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It is the first mosaic of Rhea to be created using mostly only","geoform":["Global Mosaic","Raster Data","Remote-sensing Data"],"name":"rhea_cassini_voyager_global_mosaic_417m","onlink":"https://astrogeology.usgs.gov/search/map/rhea_cassini_voyager_global_mosaic_417m","pubdate":null,"thumb":"https://astrogeology.usgs.gov/ckan/dataset/22bc1015-d9c9-4212-86c3-e42061b204d4/resource/0e8b4c67-c465-4f99-a60b-8be5e18761c6/download/thumb.png","title":"Rhea Cassini - Voyager Global Mosaic 417m"},{"abstract":"<b>Product Information:</b> 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]). 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This mosaic was created from the Magellan Full resolution Basic Image Data Records (F-BIDRs),","geoform":["Global Mosaic"],"name":"venus_magellan_global_c3_mdir_synthetic_color_mosaic_4641m","onlink":"https://astrogeology.usgs.gov/search/map/venus_magellan_global_c3_mdir_synthetic_color_mosaic_4641m","pubdate":null,"thumb":"https://astrogeology.usgs.gov/ckan/dataset/128fc727-4864-4086-bf74-651d6108ce02/resource/4701f914-c19d-4376-bddb-fca8c5039ed0/download/thumb.png","title":"Venus Magellan Global C3-MDIR Synthetic Color Mosaic 4641m"},{"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 pixel","geoform":["Digital Elevation Model"],"name":"moon_lro_south_pole_dem","onlink":"https://astrogeology.usgs.gov/search/map/moon_lro_south_pole_dem","pubdate":null,"thumb":"https://astrogeology.usgs.gov/ckan/dataset/61d426ba-9e84-47cd-b2dc-8b73282a0ae1/resource/32bafc49-a2f5-4ab7-858e-6a72b20f2536/download/thumb.png","title":"Moon LRO South Pole DEM"},{"abstract":"<b>Product Information:</b> Lunar Reconnaissance Orbiter Camera (LROC) Wide Angle Camera (WAC) aboard the Lunar Reconnaissance Orbiter (LRO) has allowed the instrument team to create a global mosaic comprised of over 15,000 images","geoform":["Global Mosaic","Raster Data","Remote-sensing Data"],"name":"moon_lro_lroc_wac_global_morphology_mosaic_100m","onlink":"https://astrogeology.usgs.gov/search/map/moon_lro_lroc_wac_global_morphology_mosaic_100m","pubdate":null,"thumb":"https://astrogeology.usgs.gov/ckan/dataset/db948a2d-4d6a-4775-a0d3-12613d36f9e7/resource/9c0ea819-5bbd-464d-b402-bf36621c7bdb/download/moon_lro_lroc-wac_mosaic_global_100.jpg","title":"Moon LRO LROC WAC Global Morphology Mosaic 100m"},{"abstract":"In 2003-2005, the USGS worked under the guidance of NASA's Mars Critical Data Products Initiative to conduct research on how controlled large area or global 2001 Mars Odyssey THEMIS IR image mosaics","geoform":["Regional Mosaic"],"name":"gusev_crater_mer_landing_site_ellipse_themis_ir_mosaic","onlink":"https://astrogeology.usgs.gov/search/map/gusev_crater_mer_landing_site_ellipse_themis_ir_mosaic","pubdate":null,"thumb":"https://astrogeology.usgs.gov/ckan/dataset/ba617985-c55e-4ad1-b6a2-be63de7d4841/resource/78b0fc80-9db7-423f-a343-364d2ec6c353/download/thumb.png","title":"Gusev Crater MER Landing Site Ellipse THEMIS IR Mosaic"},{"abstract":"This mosaic represents the Thermal Emission Imaging System (THEMIS) -daytime infrared (IR) 100 meter/pixel mosaic (version 12) released in the summer of 2014 by Arizona State University. 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