1 Ceres Information Page

Derived 1 Ceres Data

The data sets listed in the table below are PDS3 legacy data sets. Once these data sets have been migrated to PDS4 they will be listed in the section above.

Data Set Name	Data Set Description	Data Resource Page	Citation
Dawn GRaND Ceres Maps	This data set contains the Dawn Ceres high level map products including Water Equivalent Hydrogen (WEH) Map, Smoothed Water Equivalent Hydrogen (WEH) Map, Thermal & Epithermal Neutron Counts Map, Iron Concentration Map, and Iron Gamma Counts Map. These maps have been generated from the GRaND L1B data taken during the Ceres Low Altitude Mapping Orbit phase of the Dawn mission.	Browse	"Prettyman, T.H., Dawn GRaND hydrogen map, DAWN-A-GRAND-5-CERES-HYDROGEN-MAP_V1.0, NASA Planetary Data System, 2017."
HST Images, Albedo Maps, and Shape of 1 Ceres	This dataset contains 267 HST ACS/HRC images of asteroid (1) Ceres obtained in 2003/2004 at three wavelengths, 535 nm, 335 nm, and 223 nm. They have been photometrically calibrated to standard reflectance unit I/F. The dataset also includes a shape for Ceres, as well as three surface albedo maps covering the area between +/-50 deg latitude, derived from these images.	Browse	"Li, J.-Y., Young, E. F., Thomas, P. C., Parker, J. Wm., McFadden, L. A., Russell, C. T., Stern, S. A., and Sykes, M. V., HST Images, Albedo Maps, and Shape of 1 Ceres V1.0. EAR-A-HSTACS-5-CERESHST-V1.0. NASA Planetary Data System, 2006."
Dawn VIR Ceres Global Maps	This data set contains global mosaics of the Dawn VIR band centers and depths of phyllosilicate absorption bands, located at 2.7 (OH band) and 3.1 microns (NH4 band), from the Ceres encounter. The data set was acquired during the Survey and Ceres Science RC3 (CSR) phases between 2015-04-25 and 2015-06-27.	Browse	"De Sanctis, M.C., M.T. Capria, E. Ammannito, A. Frigeri, F. Tosi, M. Giardino, S. Fonte, F. Zambon, DAWN VIR DERIVED CERES GLOBAL MOSAICS V1.0, DAWN-A-VIR-5-DDR-CERES-MOSAIC-V1.0, NASA Planetary Data System, 2018."
Dawn Shape Models of Ceres LAMO	This data set contains a Ceres regional digital terrain models and associated clear filter mosaics based on the Dawn Low Altitude Mapping orbit (LAMO) Framing Camera 2 (FC2) images and derived by using the stereo photo-grametric (SPG) method. The LAMO DTMs/mosaics covers the regions around the following features: Ahuna Mons and the Occator, Ernutet, Haulani, Ikapati, Kupalo/Juling, and Yalode craters. The DTM has a lateral spacing of 32 m/pixel (256 pixel/degree) and a vertical accuracy of about 1.5 m.	Browse	"Park, R.S. and Buccino, D.R., Ceres SPC Shape Model Dataset V1.0. DAWN-A-FC2-5-CERESSHAPESPC-V1.0. NASA Planetary Data System, 2018."
Dawn Shape Models of Ceres HAMO	This data set contains the Ceres digital terrain model based on the Dawn High Altitude Mapping orbit (HAMO) Framing Camera 2 (FC2) images and derived by using the stereo photo-grametric (SPG) method. The HAMO DTM covers approximately 98% of the Ceres surface (few permanently shadowed areas near the poles required interpolation). The a DTM has a lateral spacing of ~136.7 m/pixel (60 pixel/degree) and a vertical accuracy of about 10 m.	Browse	"Park, R.S. and Buccino, D.R., Ceres SPC Shape Model Dataset V1.0. DAWN-A-FC2-5-CERESSHAPESPC-V1.0. NASA Planetary Data System, 2018."
Dawn Ceres Gravity Models	This data set contains archival results from gravity investigations conducted during the Dawn mission while the spacecraft was in orbit around the asteroid Ceres. Radio measurements were made using the Dawn spacecraft and Earth-based stations of the NASA Deep Space Network (DSN). The data set includes a spherical harmonic model of Ceres's gravity field generated by the Jet Propulsion Laboratory, radial gravity acceleration map, and Bouguet map; these results were derived from raw radio tracking data.	Browse	"Park, R.S., Konopliv, A.S., Asmar, S.W., and Buccino, D.R., Dawn Ceres Derived Gravity Data, NASA Planetary Data System, DAWN-A-RSS-5-CEGR-V3.0, 2018."
Dawn Framing Camera Ceres Image Mosaics	This accumulating data set includes Ceres global mosaics and quadrangles derived from images acquired by the Framing Camera 2 (FC2) on the NASA Dawn spacecraft. Global mosaics are provided in cylindrical and polar stereographic projections. The quadrangle mosaics use Mercator (equatorial), Lambert conformal (mid-latitude) and stereographic projections. Clear and color mosaics are provided for high altitude mapping orbit (HAMO) and clear filter mosaics only in the low altitude mapping orbit (LAMO) science phases.	Browse	"Roatsch,T., E. Kersten,K.-D. Matz,F. Preusker, F. Scholten, S. Elgner, S.E. Schroeder, R. Jaumann, C.A. Raymond, C.T. Russell, DAWN FC2 DERIVED CERES MOSAICS V1.0, DAWN-A-FC2-5-CERESMOSAIC-V1.0, NASA Planetary Data System, 2016."