{"collections":[{"abstract":"This page introduces the Kaguya Multiband Imager derived spectral and derived mineral maps by the Japan Aerospace Exploration Agency (JAXA) and the University of Hawaii. The mosaics were created from topographically-corrected MI","geoform":["Collection"],"name":"lunar-kaguya-multiband-imager-mosaics","onlink":"https://astrogeology.usgs.gov/search/map/lunar-kaguya-multiband-imager-mosaics","pubdate":"2015-01-01","thumb":"https://astrogeology.usgs.gov/ckan/dataset/a53c9dbf-e03a-4d7a-8641-fc7af97a75c2/resource/a7e1a610-f8ef-4080-99e0-1b637d6c269f/download/moon-selene-kaguya-mi-thumb.jpg","title":"Lunar Kaguya Multiband Imager Mosaics"},{"abstract":"The following products were the first step of cartography planning in support of the Cassini-Huygens mission to the Saturian System. Five of Saturans moons are linked below in a standard cartographic","geoform":["Collection"],"name":"saturn-voyager-airbrush-global-products","onlink":"https://astrogeology.usgs.gov/search/map/saturn-voyager-airbrush-global-products","pubdate":"2023-10-05","thumb":"https://astrogeology.usgs.gov/ckan/dataset/0872355e-41d2-48be-a3f3-474c571911e0/resource/fe0f7b0d-3a95-40f3-ad90-103ee20b2342/download/rhea-voyager-thumb.png","title":"Saturn Voyager Airbrush Global Products"},{"abstract":"Distributed here are control network data for solar system bodies (planets, moons, and asteroids) other than the Earth. Each control network is essentially a set of photogrammetric or radargrammetric solution (input","geoform":["Collection"],"name":"control-networks","onlink":"https://astrogeology.usgs.gov/search/map/control-networks","pubdate":null,"thumb":"https://astrogeology.usgs.gov/ckan/dataset/c14e7072-decf-4997-925f-c7f305d2dd44/resource/f41d1d4e-daa4-484b-b6e2-439a93c3af58/download/control-networks-thumb.jpeg","title":"Control Networks"},{"abstract":"This gallery features several digitized photographs from Apollo Mission explorations of the lunar surface. Anaglyph or 3D images require red-blue or red-green 3D glasses. The imagery and maps were prepared as","geoform":["Collection"],"name":"moon-apollo-anaglyph-3d-images","onlink":"https://astrogeology.usgs.gov/search/map/moon-apollo-anaglyph-3d-images","pubdate":"2023-10-20","thumb":"https://astrogeology.usgs.gov/ckan/dataset/8cd5663b-8ad1-44d4-9ef9-bac956de07a4/resource/2adf2528-8613-4545-a184-c8b31e08669f/download/apollo_stereo-thumb.jpg","title":"Moon Apollo Anaglyph 3D Images"},{"abstract":"This page features several maps showing routes the astronauts took during extravehicular activities (EVAs). The imagery and maps were prepared as part of a project by a USGS team under funding","geoform":["Collection"],"name":"moon-apollo-traverse-maps","onlink":"https://astrogeology.usgs.gov/search/map/moon-apollo-traverse-maps","pubdate":"2023-10-16","thumb":"https://astrogeology.usgs.gov/ckan/dataset/b499160d-149f-4a79-8aee-e4a09d50fb80/resource/af3a32f8-eb16-48cc-8fd4-0b0881d440d5/download/apollo14_traverse-thumb.jpg","title":"Moon Apollo Traverse Maps"},{"abstract":"The USGS Astrogeology Science Center created some of the finest cartographic products of Mars using data from Viking Oribter. Some of these products include global mosaics, north and south polar stereographic","geoform":["Collection"],"name":"mars-viking-global-products","onlink":"https://astrogeology.usgs.gov/search/map/mars-viking-global-products","pubdate":"2023-10-16","thumb":"https://astrogeology.usgs.gov/ckan/dataset/817ca072-b931-49d2-9056-c07e62c4038f/resource/9c90727e-5452-465d-9bb3-9d5a260b4607/download/mars-viking-thumb.jpg","title":"Mars Viking Global Products"},{"abstract":"The objective of this work is to assemble and cartographically control Thermal Emission Imaging System (THEMIS; Christensen et al. 2004) daytime infrared (IR) and nighttime IR images. 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The spacecraft will help scientists back on Earth study the surface and atmosphere of the dwarf planet","geoform":["Collection"],"name":"new-horizon-global-mosaics","onlink":"https://astrogeology.usgs.gov/search/map/new-horizon-global-mosaics","pubdate":"2023-10-06","thumb":"https://astrogeology.usgs.gov/ckan/dataset/ee77b8eb-73c4-48c8-8c96-8692c9f03149/resource/0e9e8592-ab83-42d5-ad64-78d683f54f34/download/pluto-new-horizon-thumb.jpg","title":"New Horizon Global Mosaics"}],"facets":{"geoform":{"facet":{"3D":4,"Airbrush":5,"Anaglyph":4,"Archive":3,"Collection":18,"Color":2,"Control Network":24,"Data":3,"Digital Elevation Model":55,"Document":18,"Geologic Map":245,"Global Mosaic":116,"Globe":9,"Grey Scale":7,"Image":46,"Landing Site Map":31,"Mineral Map":11,"Nomenclature":272,"Panorama":38,"Polar Map":6,"Poster":5,"Presentation":4,"Raster Data":431,"Regional Mosaic":622,"Remote-sensing Data":129,"Shaded-Relief Map":128,"Tabular Data":4,"Topographic Map":16,"Traverse Map":5,"Vector Data":242},"label":"Geo Format"},"mapprojn":{"facet":{"":12,"Equirectangular":86,"Lambert Conformal":240,"Mercator":214,"Orthographic":3,"Polar Stereographic":64,"Simple Cylindrical":206,"Sinusoidal":5,"Stereographic":2,"Transverse Mercator":222},"label":"Map Projection"},"missikey":{"facet":{"Apollo":55,"Artemis":2,"Cassini-Huygens":26,"Chandrayaan":1,"Clementine":11,"Dawn":9,"Galileo":36,"Kaguya":21,"Lunar Orbiter":4,"Lunar Reconnaissance Orbiter":168,"MESSENGER":26,"Magellan":76,"Mariner":3,"Mariner 9":12,"Mars 2020":7,"Mars Express":8,"Mars Global Surveyor":10,"Mars Odyssey":119,"Mars Reconnaissance Orbiter":58,"NEAR":2,"New Horizons":6,"OSIRIS-REx":2,"Viking":16,"Viking Lander":2,"Viking Orbiter":337,"Voyager":107},"label":"Mission"}},"page":null,"results":[{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed 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identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"tethys_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/tethys_nomenclature","pubdate":"2009-01-20","thumb":"https://astrogeology.usgs.gov/ckan/dataset/4143d203-4fc1-4691-a8cb-65f5976bf98f/resource/9e4683e0-929a-4cd2-84a2-96d7f94e6c89/download/thumb.png","title":"Tethys Nomenclature"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed 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(Hargitai","geoform":["Nomenclature"],"name":"titan_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/titan_nomenclature","pubdate":"2017-09-15","thumb":"https://astrogeology.usgs.gov/ckan/dataset/a339f989-d5a0-4244-bc3c-3e36cb6e2fd1/resource/0fdc6bad-5acd-42da-a2a3-a63b744243dd/download/thumb.png","title":"Titan Nomenclature"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"triton_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/triton_nomenclature","pubdate":"2013-03-22","thumb":"https://astrogeology.usgs.gov/ckan/dataset/5435ceb4-ccc7-402d-ac74-f541ef46b26b/resource/bb47084d-fad9-4127-ae32-a6df1349a4b8/download/thumb.png","title":"Triton Nomenclature"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"umbriel_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/umbriel_nomenclature","pubdate":"2013-03-22","thumb":"https://astrogeology.usgs.gov/ckan/dataset/1f433305-416a-481b-96cd-0c97a870fa9a/resource/e74c8c68-7106-4b56-96d9-eedc29224d03/download/thumb.png","title":"Umbriel Nomenclature"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"vesta_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/vesta_nomenclature","pubdate":"2014-10-07","thumb":"https://astrogeology.usgs.gov/ckan/dataset/56966deb-f918-4e24-981f-87392896ba19/resource/e6919dc3-5300-414d-b624-867ab72694c8/download/thumb.png","title":"Vesta Nomenclature"},{"abstract":"","geoform":["Image"],"name":"moc_movie_showing_seasonal_variations","onlink":"https://astrogeology.usgs.gov/search/map/moc_movie_showing_seasonal_variations","pubdate":null,"thumb":"https://astrogeology.usgs.gov/ckan/dataset/dbbe5e52-6eb7-4dae-b887-1c8ceaa6f60c/resource/1a948570-82bc-4ac8-a96a-63ec11b4fc6a/download/thumb.png","title":"MOC movie showing seasonal variations"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"miranda_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/miranda_nomenclature","pubdate":"2020-01-31","thumb":"https://astrogeology.usgs.gov/ckan/dataset/b4edafac-65b1-43ec-8feb-67f4bc4ede2d/resource/a8d6d37b-9ae4-4e07-8916-8c2731bb5943/download/thumb.png","title":"Miranda Nomenclature"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"mimas_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/mimas_nomenclature","pubdate":"2010-07-13","thumb":"https://astrogeology.usgs.gov/ckan/dataset/9ed3ca4a-cc5d-4121-a5cf-4927b8918260/resource/533bc0cd-8fda-4287-9c65-2194a67d781b/download/thumb.png","title":"Mimas Nomenclature"},{"abstract":"","geoform":["Global 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The elevated","geoform":["Geologic Map","Raster Data","Vector Data"],"name":"venus_geologic_map_of_the_lakshmi_planum_quadrangle","onlink":"https://astrogeology.usgs.gov/search/map/venus_geologic_map_of_the_lakshmi_planum_quadrangle","pubdate":"2010-02-10","thumb":"https://astrogeology.usgs.gov/ckan/dataset/74f9d9be-78b3-4531-af4c-15dc3be74af5/resource/6bfbadfb-c82b-4b45-b83a-65ab5046a1dc/download/thumb.png","title":"Venus Geologic Map of the Lakshmi Planum Quadrangle"},{"abstract":"","geoform":["Geologic Map","Raster Data","Vector Data"],"name":"io_geologic_map_of_the_lerna_region","onlink":"https://astrogeology.usgs.gov/search/map/io_geologic_map_of_the_lerna_region","pubdate":"2021-12-30","thumb":"https://astrogeology.usgs.gov/ckan/dataset/6c4edc37-cc44-4a9b-abfd-5605d30388ae/resource/fe9839be-62fa-4c2b-8923-73622d0f2999/download/thumb.png","title":"Io Geologic Map of the Lerna Region"},{"abstract":"Introduction The Lavinia Planitia quadrangle (V-55) is in the southern hemisphere of Venus and extends from 25 to 50 south latitude and from 330 to 360 longitude. It covers the central and","geoform":["Geologic Map","Raster Data","Vector Data"],"name":"venus_geologic_map_of_the_lavinia_planitia_quadrangle","onlink":"https://astrogeology.usgs.gov/search/map/venus_geologic_map_of_the_lavinia_planitia_quadrangle","pubdate":"2001-01-01","thumb":"https://astrogeology.usgs.gov/ckan/dataset/21fe4cf0-a705-4cc4-b84a-75a0255e5035/resource/47c9f057-4549-43fb-8e8a-fcee43a80cdb/download/thumb.png","title":"Venus Geologic Map of the Lavinia Planitia Quadrangle"},{"abstract":"The Magellan spacecraft orbited Venus from August 10, 1990, until it plunged into the Venusian atmosphere on October 12, 1994. 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Magellan Mission objectives included (1) improving the knowledge of the geological processes,","geoform":["Geologic Map","Raster Data","Vector Data"],"name":"venus_geologic_map_of_the_mead_quadrangle","onlink":"https://astrogeology.usgs.gov/search/map/venus_geologic_map_of_the_mead_quadrangle","pubdate":"2006-01-06","thumb":"https://astrogeology.usgs.gov/ckan/dataset/2bcd1596-786f-4358-90e5-1e127ec9b783/resource/51b8961d-334c-4c3d-a6f4-901fb70c75d9/download/thumb.png","title":"Venus Geologic Map of the Mead Quadrangle"},{"abstract":"The Magellan spacecraft orbited Venus from August 10, 1990, until it plunged into the Venusian atmosphere on October 12, 1994. Magellan Mission objectives included (1) improving the knowledge of the geological processes,","geoform":["Geologic Map","Raster Data","Vector Data"],"name":"venus_geologic_map_of_the_sif_mons_quadrangle","onlink":"https://astrogeology.usgs.gov/search/map/venus_geologic_map_of_the_sif_mons_quadrangle","pubdate":"2007-01-07","thumb":"https://astrogeology.usgs.gov/ckan/dataset/8ad16313-6d63-48d9-aa11-ecea5d6aaa70/resource/83d80021-3193-4613-9404-09d74fe2306b/download/thumb.png","title":"Venus Geologic Map of the Sif Mons Quadrangle"},{"abstract":"The Greenaway quadrangle (V-24; lat 0 degrees -25 degrees N., long 120 degrees -150 degrees E.), Venus, derives its name from the impact crater Greenaway, centered at lat 22.9 degrees N., long","geoform":["Geologic Map","Raster Data","Vector 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Along with the uplifted rim and huge,","geoform":["Geologic Map","Raster Data","Vector Data"],"name":"mars_geologic_map_of_the_hellas_region","onlink":"https://astrogeology.usgs.gov/search/map/mars_geologic_map_of_the_hellas_region","pubdate":"2001-01-01","thumb":"https://astrogeology.usgs.gov/ckan/dataset/59019a4d-cf38-4f7c-b936-02d0f45e2bed/resource/28596e7b-2290-4819-8000-128fafb1a168/download/thumb.png","title":"Mars Geologic Map of the Hellas Region"},{"abstract":"Introduction Rock units were deposited on Mars by meteorite impact, volcanism, wind, flowing water, standing water, and ice, acting separately or in concert. Hellas Planitia, the deepest tract on Mars, is a","geoform":["Geologic Map","Raster Data","Vector Data"],"name":"mars_geologic_map_of_part_of_western_hellas_planitia","onlink":"https://astrogeology.usgs.gov/search/map/mars_geologic_map_of_part_of_western_hellas_planitia","pubdate":"2007-01-07","thumb":"https://astrogeology.usgs.gov/ckan/dataset/957da65c-2f5f-4585-b828-160adbdc9b18/resource/60716230-033a-4778-90c4-b85f5a3cd70c/download/thumb.png","title":"Mars Geologic Map of Part of Western Hellas Planitia"},{"abstract":"The northern plains of Mars cover nearly a third of the planet and constitute the planet's broadest region of lowlands. Apparently formed early in Mars' history, the northern lowlands served as a","geoform":["Geologic Map","Raster Data","Vector Data"],"name":"mars_geologic_map_of_the_northern_plains","onlink":"https://astrogeology.usgs.gov/search/map/mars_geologic_map_of_the_northern_plains","pubdate":"2005-01-05","thumb":"https://astrogeology.usgs.gov/ckan/dataset/5ba03530-5c08-4406-b4bb-177ab6e1fa21/resource/036a8bbb-d134-4a23-923c-58c95ffe9a25/download/thumb.png","title":"Mars Geologic Map of the Northern Plains"},{"abstract":"The north polar region of Mars occurs within the central and lowest part of the vast northern plains of Mars and is dominated by the roughly circular north polar plateau, Planum Boreum.","geoform":["Geologic Map","Polar Map","Raster Data","Vector Data"],"name":"mars_geologic_map_of_the_north_polar_region","onlink":"https://astrogeology.usgs.gov/search/map/mars_geologic_map_of_the_north_polar_region","pubdate":"2012-02-12","thumb":"https://astrogeology.usgs.gov/ckan/dataset/83516f10-1634-4f93-b6c8-ed6093636d04/resource/68c7ff90-e1a6-456a-a4ac-ea0d201ea383/download/thumb.png","title":"Mars Geologic Map of the North Polar Region"},{"abstract":"","geoform":["Geologic Map","Raster Data","Vector Data"],"name":"mars_geologic_map_of_the_tempe_mareotis_region","onlink":"https://astrogeology.usgs.gov/search/map/mars_geologic_map_of_the_tempe_mareotis_region","pubdate":"2001-01-01","thumb":"https://astrogeology.usgs.gov/ckan/dataset/47f1490e-4aa8-41bd-b6bd-ec338db33ce0/resource/7de48809-71db-46d5-9e74-1559ce2fb7b8/download/thumb.png","title":"Mars Geologic Map of the Tempe-Mareotis Region"},{"abstract":"The Metis Mons quadrangle (V6) in the northern hemisphere of Venus (lat 50\u00b0 to 75\u00b0 N., long 240\u00b0 to 300\u00b0 E.) includes a variety of coronae, large volcanoes, ridge and fracture (structure)","geoform":["Geologic Map","Raster Data","Vector Data"],"name":"venus_geologic_map_of_the_metis_mons_quadrangle","onlink":"https://astrogeology.usgs.gov/search/map/venus_geologic_map_of_the_metis_mons_quadrangle","pubdate":"2011-02-11","thumb":"https://ckan.astrogeology.usgs.gov/ckan/dataset/10dc0bda-32eb-4d42-9d22-561228364097/resource/9b350418-8bb6-4809-aafa-1af5e9309d88/download/venus-geologic-map-of-the-metis-mons-quadrangle-v-6-thumb.jpg","title":"Venus Geologic Map of the Metis Mons Quadrangle"},{"abstract":"The Snegurochka Planitia region is a predominantly low-lying terrain that covers the north polar region of Venus, extending from lat 75\u00b0 N. to 90\u00b0 N. and from long 0\u00b0 E. to 360\u00b0","geoform":["Geologic Map","Raster Data","Vector Data"],"name":"venus_geologic_map_of_the_snegurochka_planitia_quadrangle","onlink":"https://astrogeology.usgs.gov/search/map/venus_geologic_map_of_the_snegurochka_planitia_quadrangle","pubdate":"2012-02-12","thumb":"https://astrogeology.usgs.gov/ckan/dataset/d9ab239f-d43e-4fe5-8ca6-2682d01effdf/resource/da0f5030-ceb5-4f9b-bf27-a84d2960d125/download/venus-geologic-map-of-the-snegurochka-planitia-quadrangle-v-1-thumb.jpg","title":"Venus Geologic Map of the Snegurochka Planitia Quadrangle"},{"abstract":"The Themis Regio quadrangle (V-53), Venus, has been geologically mapped at 1:5,000,000 scale as part of the NASA Planetary Geologic Mapping Program. The quadrangle extends from lat 25\u00b0 to 50\u00b0 S. and","geoform":["Geologic Map","Raster Data","Vector Data"],"name":"venus_geologic_map_of_the_themis_regio_quadrangle","onlink":"https://astrogeology.usgs.gov/search/map/venus_geologic_map_of_the_themis_regio_quadrangle","pubdate":"2012-02-12","thumb":"https://ckan.astrogeology.usgs.gov/ckan/dataset/e7b6c0ce-ee0c-4f6a-b984-0425f014f663/resource/0c9dbf68-54fc-434f-9187-901cc68c07d8/download/thumb.png","title":"Venus Geologic Map of the Themis Regio Quadrangle"},{"abstract":"This publication provides a geological map of Lada Terra quadrangle (V56), a portion of the southern hemisphere of Venus that extends from lat 50\u00b0 S. to 70\u00b0 S. and from long 0\u00b0","geoform":["Geologic Map"],"name":"venus_geologic_map_of_the_lada_terra_quadrangle","onlink":"https://astrogeology.usgs.gov/search/map/venus_geologic_map_of_the_lada_terra_quadrangle","pubdate":"2013-02-13","thumb":"https://ckan.astrogeology.usgs.gov/ckan/dataset/18c58974-6948-4004-a287-d765180641b0/resource/08ed045a-7f1d-47f0-8d1f-d0dd2c2341b0/download/venus-geologic-map-of-the-lada-terra-quadrangle-v-56-thumb.jpg","title":"Venus Geologic Map of the Lada Terra Quadrangle"},{"abstract":"","geoform":["Geologic Map","Raster Data","Vector Data"],"name":"moon_geologic_map_of_the_geminus_quadrangle","onlink":"https://astrogeology.usgs.gov/search/map/moon_geologic_map_of_the_geminus_quadrangle","pubdate":"1974-10-13","thumb":"https://astrogeology.usgs.gov/ckan/dataset/77514efe-78b5-4b9e-8ae5-d4eb38b4115a/resource/1f073c33-94b2-4e36-a164-f74543171db8/download/thumb.png","title":"Moon Geologic Map of the Geminus Quadrangle"},{"abstract":"Ganymede is the largest (~5,200 km diameter) known satellite in the Solar System and the third Galilean satellite outward from Jupiter. Its density (1.93 g/cm3) and surface spectral characteristics indicate that its","geoform":["Geologic Map","Raster Data","Vector Data"],"name":"ganymede_geologic_map_of_the_osiris_quadrangles","onlink":"https://astrogeology.usgs.gov/search/map/ganymede_geologic_map_of_the_osiris_quadrangles","pubdate":"1998-01-05","thumb":"https://astrogeology.usgs.gov/ckan/dataset/d00c9db3-c952-4688-bbee-4d6bfc8fbb70/resource/cff31baf-6793-46c9-b4f9-c48c43ff779e/download/thumb.png","title":"Ganymede Geologic Map of the Osiris Quadrangles"},{"abstract":"Ganymede is the largest (~5,200 km diameter) known satellite in the Solar System and the third Galilean satellite outward from Jupiter. Its density (1.93 g/cm3) and surface spectral characteristics indicate that its","geoform":["Geologic Map","Raster Data","Vector Data"],"name":"ganymede_geologic_map_of_the_hathor_region","onlink":"https://astrogeology.usgs.gov/search/map/ganymede_geologic_map_of_the_hathor_region","pubdate":"1995-01-02","thumb":"https://astrogeology.usgs.gov/ckan/dataset/3028c753-c420-4ad0-b5d2-e8ab595a1413/resource/e2e94441-30ec-4574-a786-d17fc8719589/download/thumb.png","title":"Ganymede Geologic Map of the Hathor Region"},{"abstract":"Ganymede is the largest (~5,200 km diameter) known satellite in the Solar System and the third Galilean satellite outward from Jupiter. Its density (1.93 g/cm3) and surface spectral characteristics indicate that its","geoform":["Geologic Map","Raster Data","Vector Data"],"name":"ganymede_geologic_map_of_the_tiamat_sulcus_quadrangle","onlink":"https://astrogeology.usgs.gov/search/map/ganymede_geologic_map_of_the_tiamat_sulcus_quadrangle","pubdate":null,"thumb":"https://astrogeology.usgs.gov/ckan/dataset/259fc483-81aa-4d02-aa3e-798334c2776c/resource/4f916e6f-3f30-4dd8-b27e-5d2fb947e20b/download/thumb.png","title":"Ganymede Geologic Map of the Tiamat Sulcus Quadrangle"},{"abstract":"Ganymede is the largest (~5,200 km diameter) known satellite in the Solar System and the third Galilean satellite outward from Jupiter. Its density (1.93 g/cm3) and surface spectral characteristics indicate that its","geoform":["Geologic Map","Raster Data","Vector Data"],"name":"ganymede_geologic_map_of_the_perrine_quadrangles","onlink":"https://astrogeology.usgs.gov/search/map/ganymede_geologic_map_of_the_perrine_quadrangles","pubdate":"1998-01-05","thumb":"https://astrogeology.usgs.gov/ckan/dataset/47618293-e331-4310-adfe-2037b8c59c33/resource/54f68fab-3dd1-445c-873d-6d9a12c4e8e7/download/thumb.png","title":"Ganymede Geologic Map of the Perrine Quadrangles"},{"abstract":"Ganymede is the largest (~5,200 km diameter) known satellite in the Solar System and the third Galilean satellite outward from Jupiter. Its density (1.93 g/cm3) and surface spectral characteristics indicate that its","geoform":["Geologic Map","Raster Data","Vector Data"],"name":"ganymede_geologic_map_of_the_philus_sulcus_quadrangle","onlink":"https://astrogeology.usgs.gov/search/map/ganymede_geologic_map_of_the_philus_sulcus_quadrangle","pubdate":null,"thumb":"https://astrogeology.usgs.gov/ckan/dataset/669b7c13-80dc-4a1c-b3de-014109cfd956/resource/0f1e5314-90fc-44e1-bc8a-3be740ee62dc/download/thumb.png","title":"Ganymede Geologic Map of the Philus Sulcus Quadrangle"},{"abstract":"Ganymede is the largest (~5,200 km diameter) known satellite in the Solar System and the third Galilean satellite outward from Jupiter. Its density (1.93 g/cm3) and surface spectral characteristics indicate that its","geoform":["Geologic Map","Raster Data","Vector Data"],"name":"ganymede_geologic_map_of_the_uruk_sulcus_quadrangle","onlink":"https://astrogeology.usgs.gov/search/map/ganymede_geologic_map_of_the_uruk_sulcus_quadrangle","pubdate":null,"thumb":"https://astrogeology.usgs.gov/ckan/dataset/3268d1ee-e733-4452-b271-8cde7aa872cb/resource/0d5d3005-c4e9-4f1a-a310-af68f3c8f5ea/download/thumb.png","title":"Ganymede Geologic Map of the Uruk Sulcus Quadrangle"},{"abstract":"","geoform":["Global Mosaic"],"name":"ganymede_preliminary_pictorial_map","onlink":"https://astrogeology.usgs.gov/search/map/ganymede_preliminary_pictorial_map","pubdate":"1979-12-31","thumb":"https://astrogeology.usgs.gov/ckan/dataset/776a8845-aa04-4565-b1bb-996ba7990e92/resource/3fbd4f87-4bd2-41e4-ba50-18d9b9ce2104/download/thumb.png","title":"Ganymede Preliminary Pictorial Map"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"ganymede_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/ganymede_nomenclature","pubdate":"2016-07-11","thumb":"https://astrogeology.usgs.gov/ckan/dataset/5ffdee5e-8722-465d-a3d1-5dbba9a568f5/resource/cb338d68-e7d1-4464-a957-224e9b18afb8/download/thumb.png","title":"Ganymede Nomenclature"},{"abstract":"The Ganiki Planitia (V-14) quadrangle on Venus, which extends from 25\u00c2\u00b0 N. to 50\u00c2\u00b0 N. and from 180\u00c2\u00b0 E. to 210\u00c2\u00b0 E., derives its name from the extensive suite of plains that","geoform":["Geologic Map","Raster Data","Vector Data"],"name":"venus_geologic_map_of_the_ganiki_planitia_quadrangle","onlink":"https://astrogeology.usgs.gov/search/map/venus_geologic_map_of_the_ganiki_planitia_quadrangle","pubdate":"2011-02-11","thumb":"https://astrogeology.usgs.gov/ckan/dataset/59fe7e04-4111-4238-90f9-8073f30c72d4/resource/2415e4ca-e96f-4179-a4a0-784433640057/download/venus-geologic-map-of-the-ganiki-planitia-quadrangle-v-14-thumb.jpg","title":"Venus Geologic Map of the Ganiki Planitia Quadrangle"},{"abstract":"The Magellan spacecraft orbited Venus from August 10, 1990, until it plunged into the venusian atmosphere on October 12, 1994. Magellan had the objectives of (1) improving knowledge of the geologic processes,","geoform":["Geologic Map","Raster Data","Vector Data"],"name":"venus_geologic_geomorphic_map_of_the_galindo_quadrangle","onlink":"https://astrogeology.usgs.gov/search/map/venus_geologic_geomorphic_map_of_the_galindo_quadrangle","pubdate":"2000-01-07","thumb":"https://astrogeology.usgs.gov/ckan/dataset/c728b8e4-1f6d-466d-9467-1d3ed7f52291/resource/2fb44793-70b3-4385-b18b-a546b5fe6038/download/thumb.png","title":"Venus Geologic Geomorphic Map of the Galindo Quadrangle"},{"abstract":"Ganymede is the largest (~5,200 km diameter) known satellite in the Solar System and the third Galilean satellite outward from Jupiter. Its density (1.93 g/cm3) and surface spectral characteristics indicate that its","geoform":["Geologic Map","Raster Data","Vector Data"],"name":"ganymede_geologic_map_of_the_galileo_regio_quadrangle","onlink":"https://astrogeology.usgs.gov/search/map/ganymede_geologic_map_of_the_galileo_regio_quadrangle","pubdate":"1998-01-05","thumb":"https://astrogeology.usgs.gov/ckan/dataset/2d39c2ec-acb3-4b9d-8500-5f52915a00a9/resource/e72cb39a-0f06-4257-b9a3-0913723f531a/download/thumb.png","title":"Ganymede Geologic Map of the Galileo Regio Quadrangle"},{"abstract":"This global map base of Ganymede utilizes the best image quality and moderate resolution coverage supplied by Galileo SSI (Solid State Imaging instrument) and Voyager 1 and 2. The image processing was","geoform":["Global Mosaic"],"name":"ganymede_voyager_galileo_south_polar_stereographic","onlink":"https://astrogeology.usgs.gov/search/map/ganymede_voyager_galileo_south_polar_stereographic","pubdate":null,"thumb":"https://astrogeology.usgs.gov/ckan/dataset/c69f2f2f-386f-44ae-9fea-11345e19f158/resource/d9bb5154-1e60-4aa3-a15d-9d8e1825c0aa/download/thumb.png","title":"Ganymede Voyager / Galileo South Polar Stereographic"},{"abstract":"This global map base of Ganymede utilizes the best image quality and moderate resolution coverage supplied by Galileo SSI (Solid State Imaging instrument) and Voyager 1 and 2. The image processing was","geoform":["Global Mosaic"],"name":"ganymede_voyager_galileo_north_polar_stereographic","onlink":"https://astrogeology.usgs.gov/search/map/ganymede_voyager_galileo_north_polar_stereographic","pubdate":null,"thumb":"https://astrogeology.usgs.gov/ckan/dataset/4037109c-c86c-47b5-8388-ce0776a2995b/resource/9cc2fa80-71b6-4451-8c62-12afe21edbd8/download/thumb.png","title":"Ganymede Voyager / Galileo North Polar Stereographic"},{"abstract":"This global map base of Ganymede utilizes the best image quality and moderate resolution coverage supplied by Galileo SSI (Solid State Imaging instrument) and Voyager 1 and 2. The image processing was","geoform":["Global Mosaic"],"name":"ganymede_voyager_galileo_global_mosaic_mercator","onlink":"https://astrogeology.usgs.gov/search/map/ganymede_voyager_galileo_global_mosaic_mercator","pubdate":null,"thumb":"https://astrogeology.usgs.gov/ckan/dataset/bc2ebb05-4e2d-4542-8449-f561450aa4d2/resource/42a1057b-0d94-499f-b89b-043ff2475a17/download/thumb.png","title":"Ganymede Voyager / Galileo Global Mosaic Mercator"},{"abstract":"The images used for the base of this globe were chosen from coverage supplied by the Galileo solid-state imaging (SSI) camera and Voyager 1 and 2 spacecraft. The monochrome and color data","geoform":["Global Mosaic","Globe"],"name":"ganymede_voyager_galileo_image_mosaic_globe","onlink":"https://astrogeology.usgs.gov/search/map/ganymede_voyager_galileo_image_mosaic_globe","pubdate":null,"thumb":"https://astrogeology.usgs.gov/ckan/dataset/8c47a7c4-933b-4e0c-8218-b34277770c59/resource/f4762b3b-7c03-4675-83e2-fb8ff340ffde/download/thumb.png","title":"Ganymede Voyager Galileo Image Mosaic Globe"},{"abstract":"A global monochrome mosaic of the best resolution images from both Galileo and Voyager 1 was created that includes 51 Voyager 1 images with spatial resolutions sometimes exceeding the 1 km/pixel scale","geoform":["Global Mosaic","Globe"],"name":"io_voyager_galileo_image_mosaic_globe","onlink":"https://astrogeology.usgs.gov/search/map/io_voyager_galileo_image_mosaic_globe","pubdate":null,"thumb":"https://astrogeology.usgs.gov/ckan/dataset/11dcdc82-4269-4ba9-82fa-61969f4fe9d9/resource/07edb545-3d72-427a-a627-e1eb7c2985d9/download/thumb.png","title":"Io Voyager / Galileo Image Mosaic Globe"},{"abstract":"The Galaxias region (MTM 35217) is one of a series of 1:500,000-scale science study areas on Mars sponsored by NASA's Planetary Geology and Geophysics Program. Situated near the northern limit of lava","geoform":["Geologic Map","Raster Data","Vector Data"],"name":"mars_geologic_map_of_the_galaxias_quadrangle","onlink":"https://astrogeology.usgs.gov/search/map/mars_geologic_map_of_the_galaxias_quadrangle","pubdate":"2000-01-07","thumb":"https://astrogeology.usgs.gov/ckan/dataset/5e5d2497-084c-4466-b1c9-26dc8e3befb2/resource/04dae3d7-a24b-44e1-bf7d-8680303353fa/download/thumb.png","title":"Mars Geologic Map of the Galaxias Quadrangle"},{"abstract":"","geoform":["Geologic Map","Raster Data","Vector Data"],"name":"moon_geologic_map_of_the_maestlin_g_region","onlink":"https://astrogeology.usgs.gov/search/map/moon_geologic_map_of_the_maestlin_g_region","pubdate":"1969-09-07","thumb":"https://astrogeology.usgs.gov/ckan/dataset/f9ca1cbf-0e7f-4980-bd55-697184559cdb/resource/c03c67a8-0848-4b6d-8a5c-a4c2b33cf3a9/download/thumb.png","title":"Moon Geologic Map of the Maestlin G Region"},{"abstract":"","geoform":["Geologic Map","Raster Data","Vector 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Prior to NASA’s Dawn mission, the dwarf planet Ceres was widely believed to contain a substantial ice-rich layer below its rocky surface. 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Quadrangle"},{"abstract":"","geoform":["Regional Mosaic"],"name":"mars_controlled_photomosaic_of_the_thaumasia_southwest_quadrangle","onlink":"https://astrogeology.usgs.gov/search/map/mars_controlled_photomosaic_of_the_thaumasia_southwest_quadrangle","pubdate":"1984-11-23","thumb":"https://astrogeology.usgs.gov/ckan/dataset/d618abdc-24ec-4a11-8972-e5dd4477de0a/resource/57cb7a8c-441b-4125-aa7e-d6ea379d3ecb/download/thumb.png","title":"Mars Controlled Photomosaic of the Thaumasia Southwest Quadrangle"},{"abstract":"","geoform":["Regional Mosaic"],"name":"mars_controlled_photomosaic_of_the_thaumasia_northwest_quadrangle","onlink":"https://astrogeology.usgs.gov/search/map/mars_controlled_photomosaic_of_the_thaumasia_northwest_quadrangle","pubdate":"1980-11-19","thumb":"https://astrogeology.usgs.gov/ckan/dataset/ab7fdf58-fb3b-447b-9a8e-f791a4bdba83/resource/0eb75553-e3c0-4c04-a685-0e81ab4b078e/download/thumb.png","title":"Mars Controlled Photomosaic of the Thaumasia Northwest Quadrangle"},{"abstract":"

