Product Information: Update: Oct. 14, 2021 to version 2 which includes polygonal impact craters (Excel table) as described in Zeilnhofer, 2021. The Cerean crater database contains 44,594 craters…

Product Information: This digital terrain model (DTM) of Ceres based on the Dawn High Altitude Mapping Orbit (HAMO) Framing Camera 2 (FC2) images and derived by using the stereo photogrammetry (SPG)…

This is a grayscale hillshade of the original Ceres digital terrain model (DTM). This DTM was created from the Dawn High Altitude Mapping orbit (HAMO) Framing Camera 2 (FC2) images and derived by…

Product Information: The Dawn Framing Camera (FC) captured images of Ceres with a resolution of about 140 meters per pixel (m) in 2015 (Preusker et al., 2016). German Aerospace Center (DLR)…

Product Information: DAWN orbited Vesta during HAMO in 21 cycles between December 2011 and end of April 2012. Dawn orbited Vesta during HAMO in 6 cycles between end of September end early November…

Product Information: This is a colorized shaded-relief of the original stereo-derived High Altitude Mapping Orbit (HAMO) digital terrain model (DTM). DAWN orbited Vesta during HAMO in 21 cycles…

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 took about 2,500…

Product Information: The Dawn framing camera (FC) acquired images of Ceres with a resolution of about 400 meters per pixel (m) during approach in 2015 (Preusker et al., 2016). German Aerospace…

Prior to NASA’s Dawn mission, the dwarf planet Ceres was widely believed to contain a substantial ice-rich layer below its rocky surface. The existence of such a layer has significant…

History: The IAU Working Group on Cartographic Coordinates and Rotational Elements of the Planets and Satellites was established as a consequence of a resolution adopted by Commissions 4 and 16 at…