WMS Planetary WMS service hosted by Astrogeology, USGS 4096 4096 text/xml image/png image/jpeg image/png; mode=8bit image/vnd.jpeg-png image/vnd.jpeg-png8 application/x-pdf image/svg+xml image/tiff application/json text/plain application/vnd.ogc.gml text/xml image/png image/jpeg image/png; mode=8bit image/vnd.jpeg-png image/vnd.jpeg-png8 text/xml XML INIMAGE BLANK Ceres_North_Pole_Rasters Planetary WMS service hosted by Astrogeology, USGS EPSG:32661 -70.174228 -19.825772 53.759891 76.557684 Ceres_FC_HAMO_NPole The Dawn framing camera (FC) acquired clear filter images of Ceres with a resolution of about 140 m/pixels during the High Altitude Mapping Orbit (HAMO). DLR ortho-rectified these images and produced polar controlled mosaics of Ceres at 140m/p. Image credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA Reference: High resolution Ceres High Altitude Mapping Orbit (HAMO) atlas derived from Dawn framing camera images Planetary and Space Science, Volume 73, Issue 1, December 2012, ISSN 0032-0633 http://dx.doi.org/10.1016/j.pss.2012.08.021 Authors: Th. Roatsch(1), E. Kersten(1), K.-D. Matz(1), F. Preusker(1), F. Scholten(1), R. Jaumann(1), C. A. Raymond(2), and C. T. Russell(3) (1) Institute of Planetary Research, German Aerospace Center (DLR), Berlin, Germany; (2) Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA; (3) Institute of Geophysics, UCLA, Los Angeles, CA. -70.174228 -19.825772 53.759891 76.557684 text/xml