This page has been created as part of a project to put planetary control networks on the web. This control network for asteroid 243 Ida originated from Merton Davies and Tim Colvin","geoform":["Control Network"],"name":"ida_image_control_network","onlink":"https://astrogeology.usgs.gov/search/map/ida_image_control_network","pubdate":null,"thumb":"https://astrogeology.usgs.gov/ckan/dataset/1dc57ae5-68de-456c-988b-a73a76469a23/resource/2cbf3c4b-a874-474b-9a45-c0ca8d22bdfc/download/ida_100.jpg","title":"Ida Image Control Network"},{"abstract":"This product is a cartographically controlled mosaic of Mars Charts (MC) 08 through 23, covering 50.0 percent of Mars' surface, from -30 deg N to +30 deg N latitude and 0\u00e2\u0080\u0093360 deg","geoform":["Raster Data","Regional Mosaic","Remote-sensing Data"],"name":"mars_ctx_controlled_equatorial_mosaics","onlink":"https://astrogeology.usgs.gov/search/map/mars_ctx_controlled_equatorial_mosaics","pubdate":"2023-12-20","thumb":"https://astrogeology.usgs.gov/ckan/dataset/43673811-b1f8-4e15-a238-4e838dd038f2/resource/95266fde-3880-46d0-b14e-a8ad1a79a1ff/download/thumb.png","title":"Mars CTX Controlled Equatorial Mosaics"},{"abstract":"

This page has been created as part of a project to put planetary control networks on the web. This control network for asteroid 951 Gaspra originated from Merton Davies and Tim Colvin","geoform":["Control Network"],"name":"gaspra_image_control_network","onlink":"https://astrogeology.usgs.gov/search/map/gaspra_data_zip","pubdate":null,"thumb":"https://astrogeology.usgs.gov/ckan/dataset/9fb8c04d-5a2c-4ed3-b6c3-a9740bc4ceb3/resource/814409b9-9fea-4dab-8f87-5df3998efe52/download/gaspa_100.jpg","title":"Gaspra Image Control Network"},{"abstract":"

This page has been created as part of a project to put planetary control networks on the web. This control network for Venus originated from Merton Davies, Tim Colvin and others, and","geoform":["Control Network"],"name":"venus_magellan_control_network","onlink":"https://astrogeology.usgs.gov/search/map/venus_magellan_control_network","pubdate":null,"thumb":"https://astrogeology.usgs.gov/ckan/dataset/b085eccc-2248-4e16-a6a7-950b9e055f2d/resource/72cd32eb-591b-457c-ab0d-c49f9caa4c59/download/venusmap_100.jpg","title":"Venus Magellan Control Network"},{"abstract":"

This page has been created as part of a project to put planetary control networks on the web. These control network measurements for Saturn\u00e2\u0080\u0099s moon, Hyperion, originated from Merton Davies and Tim","geoform":["Control Network"],"name":"hyperion_image_control_network","onlink":"https://astrogeology.usgs.gov/search/map/hyperion_image_control_network","pubdate":null,"thumb":"https://astrogeology.usgs.gov/ckan/dataset/b51e2056-513d-47af-88c3-0104dfaf2495/resource/582a97e9-ff7c-464a-9f1d-b34347f23ad0/download/hyperion_voyager.jpg","title":"Hyperion Image Control Network"},{"abstract":"Lunar Orbiter Lunar Control Network 2004: The USGS worked to digitize and restore a global set of Lunar Orbiter images and to assemble this into a global digital Lunar Orbiter mosaic of","geoform":["Control Network"],"name":"unified_lunar_control_network_solution_output_files","onlink":"https://astrogeology.usgs.gov/search/map/unified_lunar_control_network_solution_output_files","pubdate":null,"thumb":"https://astrogeology.usgs.gov/ckan/dataset/20fd9c30-76db-4116-84cf-7bda7624f848/resource/837c60e5-7960-4ec8-a24d-baee1333949e/download/ulcn-thumb.jpg","title":"Unified Lunar Control Network solution output files"},{"abstract":"Positional control for the MDIM 2.1 global mosaic came from a geodetic/photogrammetric solution of the global Mars Mariner 9 and Viking image control network. The details of this network solution are described","geoform":["Control Network"],"name":"mars-image-control-network","onlink":"https://astrogeology.usgs.gov/search/map/mars-image-control-network","pubdate":null,"thumb":"https://astrogeology.usgs.gov/ckan/dataset/dafdc7b5-7e22-4a2e-997c-05cdff4927b7/resource/be16e9c2-860b-4db6-aff1-4d0c3decba3f/download/arcglobe_mola_tracks-thumb.jpg","title":"Mars Image Control Network"},{"abstract":"Distributed here are control network data for solar system bodies (planets, moons, and asteroids) other than the Earth. Each control network is essentially a set of photogrammetric or radargrammetric solution (input","geoform":["Collection"],"name":"control-networks","onlink":"https://astrogeology.usgs.gov/search/map/control-networks","pubdate":null,"thumb":"https://astrogeology.usgs.gov/ckan/dataset/c14e7072-decf-4997-925f-c7f305d2dd44/resource/f41d1d4e-daa4-484b-b6e2-439a93c3af58/download/control-networks-thumb.jpeg","title":"Control Networks"},{"abstract":"The Solid State Imager (SSI) on NASA's Galileo spacecraft acquired more than 500 images of Jupiter's moon, Europa, providing the only moderate- to high-resolution images of the moon's surface. Images were acquired","geoform":["Regional Mosaic"],"name":"photogrammetrically_controlled_galileo_image_mosaics_of_europa","onlink":"https://astrogeology.usgs.gov/search/map/photogrammetrically_controlled_galileo_image_mosaics_of_europa","pubdate":"2021-03-22","thumb":"https://astrogeology.usgs.gov/ckan/dataset/cc38d1df-db15-41f3-90d6-4e63e3c4420f/resource/622a0c7f-c382-4c5d-9c3b-fa1306f7e154/download/europa_mosaic_thumbnail_100.jpg","title":"Photogrammetrically Controlled Galileo Image Mosaics of Europa"},{"abstract":"

