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Fourteen More Names Approved for Surface Features on Vesta

Tuesday, December 27, 2011

The Working Group for Planetary System Nomenclature has approved names for seven craters, two fossae, one tholus, one terra, one planitia, and two rupēs on Vesta. For details, see the list of Vesta feature names and the image of Vesta in the Gazetteer of Planetary Nomenclature. Coordinates for these names are in a system used by the Dawn Team.

Two New Names Approved for Craters on Titan

Friday, December 23, 2011

The names Hano and Momoy have been approved for craters on Titan. For more information, see the Titan page in the Gazetteer of Planetary Nomenclature.

New Names for Montes and Undae on Titan

Monday, December 5, 2011

The names of six montes (Angmar, Dolmed, Echoriath, Gram, Merlock, and Rerir Montes) and four undae (Boreas, Eurus, Notus, and Zephyrus Undae) have been approved for Titan. For details, see the list of Titan feature names in the Gazetteer of Planetary Nomenclature.

First Names for Vesta Approved

Monday, October 3, 2011

The names of fourteen craters and one tholus have been approved for Vesta. For details, see the list of Vesta feature names in the Gazetteer of Planetary Nomenclature. Coordinates for these names are in a system used by the Dawn Team.

Four New Names Approved for use on Mars

Thursday, September 29, 2011

The names Corozal, Palikir, Raga, and Tivat have been approved for use on Mars. For more information, see the maps of Mars in the Gazetteer of Planetary Nomenclature.

Longitude Defining Crater on Lutetia Named Lauriacum

Friday, September 2, 2011

The name Lauriacum has been approved for the small crater that defines zero degrees longitude on asteroid (21) Lutetia. For more information, see the Lutetia page in the Gazetteer of Planetary Nomenclature.

Mars Feature Coordinates Updated to MDIM 2.1

Thursday, August 11, 2011

The Mars portion of the Gazetteer of Planetary Nomenclature now defaults to a new set of coordinates; all of the Martian features now match the Mars Digital Image Mosaic (MDIM) 2.1 control network.

In late 2010, the coordinates of the named craters in the Martian portion of the nomenclature database were updated from values from the MDIM 2.0 control network to values in the MDIM 2.1 control network. In the spring of 2011, the remaining Martian features (i.e., all the named features that are not craters) were also updated to MDIM 2.1. Since the MDIM 2.1 network was tied to local Digital Elevation Models (DEMs) generated from Mars Orbiter Laser Altimeter (MOLA) data, this implies the features now match MOLA data products and other products in that reference frame. The GIS download that contains all of the features in the MDIM 2.0 control network is still retained in the gazetteer, but is now considered archival and will not be updated with new names or changes to approved names.

The extents and sizes of the named features were also updated, and vectors describing feature boundaries were drawn; these data are approximate and are intended solely to give the user sufficient information to identify named features and their rough extents.

This work was accomplished using ArcMap version 9.3.1 and the Mars Digital Image Mosaic 2.1. Some features are not resolved well in the 2.1 mosaic; for these cases, feature coordinates were derived from the Thermal Emission Imaging System (THEMIS) Day IR 100m global mosaic. We would like to thank Stuart Robbins (University of Colorado, Boulder) for sharing a portion of his global crater database, which provided a valuable and time-saving starting point for the crater portion of this work.

Four New Names Approved for Phobos

Thursday, July 28, 2011

Names for two craters (Öpik and Shklovsky), one planitia (Lagado Planitia), and one regio (Laputa Regio) have been approved for use on Phobos. For more information, see the Phobos page and the map of Phobos in the Gazetteer of Planetary Nomenclature.

Three New Names for Features on Mars and Changes to an Approved Name

Tuesday, June 14, 2011

The names Lipany, Oenotria Plana, and Zarqa Valles have been approved for use on Mars. The name Oenotria Scopulus has been changed to the plural form, Oenotria Scopuli, to accomodate the addition of several scarps to this feature. For more information, see the maps of MC-13 and MC-21 in the Gazetteer of Planetary Nomenclature.

Martian Crater Named Dogana

Tuesday, April 19, 2011

The name Dogana has been approved for the Martian crater located at 10.0S, 306.35E. For more information, see the database information and the map of MC-18 in the Gazetteer of Planetary Nomenclature.

Three New Lacus Names Approved on Titan

Thursday, April 7, 2011

Three new lacus names (Cardiel Lacus, Freeman Lacus, and Towada Lacus) have been approved for use on Titan. For more information, see the Titan page and the map of the north polar region of Titan in the Gazetteer of Planetary Nomenclature.

Names Approved for 36 Features on Lutetia

Tuesday, April 5, 2011

Names for 18 craters, 1 dorsum, 2 fossae, 3 labēs, 8 regiones, 2 rimae, and 2 rupēs have been approved on asteroid (21) Lutetia. For more information, see the Lutetia page in the Gazetteer of Planetary Nomenclature.

Mercury Feature Coordinates Updated to MESSENGER

Monday, March 7, 2011

In late 2010, the coordinates of the named features in the Mercury portion of the nomenclature database were updated from values from historical sources to values in the preliminary MESSENGER control network. The purpose of this work was to facilitate the identification of named features on Mercury. Dots representing the coordinates of the centers of named features will fall in the centers of the features when displayed on any map product that was created using the same control network.

The extents and sizes of the named features were also updated; these data are approximate and are intended solely to give the user sufficient information to identify named features and their rough extents.

This new set of coordinates was derived using ArcMap version 9.3.1 and the global map of Mercury.  Because MESSENGER does not yet have global coverage of Mercury, Mariner 10 data were used to fill in areas where MESSENGER has not yet collected image data.  In order for the two data sets to align, the preliminary MESSENGER control network was tied to the Mariner 10 map using several ground truth points.

The Mercury portion of the Gazetteer of Planetary Nomenclature web site now defaults to showing feature coordinates in the frame of the preliminary MESSENGER control network. The original ‘unknown’ source coordinates are still retained in the gazetteer, but this data set is now considered archival and will not be updated with new names or changes to approved names.

Themes Approved for Asteroid (21) Lutetia

Tuesday, March 1, 2011

The following themes have been approved for naming surface features on asteroid (21) Lutetia:

Craters: Cities of the Roman Empire and the adjacent parts of Europe at the time of Lutetia (52 BC - 360 AD)

Regiones: Discoverer of Lutetia, and provinces of the Roman Empire at the time of Lutetia

Other features: Rivers of the Roman Empire and the adjacent parts of Europe at the time of Lutetia

Please visit the surface features categories page in the Gazetteer of Planetary Nomenclature to see the themes for other bodies in the solar system.

Sixteen New Names Approved on Dione

Friday, February 25, 2011

New names for 13 craters and 3 fossae have been approved for Dione. For more information, see the Dione page and the map of Dione in the Gazetteer of Planetary Nomenclature.