This archive has been created as part of a project to put planetary control networks on the web. These control networks originated from the RAND corporation (Merton Davies and Tim Colvin) and","geoform":["Control Network"],"name":"dione_voyager_image_control_network","onlink":"https://astrogeology.usgs.gov/search/map/dione_voyager_image_control_network","pubdate":"2025-04-01","thumb":"https://astrogeology.usgs.gov/ckan/dataset/f3415e7b-a190-4675-b4de-f8cededdce66/resource/1be4480b-5fb0-4ca6-bf9f-fd185c57a265/download/dione-control-network-100.jpg","title":"Dione Voyager Image Control Network"},{"abstract":"

This archive has been created as part of a project to put planetary control networks on the web. These control networks originated from the RAND corporation (Merton Davies and Tim Colvin) and","geoform":["Control Network"],"name":"ganymede_voyager_image_control_network","onlink":"https://astrogeology.usgs.gov/search/map/ganymede_voyager_image_control_network","pubdate":"2025-04-01","thumb":"https://astrogeology.usgs.gov/ckan/dataset/d0b5b3e2-b755-422b-92c9-b32724feb5de/resource/5176ace4-86f5-4c8d-93f1-b861a5c8512d/download/ganymede_controlled-100.jpg","title":"Ganymede Voyager Image Control Network"},{"abstract":"

This archive has been created as part of a project to put planetary control networks on the web. These control networks originated from the RAND corporation (Merton Davies and Tim Colvin) and","geoform":["Control Network"],"name":"enceladus_voyager_image_control_network","onlink":"https://astrogeology.usgs.gov/search/map/enceladus_voyager_image_control_network","pubdate":"2025-04-01","thumb":"https://astrogeology.usgs.gov/ckan/dataset/9294baf9-d267-4f77-a5e7-3f714db47349/resource/7dc67e8f-4347-4650-9e73-473d607acbd3/download/enceladus_photomosaic_100.jpg","title":"Enceladus Voyager Image Control Network"},{"abstract":"

This archive has been created as part of a project to put planetary control networks on the web. These control networks originated from the RAND corporation (Merton Davies and Tim Colvin) and","geoform":["Control Network"],"name":"tethys_voyager_image_control_network","onlink":"https://astrogeology.usgs.gov/search/map/tethys_voyager_image_control_network","pubdate":"2025-04-01","thumb":"https://astrogeology.usgs.gov/ckan/dataset/91ea2858-8830-4f7a-9cbc-90b601f5ada2/resource/07f90f06-0cb8-40fd-b0d1-233365db298f/download/tethys_photomosaic_100.jpg","title":"Tethys Voyager Image Control Network"},{"abstract":"

This archive has been created as part of a project to put planetary control networks on the web. These control networks originated from the RAND corporation (Merton Davies and Tim Colvin) and","geoform":["Control Network"],"name":"iapetus_voyager_image_control_network","onlink":"https://astrogeology.usgs.gov/search/map/iapetus_voyager_image_control_network","pubdate":"2025-04-01","thumb":"https://astrogeology.usgs.gov/ckan/dataset/6abd15c6-8b5d-43e3-9ca5-2ed92994cacf/resource/5facab0f-12cf-441d-8c04-1555b5f66693/download/iapetus_photomosaic_100.jpg","title":"Iapetus Voyager Image Control Network"},{"abstract":"

This archive has been created as part of a project to put planetary control networks on the web. These control networks originated from the RAND corporation (Merton Davies and Tim Colvin) and","geoform":["Control Network"],"name":"rhea_voyager_image_control_network","onlink":"https://astrogeology.usgs.gov/search/map/rhea_voyager_image_control_network","pubdate":"2025-04-01","thumb":"https://astrogeology.usgs.gov/ckan/dataset/f7389346-18c6-4690-b257-1f97de636a1a/resource/a883d5ce-833a-437f-9fc9-ecd836eeaf58/download/rhea_photomosaics_100.jpg","title":"Rhea Voyager Image Control Network"},{"abstract":"

This archive has been created as part of a project to put planetary control networks on the web. These control networks originated from the RAND corporation (Merton Davies and Tim Colvin) and","geoform":["Control Network"],"name":"io_voyager_image_control_network","onlink":"https://astrogeology.usgs.gov/search/map/io_voyager_image_control_network","pubdate":"2025-04-01","thumb":"https://astrogeology.usgs.gov/ckan/dataset/cdd61d89-27e9-424a-9ed5-cc3bb74c842a/resource/409a995e-863f-4f16-b86c-bb195967074a/download/io_controlled-100.jpg","title":"Io Voyager Image Control Network"},{"abstract":"

This archive has been created as part of a project to put planetary control networks on the web. These control networks originated from the RAND corporation (Merton Davies and Tim Colvin) and","geoform":["Control Network"],"name":"mimas_voyager_image_control_network","onlink":"https://astrogeology.usgs.gov/search/map/mimas_voyager_image_control_network","pubdate":"2025-04-01","thumb":"https://astrogeology.usgs.gov/ckan/dataset/c8dfa599-2376-4d0c-9c70-baec9b037394/resource/2bc9123e-ef71-4cd9-b0ee-cde6e43ab3ee/download/mimas_photomosaic_512.jpg","title":"Mimas Voyager Image Control Network"},{"abstract":"

This archive has been created as part of a project to put planetary control networks on the web. These control networks originated from the RAND corporation (Merton Davies and Tim Colvin) and","geoform":["Control Network"],"name":"europa_control_network","onlink":"https://astrogeology.usgs.gov/search/map/europa_control_network","pubdate":"2025-04-01","thumb":"https://astrogeology.usgs.gov/ckan/dataset/384b9083-bafd-48e8-b586-1ffd88e42e05/resource/f77e26d5-a4f0-4fae-8ae4-670bf6ff2135/download/europa_controlled-100.jpg","title":"Europa Voyager Image Control Network"},{"abstract":"We describe work to rigorously register LRO LROC NAC and LOLA [1, 2, 3] image and lidar data to make high resolution lunar digital terrain models (DTMs) suitable for landing site planning,","geoform":["Control Network"],"name":"lro-lidar-improved-lunar-control-networks","onlink":"","pubdate":"2025-04-01","thumb":"/search/images/astropedia/astropedia-logo-small.png","title":"LRO LIDAR-improved lunar control networks"},{"abstract":"

This archive has been created as part of a project to put planetary control networks on the web. These control networks originated from the RAND corporation (Merton Davies and Tim Colvin) and","geoform":["Control Network"],"name":"umbriel_voyager_image_control_network","onlink":"https://astrogeology.usgs.gov/search/map/umbriel_voyager_image_control_network","pubdate":"2025-04-01","thumb":"https://astrogeology.usgs.gov/ckan/dataset/0fb5fd67-a5e2-47d3-baa6-08dde50be631/resource/b1e5b42c-e9ea-46f1-8f4f-d72a79660847/download/davies_umbriel_controlnetwork.jpg","title":"Umbriel Voyager Image Control Network"},{"abstract":"

This archive has been created as part of a project to put planetary control networks on the web. These control networks originated from the RAND corporation (Merton Davies and Tim Colvin) and","geoform":["Control Network"],"name":"titania_voyager_image_control_network","onlink":"https://astrogeology.usgs.gov/search/map/titania_voyager_image_control_network","pubdate":"2025-04-01","thumb":"https://astrogeology.usgs.gov/ckan/dataset/f3a3fe34-d076-4643-a4ad-e6c07efe10aa/resource/2d4ac5f5-a499-4ce4-bd48-4f2713ffdb3d/download/davies_titania_controlnetwork.jpg","title":"Titania Voyager Image Control Network"},{"abstract":"

This archive has been created as part of a project to put planetary control networks on the web. These control networks originated from the RAND corporation (Merton Davies and Tim Colvin) and","geoform":["Control Network"],"name":"oberon_voyager_image_control_network","onlink":"https://astrogeology.usgs.gov/search/map/oberon_voyager_image_control_network","pubdate":"2025-04-01","thumb":"https://astrogeology.usgs.gov/ckan/dataset/7c19335f-3b5e-495c-bdc2-dd259e1e8711/resource/0df4e8d8-2e2f-4276-81d9-52a4c52589d1/download/davies_oberon_controlnetwork2.jpg","title":"Oberon Voyager Image Control Network"},{"abstract":"

This archive has been created as part of a project to put planetary control networks on the web. These control networks originated from the RAND corporation (Merton Davies and Tim Colvin) and","geoform":["Control Network"],"name":"miranda_voyager_image_control_network","onlink":"https://astrogeology.usgs.gov/search/map/miranda_voyager_image_control_network","pubdate":"2025-04-01","thumb":"https://astrogeology.usgs.gov/ckan/dataset/292615a7-a182-4da1-8389-95f532b7a138/resource/8c06d0e6-e949-478f-8085-2bfca957c821/download/davies_miranda_controlnetwork.jpg","title":"Miranda Voyager Image Control Network"},{"abstract":"This orthorectified image was created by projecting an image from the Mars Reconnaissance Orbiter Context Camera (CTX) onto a Digital Terrain Model (DTM). The DTM is available under the \u00e2\u0080\u009cDerived From\u00e2\u0080\u009d section","geoform":["Digital Elevation Model","Raster Data"],"name":"ctx_orthoimage_northwest_kasei_valles_constriction","onlink":"https://astrogeology.usgs.gov/search/map/ctx_orthoimage_northwest_kasei_valles_constriction","pubdate":"2018-04-09","thumb":"https://astrogeology.usgs.gov/ckan/dataset/605e3901-beea-4df3-a09b-ca5970fe9c04/resource/c972f34f-2c4d-4134-8a58-33fcd8d0edc4/download/g19_025758_2047_xi_24n072w_6m_o-thumb.jpg","title":"CTX Orthoimage Northwest Kasei Valles Constriction"},{"abstract":"This Digital Terrain Model (DTM) was produced as part of a project to understand Martian lava flows. It was constructed from a pair of Mars Reconnaissance Orbiter Context Camera (CTX) images using","geoform":["Digital Elevation Model","Raster Data"],"name":"ctx_dtm_northwest_kasei_valles_constriction","onlink":"https://astrogeology.usgs.gov/search/map/ctx_dtm_northwest_kasei_valles_constriction","pubdate":"2018-04-09","thumb":"https://astrogeology.usgs.gov/ckan/dataset/e7c4c515-d687-4a02-9f87-b27f511921a9/resource/31800cd6-c589-4788-8c1e-932ff7a62090/download/dem_18m_nw_kasei_constriction-thumb.jpg","title":"CTX DTM Northwest Kasei Valles Constriction"},{"abstract":"This sheet is one in a series of maps of the Galilean satellites of Jupiter at a nominal scale of 1:15,000,000. This series is based on data from the Galileo Orbiter Solid-State","geoform":["Global Mosaic"],"name":"ganymede_controlled_color_photomosaic_map","onlink":"https://astrogeology.usgs.gov/search/map/ganymede_controlled_color_photomosaic_map","pubdate":"2002-01-02","thumb":"https://astrogeology.usgs.gov/ckan/dataset/4d7e6c95-dae7-4603-9afa-fc33c7e5d9a4/resource/779ab575-8bcd-4425-b77a-7119dddae58a/download/thumb.png","title":"Ganymede Controlled Color Photomosaic Map"},{"abstract":"","geoform":["Geologic Map","Raster Data","Vector Data"],"name":"moon_geologic_map_of_the_colombo_quadrangle","onlink":"https://astrogeology.usgs.gov/search/map/moon_geologic_map_of_the_colombo_quadrangle","pubdate":"1972-10-11","thumb":"https://astrogeology.usgs.gov/ckan/dataset/caf3d8a3-2407-48d6-a054-c7f1801bfd24/resource/99a18aa5-ea44-4ba9-a1db-ac5e143f5033/download/thumb.png","title":"Moon Geologic Map of the Colombo Quadrangle"},{"abstract":"","geoform":["Geologic Map","Raster Data","Vector Data"],"name":"moon_geologic_map_of_the_cleomedes_quadrangle","onlink":"https://astrogeology.usgs.gov/search/map/moon_geologic_map_of_the_cleomedes_quadrangle","pubdate":"1972-10-11","thumb":"https://astrogeology.usgs.gov/ckan/dataset/fe4f850b-c9b6-4c7c-8ece-f5780a34e148/resource/db65cfca-09d3-4405-b042-6f5cbbe0a3e5/download/thumb.png","title":"Moon Geologic Map of the Cleomedes Quadrangle"},{"abstract":"The photomosaic that forms the base for this globe combines a gray-shaded relief airbrush image with color-coded topographic data. The shaded relief data provide interpretations of lunar morphology based on lunar images","geoform":["Globe","Topographic Map"],"name":"moon_clementine_topographic_globe","onlink":"https://astrogeology.usgs.gov/search/map/moon_clementine_topographic_globe","pubdate":null,"thumb":"https://astrogeology.usgs.gov/ckan/dataset/114b828d-b993-4614-ae9b-cea3f8513e9b/resource/dd2f2a3b-0fdc-4857-9422-d7b956ee4d8c/download/thumb.png","title":"Moon Clementine Topographic Globe"},{"abstract":"In May and June of 1994, the NASA/DoD Clementine Mission acquired global, 11-band, multispectral data of the lunar surface using the ultraviolet-visible (UVVIS) and near-infrared (NIR) camera systems (e.g., Nozette et","geoform":["Collection"],"name":"moon-clementine-nir-global-map","onlink":"https://astrogeology.usgs.gov/search/map/moon-clementine-nir-global-map","pubdate":"2023-10-06","thumb":"https://astrogeology.usgs.gov/ckan/dataset/d6325dc3-6dd3-466e-b3fe-338723e8ea8a/resource/e88bd63b-d122-48a7-a87d-94805c6847ea/download/moon-clementine-nir-thumb.jpg","title":"Moon Clementine NIR Global Map"},{"abstract":"The Clementine Lunar Control Network (CLCN) includes 543,245 measurements of 271,634 points on 43,871 Clementine 750-nm images-the largest planetary control network ever computed. 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Sources for the series were Voyager","geoform":["Regional Mosaic"],"name":"callisto_controlled_photomosaic_of_the_askr_quadrangle","onlink":"https://astrogeology.usgs.gov/search/map/callisto_controlled_photomosaic_of_the_askr_quadrangle","pubdate":null,"thumb":"https://astrogeology.usgs.gov/ckan/dataset/57dc61c7-87f1-4139-b7f7-5e0d1d341d4c/resource/6fb02a11-cb12-4944-a6ff-5509af695a63/download/thumb.png","title":"Callisto Controlled Photomosaic of the Askr Quadrangle"},{"abstract":"This sheet is one in a series of maps that covers the surface of Galilean satellites of Jupiter at nominal scale of 1:5,000,000(Batson and others, 1980). Sources for the series were Voyager","geoform":["Regional Mosaic"],"name":"callisto_controlled_photomosaic_of_the_asgard_quadrangle","onlink":"https://astrogeology.usgs.gov/search/map/callisto_controlled_photomosaic_of_the_asgard_quadrangle","pubdate":null,"thumb":"https://astrogeology.usgs.gov/ckan/dataset/27ba8600-72c9-4af9-8263-6f0bfe2b7cb6/resource/da67f670-c1de-4fbb-a5f5-06e7f709e4f4/download/thumb.png","title":"Callisto Controlled Photomosaic of the Asgard Quadrangle"},{"abstract":"Artemis, named for the Greek goddess of the hunt, represents an approximately 2,600 km diameter circular feature on Venus, and it may represent the largest circular structure in our solar system. Artemis,","geoform":["Geologic Map","Raster Data","Vector Data"],"name":"venus_geologic_map_of_the_artemis_chasma_quadrangle","onlink":"https://astrogeology.usgs.gov/search/map/venus_geologic_map_of_the_artemis_chasma_quadrangle","pubdate":"2010-02-10","thumb":"https://astrogeology.usgs.gov/ckan/dataset/cacbf624-ae60-4da7-a5de-774c4e847863/resource/c7898804-5dc4-4dea-8e29-118603640ee6/download/thumb.png","title":"Venus Geologic Map of the Artemis Chasma Quadrangle"},{"abstract":"USGS is assessing the feasibility of map projections and grid systems for lunar surface operations. We propose developing a new Lunar Transverse Mercator (LTM), the Lunar Polar Stereographic (LPS), and the Lunar","geoform":["Grids"],"name":"lunar-grid-reference-system-artemis-iii-candidate-landing-site-navigational-grids","onlink":"https://astrogeology.usgs.gov/search/map/lunar-grid-reference-system-artemis-iii-candidate-landing-site-navigational-grids","pubdate":"2024-11-05","thumb":"https://astrogeology.usgs.gov/ckan/dataset/895dda47-db5d-43c6-b487-032d7bf4698c/resource/0d70cfd9-081e-4832-9d16-9537e725e14a/download/mcclernan_lunar-thumb2.jpg","title":"Lunar Grid Reference System Artemis III Candidate Landing Site Navigational Grids"},{"abstract":"","geoform":["Geologic Map","Raster Data","Vector Data"],"name":"mars_geologic_map_of_arsia_mons_volcano","onlink":"https://astrogeology.usgs.gov/search/map/mars_geologic_map_of_arsia_mons_volcano","pubdate":"1996-01-03","thumb":"https://astrogeology.usgs.gov/ckan/dataset/eabb715f-b2e0-4c14-b7bd-8c25e4f957af/resource/a814f993-957d-44cd-bc76-cfffbae881d6/download/thumb.png","title":"Mars Geologic Map of Arsia Mons Volcano"},{"abstract":"","geoform":["Geologic Map","Raster Data","Vector Data"],"name":"moon_geologic_map_of_the_aristoteles_quadrangle","onlink":"https://astrogeology.usgs.gov/search/map/moon_geologic_map_of_the_aristoteles_quadrangle","pubdate":"1972-10-11","thumb":"https://astrogeology.usgs.gov/ckan/dataset/c6a1ff38-190f-4352-90ad-a8d576c7d5ff/resource/7a697944-d043-4751-acde-91b232b76f20/download/thumb.png","title":"Moon Geologic Map of the Aristoteles Quadrangle"},{"abstract":"","geoform":["Geologic Map","Raster Data","Vector Data"],"name":"moon_geologic_map_of_the_aristarchus_region","onlink":"https://astrogeology.usgs.gov/search/map/moon_geologic_map_of_the_aristarchus_region","pubdate":"2021-09-03","thumb":"https://astrogeology.usgs.gov/ckan/dataset/a83f3fd7-f126-42e8-ae1a-9279fc8f3ac2/resource/134ff925-6de0-4f06-abc4-6de29c576453/download/thumb.png","title":"Moon Geologic Map of the Aristarchus Region"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"ariel_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/ariel_nomenclature","pubdate":"2013-03-20","thumb":"https://astrogeology.usgs.gov/ckan/dataset/fd9250e1-35c3-4090-a12e-9a7c87b506a0/resource/90205719-6e83-4d63-a0f3-6eb1ba2caa4d/download/thumb.png","title":"Ariel Nomenclature"},{"abstract":"

This archive has been created as part of a project to put planetary control networks on the web. These control networks originated from the RAND corporation (Merton Davies and Tim Colvin) and","geoform":["Control Network"],"name":"ariel_voyager_image_control_network","onlink":"https://astrogeology.usgs.gov/search/map/ariel_voyager_image_control_network","pubdate":"2025-04-01","thumb":"https://astrogeology.usgs.gov/ckan/dataset/5785f59b-09f8-41ae-b522-e5b2edcb1df0/resource/40d6a9bb-7869-4fac-94c7-e4c0346032f2/download/davies_ariel_controlnetwork.jpg","title":"Ariel Voyager Image Control Network"},{"abstract":"","geoform":["Geologic Map","Raster Data","Vector Data"],"name":"mars_geologic_map_of_the_argyre_quadrangle","onlink":"https://astrogeology.usgs.gov/search/map/mars_geologic_map_of_the_argyre_quadrangle","pubdate":"1980-11-19","thumb":"https://astrogeology.usgs.gov/ckan/dataset/00f999c7-728a-4749-af23-7d389f75f9d3/resource/fc082843-9b19-4c7b-886b-620442cd6f14/download/thumb.png","title":"Mars Geologic Map of the Argyre Quadrangle"},{"abstract":"","geoform":["Regional Mosaic"],"name":"mars_controlled_photomosaic_of_the_argyre_north_central_quadrangle","onlink":"https://astrogeology.usgs.gov/search/map/mars_controlled_photomosaic_of_the_argyre_north_central_quadrangle","pubdate":"1979-10-18","thumb":"https://astrogeology.usgs.gov/ckan/dataset/ab864c1d-29d0-4002-88ac-aabf85314c09/resource/4df8e93b-9ca5-4238-82fc-68bb257984ab/download/thumb.png","title":"Mars Controlled Photomosaic of the Argyre North-Central Quadrangle"},{"abstract":"","geoform":["Regional Mosaic"],"name":"mars_controlled_photomosaic_of_the_argyre_northwest_quadrangle","onlink":"https://astrogeology.usgs.gov/search/map/mars_controlled_photomosaic_of_the_argyre_northwest_quadrangle","pubdate":"1979-10-18","thumb":"https://astrogeology.usgs.gov/ckan/dataset/e2294261-4366-4381-8ffa-c341760f11c8/resource/10cedc0c-ba5b-4680-814b-c52be962752a/download/thumb.png","title":"Mars Controlled Photomosaic of the Argyre Northwest Quadrangle"},{"abstract":"","geoform":["Regional Mosaic"],"name":"mars_controlled_photomosaic_of_the_argyre_northeast_quadrangle","onlink":"https://astrogeology.usgs.gov/search/map/mars_controlled_photomosaic_of_the_argyre_northeast_quadrangle","pubdate":"1979-10-18","thumb":"https://astrogeology.usgs.gov/ckan/dataset/a995715b-8920-4891-a8bb-423e3c940c89/resource/20adf5eb-78cf-43a2-ade4-99538a46a28c/download/thumb.png","title":"Mars Controlled Photomosaic of the Argyre Northeast Quadrangle"},{"abstract":"","geoform":["Regional Mosaic"],"name":"mars_controlled_photomosaic_of_the_argyre_southeast_quadrangle","onlink":"https://astrogeology.usgs.gov/search/map/mars_controlled_photomosaic_of_the_argyre_southeast_quadrangle","pubdate":"1985-11-24","thumb":"https://astrogeology.usgs.gov/ckan/dataset/58524b9d-3560-44a7-a443-20e3d9c1f036/resource/02093647-ee88-44e3-af06-a3b137cedb72/download/thumb.png","title":"Mars Controlled Photomosaic of the Argyre Southeast Quadrangle"},{"abstract":"","geoform":["Regional Mosaic"],"name":"mars_controlled_photomosaic_of_the_argyre_southwest_quadrangle","onlink":"https://astrogeology.usgs.gov/search/map/mars_controlled_photomosaic_of_the_argyre_southwest_quadrangle","pubdate":"1985-11-24","thumb":"https://astrogeology.usgs.gov/ckan/dataset/1ad6069b-0556-4c26-997d-95dd88d5e160/resource/6ad25662-1582-4250-9b3d-c5462533c6ab/download/thumb.png","title":"Mars Controlled Photomosaic of the Argyre Southwest Quadrangle"},{"abstract":"","geoform":["Shaded-Relief Map"],"name":"mars_shaded_relief_map_of_the_argyre_planitia","onlink":"https://astrogeology.usgs.gov/search/map/mars_shaded_relief_map_of_the_argyre_planitia","pubdate":"1980-11-19","thumb":"https://astrogeology.usgs.gov/ckan/dataset/415d06b5-22d3-4b11-bbcd-774f442a0664/resource/0ae4db23-9d81-4588-b84e-311b9192b52a/download/thumb.png","title":"Mars Shaded Relief Map of the Argyre Planitia"},{"abstract":"","geoform":["Shaded-Relief Map"],"name":"mars_shaded_relief_map_of_the_argyre_quadrangle","onlink":"https://astrogeology.usgs.gov/search/map/mars_shaded_relief_map_of_the_argyre_quadrangle","pubdate":"1975-10-14","thumb":"https://astrogeology.usgs.gov/ckan/dataset/fd36cce9-5aef-475d-8a13-53f7c1856e46/resource/477d81dd-07f0-4d17-b9de-02b6788c1205/download/thumb.png","title":"Mars Shaded Relief Map of the Argyre Quadrangle"},{"abstract":"","geoform":["Regional Mosaic"],"name":"mars_topographic_map_of_the_argyre_quadrangle","onlink":"https://astrogeology.usgs.gov/search/map/mars_topographic_map_of_the_argyre_quadrangle","pubdate":"1976-10-15","thumb":"https://astrogeology.usgs.gov/ckan/dataset/e1dfad7e-bc98-44a7-ab75-c88359789abd/resource/e96b9195-3c9f-4437-868e-114557e9a9c7/download/thumb.png","title":"Mars Topographic Map of the Argyre Quadrangle"},{"abstract":"Io is one of the most geologically active planetary objects observed so far in the exploration of the Solar System. It is dominated by volcanism, and it shows only minor surface modification","geoform":["Geologic Map","Raster Data","Vector Data"],"name":"io_geologic_map_of_the_ra_patera_area","onlink":"https://astrogeology.usgs.gov/search/map/io_geologic_map_of_the_ra_patera_area","pubdate":null,"thumb":"https://astrogeology.usgs.gov/ckan/dataset/06ad74cb-eb79-4651-834a-8a083841c4b4/resource/9c52ea31-b1e9-48be-ae74-fa8fd59b20a6/download/thumb.png","title":"Io Geologic Map of the Ra Patera Area"},{"abstract":"Io, the innermost Galilean satellite of Jupiter, is about the same size as Earth\u00e2\u0080\u0099s Moon, but its surface properties and geologic processes are significantly different. Impact craters and basins, which dominate the","geoform":["Geologic Map","Raster Data","Vector Data"],"name":"io_geologic_map_of_the_maasaw_patera_area","onlink":"https://astrogeology.usgs.gov/search/map/io_geologic_map_of_the_maasaw_patera_area","pubdate":"2021-11-13","thumb":"https://astrogeology.usgs.gov/ckan/dataset/f450d0c4-b1ec-45af-9684-df5deda64d64/resource/aa2d2582-9b06-415b-9b23-20cc01152be8/download/thumb.png","title":"Io Geologic Map of the Maasaw Patera Area"},{"abstract":"","geoform":["Shaded-Relief Map"],"name":"mercury_shaded_relief_map_of_the_borealis_area","onlink":"https://astrogeology.usgs.gov/search/map/mercury_shaded_relief_map_of_the_borealis_area","pubdate":"1977-10-16","thumb":"https://astrogeology.usgs.gov/ckan/dataset/c08c1caa-7895-4cc9-b1ae-f303864f7ae5/resource/bad57990-7dd8-41e5-9038-6ab206f0ed69/download/thumb.png","title":"Mercury Shaded Relief Map of the Borealis Area"},{"abstract":"","geoform":["Shaded-Relief 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Data"],"name":"mars_geologic_map_of_the_mare_australe_area","onlink":"https://astrogeology.usgs.gov/search/map/mars_geologic_map_of_the_mare_australe_area","pubdate":"2019-10-17","thumb":"https://astrogeology.usgs.gov/ckan/dataset/7cc688f1-0337-41ee-97f0-331b6b37fbe8/resource/70b88c81-269f-4a9d-b84f-93be41729666/download/thumb.png","title":"Mars Geologic Map of the Mare Australe Area"},{"abstract":"","geoform":["Geologic Map","Raster Data","Vector Data"],"name":"mars_geologic_map_of_the_mare_boreum_area","onlink":"https://astrogeology.usgs.gov/search/map/mars_geologic_map_of_the_mare_boreum_area","pubdate":"2019-11-23","thumb":"https://astrogeology.usgs.gov/ckan/dataset/3e89379e-52c7-4a3c-9fbb-dccc1032fd53/resource/79b12f7a-7687-46c3-a2c9-8be9acebcbf7/download/thumb.png","title":"Mars Geologic Map of the Mare Boreum Area"},{"abstract":"","geoform":["Polar Map","Regional Mosaic"],"name":"mars_controlled_photomosaic_of_the_south_polar_area_planum_australe_region","onlink":"https://astrogeology.usgs.gov/search/map/mars_controlled_photomosaic_of_the_south_polar_area_planum_australe_region","pubdate":"1991-12-30","thumb":"https://astrogeology.usgs.gov/ckan/dataset/9a26bc89-9f89-417d-9c54-7613bb623d12/resource/8af97736-9b21-43ee-a731-918dbd64cac4/download/thumb.png","title":"Mars Controlled Photomosaic of the South Polar Area , Planum Australe Region"},{"abstract":"","geoform":["Shaded-Relief Map"],"name":"mars_shaded_relief_map_of_the_mare_australe_area","onlink":"https://astrogeology.usgs.gov/search/map/mars_shaded_relief_map_of_the_mare_australe_area","pubdate":"1976-10-15","thumb":"https://astrogeology.usgs.gov/ckan/dataset/d47e349d-f19e-4757-a738-acb5ae52fab2/resource/41a87e1b-3d43-484d-a3bf-9fef06f8243f/download/thumb.png","title":"Mars Shaded Relief Map of the Mare Australe Area"},{"abstract":"","geoform":["Shaded-Relief Map"],"name":"mars_shaded_relief_map_of_the_mare_boreum_area","onlink":"https://astrogeology.usgs.gov/search/map/mars_shaded_relief_map_of_the_mare_boreum_area","pubdate":"1976-10-15","thumb":"https://astrogeology.usgs.gov/ckan/dataset/a221732d-209d-49d0-9a68-e6903413b39f/resource/6855318c-4a5d-465f-93f9-eb83bbd37b04/download/thumb.png","title":"Mars Shaded Relief Map of the Mare Boreum Area"},{"abstract":"","geoform":["Regional Mosaic"],"name":"mars_topographic_map_of_the_mare_boreum_area","onlink":"https://astrogeology.usgs.gov/search/map/mars_topographic_map_of_the_mare_boreum_area","pubdate":"1977-10-16","thumb":"https://astrogeology.usgs.gov/ckan/dataset/3d3ea5ba-dc82-46b5-b5ac-37ca8d503eb9/resource/453b362d-b9ff-4d2b-9493-3dc7b281db33/download/thumb.png","title":"Mars Topographic Map of the Mare Boreum Area"},{"abstract":"Assorted Lunar Images and Data from 1965 to 1992 Presented here are safed versions of variety of data selected from a collection of data commonly referred to as the Lunar Consortium Data.","geoform":["Digital Elevation Model","Raster Data","Remote-sensing Data"],"name":"lunar_consortium_data_historical_archive","onlink":"https://astrogeology.usgs.gov/search/map/lunar_consortium_data_historical_archive","pubdate":null,"thumb":"https://astrogeology.usgs.gov/ckan/dataset/29df8aa7-4039-426d-ad4e-6f764cab92d5/resource/dde0fe4c-4f52-4629-8e5f-fd6537ae2c26/download/lunarconsortiumdata_historic_archive_thumb.jpg","title":"Lunar Consortium Data Historical Archive"},{"abstract":"These new NIMS map cubes (rasters) of Callisto come in three varieties: CUB, CIOF, and COC. The CUB files contain the original spectral radiance values in units of mW/(cm2 str \u03bcm). The","geoform":["Archive","Data","Image","Raster Data","Remote-sensing Data"],"name":"callisto-galileo-nims-hyperspectral-map-products-registered-archive","onlink":"https://astrogeology.usgs.gov/search/map/callisto-galileo-nims-hyperspectral-map-products-registered-archive#open","pubdate":"2024-07-05","thumb":"https://astrogeology.usgs.gov/ckan/dataset/eb8d3757-c9f1-43ba-a91d-56394796c9d9/resource/2ea9596d-4adf-49f1-a5b4-de1e24076ec0/download/callisto_nims_composite_100.jpg","title":"Callisto Galileo NIMS Hyperspectral Map Products Registered Archive"},{"abstract":"These new NIMS map cubes (rasters) of Europa come in three varieties: CUB, CIOF, and COC. The CUB files contain the original spectral radiance values in units of mW/(cm2 str \u03bcm). The","geoform":["Archive","Data","Image","Raster Data","Remote-sensing Data"],"name":"europa-galileo-nims-hyperspectral-map-products-registered-archive","onlink":"https://astrogeology.usgs.gov/search/map/europa-galileo-nims-hyperspectral-map-products-registered-archive#open","pubdate":"2024-07-25","thumb":"https://astrogeology.usgs.gov/ckan/dataset/ea4a5a5c-b491-4b52-a5ef-84b518bc86f5/resource/97584861-99dc-4dce-9a21-367e22911f74/download/europa_nims_composite_100.jpg","title":"Europa Galileo NIMS Hyperspectral Map Products Registered Archive"},{"abstract":"","geoform":["Geologic Map","Raster Data","Vector Data"],"name":"mars_geologic_map_of_the_arcadia_quadrangle","onlink":"https://astrogeology.usgs.gov/search/map/mars_geologic_map_of_the_arcadia_quadrangle","pubdate":"2019-10-18","thumb":"https://astrogeology.usgs.gov/ckan/dataset/17b9db40-e4ec-4de9-bf19-757b70858b3d/resource/0c3b3d82-0cdb-4a3f-b93c-1e50d4bdb6f2/download/thumb.png","title":"Mars Geologic Map of the Arcadia Quadrangle"},{"abstract":"","geoform":["Geologic Map","Raster Data","Vector Data"],"name":"mars_map_showing_lava_flows_in_the_southwest_part_of_the_arcadia_quadrangle","onlink":"https://astrogeology.usgs.gov/search/map/mars_map_showing_lava_flows_in_the_southwest_part_of_the_arcadia_quadrangle","pubdate":"1981-11-20","thumb":"https://astrogeology.usgs.gov/ckan/dataset/7ad7f12d-28a5-4d31-9438-bac26079d676/resource/bb2d3730-1c1e-4c5a-85b1-1fecf941e88c/download/thumb.png","title":"Mars Map Showing Lava Flows in the Southwest Part of the Arcadia Quadrangle"},{"abstract":"","geoform":["Regional Mosaic"],"name":"mars_controlled_photomosaic_of_the_arcadia_southwest_quadrangle","onlink":"https://astrogeology.usgs.gov/search/map/mars_controlled_photomosaic_of_the_arcadia_southwest_quadrangle","pubdate":"1984-11-23","thumb":"https://astrogeology.usgs.gov/ckan/dataset/edc90a2b-b9d6-4e3c-8e89-fb7055e61646/resource/a2755437-7093-4839-8006-a258c6c7a16f/download/thumb.png","title":"Mars Controlled Photomosaic of the Arcadia Southwest Quadrangle"},{"abstract":"","geoform":["Regional Mosaic"],"name":"mars_controlled_photomosaic_of_the_arcadia_southeast_quadrangle","onlink":"https://astrogeology.usgs.gov/search/map/mars_controlled_photomosaic_of_the_arcadia_southeast_quadrangle","pubdate":"1981-11-20","thumb":"https://astrogeology.usgs.gov/ckan/dataset/4bebf12e-ddd0-48b8-bdf1-72d0ecdc6da5/resource/7cc3f1a5-9ab4-4994-8ef8-9a111592415d/download/thumb.png","title":"Mars Controlled Photomosaic of the Arcadia Southeast Quadrangle"},{"abstract":"","geoform":["Regional Mosaic"],"name":"mars_controlled_photomosaic_of_the_arcadia_northwest_quadrangle","onlink":"https://astrogeology.usgs.gov/search/map/mars_controlled_photomosaic_of_the_arcadia_northwest_quadrangle","pubdate":"1981-11-20","thumb":"https://astrogeology.usgs.gov/ckan/dataset/0a1d494c-fffe-4a18-b87c-6aa0fa018b58/resource/38589154-b5d5-4c56-b81e-29387a1ff064/download/thumb.png","title":"Mars Controlled Photomosaic of the Arcadia Northwest Quadrangle"},{"abstract":"","geoform":["Regional Mosaic"],"name":"mars_controlled_photomosaic_of_the_arcadia_northeast_quadrangle","onlink":"https://astrogeology.usgs.gov/search/map/mars_controlled_photomosaic_of_the_arcadia_northeast_quadrangle","pubdate":"1981-11-20","thumb":"https://astrogeology.usgs.gov/ckan/dataset/f58fd60d-c532-4266-b437-035922dc69f0/resource/cd61c9ad-cdee-4e4a-9d59-207644e46c7c/download/thumb.png","title":"Mars Controlled Photomosaic of the Arcadia Northeast Quadrangle"},{"abstract":"","geoform":["Shaded-Relief Map"],"name":"mars_shaded_relief_map_of_the_arcadia_quadrangle","onlink":"https://astrogeology.usgs.gov/search/map/mars_shaded_relief_map_of_the_arcadia_quadrangle","pubdate":"1982-11-21","thumb":"https://astrogeology.usgs.gov/ckan/dataset/58353bf4-e7ec-4268-b875-0c6aee215945/resource/3322c26b-3147-4890-a50c-066461f01a4a/download/thumb.png","title":"Mars Shaded Relief Map of the Arcadia Quadrangle"},{"abstract":"","geoform":["Geologic Map","Raster Data","Vector Data"],"name":"mars_geologic_map_of_the_arabia_quadrangle","onlink":"https://astrogeology.usgs.gov/search/map/mars_geologic_map_of_the_arabia_quadrangle","pubdate":"2019-10-16","thumb":"https://astrogeology.usgs.gov/ckan/dataset/01cde386-048d-4d10-a7bf-6f78286d2fc5/resource/7d39622a-8fa1-4c4d-b7fb-d99cffec59a5/download/thumb.png","title":"Mars Geologic Map of the Arabia Quadrangle"},{"abstract":"Arabia Terra is a large region of cratered terrane extending from about 20\u00c3\u0082\u00c2\u00b0 W. longitude eastward across the prime meridian to about 300\u00c3\u0082\u00c2\u00b0 W. longitude for an average east-west width of about","geoform":["Geologic Map","Raster Data","Vector Data"],"name":"mars_geologic_map_transecting_the_highland_lowland_boundary_zone_arabia_terra","onlink":"https://astrogeology.usgs.gov/search/map/mars_geologic_map_transecting_the_highland_lowland_boundary_zone_arabia_terra","pubdate":"2002-01-02","thumb":"https://astrogeology.usgs.gov/ckan/dataset/33ca8647-34ef-46fa-b0e4-bc363e03da35/resource/feb01fde-0508-4c08-80a3-c97535f4d965/download/thumb.png","title":"Mars Geologic Map Transecting the Highland/Lowland Boundary Zone, Arabia Terra"},{"abstract":"","geoform":["Regional Mosaic"],"name":"mars_controlled_photomosaic_of_the_arabia_northeast_quadrangle","onlink":"https://astrogeology.usgs.gov/search/map/mars_controlled_photomosaic_of_the_arabia_northeast_quadrangle","pubdate":"1982-11-21","thumb":"https://astrogeology.usgs.gov/ckan/dataset/3726eaa5-4de9-47f5-bcb2-274dc0745ed9/resource/c08ffbe2-f1a1-4e26-b5cf-c7b186a34355/download/thumb.png","title":"Mars Controlled Photomosaic of the Arabia Northeast Quadrangle"},{"abstract":"","geoform":["Regional Mosaic"],"name":"mars_controlled_photomosaic_of_the_arabia_northwest_quadrangle","onlink":"https://astrogeology.usgs.gov/search/map/mars_controlled_photomosaic_of_the_arabia_northwest_quadrangle","pubdate":"1982-11-21","thumb":"https://astrogeology.usgs.gov/ckan/dataset/fa1d70c7-ba76-48f1-8169-0682bc8f9bbe/resource/a9c30716-1dff-4569-8a0e-cd2cb9350251/download/thumb.png","title":"Mars Controlled Photomosaic of the Arabia Northwest Quadrangle"},{"abstract":"","geoform":["Regional Mosaic"],"name":"mars_controlled_photomosaic_of_the_arabia_southwest_quadrangle","onlink":"https://astrogeology.usgs.gov/search/map/mars_controlled_photomosaic_of_the_arabia_southwest_quadrangle","pubdate":"1982-11-21","thumb":"https://astrogeology.usgs.gov/ckan/dataset/6221fee7-1886-4f25-8674-38278dc1efbd/resource/825bc78a-e7e2-4070-99b9-6d4b53b01bc3/download/thumb.png","title":"Mars Controlled Photomosaic of the Arabia Southwest Quadrangle"},{"abstract":"","geoform":["Regional Mosaic"],"name":"mars_controlled_photomosaic_of_the_arabia_southeast_quadrangle","onlink":"https://astrogeology.usgs.gov/search/map/mars_controlled_photomosaic_of_the_arabia_southeast_quadrangle","pubdate":"1982-11-21","thumb":"https://astrogeology.usgs.gov/ckan/dataset/1a9cc26c-8730-493b-9fe8-d3e6eaf8f8f2/resource/2cac2a2b-4c2d-411d-b3b5-2373a4d21606/download/thumb.png","title":"Mars Controlled Photomosaic of the Arabia Southeast Quadrangle"},{"abstract":"","geoform":["Shaded-Relief Map"],"name":"mars_shaded_relief_map_of_the_arabia_quadrangle","onlink":"https://astrogeology.usgs.gov/search/map/mars_shaded_relief_map_of_the_arabia_quadrangle","pubdate":"1984-11-23","thumb":"https://astrogeology.usgs.gov/ckan/dataset/41789e11-0dab-4312-944c-b6614adc8f5e/resource/b4dd6c8a-b06d-46c1-9086-5915442096d5/download/thumb.png","title":"Mars Shaded Relief Map of the Arabia Quadrangle"},{"abstract":"","geoform":["Regional Mosaic"],"name":"mars_topographic_map_of_the_arabia_southeast_quadrangle","onlink":"https://astrogeology.usgs.gov/search/map/mars_topographic_map_of_the_arabia_southeast_quadrangle","pubdate":"1991-12-30","thumb":"https://astrogeology.usgs.gov/ckan/dataset/ab5cf18b-f0d6-4537-a12d-cae79b9aa48c/resource/e2d10ee1-bb86-427b-b232-d7dd67946faf/download/thumb.png","title":"Mars Topographic Map of the Arabia Southeast Quadrangle"},{"abstract":"","geoform":["Regional Mosaic"],"name":"mars_topographic_map_of_the_arabia_northwest_quadrangle","onlink":"https://astrogeology.usgs.gov/search/map/mars_topographic_map_of_the_arabia_northwest_quadrangle","pubdate":"1991-12-30","thumb":"https://astrogeology.usgs.gov/ckan/dataset/46857132-b47b-43ba-b470-630a81da7a3b/resource/80314f4a-53b6-4f15-a9fc-be668eff8efc/download/thumb.png","title":"Mars Topographic Map of the Arabia Northwest Quadrangle"},{"abstract":"","geoform":["Regional Mosaic"],"name":"mars_topographic_map_of_the_arabia_northeast_quadrangle","onlink":"https://astrogeology.usgs.gov/search/map/mars_topographic_map_of_the_arabia_northeast_quadrangle","pubdate":"1991-12-30","thumb":"https://astrogeology.usgs.gov/ckan/dataset/63b1a811-c413-40b2-bd92-8d9f5c0c23c9/resource/18d231b5-a5ec-4ce7-8ed4-8222f999df7f/download/thumb.png","title":"Mars Topographic Map of the Arabia Northeast Quadrangle"},{"abstract":"","geoform":["Regional Mosaic"],"name":"mars_topographic_map_of_the_arabia_southwest_quadrangle","onlink":"https://astrogeology.usgs.gov/search/map/mars_topographic_map_of_the_arabia_southwest_quadrangle","pubdate":"1991-12-30","thumb":"https://astrogeology.usgs.gov/ckan/dataset/c613c732-0a0b-495d-9a33-e5e70658a49b/resource/5cb5b827-ffce-4556-b495-5177f5112c3f/download/thumb.png","title":"Mars Topographic Map of the Arabia Southwest Quadrangle"},{"abstract":"The following 360\u00b0 panoramas were created using digitized photographs collected by the astronauts during the Apollo 11 - 17 lunar exploration missions. The imagery and maps were prepared as part of a","geoform":["Collection"],"name":"moon-apollo-landing-panoramas","onlink":"https://astrogeology.usgs.gov/search/map/moon-apollo-landing-panoramas","pubdate":"2023-06-22","thumb":"https://astrogeology.usgs.gov/ckan/dataset/77ce00c9-30b3-42ec-89a4-ce38d5140eba/resource/cd766698-d203-430f-a573-dcfb28ba9e3d/download/apollo11-thumb.jpg","title":"Moon Apollo Landing Panoramas"},{"abstract":"The Apollo Metric Mapping Cameras were carried on the Apollo 15, 16, and 17 missions to map Earth\u00e2\u0080\u0099s Moon with a high degree of geometric fidelity. This archive collection consists of 7247","geoform":["Grey Scale"],"name":"moon_apollo_metric_mapping_camera_data","onlink":"https://astrogeology.usgs.gov/search/map/moon_apollo_metric_mapping_camera_data","pubdate":"2012-09-25","thumb":"https://astrogeology.usgs.gov/ckan/dataset/f6982164-5ba7-483f-81ac-de1d4ae6129c/resource/b6430f9f-889e-4839-96e3-ecbe567b6e8f/download/thumb.png","title":"Moon Apollo Metric Mapping Camera Data"},{"abstract":"Product Information: This set of archive volumes contains digital scanned versions of original film photographs of rock, soil, and core samples collected from the lunar surface during the Apollo 11, 12, 14,","geoform":["Archive","Image"],"name":"moon_apollo_lunar_sample_photographs","onlink":"https://astrogeology.usgs.gov/search/map/moon_apollo_lunar_sample_photographs","pubdate":null,"thumb":"https://astrogeology.usgs.gov/ckan/dataset/5a02c7c7-90ae-412e-953a-dd6df1bae0e8/resource/384727fa-8f9d-4a7d-9a5a-132a5c5daa75/download/thumb.png","title":"Moon Apollo Lunar Sample Photographs"},{"abstract":"This page features several maps showing routes the astronauts took during extravehicular activities (EVAs). The imagery and maps were prepared as part of a project by a USGS team under funding","geoform":["Collection"],"name":"moon-apollo-traverse-maps","onlink":"https://astrogeology.usgs.gov/search/map/moon-apollo-traverse-maps","pubdate":"2023-10-16","thumb":"https://astrogeology.usgs.gov/ckan/dataset/b499160d-149f-4a79-8aee-e4a09d50fb80/resource/af3a32f8-eb16-48cc-8fd4-0b0881d440d5/download/apollo14_traverse-thumb.jpg","title":"Moon Apollo Traverse Maps"},{"abstract":"","geoform":["Regional Mosaic"],"name":"venus_in_four_map_sheets_the_aphrodite_planitia_region","onlink":"https://astrogeology.usgs.gov/search/map/venus_in_four_map_sheets_the_aphrodite_planitia_region","pubdate":"1999-01-06","thumb":"https://astrogeology.usgs.gov/ckan/dataset/f90fad41-48fc-4b3a-982f-88711e519e90/resource/61d7805b-2ec5-48d1-b00c-13953a9c9990/download/thumb.png","title":"Venus in Four Map Sheets: The Aphrodite Planitia Region"},{"abstract":"","geoform":["Geologic Map","Raster Data","Vector Data"],"name":"moon_geologic_map_of_the_montes_apenninus_region","onlink":"https://astrogeology.usgs.gov/search/map/moon_geologic_map_of_the_montes_apenninus_region","pubdate":"1966-09-04","thumb":"https://astrogeology.usgs.gov/ckan/dataset/acf0c0be-4efc-4065-97a8-f0efb27c92dc/resource/a44f5a5e-ca5b-4520-bd58-0c45b1644338/download/thumb.png","title":"Moon Geologic Map of the Montes Apenninus Region"},{"abstract":"","geoform":["Geologic Map","Raster Data","Vector Data"],"name":"moon_geologic_maps_of_the_apennine_hadley_region","onlink":"https://astrogeology.usgs.gov/search/map/moon_geologic_maps_of_the_apennine_hadley_region","pubdate":"1971-10-10","thumb":"https://astrogeology.usgs.gov/ckan/dataset/11204c0a-3827-427f-a945-50a342197cce/resource/106f3cb9-dc2a-437f-b879-6acb1ef21a28/download/thumb.png","title":"Moon Geologic Maps of the Apennine-Hadley Region"},{"abstract":"This basemap of Jupiter\u00e2\u0080\u0099s moon Io was produced by combining the best images from both the Voyager 1 and Galileo Missions. Although the subjovian hemisphere of Io was poorly seen by Galileo,","geoform":["Global Mosaic"],"name":"io_voyager_galileo_global_mosaic_rotation_animation","onlink":"https://astrogeology.usgs.gov/search/map/io_voyager_galileo_global_mosaic_rotation_animation","pubdate":null,"thumb":"https://astrogeology.usgs.gov/ckan/dataset/5f72107a-5a9c-4844-aa50-2194cae94eeb/resource/1aaa41e2-e2e9-4835-b052-1d0c5c3ef863/download/thumb.png","title":"Io Voyager - Galileo Global Mosaic Rotation Animation"},{"abstract":"The Lunar Reconnaissance Orbiter Camera (LROC) consists of one Wide Angle Camera (WAC) for synoptic multispectral imaging and two Narrow Angle Cameras (NAC) that provide high-resolution images (0.5 to 2.0 m 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pixel","geoform":["Document"],"name":"moon_lro_south_pole_dem_from_narrow_angle_camera","onlink":"https://astrogeology.usgs.gov/search/map/moon_lro_south_pole_dem_from_narrow_angle_camera","pubdate":null,"thumb":"https://astrogeology.usgs.gov/ckan/dataset/a0bf8e37-6c28-48e1-a381-ee2b91f7f613/resource/3c76fc50-a6f5-4772-a9ec-63b8aeada88f/download/thumb.png","title":"Moon LRO South Pole DEM from Narrow Angle Camera"},{"abstract":"NOTES ON BASE: This sheet is one in a series of maps that covers the surface of Galilean satellites of Jupiter at a nominal scale of 1: 5,000,000 (Batson and others, 1980).","geoform":["Polar Map","Shaded-Relief Map"],"name":"ganymede_shaded_relief_and_surface_markings_maps_of_the_polar_western_and_eastern_regions","onlink":"https://astrogeology.usgs.gov/search/map/ganymede_shaded_relief_and_surface_markings_maps_of_the_polar_western_and_eastern_regions","pubdate":"1992-12-31","thumb":"https://astrogeology.usgs.gov/ckan/dataset/1d3d3894-bf4f-431c-9687-3eb891226f53/resource/72f0382f-0b8e-4fdf-830f-534af2d9a401/download/thumb.png","title":"Ganymede Shaded Relief and Surface Markings Maps of the Polar, Western, and Eastern Regions"},{"abstract":"NOTES ON BASE: This sheet is one in a series of maps that covers the surface of Galilean satellites of Jupiter at a nominal scale of 1: 5,000,000 (Batson and others, 1980).","geoform":["Shaded-Relief 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Map"],"name":"ganymede_shaded_relief_and_surface_markings_of_the_galileo_regio_quadrangle","onlink":"https://astrogeology.usgs.gov/search/map/ganymede_shaded_relief_and_surface_markings_of_the_galileo_regio_quadrangle","pubdate":null,"thumb":"https://astrogeology.usgs.gov/ckan/dataset/be16a478-103f-4dd8-aa7c-d84732325618/resource/1fa9cb8b-27f3-4654-ab65-24360d909681/download/thumb.png","title":"Ganymede Shaded Relief and Surface Markings of the Galileo Regio Quadrangle"},{"abstract":"NOTES ON BASE: This sheet is one in a series of maps that covers the surface of Galilean satellites of Jupiter at a nominal scale of 1: 5,000,000 (Batson and others, 1980).","geoform":["Shaded-Relief 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The map is a Simple Cylindrical projection and has","geoform":["Global Mosaic","Raster Data","Remote-sensing Data"],"name":"iapetus_cassini_voyager_global_mosaic_803m","onlink":"https://astrogeology.usgs.gov/search/map/iapetus_cassini_voyager_global_mosaic_803m","pubdate":null,"thumb":"https://astrogeology.usgs.gov/ckan/dataset/6ac8ecfb-36e7-4113-8d16-c92ba857c3d7/resource/e1178cdb-41bb-49ed-a064-fd65e8378d7b/download/thumb.png","title":"Iapetus Cassini - Voyager Global Mosaic 803m"},{"abstract":"","geoform":["Regional Mosaic"],"name":"mars_mtm_80270_controlled_photomosaic_of_part_of_the_planum_australe_region","onlink":"https://astrogeology.usgs.gov/search/map/mars_mtm_80270_controlled_photomosaic_of_part_of_the_planum_australe_region","pubdate":"1987-11-26","thumb":"https://astrogeology.usgs.gov/ckan/dataset/617c1c14-b970-4eed-874d-725b15ca1271/resource/0835ab91-a229-43e5-99b3-39eb1590c3c6/download/thumb.png","title":"Mars MTM -80270 Controlled Photomosaic of Part of the Planum 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Boreale Region"},{"abstract":"","geoform":["Regional Mosaic"],"name":"mars_mtm_80050_controlled_photomosaic_of_part_of_the_planum_australe_region","onlink":"https://astrogeology.usgs.gov/search/map/mars_mtm_80050_controlled_photomosaic_of_part_of_the_planum_australe_region","pubdate":"1987-11-26","thumb":"https://astrogeology.usgs.gov/ckan/dataset/ea79cb19-4d0f-4cea-ac57-0b5aa026a771/resource/8b1e1d9f-9078-4a94-aba0-f1341dacf825/download/thumb.png","title":"Mars MTM -80050 Controlled Photomosaic of Part of the Planum Australe Region"},{"abstract":"","geoform":["Regional Mosaic"],"name":"mars_mtm_80030_controlled_photomosaic_of_part_of_the_chasma_boreale_region","onlink":"https://astrogeology.usgs.gov/search/map/mars_mtm_80030_controlled_photomosaic_of_part_of_the_chasma_boreale_region","pubdate":"1986-11-25","thumb":"https://astrogeology.usgs.gov/ckan/dataset/e040c81c-2b0d-478f-83e3-ccb660f1abf4/resource/b443dfd7-3ec7-4740-a721-98a04674a70b/download/thumb.png","title":"Mars MTM 80030 Controlled Photomosaic of Part of the Chasma Boreale Region"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"moon_lac_80_langrenus_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/moon_lac_80_langrenus_nomenclature","pubdate":"2013-01-25","thumb":"https://astrogeology.usgs.gov/ckan/dataset/7ca227d1-b8f0-45da-9bad-83d262691d2b/resource/1f527f97-1eb0-4de9-83b5-b57b4d88931e/download/thumb.png","title":"Moon LAC-80 Langrenus Nomenclature"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"venus_v_8_bereghinya_planitia_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/venus_v_8_bereghinya_planitia_nomenclature","pubdate":"2012-06-07","thumb":"https://astrogeology.usgs.gov/ckan/dataset/50636695-98ba-4624-85a0-8f6668acc154/resource/462f3a99-1f9d-4054-9e29-0f51945e0511/download/thumb.png","title":"Venus V-8 Bereghinya Planitia Nomenclature"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"mercury_h_8_tolstoj_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/mercury_h_8_tolstoj_nomenclature","pubdate":"2016-05-25","thumb":"https://astrogeology.usgs.gov/ckan/dataset/83f8d915-0846-4d3c-8993-863881fb05ba/resource/806b931d-d740-40df-a836-b0f1ea825d1c/download/thumb.png","title":"Mercury H-8 Tolstoj Nomenclature"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"moon_lac_8_kirkwood_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/moon_lac_8_kirkwood_nomenclature","pubdate":"2013-01-25","thumb":"https://astrogeology.usgs.gov/ckan/dataset/301ca1c3-a078-4f46-8cd5-05c39857a504/resource/bb093f01-1c2c-45cf-acd7-3875c19f55ca/download/thumb.png","title":"Moon LAC-8 Kirkwood Nomenclature"},{"abstract":"","geoform":["Geologic Map","Raster Data","Vector Data"],"name":"mars_geologic_map_of_science_study_area_8_apollinaris_patera_region","onlink":"https://astrogeology.usgs.gov/search/map/mars_geologic_map_of_science_study_area_8_apollinaris_patera_region","pubdate":"1994-01-01","thumb":"https://astrogeology.usgs.gov/ckan/dataset/e746b80d-86d1-4002-aea1-4415a8bea0b6/resource/0b6516cc-eaf5-4563-a38a-dceb10108a94/download/thumb.png","title":"Mars Geologic Map of Science Study Area 8, Apollinaris Patera Region"},{"abstract":"This digital terrain model (DTM) was produced as part of an effort to characterize topography within candidate landing ellipses for the Mars InSight mission and to aid entry, descent, and landing simulations","geoform":["Digital Elevation Model","Landing Site Map","Raster Data"],"name":"ctx_digital_terrain_model_of_mars_insight_landing_site_ellipse_8_west","onlink":"https://astrogeology.usgs.gov/search/map/ctx_digital_terrain_model_of_mars_insight_landing_site_ellipse_8_west","pubdate":"2016-10-11","thumb":"https://astrogeology.usgs.gov/ckan/dataset/2288fda4-2217-4c3f-8093-fab0fd8bd3d1/resource/6da9fd81-aedf-4b68-82b9-7d9fc4cb9b01/download/d18_034427_1842_d17_033939_1843_20m_dtm-thumb.jpg","title":"CTX Digital Terrain Model of Mars InSight Landing Site Ellipse 8 West"},{"abstract":"This product represents adirectional topographic slopes over 20 meter horizontal baselines within part of a candidate landing site for the Mars InSight mission. The slope map was derived from a CTX-based digital","geoform":["Digital Elevation Model","Landing Site Map","Raster Data"],"name":"topographic_slopes_of_mars_insight_landing_site_ellipse_8_west","onlink":"https://astrogeology.usgs.gov/search/map/topographic_slopes_of_mars_insight_landing_site_ellipse_8_west","pubdate":"2016-10-11","thumb":"https://astrogeology.usgs.gov/ckan/dataset/02b4b95e-57a4-4b80-aabb-708a19a053ab/resource/ebdf968a-9dd2-4695-b7ec-a9626a1971be/download/d18_034427_1842_d17_033939_1843_20m_slope_20m-thumb.jpg","title":"Topographic Slopes of Mars InSight Landing Site Ellipse 8 West"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"mars_mc_8_amazonis_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/mars_mc_8_amazonis_nomenclature","pubdate":"2017-07-11","thumb":"https://astrogeology.usgs.gov/ckan/dataset/f5942ebf-7877-44f2-9a85-21be057dabfe/resource/705c1a09-adfd-45ee-84a0-2f5ee7861f0a/download/thumb.png","title":"Mars MC-8 Amazonis Nomenclature"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"moon_lac_79_colombo_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/moon_lac_79_colombo_nomenclature","pubdate":"2013-10-25","thumb":"https://astrogeology.usgs.gov/ckan/dataset/73d8ffe4-30c6-4e51-a8ef-d63f1b50b4df/resource/e1e3899b-6b2b-483d-8a59-d982dc932a5f/download/thumb.png","title":"Moon LAC-79 Colombo Nomenclature"},{"abstract":"This image mosaic is one of several products created as the first step of cartography planning in support of the Cassini-Huygens Mission to Saturn & Titan. The data included in these mosaics","geoform":["Airbrush","Global Mosaic","Raster Data","Remote-sensing Data"],"name":"iapetus_voyager_airbrush_global_mosaic_783m","onlink":"https://astrogeology.usgs.gov/search/map/iapetus_voyager_airbrush_global_mosaic_783m","pubdate":null,"thumb":"https://astrogeology.usgs.gov/ckan/dataset/65d92f60-6239-46ca-b3e1-14a757c64f62/resource/41ee316c-8ccc-4c06-8856-0e66aa25e849/download/thumb.png","title":"Iapetus Voyager Airbrush Global Mosaic 783m"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"moon_lac_78_theophilus_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/moon_lac_78_theophilus_nomenclature","pubdate":"2013-01-25","thumb":"https://astrogeology.usgs.gov/ckan/dataset/8d1b2acf-1297-4aa0-90c8-8ff5712ff87e/resource/fd9efc02-b1ac-46c3-bbdd-91d7de2a74fd/download/thumb.png","title":"Moon LAC-78 Theophilus Nomenclature"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"moon_lac_77_ptolemaeus_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/moon_lac_77_ptolemaeus_nomenclature","pubdate":"2013-01-25","thumb":"https://astrogeology.usgs.gov/ckan/dataset/3f0c347d-63a5-4e7e-87db-09e5fc2df95c/resource/8db73242-7936-4886-93ee-d003f4b15c21/download/thumb.png","title":"Moon LAC-77 Ptolemaeus Nomenclature"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"moon_lac_76_montes_riphaeus_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/moon_lac_76_montes_riphaeus_nomenclature","pubdate":"2013-01-25","thumb":"https://astrogeology.usgs.gov/ckan/dataset/5a01a4af-4128-49bc-9dbd-de01ab903183/resource/5dfdc69f-8522-4744-8345-dbe0b5de0c30/download/thumb.png","title":"Moon LAC-76 Montes Riphaeus Nomenclature"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"moon_lac_75_letronne_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/moon_lac_75_letronne_nomenclature","pubdate":"2013-01-25","thumb":"https://astrogeology.usgs.gov/ckan/dataset/3875f6b3-7e30-4af1-9e60-8ddb961db9b9/resource/0b9b6168-89de-4027-9432-74ddc5ecac89/download/thumb.png","title":"Moon LAC-75 Letronne Nomenclature"},{"abstract":"Product Information: This mosaic was created from the Magellan F-BIDRs, (Full resolution Basic Image Data Records), the highest resolution radar images of the Venus surface (~75 m/pixel). For a smaller download, this","geoform":["Global Mosaic","Raster Data","Remote-sensing Data"],"name":"venus_magellan_sar_fmap_left_look_global_mosaic_75m","onlink":"https://astrogeology.usgs.gov/search/map/venus_magellan_sar_fmap_left_look_global_mosaic_75m","pubdate":"2015-08-01","thumb":"https://astrogeology.usgs.gov/ckan/dataset/dbef2da4-5ed3-4d99-b7bb-5391ee8d5f10/resource/dfde201a-cf22-4be5-97ea-8335a92acce8/download/thumb.png","title":"Venus Magellan SAR FMAP Left Look Global Mosaic 75m"},{"abstract":"Product Information: This mosaic was created from the Magellan Full resolution Basic Image Data Records (F-BIDRs), the highest resolution radar images of the Venus surface (~75 meters per pixel [m]). Even though","geoform":["Global Mosaic","Raster Data","Remote-sensing Data"],"name":"venus_magellan_sar_fmap_right_look_global_mosaic_75m","onlink":"https://astrogeology.usgs.gov/search/map/venus_magellan_sar_fmap_right_look_global_mosaic_75m","pubdate":"2015-08-01","thumb":"https://astrogeology.usgs.gov/ckan/dataset/4550c68e-dfec-4c41-82f8-d5535ef7508d/resource/330266fa-6e43-4918-9b87-40bb082d8650/download/thumb.png","title":"Venus Magellan SAR FMAP Right Look Global Mosaic 75m"},{"abstract":"Product Information: This mosaic was created from the Magellan Full resolution Basic Image Data Records (F-BIDRs), the highest resolution radar images of the Venus surface (~75 meters per pixel [m]). Even though","geoform":["Global Mosaic","Image","Raster Data","Remote-sensing Data"],"name":"venus_magellan_sar_fmap_stereo_look_global_mosaic_75m","onlink":"https://astrogeology.usgs.gov/search/map/venus_magellan_sar_fmap_stereo_look_global_mosaic_75m","pubdate":"2015-08-30","thumb":"https://astrogeology.usgs.gov/ckan/dataset/1518f376-96fe-452b-8afb-4114d207e71f/resource/a07daca9-b804-470d-8e59-409b998eb809/download/thumb.png","title":"Venus Magellan SAR FMAP Stereo Look Global Mosaic 75m"},{"abstract":"Product Information: The Mars Global Surveyor (MGS) Thermal Emission Spectrometer (TES) has acquired a variety of observations, including broadband visible/near-IR (VISIR) data (0.3 to 2.9 micrometers) and broadband thermal IR data (5.1","geoform":["Global Mosaic","Raster Data","Remote-sensing Data"],"name":"mars_mgs_tes_global_bolometric_albedo_map_7410m","onlink":"https://astrogeology.usgs.gov/search/map/mars_mgs_tes_global_bolometric_albedo_map_7410m","pubdate":null,"thumb":"https://astrogeology.usgs.gov/ckan/dataset/a5083068-715f-448d-9ff7-463a72d7c903/resource/537fa61c-e646-4d7b-83b0-ae607cac030f/download/thumb.png","title":"Mars MGS TES Global Bolometric Albedo Map 7410m"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"moon_lac_74_grimaldi_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/moon_lac_74_grimaldi_nomenclature","pubdate":"2013-01-25","thumb":"https://astrogeology.usgs.gov/ckan/dataset/b8fb610d-445c-4168-8d55-d1537e99ae9d/resource/934e624e-6f19-4fd6-a385-75ddc286345a/download/thumb.png","title":"Moon LAC-74 Grimaldi Nomenclature"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"moon_lac_73_riccioli_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/moon_lac_73_riccioli_nomenclature","pubdate":"2013-01-25","thumb":"https://astrogeology.usgs.gov/ckan/dataset/dcb51ca9-a89d-4f5d-88f4-30e3cb2c5b45/resource/6ecd69c2-c6dd-4ae9-98e6-fb32bf057ac1/download/thumb.png","title":"Moon LAC-73 Riccioli Nomenclature"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"moon_lac_72_nobel_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/moon_lac_72_nobel_nomenclature","pubdate":"2015-05-26","thumb":"https://astrogeology.usgs.gov/ckan/dataset/05fbfa22-c7ce-49f7-b45b-0e3484839ae2/resource/a6a6f983-e7e4-4339-b3fc-ec5fc4c35088/download/thumb.png","title":"Moon LAC-72 Nobel Nomenclature"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"moon_lac_71_michelson_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/moon_lac_71_michelson_nomenclature","pubdate":"2017-07-25","thumb":"https://astrogeology.usgs.gov/ckan/dataset/29f88aad-5487-4957-9ad0-3a22518dc692/resource/946b9f26-1676-4155-8751-11171334ea74/download/thumb.png","title":"Moon LAC-71 Michelson Nomenclature"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"moon_lac_70_kibalchich_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/moon_lac_70_kibalchich_nomenclature","pubdate":"2013-01-25","thumb":"https://astrogeology.usgs.gov/ckan/dataset/59186b61-9fcd-4adb-944b-cb7ab4fc31e9/resource/4ec7e410-18cf-4da4-b413-a9a858320782/download/thumb.png","title":"Moon LAC-70 Kibalchich Nomenclature"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"venus_v_7_lakshmi_planum_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/venus_v_7_lakshmi_planum_nomenclature","pubdate":"2012-06-07","thumb":"https://astrogeology.usgs.gov/ckan/dataset/1ec2c0cf-65eb-433d-8733-002c359dfae8/resource/c0f2782c-a92f-4424-bcd0-21c3014310ba/download/thumb.png","title":"Venus V-7 Lakshmi Planum Nomenclature"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"mercury_h_7_beethoven_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/mercury_h_7_beethoven_nomenclature","pubdate":"2017-03-15","thumb":"https://astrogeology.usgs.gov/ckan/dataset/8ba60484-646e-4501-8f3d-0186710f4f64/resource/5c76be30-8e91-426a-9a7c-39a495955aae/download/thumb.png","title":"Mercury H-7 Beethoven Nomenclature"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"moon_lac_7_karpinskij_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/moon_lac_7_karpinskij_nomenclature","pubdate":"2013-01-25","thumb":"https://astrogeology.usgs.gov/ckan/dataset/ce77c7b9-88ec-42c0-bb86-8512a07a421d/resource/92d49ff1-d473-4ca7-a447-b7cdd4c29c0d/download/thumb.png","title":"Moon LAC-7 Karpinskij Nomenclature"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"mars_mc_7_cebrenia_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/mars_mc_7_cebrenia_nomenclature","pubdate":"2017-07-11","thumb":"https://astrogeology.usgs.gov/ckan/dataset/b1a6b234-ba5d-4d38-aa66-578140de4520/resource/9ad5560a-87e6-4477-92b4-a729d31f3947/download/thumb.png","title":"Mars MC-7 Cebrenia Nomenclature"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"moon_lac_69_zhukovskij_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/moon_lac_69_zhukovskij_nomenclature","pubdate":"2017-07-25","thumb":"https://astrogeology.usgs.gov/ckan/dataset/32ef413f-361f-465c-80b8-46f099364620/resource/57b16ecf-4fd2-425f-9dec-dfa9a0427ee8/download/thumb.png","title":"Moon LAC-69 Zhukovskij Nomenclature"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"moon_lac_68_sharonov_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/moon_lac_68_sharonov_nomenclature","pubdate":"2017-05-02","thumb":"https://astrogeology.usgs.gov/ckan/dataset/b846faf6-45d4-44f2-92db-19ddd90f7a43/resource/bc5799b2-ee3f-444f-a957-bea3da74f1fe/download/thumb.png","title":"Moon LAC-68 Sharonov Nomenclature"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"moon_lac_67_mandel_shtam_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/moon_lac_67_mandel_shtam_nomenclature","pubdate":"2017-07-25","thumb":"https://astrogeology.usgs.gov/ckan/dataset/d85e28ab-e3f1-49f4-9315-141f891d7c7e/resource/a1a73802-2121-4fab-a8fe-4f4fe414d418/download/thumb.png","title":"Moon LAC-67 Mandel'shtam Nomenclature"},{"abstract":"Product Information: This color mosaic is comprised of photometrically corrected I/F (radiance factor) for 3 narrow-band color filters of the Mercury Dual Imaging System (MDIS) Wide Angle Camera (WAC), placing the 1000-nm,","geoform":["Global Mosaic","Remote-sensing Data"],"name":"mercury_messenger_mdis_global_color_mosaic_665m","onlink":"https://astrogeology.usgs.gov/search/map/mercury_messenger_mdis_global_color_mosaic_665m","pubdate":null,"thumb":"https://astrogeology.usgs.gov/ckan/dataset/b8ad92a0-5cb2-4db9-ae66-d0ef3a747bb7/resource/22f86f44-3efe-4f87-a32f-961bfc8071c1/download/thumb.png","title":"Mercury MESSENGER MDIS Global Color Mosaic 665m"},{"abstract":"This mosaic shows Mercury's surface in \"enhanced color,\" a term used to describe a color scheme created to emphasize color differences on Mercury's surface. This is not what Mercury would look like","geoform":["Global Mosaic","Raster Data","Remote-sensing Data"],"name":"mercury_messenger_mdis_basemap_enhanced_color_global_mosaic_665m","onlink":"https://astrogeology.usgs.gov/search/map/mercury_messenger_mdis_basemap_enhanced_color_global_mosaic_665m","pubdate":"2016-05-13","thumb":"https://astrogeology.usgs.gov/ckan/dataset/3599a192-1df1-49c7-a328-f5936df16155/resource/6c5fddc9-a8a0-422a-a585-d6e09fd227e6/download/thumb.png","title":"Mercury MESSENGER MDIS Basemap Enhanced Color Global Mosaic 665m"},{"abstract":"Product Information: Using the Integrated Software for Imagers and Spectrometers (ISIS3) and observations from Mercury Dual Imaging System (MDIS) narrow-angle camera (NAC) and multispectral wide-angle camera (WAC), we derived a global digital","geoform":["Digital Elevation Model","Raster Data","Topographic Map"],"name":"mercury_messenger_global_dem_665m","onlink":"https://astrogeology.usgs.gov/search/map/mercury_messenger_global_dem_665m","pubdate":"2016-10-21","thumb":"https://astrogeology.usgs.gov/ckan/dataset/75db9745-e9c5-4a6d-8dea-39f704a163cc/resource/cb55826f-bc9a-4e09-ad3d-22ee3e1d22fd/download/thumb.png","title":"Mercury MESSENGER Global DEM 665m"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"moon_lac_66_mendeleev_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/moon_lac_66_mendeleev_nomenclature","pubdate":"2013-01-25","thumb":"https://astrogeology.usgs.gov/ckan/dataset/146975ba-b772-42d5-86b6-e506b3fea3b4/resource/31f86def-6015-40d3-b05f-e84933b73f07/download/thumb.png","title":"Moon LAC-66 Mendeleev Nomenclature"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"moon_lac_65_ostwald_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/moon_lac_65_ostwald_nomenclature","pubdate":"2013-01-25","thumb":"https://astrogeology.usgs.gov/ckan/dataset/4857eaa3-ddd0-4ff9-9ce4-48dfe32dbd75/resource/f8f1e456-e528-4fb2-8bc7-67b067da33ee/download/thumb.png","title":"Moon LAC-65 Ostwald Nomenclature"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"moon_lac_64_babcock_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/moon_lac_64_babcock_nomenclature","pubdate":"2013-01-25","thumb":"https://astrogeology.usgs.gov/ckan/dataset/54149dc6-04e6-4a2f-9531-f1125261e688/resource/f6dfd1a9-beb3-4236-ab08-9e40329d55e7/download/thumb.png","title":"Moon LAC-64 Babcock Nomenclature"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"moon_lac_63_neper_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/moon_lac_63_neper_nomenclature","pubdate":"2013-01-25","thumb":"https://astrogeology.usgs.gov/ckan/dataset/98bcb7e7-77ef-45f2-a6f6-e0c680641edd/resource/0b6a8362-7bd4-4dc2-a7ef-5aae43a11ad4/download/thumb.png","title":"Moon LAC-63 Neper Nomenclature"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"venus_v_62_hurston_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/venus_v_62_hurston_nomenclature","pubdate":"2012-06-08","thumb":"https://astrogeology.usgs.gov/ckan/dataset/69df7804-d59c-4e80-956d-04b2d79fc68f/resource/9c0afb9c-8636-40fb-8205-5d7ec5a45481/download/thumb.png","title":"Venus V-62 Hurston Nomenclature"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"moon_lac_62_mare_undarum_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/moon_lac_62_mare_undarum_nomenclature","pubdate":"2013-01-25","thumb":"https://astrogeology.usgs.gov/ckan/dataset/d618530c-6130-4eed-90a8-0f7db99a832f/resource/fd640568-f696-4069-aff4-4733f7516df4/download/thumb.png","title":"Moon LAC-62 Mare Undarum Nomenclature"},{"abstract":"This image mosaic is one of several products created as the first step of cartography planning in support of the Cassini-Huygens Mission to Saturn & Titan. The data included in this mosaic","geoform":["Airbrush","Global Mosaic"],"name":"dione_voyager_airbrush_mosaic_610m","onlink":"https://astrogeology.usgs.gov/search/map/dione_voyager_airbrush_mosaic_610m","pubdate":null,"thumb":"https://astrogeology.usgs.gov/ckan/dataset/98d2aad1-bb01-45da-b622-75d176f777e1/resource/7f67d299-66d9-48a9-891c-25c6e4b52988/download/thumb.png","title":"Dione Voyager Airbrush Mosaic 610m"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"venus_v_61_mylitta_fluctus_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/venus_v_61_mylitta_fluctus_nomenclature","pubdate":"2012-06-08","thumb":"https://astrogeology.usgs.gov/ckan/dataset/c2cec3ea-1e74-4ecc-9bdb-b3340d023572/resource/d7a838eb-ae5a-4430-9aa3-02821b60c2e8/download/thumb.png","title":"Venus V-61 Mylitta Fluctus Nomenclature"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"moon_lac_61_taruntius_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/moon_lac_61_taruntius_nomenclature","pubdate":"2017-07-26","thumb":"https://astrogeology.usgs.gov/ckan/dataset/c9a16e56-6bd2-4dc3-827e-b06bcd2151c3/resource/0dc64594-3801-4737-a391-d796314fd204/download/thumb.png","title":"Moon LAC-61 Taruntius Nomenclature"},{"abstract":"Product Information: DAWN orbited Vesta during HAMO in 21 cycles between December 2011 and end of April 2012 and in 6 cycles between end of September end early November 2011. The FC","geoform":["Global Mosaic","Raster Data","Remote-sensing Data"],"name":"vesta_dawn_fc_hamo_global_mosaic_60m","onlink":"https://astrogeology.usgs.gov/search/map/vesta_dawn_fc_hamo_global_mosaic_60m","pubdate":"2013-12-10","thumb":"https://astrogeology.usgs.gov/ckan/dataset/ec63e420-a8bd-4a90-9341-a5754b551574/resource/3a4dc1df-3257-468f-874a-cdcc3c793927/download/thumb.png","title":"Vesta Dawn FC HAMO Global Mosaic 60m"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"venus_v_60_godiva_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/venus_v_60_godiva_nomenclature","pubdate":"2012-06-08","thumb":"https://astrogeology.usgs.gov/ckan/dataset/7a8aefb4-819d-4089-992d-948aad602759/resource/5f58f803-5b2f-4c0c-b05d-cd9600e8a55f/download/thumb.png","title":"Venus V-60 Godiva Nomenclature"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"moon_lac_60_julius_caesar_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/moon_lac_60_julius_caesar_nomenclature","pubdate":"2017-07-26","thumb":"https://astrogeology.usgs.gov/ckan/dataset/2e78ea26-6368-403c-8e46-c1e9989446e9/resource/f1885212-c1ac-49b7-8988-1efccfc54abe/download/thumb.png","title":"Moon LAC-60 Julius Caesar Nomenclature"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"venus_v_6_metis_mons_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/venus_v_6_metis_mons_nomenclature","pubdate":"2012-06-07","thumb":"https://astrogeology.usgs.gov/ckan/dataset/6701b917-51a5-4770-b207-f0db1b3309e9/resource/85b8bcc0-ee89-4316-a11a-bc1800cff894/download/thumb.png","title":"Venus V-6 Metis Mons Nomenclature"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"mercury_h_6_kuiper_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/mercury_h_6_kuiper_nomenclature","pubdate":"2017-03-15","thumb":"https://astrogeology.usgs.gov/ckan/dataset/aedcc76c-8846-4bc9-8e1f-a27930190936/resource/d8c2bf74-7e0d-444f-a0ac-2349d02d1eec/download/thumb.png","title":"Mercury H-6 Kuiper Nomenclature"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"moon_lac_6_schwarzschild_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/moon_lac_6_schwarzschild_nomenclature","pubdate":"2013-01-25","thumb":"https://astrogeology.usgs.gov/ckan/dataset/52feb332-b19b-4f1b-896a-33a5ccd94900/resource/3c86435f-c4ae-4361-a7f6-bb74a38c221b/download/thumb.png","title":"Moon LAC-6 Schwarzschild Nomenclature"},{"abstract":"","geoform":["Geologic Map","Raster Data","Vector Data"],"name":"mars_geologic_map_of_science_study_area_6_memnonia_region","onlink":"https://astrogeology.usgs.gov/search/map/mars_geologic_map_of_science_study_area_6_memnonia_region","pubdate":"1991-12-30","thumb":"https://astrogeology.usgs.gov/ckan/dataset/e63c77bd-633f-46c1-81a0-5ef08cc9e8f5/resource/d38b6050-3bf3-411e-b14e-0c3b049b179b/download/thumb.png","title":"Mars Geologic Map of Science Study Area 6. Memnonia Region"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"mars_mc_6_casius_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/mars_mc_6_casius_nomenclature","pubdate":"2017-07-11","thumb":"https://astrogeology.usgs.gov/ckan/dataset/da67f3df-9a17-4646-876d-ee98d2577cf1/resource/02989d55-fb29-49c6-b659-d17e3c7372e0/download/thumb.png","title":"Mars MC-6 Casius Nomenclature"},{"abstract":"The Ice Favorability Index (IFI) maps below are based on a geologic system model for ice deposition and evolution (Cannon and Britt 2020). The index maps are predictive, not based on surface","geoform":["Model","Raster Data"],"name":"moon_ice_favorability_index_north_pole_591mp","onlink":"https://astrogeology.usgs.gov/search/map/moon_ice_favorability_index_north_pole_591mp","pubdate":"2020-09-01","thumb":"https://astrogeology.usgs.gov/ckan/dataset/9d54fbc9-e5fa-4177-8bff-c7fb26dd2d60/resource/8b11dca7-1f44-4223-9e0f-9cde905b2f25/download/moon_icefavorabilityindex_90n000e_thumb.jpg","title":"Moon Ice Favorability Index North Pole 591mp"},{"abstract":"The Ice Favorability Index (IFI) maps below are based on a geologic system model for ice deposition and evolution (Cannon and Britt 2020). The index maps are predictive, not based on surface","geoform":["Model","Raster Data"],"name":"moon_ice_favorability_index_south_pole_591mp","onlink":"https://astrogeology.usgs.gov/search/map/moon_ice_favorability_index_south_pole_591mp","pubdate":"2020-09-01","thumb":"https://astrogeology.usgs.gov/ckan/dataset/ec96b436-480e-44c9-a62e-9b2682363d71/resource/c8621b64-091c-490e-a619-80b9af918155/download/moon_icefavorabilityindex_90s000e_thumb.jpg","title":"Moon Ice Favorability Index South Pole 591mp"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"venus_v_59_barrymore_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/venus_v_59_barrymore_nomenclature","pubdate":"2012-06-08","thumb":"https://astrogeology.usgs.gov/ckan/dataset/e868c105-111f-4aa3-ba12-ba8118f6874c/resource/d802cb8b-4021-4997-98ff-9b6168d60444/download/thumb.png","title":"Venus V-59 Barrymore Nomenclature"},{"abstract":"Product Information: This Lunar Orbiter (LO) mosaic of the Moon was constructed using photographs acquired by LO III, IV and V. Work towards constructing the global mosaic spanned over seven years. Earlier","geoform":["Global Mosaic","Grey Scale","Remote-sensing Data"],"name":"moon_lunar_orbiter_digital_photographic_global_mosaic_59m","onlink":"https://astrogeology.usgs.gov/search/map/moon_lunar_orbiter_digital_photographic_global_mosaic_59m","pubdate":"2010-02-01","thumb":"https://astrogeology.usgs.gov/ckan/dataset/5f5fae52-db25-4ac5-8c56-95cd6615cfde/resource/13e9f406-31df-4c80-a94f-7b15e17b0284/download/lunar_lo_mr_mosaic_global_100.jpg","title":"Moon Lunar Orbiter Digital Photographic Global Mosaic 59m"},{"abstract":"Product Information: This mosaic represents SELenological and Engineering Explorer (SELENE) Kaguya Multiband Imager (MI) derived submicroscopic metallic iron (SMFe; Taylor et al., 2010). The mosaic was created from topographically-corrected MI reflectance data","geoform":["Grey Scale","Mineral Map","Raster Data","Remote-sensing Data"],"name":"moon_selene_kaguya_mi_derived_submicroscopic_metallic_iron_mosaic_59m","onlink":"https://astrogeology.usgs.gov/search/map/moon_selene_kaguya_mi_derived_submicroscopic_metallic_iron_mosaic_59m","pubdate":"2016-09-01","thumb":"https://astrogeology.usgs.gov/ckan/dataset/f0baa135-fe11-4bba-8f8e-547a353c3a13/resource/f004d7f0-a638-4354-ac24-b7d686d24ff8/download/thumb.png","title":"Moon SELENE Kaguya MI Derived Submicroscopic Metallic Iron Mosaic 59m"},{"abstract":"This mosaic represents the abundance of the mineral clinopyroxene on the surface of the Moon, expressed as weight percent (wt%). The mosaic was created from topographically-corrected MI reflectance data acquired by the","geoform":["Mineral Map","Raster Data","Remote-sensing Data"],"name":"kaguya_lunar_multiband_imager_59mpp","onlink":"https://astrogeology.usgs.gov/search/map/kaguya_lunar_multiband_imager_59mpp","pubdate":"2016-09-01","thumb":"https://astrogeology.usgs.gov/ckan/dataset/e821546d-9b35-467a-bf93-6cdd2c7b1151/resource/c7b385bf-3815-4b40-a2ec-36442fd7b192/download/lunar_kaguya_mimap_mineraldeconv_clinopyroxenepercent_50n50s_100.jpg","title":"Kaguya Lunar Multiband Imager 59mpp"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"moon_lac_59_mare_vaporum_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/moon_lac_59_mare_vaporum_nomenclature","pubdate":"2013-01-25","thumb":"https://astrogeology.usgs.gov/ckan/dataset/fbfcd350-3926-4b1f-abe4-24201a765179/resource/bb1c75cf-bde0-43a7-b76c-f5abaeab2568/download/thumb.png","title":"Moon LAC-59 Mare Vaporum Nomenclature"},{"abstract":"Product Information: The Lunar Orbiter Laser Altimeter (LOLA) and SELenological and Engineering Explorer (SELENE) Kaguya Teams have created an improved lunar digital elevation model (DEM) covering latitudes within \u00b160\u00b0, at a horizontal","geoform":["Digital Elevation Model","Remote-sensing Data","Topographic Map"],"name":"moon_lro_lola_selene_kaguya_tc_dem_merge_60n60s_59m","onlink":"https://astrogeology.usgs.gov/search/map/moon_lro_lola_selene_kaguya_tc_dem_merge_60n60s_59m","pubdate":"2015-02-04","thumb":"https://astrogeology.usgs.gov/ckan/dataset/21cbb67a-ea2b-445b-8ff7-c69cae74689e/resource/cca0f639-2d71-49ac-bac5-26f3ac5e0b27/download/thumb.png","title":"Moon LRO LOLA - SELENE Kaguya TC DEM Merge 60N60S 59m"},{"abstract":"Product Information: The Lunar Orbiter Laser Altimeter (LOLA) and SELenological and Engineering Explorer (SELENE) Kaguya Teams have created this shaded relief of the improved lunar digital elevation model (DEM) covering latitudes within","geoform":["Remote-sensing Data","Topographic Map"],"name":"moon_lro_lola_selene_kaguya_tc_shaded_relief_merge_60n60s_59m","onlink":"https://astrogeology.usgs.gov/search/map/moon_lro_lola_selene_kaguya_tc_shaded_relief_merge_60n60s_59m","pubdate":"2015-09-08","thumb":"https://astrogeology.usgs.gov/ckan/dataset/7fbb2043-f438-4f03-b02b-a9ccb395af39/resource/f7320e0a-585a-4b0b-8b51-95c92113224e/download/thumb.png","title":"Moon LRO LOLA - SELENE Kaguya TC Shaded Relief Merge 60N60S 59m"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"venus_v_58_henie_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/venus_v_58_henie_nomenclature","pubdate":"2012-06-08","thumb":"https://astrogeology.usgs.gov/ckan/dataset/047b0407-42a2-44d5-aa54-a3890ba9999b/resource/9e51f05a-f227-474b-a506-0601c45c2435/download/thumb.png","title":"Venus V-58 Henie Nomenclature"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"moon_lac_58_copernicus_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/moon_lac_58_copernicus_nomenclature","pubdate":"2013-01-25","thumb":"https://astrogeology.usgs.gov/ckan/dataset/ae2273c5-42ce-4585-b59f-ca25f748c96f/resource/bf8e5973-c272-4eec-837f-96598bcc1aeb/download/thumb.png","title":"Moon LAC-58 Copernicus Nomenclature"},{"abstract":"The data included in this mosaic were collected by both Voyager I and Voyager II missions and then airbrushed for cosmetic purposes.","geoform":["Airbrush","Global Mosaic","Remote-sensing Data"],"name":"tethys_voyager_global_airbrush_mosaic_572m","onlink":"https://astrogeology.usgs.gov/search/map/tethys_voyager_global_airbrush_mosaic_572m","pubdate":null,"thumb":"https://astrogeology.usgs.gov/ckan/dataset/174b2f81-9af9-4bd2-893f-2560a53024ab/resource/418995ff-8fab-48e8-b3f2-d6d4f98012af/download/thumb.png","title":"Tethys Voyager Global Airbrush Mosaic 572m"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"venus_v_57_fredegonde_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/venus_v_57_fredegonde_nomenclature","pubdate":"2012-06-08","thumb":"https://astrogeology.usgs.gov/ckan/dataset/6d9d6234-1904-41d2-bc9c-3670109c93f1/resource/c4416c0c-ba52-42b1-bd60-b48458526741/download/thumb.png","title":"Venus V-57 Fredegonde Nomenclature"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"moon_lac_57_kepler_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/moon_lac_57_kepler_nomenclature","pubdate":"2013-01-25","thumb":"https://astrogeology.usgs.gov/ckan/dataset/d1c91c09-36c7-4d43-b4cc-14ff914e7c2e/resource/37fd7c48-d5c1-4534-b5ca-507835b24669/download/thumb.png","title":"Moon LAC-57 Kepler Nomenclature"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"venus_v_56_lada_terra_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/venus_v_56_lada_terra_nomenclature","pubdate":"2012-06-08","thumb":"https://astrogeology.usgs.gov/ckan/dataset/aab24a8b-a021-4b79-ad63-981954e44c20/resource/b5d42d2d-1967-42fd-b6c6-150488fbdebe/download/thumb.png","title":"Venus V-56 Lada Terra Nomenclature"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"moon_lac_56_hevelius_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/moon_lac_56_hevelius_nomenclature","pubdate":"2013-01-25","thumb":"https://astrogeology.usgs.gov/ckan/dataset/6f886606-437e-4158-a8f3-869f2643cb1c/resource/ab0d5756-0831-41b6-9f34-aab8749a2cd1/download/thumb.png","title":"Moon LAC-56 Hevelius Nomenclature"},{"abstract":"","geoform":["Regional Mosaic"],"name":"mars_controlled_photomosaic_of_the_mtm_55043_quadrangle_argyre_planitia_region","onlink":"https://astrogeology.usgs.gov/search/map/mars_controlled_photomosaic_of_the_mtm_55043_quadrangle_argyre_planitia_region","pubdate":"1992-12-31","thumb":"https://astrogeology.usgs.gov/ckan/dataset/97ca7f21-85d6-4dcc-9174-b8daa621985a/resource/8efa6f08-b885-490c-bb9a-2e301299ac86/download/thumb.png","title":"Mars Controlled Photomosaic of the MTM -55043 Quadrangle, Argyre Planitia Region"},{"abstract":"","geoform":["Regional Mosaic"],"name":"mars_controlled_photomosaic_of_the_mtm_55036_quadrangle_argyre_planitia_region","onlink":"https://astrogeology.usgs.gov/search/map/mars_controlled_photomosaic_of_the_mtm_55036_quadrangle_argyre_planitia_region","pubdate":"1992-12-31","thumb":"https://astrogeology.usgs.gov/ckan/dataset/b194ec4f-1523-4759-b6cf-0a6b61907d4c/resource/c4acae23-59dc-4053-af84-be4ee3a9d2c5/download/thumb.png","title":"Mars Controlled Photomosaic of the MTM -55036 Quadrangle, Argyre Planitia Region"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"venus_v_55_lavinia_planitia_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/venus_v_55_lavinia_planitia_nomenclature","pubdate":"2012-06-08","thumb":"https://astrogeology.usgs.gov/ckan/dataset/c928c013-754a-490c-95fb-b3add400d840/resource/87da1082-59b7-409a-b968-17f04db638a5/download/thumb.png","title":"Venus V-55 Lavinia Planitia Nomenclature"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"moon_lac_55_vasco_a_gama_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/moon_lac_55_vasco_a_gama_nomenclature","pubdate":"2013-01-25","thumb":"https://astrogeology.usgs.gov/ckan/dataset/721fc144-e2c0-4ff8-99c6-30a67f1fa75f/resource/54ee026a-10ca-448d-a811-dab37b275652/download/thumb.png","title":"Moon LAC-55 Vasco a Gama Nomenclature"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"venus_v_54_nepthys_mons_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/venus_v_54_nepthys_mons_nomenclature","pubdate":"2012-06-08","thumb":"https://astrogeology.usgs.gov/ckan/dataset/f440236e-e08e-4e38-8923-eab50d2ec75c/resource/55a7497a-7945-4b57-a681-4d78fd14a0d4/download/thumb.png","title":"Venus V-54 Nepthys Mons Nomenclature"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"moon_lac_54_robertson_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/moon_lac_54_robertson_nomenclature","pubdate":"2013-01-25","thumb":"https://astrogeology.usgs.gov/ckan/dataset/fa28c165-4b63-4f84-bb26-fd96a06643a6/resource/51a8660e-96c3-472a-8e73-bce257a44c80/download/thumb.png","title":"Moon LAC-54 Robertson Nomenclature"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"venus_v_53_themis_regio_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/venus_v_53_themis_regio_nomenclature","pubdate":"2012-06-08","thumb":"https://astrogeology.usgs.gov/ckan/dataset/0873f62c-f51b-464e-8dcb-23c8fe6178b1/resource/6c131d68-a4a3-4337-8304-15c45d33ce12/download/thumb.png","title":"Venus V-53 Themis Regio 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(Hargitai","geoform":["Nomenclature"],"name":"venus_v_52_helen_planitia_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/venus_v_52_helen_planitia_nomenclature","pubdate":"2012-06-08","thumb":"https://astrogeology.usgs.gov/ckan/dataset/b0340629-b96d-4749-aabc-90fe2c2553dd/resource/49fe8f33-c713-46ba-9c1f-e6b438073a1e/download/thumb.png","title":"Venus V-52 Helen Planitia Nomenclature"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"moon_lac_52_joule_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/moon_lac_52_joule_nomenclature","pubdate":"2017-07-25","thumb":"https://astrogeology.usgs.gov/ckan/dataset/d8cd1b35-abdb-4ead-98a0-cf13436906e1/resource/67fd67e7-5d95-4180-b149-de3d99de0f32/download/thumb.png","title":"Moon LAC-52 Joule 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(Hargitai","geoform":["Nomenclature"],"name":"venus_v_51_imdr_regio_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/venus_v_51_imdr_regio_nomenclature","pubdate":"2012-06-08","thumb":"https://astrogeology.usgs.gov/ckan/dataset/b78795ed-ba7d-4ac5-8bba-d6019c2dd14c/resource/cf41a822-5424-4b51-b925-3257697995f0/download/thumb.png","title":"Venus V-51 Imdr Regio Nomenclature"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"moon_lac_51_cockcroft_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/moon_lac_51_cockcroft_nomenclature","pubdate":"2013-01-25","thumb":"https://astrogeology.usgs.gov/ckan/dataset/b848cf2c-767e-4da6-8eb4-154c10fadb69/resource/c02d8a39-9449-42d8-abb8-af988a18fdfb/download/thumb.png","title":"Moon LAC-51 Cockcroft Nomenclature"},{"abstract":"","geoform":["Regional Mosaic"],"name":"mars_controlled_photomosaic_of_the_mtm_50063_quadrangle_tempe_fossae_region","onlink":"https://astrogeology.usgs.gov/search/map/mars_controlled_photomosaic_of_the_mtm_50063_quadrangle_tempe_fossae_region","pubdate":"1991-12-30","thumb":"https://astrogeology.usgs.gov/ckan/dataset/c949fe53-aa1c-4288-b10e-dbd09c9bf5a8/resource/13cd2fff-a0fa-413e-ae9d-645977d707ee/download/thumb.png","title":"Mars Controlled Photomosaic of the MTM 50063 Quadrangle, Tempe Fossae Region"},{"abstract":"","geoform":["Regional Mosaic"],"name":"mars_controlled_photomosaic_of_the_mtm_50043_quadrangle_argyre_planitia_region","onlink":"https://astrogeology.usgs.gov/search/map/mars_controlled_photomosaic_of_the_mtm_50043_quadrangle_argyre_planitia_region","pubdate":"1992-12-31","thumb":"https://astrogeology.usgs.gov/ckan/dataset/627716d4-7777-47e2-bae7-15a2efadcd0a/resource/9627b5cb-2d7f-4804-8bd1-ebbc5b85ccc3/download/thumb.png","title":"Mars Controlled Photomosaic of the MTM -50043 Quadrangle, Argyre Planitia Region"},{"abstract":"","geoform":["Regional Mosaic"],"name":"mars_controlled_photomosaic_of_the_mtm_50036_quadrangle_argyre_planitia_region","onlink":"https://astrogeology.usgs.gov/search/map/mars_controlled_photomosaic_of_the_mtm_50036_quadrangle_argyre_planitia_region","pubdate":"1992-12-31","thumb":"https://astrogeology.usgs.gov/ckan/dataset/bcf148be-684d-49ab-bec9-9d5a4cfb0f78/resource/0ce7b614-7051-4595-94eb-3a0e160eb6f3/download/thumb.png","title":"Mars Controlled Photomosaic of the MTM -50036 Quadrangle, Argyre Planitia Region"},{"abstract":"Product Information: This global map base of Europa utilizes the best image quality and moderate resolution coverage supplied by the Galileo SSI (Solid-State Imaging) instrument and Voyager 1 and 2. The image","geoform":["Global Mosaic","Raster Data","Remote-sensing Data"],"name":"europa_voyager_galileo_ssi_global_mosaic_500m","onlink":"https://astrogeology.usgs.gov/search/map/europa_voyager_galileo_ssi_global_mosaic_500m","pubdate":"2010-01-01","thumb":"https://astrogeology.usgs.gov/ckan/dataset/4080036f-afc5-422e-abe9-1c0c8e4f98ea/resource/f703e7d9-76c8-49a6-b195-ce8ff7a78328/download/europa_voyager_galileossi_global_mosaic_500m_100.jpg","title":"Europa Voyager - Galileo SSI Global Mosaic 500m"},{"abstract":"Product Information: This mosaic represents a reduced-resolution version of the standard calibration Clementine near-infrared (NIR) mosaic processed to 500 meters per pixel (m) as an ISIS cube (70\u00c2\u00b0 N to 70\u00c2\u00b0 S).","geoform":["Global Mosaic","Remote-sensing Data"],"name":"moon_clementine_nir_standard_calibration_500m","onlink":"https://astrogeology.usgs.gov/search/map/moon_clementine_nir_standard_calibration_500m","pubdate":null,"thumb":"https://astrogeology.usgs.gov/ckan/dataset/96e6c9a4-23c0-4995-9e49-bc485da63884/resource/6c9de6af-5fc7-437f-9df1-e88e335458b7/download/lunar_clementine_nir_cal_100.jpg","title":"Moon Clementine NIR Standard Calibration 500m"},{"abstract":"Product Information: This mosaic represents a reduced-resolution version of the empirical calibration Clementine near-infrared (NIR) mosaic processed to 500 meters per pixel (m) spatial resolution as an ISIS cube (70\u00c2\u00b0 N to","geoform":["Global Mosaic","Remote-sensing Data"],"name":"moon_clementine_nir_empirical_calibration_500m","onlink":"https://astrogeology.usgs.gov/search/map/moon_clementine_nir_empirical_calibration_500m","pubdate":null,"thumb":"https://astrogeology.usgs.gov/ckan/dataset/1236da97-7287-4c10-95b6-9857dbcc3073/resource/6dfb641d-e5c0-46a2-9f9f-2815993a823e/download/lunar_clementine_nir_cal_empcor_100.jpg","title":"Moon Clementine NIR Empirical Calibration 500m"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"venus_v_50_isabella_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/venus_v_50_isabella_nomenclature","pubdate":"2012-06-08","thumb":"https://astrogeology.usgs.gov/ckan/dataset/f1b776f4-3993-4aaf-8445-8d0f6039ed48/resource/c3668801-9af1-4f2a-ab6d-2a95ecdbb18e/download/thumb.png","title":"Venus V-50 Isabella Nomenclature"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"moon_lac_50_fitzgerald_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/moon_lac_50_fitzgerald_nomenclature","pubdate":"2013-01-25","thumb":"https://astrogeology.usgs.gov/ckan/dataset/c651cd2c-1cdf-4616-94b1-ffb1697e41f6/resource/8a79fa78-9252-424a-8d8e-b7f5a5bd4526/download/thumb.png","title":"Moon LAC-50 Fitzgerald Nomenclature"},{"abstract":"This mosaic represents the weighted criteria values associated with a collection of near-global lunar mineral maps produced by Lemelin et al using data from the Kaguya Multiband Imager (MI). 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The mosaic was created from topographically-corrected MI reflectance data","geoform":["Mineral Map","Raster Data","Remote-sensing Data"],"name":"kaguya_lunar_multiband_imager_mi_derived_feo_weight_percent_50n50s_512ppd_59mpp","onlink":"https://astrogeology.usgs.gov/search/map/kaguya_lunar_multiband_imager_mi_derived_feo_weight_percent_50n50s_512ppd_59mpp","pubdate":"2016-09-01","thumb":"https://astrogeology.usgs.gov/ckan/dataset/7b901d50-2f55-45c0-bf2f-4ca45a9a7a1a/resource/4f8f31c8-4301-458b-803c-a0dc997cdaec/download/lunar_kaguya_mimap_mineraldeconv_feoweightpercent_50n50s_100.jpg","title":"Kaguya Lunar Multiband Imager MI Derived FeO Weight Percent 50N50S 512ppd 59mpp"},{"abstract":"This digital terrain model (DTM) mosaic over the south polar region of Mars was generated by extracting three-dimensional point clouds from approximately 400 distinct CTX stereo image pairs and interpolating them to","geoform":["Digital Elevation Model","Polar Map","Remote-sensing Data"],"name":"mars_mro_ctx_south_polar_digital_terrain_model_mosaic_50m","onlink":"https://astrogeology.usgs.gov/search/map/mars_mro_ctx_south_polar_digital_terrain_model_mosaic_50m","pubdate":"2020-09-30","thumb":"https://astrogeology.usgs.gov/ckan/dataset/d7a16ff4-3a0a-4734-b8e0-3b6045218824/resource/0e7cabde-5551-4fb7-aea6-25b585462818/download/ctx_abs_align_iau_deltaradius_mosaic_thumb.jpg","title":"Mars MRO CTX South Polar Digital Terrain Model Mosaic 50m"},{"abstract":"These polygons are beased on the original created 1:5M geologic maps for Mercury as published in the late 80's and early 90's as created by several authors. The original GIS conversion was","geoform":["Geologic Map"],"name":"mercury_5m_gis_conversion","onlink":"https://astrogeology.usgs.gov/search/map/mercury_5m_gis_conversion","pubdate":"2016-05-16","thumb":"https://astrogeology.usgs.gov/ckan/dataset/9c04dcc1-e1c7-4cc0-83d2-e4ba932be6cf/resource/edd4000e-695f-4378-b24b-ae29ac501320/download/mercury_5m_gis_conversion_100.jpg","title":"Mercury 5M GIS Conversion"},{"abstract":"Product Information: This mosaic of Phobos was created by compiling updated versions of Viking high-resolution mosaics and selecting the best high-resolution images from other spacecraft to construct an entirely new mosaic. The","geoform":["Global Mosaic","Remote-sensing Data"],"name":"phobos_viking_global_mosaic_5m","onlink":"https://astrogeology.usgs.gov/search/map/phobos_viking_global_mosaic_5m","pubdate":"2012-06-01","thumb":"https://astrogeology.usgs.gov/ckan/dataset/85290c2c-7524-44ba-9251-61ea69fcd9dd/resource/a3f3dda6-a6ab-4715-8419-71fbeb997f57/download/thumb.png","title":"Phobos Viking Global Mosaic 5m"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"venus_v_5_pandrosos_dorsa_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/venus_v_5_pandrosos_dorsa_nomenclature","pubdate":"2012-06-07","thumb":"https://astrogeology.usgs.gov/ckan/dataset/e297e34c-4ae7-461e-8b57-41c777d0e20e/resource/c27d36cd-7625-422e-80f5-ab041fc45067/download/thumb.png","title":"Venus V-5 Pandrosos Dorsa Nomenclature"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"mercury_h_5_apollonia_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/mercury_h_5_apollonia_nomenclature","pubdate":"2017-03-15","thumb":"https://astrogeology.usgs.gov/ckan/dataset/edeff37a-1520-4f1d-96fd-85b891d6b55c/resource/8c8587a3-1595-4652-969e-74e5261d09fe/download/thumb.png","title":"Mercury H-5 Apollonia Nomenclature"},{"abstract":"","geoform":["Geologic Map","Raster Data","Vector Data"],"name":"moon_geologic_map_of_apollo_landing_site_5","onlink":"https://astrogeology.usgs.gov/search/map/moon_geologic_map_of_apollo_landing_site_5","pubdate":"1969-09-07","thumb":"https://astrogeology.usgs.gov/ckan/dataset/f8b94ec8-a067-4af8-b972-f3356ec85134/resource/36ade587-025e-4121-afe3-b8b4a7c81809/download/thumb.png","title":"Moon Geologic Map of Apollo Landing Site 5"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"moon_lac_5_petermann_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/moon_lac_5_petermann_nomenclature","pubdate":"2013-01-25","thumb":"https://astrogeology.usgs.gov/ckan/dataset/72e17d69-502e-444d-86f3-f3cb7cd84a01/resource/3e01cb60-322b-4249-829f-be03ce4dbe07/download/thumb.png","title":"Moon LAC-5 Petermann Nomenclature"},{"abstract":"The 1:5,000,000-scale, Mariner-9 geological maps were the first to divide mars into 30 discrete latitudinal and longitudinal areas called the \u00e2\u0080\u0098Mars Charts\u00e2\u0080\u0099 (MCs) (Skinner et al., 2006, Gaither et al., 2015; Batson,","geoform":["Geologic Map","Vector Data"],"name":"mars_mariner_9_5m_quads_gis_conversion","onlink":"https://astrogeology.usgs.gov/search/map/mars_mariner_9_5m_quads_gis_conversion","pubdate":null,"thumb":"https://astrogeology.usgs.gov/ckan/dataset/e8f0a803-14b0-4141-8717-bb8793543d5b/resource/d8ef3805-1add-447b-9210-6c50c1ccbc0a/download/mariner9_geology_globalview_100.jpg","title":"Mars Mariner 9 5M Quads GIS Conversion"},{"abstract":"This digital terrain model (DTM) was produced as part of an effort to characterize topography within candidate landing ellipses for the Mars InSight mission and to aid entry, descent, and landing simulations","geoform":["Digital Elevation Model","Landing Site Map","Raster Data"],"name":"ctx_digital_terrain_model_of_mars_insight_landing_site_ellipse_5_west","onlink":"https://astrogeology.usgs.gov/search/map/ctx_digital_terrain_model_of_mars_insight_landing_site_ellipse_5_west","pubdate":"2016-10-11","thumb":"https://astrogeology.usgs.gov/ckan/dataset/73347af3-1898-4a8b-b709-512e87807f51/resource/eca33e27-a5eb-4f8c-aa1b-860ad1ccaec1/download/d18_034150_1838_d17_033728_1838_20m_dtm_destripe-thumb.jpg","title":"CTX Digital Terrain Model of Mars InSight Landing Site Ellipse 5 West"},{"abstract":"This product represents adirectional topographic slopes over 20 meter horizontal baselines within part of a candidate landing site for the Mars InSight mission. The slope map was derived from a CTX-based digital","geoform":["Digital Elevation Model","Landing Site Map","Raster Data"],"name":"topographic_slopes_of_mars_insight_landing_site_ellipse_5_west","onlink":"https://astrogeology.usgs.gov/search/map/topographic_slopes_of_mars_insight_landing_site_ellipse_5_west","pubdate":"2016-10-11","thumb":"https://astrogeology.usgs.gov/ckan/dataset/5cb9923a-10f7-4b97-ba0b-3264a99fb892/resource/b61da67d-0fd1-4c05-a9e4-a98eaf27ecf7/download/d18_034150_1838_d17_033728_1838_20m_slope_20m-thumb.jpg","title":"Topographic Slopes of Mars InSight Landing Site Ellipse 5 West"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"mars_mc_5_ismenius_lacus_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/mars_mc_5_ismenius_lacus_nomenclature","pubdate":"2017-07-14","thumb":"https://astrogeology.usgs.gov/ckan/dataset/e95a3e04-d6e5-4ea5-9909-f7e6bd065e4c/resource/115a08f9-eda8-4dcb-8ee3-cdcbb77607d6/download/thumb.png","title":"Mars MC-5 Ismenius Lacus Nomenclature"},{"abstract":"In early 2019, NASA's OSIRIS-REx (Origins, Spectral Interpretation, Resource Identification, and SecurityRegolith Explorer) mission surveyed asteroid (101955) Bennu with a collection of instruments, including the OSIRIS-REx Camera Suite (OCAMS) PolyCam imager. Using","geoform":["Global Mosaic"],"name":"bennu_osiris_rex_ocams_global_pan_mosaic_5cm","onlink":"https://astrogeology.usgs.gov/search/map/bennu_osiris_rex_ocams_global_pan_mosaic_5cm","pubdate":"2020-02-26","thumb":"https://astrogeology.usgs.gov/ckan/dataset/1207ce04-efa6-4c3c-a7ad-13fd6b2af827/resource/a979ae3f-6e6b-49f2-b111-78f077ea6a88/download/thumb.png","title":"Bennu OSIRIS-REx OCAMS Global PAN Mosaic 5cm"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"venus_v_49_mahuea_tholus_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/venus_v_49_mahuea_tholus_nomenclature","pubdate":"2012-06-08","thumb":"https://astrogeology.usgs.gov/ckan/dataset/c252b593-b29d-4afc-be8a-d56141459d6a/resource/4df149d5-5600-408b-a948-79d9e1dfcdf9/download/thumb.png","title":"Venus V-49 Mahuea Tholus Nomenclature"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"moon_lac_49_komarov_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/moon_lac_49_komarov_nomenclature","pubdate":"2013-01-25","thumb":"https://astrogeology.usgs.gov/ckan/dataset/65ff3cbb-ddfd-4ce1-8b96-bc6b6704d331/resource/4c319874-2965-4a59-800e-13badb693f72/download/thumb.png","title":"Moon LAC-49 Komarov Nomenclature"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"venus_v_48_artemis_chasma_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/venus_v_48_artemis_chasma_nomenclature","pubdate":"2012-06-08","thumb":"https://astrogeology.usgs.gov/ckan/dataset/3c8ab22d-e777-4b26-a38d-0eafae9dbdb8/resource/c006d267-c60c-4190-af9d-f40f1dc7d94f/download/thumb.png","title":"Venus V-48 Artemis Chasma Nomenclature"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"moon_lac_48_mare_moscoviense_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/moon_lac_48_mare_moscoviense_nomenclature","pubdate":"2013-01-25","thumb":"https://astrogeology.usgs.gov/ckan/dataset/7fcff186-673d-48ed-8a87-1e19fa39dadd/resource/75b58a73-5fe4-4ca5-9446-364b1e303a7b/download/thumb.png","title":"Moon LAC-48 Mare Moscoviense Nomenclature"},{"abstract":"Product Information: This map is based on data from the Lunar Orbiter Laser Altimeter (LOLA; Smith et al., 2010), an instrument on the National Aeronautics and Space Agency (NASA) Lunar Reconnaissance Orbiter","geoform":["Digital Elevation Model","Global Mosaic","Remote-sensing Data","Shaded-Relief Map"],"name":"moon_lro_lola_color_shaded_relief_blue_steel_474m","onlink":"https://astrogeology.usgs.gov/search/map/moon_lro_lola_color_shaded_relief_blue_steel_474m","pubdate":"2015-04-13","thumb":"https://astrogeology.usgs.gov/ckan/dataset/1da32d01-c6ba-4091-a6f8-9775308fbc0c/resource/0810c93a-ce7e-4769-b037-2860863907ea/download/thumb.png","title":"Moon LRO LOLA Color Shaded Relief Blue Steel 474m"},{"abstract":"Product Information: This near-global mosaic was generated using data from the SELenological and Engineering Explorer (SELENE) \u00e2\u0080\u009cKaguya\u00e2\u0080\u009d Terrain Camera (TC) instrument. TC source data originated as map-projected tiles at ~10 meters per","geoform":["Global Mosaic","Grey Scale","Image","Raster Data"],"name":"moon_selene_kaguya_tc_global_orthomosaic_474m","onlink":"https://astrogeology.usgs.gov/search/map/moon_selene_kaguya_tc_global_orthomosaic_474m","pubdate":null,"thumb":"https://astrogeology.usgs.gov/ckan/dataset/62b3b6d8-6037-449b-bee6-b4b577299738/resource/8a15bd6e-12c2-4289-adaa-8bde213567ea/download/thumb.png","title":"Moon SELENE Kaguya TC Global Orthomosaic 474m"},{"abstract":"Product Information: This near-global mosaic was generated using data from the SELenological and Engineering Explorer (SELENE) Kaguya Terrain Camera (TC) instrument. TC source data originated as map-projected tiles at ~10 meters per","geoform":["Global Mosaic","Grey Scale","Image","Raster Data"],"name":"moon_selene_kaguya_tc_morning_global_mosaic_474m","onlink":"https://astrogeology.usgs.gov/search/map/moon_selene_kaguya_tc_morning_global_mosaic_474m","pubdate":null,"thumb":"https://astrogeology.usgs.gov/ckan/dataset/1657d6b4-ed2d-4ab5-b2f8-e3b2ede9cea1/resource/9adb9f5b-c4f0-44fd-b2b2-708aec57f331/download/thumb.png","title":"Moon SELENE Kaguya TC Morning Global Mosaic 474m"},{"abstract":"Product Information: This near-global mosaic was generated using data from the SELenological and Engineering Explorer (SELENE) Kaguya Terrain Camera (TC) instrument. TC source data originated as map-projected tiles at ~10 meters per","geoform":["Global Mosaic","Grey Scale","Image","Raster Data"],"name":"moon_selene_kaguya_tc_evening_global_mosaic_474m","onlink":"https://astrogeology.usgs.gov/search/map/moon_selene_kaguya_tc_evening_global_mosaic_474m","pubdate":null,"thumb":"https://astrogeology.usgs.gov/ckan/dataset/74ff166c-395d-4e59-88e9-31ec66970e61/resource/ac6ecd52-df03-48dc-ad08-875c284b7a3d/download/thumb.png","title":"Moon SELENE Kaguya TC Evening Global Mosaic 474m"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"venus_v_47_juno_chasma_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/venus_v_47_juno_chasma_nomenclature","pubdate":"2012-06-08","thumb":"https://astrogeology.usgs.gov/ckan/dataset/cea9a7d2-dea6-4904-a450-02b6033620cc/resource/6296a453-5562-49ce-b800-e102e7c1eab7/download/thumb.png","title":"Venus V-47 Juno Chasma Nomenclature"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"moon_lac_47_seyfert_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/moon_lac_47_seyfert_nomenclature","pubdate":"2013-01-25","thumb":"https://astrogeology.usgs.gov/ckan/dataset/c1bc2dec-ac8a-4ebe-88f2-82f1d395b3aa/resource/71e1cde4-0b92-4f4b-9207-fa692e05c248/download/thumb.png","title":"Moon LAC-47 Seyfert Nomenclature"},{"abstract":"Product Information: This Global Emissivity Data Record (GEDR) includes all Magellan measurements in which the high-gain antenna followed the nominal look-angle profile, in which the observed emission angle varied from 48 degrees","geoform":["Remote-sensing Data"],"name":"venus_magellan_global_microwave_emissivity_4641m","onlink":"https://astrogeology.usgs.gov/search/map/venus_magellan_global_microwave_emissivity_4641m","pubdate":null,"thumb":"https://astrogeology.usgs.gov/ckan/dataset/d81b186f-8ebe-4b62-a5e5-6e6df4c1f778/resource/55a8b8b3-d762-4442-b32e-79d3a3d88e58/download/thumb.png","title":"Venus Magellan Global Microwave Emissivity 4641m"},{"abstract":"Product Information: Global Reflectivity Data Record (GREDR). The power reflection coefficients are derived by fitting altimeter echoes from the fan-beam altimetry antenna as a function of time to Hagfors' radar backscatter model","geoform":["Global Mosaic","Remote-sensing Data"],"name":"venus_magellan_global_fresnel_reflectivity_4641m","onlink":"https://astrogeology.usgs.gov/search/map/venus_magellan_global_fresnel_reflectivity_4641m","pubdate":null,"thumb":"https://astrogeology.usgs.gov/ckan/dataset/09b8a22d-a6bd-40e1-be03-72c40029a9b6/resource/1a98ffa1-12f1-407d-8875-5e6469358920/download/thumb.png","title":"Venus Magellan Global Fresnel Reflectivity 4641m"},{"abstract":"Product Information: In this Global Slope Data Record (GSDR) the surface meter-scale slopes are derived by fitting altimeter echoes from the fan-beam altimetry antenna as a function of time to Hagfors' radar","geoform":["Remote-sensing Data","Topographic Map"],"name":"venus_magellan_global_meter_scale_slope_4641m","onlink":"https://astrogeology.usgs.gov/search/map/venus_magellan_global_meter_scale_slope_4641m","pubdate":null,"thumb":"https://astrogeology.usgs.gov/ckan/dataset/fe21e58b-89d2-476a-9626-4e94682bf2ee/resource/91626056-7d7a-440c-932e-05a7a815c06b/download/thumb.png","title":"Venus Magellan Global Meter Scale Slope 4641m"},{"abstract":"Product Information: The represents the version 2 (1997 release) of the Global Topographic Data Record (GTDR-SINUS.3;2). The range to surface is derived by fitting altimeter echoes from the fan-beam altimetry antenna as","geoform":["Digital Elevation Model","Global Mosaic","Remote-sensing Data","Topographic Map"],"name":"venus_magellan_global_topography_4641m","onlink":"https://astrogeology.usgs.gov/search/map/venus_magellan_global_topography_4641m","pubdate":"1997-12-18","thumb":"https://astrogeology.usgs.gov/ckan/dataset/7f4037e5-6b34-4e12-b0f5-866beda55dc1/resource/7e881826-357c-4b90-bf7e-21255096b361/download/thumb.png","title":"Venus Magellan Global Topography 4641m"},{"abstract":"Product Information: This map is based on data from the Mars Orbiter Laser Altimeter (MOLA) (Smith, et al., 2001), an instrument on NASA's Mars Global Surveyor (MGS) spacecraft (Albee, et al., 2001).","geoform":["Remote-sensing Data","Shaded-Relief Map","Topographic Map"],"name":"mars_mgs_mola_global_color_shaded_relief_463m","onlink":"https://astrogeology.usgs.gov/search/map/mars_mgs_mola_global_color_shaded_relief_463m","pubdate":null,"thumb":"https://astrogeology.usgs.gov/ckan/dataset/0c30e797-b7d7-4d06-87c2-d3b01abcd797/resource/f1f9069e-4fb9-49b7-954d-b531a1246528/download/thumb.png","title":"Mars MGS MOLA Global Color Shaded Relief 463m"},{"abstract":"Product Information: This map is based on data from the Mars Orbiter Laser Altimeter (MOLA) (Smith, et al., 2001), an instrument on NASA's Mars Global Surveyor (MGS) spacecraft (Albee, et al., 2001).","geoform":["Digital Elevation Model","Grey Scale","Shaded-Relief Map","Topographic Map"],"name":"mars_mgs_mola_global_shaded_relief_463m","onlink":"https://astrogeology.usgs.gov/search/map/mars_mgs_mola_global_shaded_relief_463m","pubdate":null,"thumb":"https://astrogeology.usgs.gov/ckan/dataset/08ba96d7-eccd-4a3c-9af3-ef270cb23937/resource/f2c4b62d-b90b-4a57-bf13-1f77ed40cd72/download/thumb.png","title":"Mars MGS MOLA Global Shaded Relief 463m"},{"abstract":"Product Information: This digital elevation model (DEM) is based on data from the Mars Orbiter Laser Altimeter (MOLA; Smith et al., 2001), an instrument on NASA's Mars Global Surveyor (MGS) spacecraft (Albee","geoform":["Digital Elevation Model","Topographic Map"],"name":"mars_mgs_mola_dem_463m","onlink":"https://astrogeology.usgs.gov/search/map/mars_mgs_mola_dem_463m","pubdate":null,"thumb":"https://astrogeology.usgs.gov/ckan/dataset/83c20dbd-e2b3-4e5b-b019-f13d4fdffa38/resource/f317869b-9ba4-4672-9fe3-e3ce246eff8c/download/thumb.png","title":"Mars MGS MOLA DEM 463m"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed (Hargitai","geoform":["Nomenclature"],"name":"venus_v_46_aino_planitia_nomenclature","onlink":"https://astrogeology.usgs.gov/search/map/venus_v_46_aino_planitia_nomenclature","pubdate":"2012-06-08","thumb":"https://astrogeology.usgs.gov/ckan/dataset/27a4b734-d054-4218-8d4c-18633f3fffe0/resource/e659f2bc-a5c1-4fe5-91e7-9719b8cbf76c/download/thumb.png","title":"Venus V-46 Aino Planitia Nomenclature"},{"abstract":"Planetary nomenclature, like terrestrial nomenclature, is used to uniquely identify a feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed 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