File:PIA20127-Ceres-DwarfPlanet-Dawn-3rdMapOrbit-HAMO-image64-20151006.jpg

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Summary

Description	English: PIA20127: Dawn HAMO Image 64 http://photojournal.jpl.nasa.gov/catalog/PIA20127 This image shows cratered terrain in the northern hemisphere of Ceres. Ikapati crater (top) appears with several flat plains filled by flows, smooth material and ejecta from the crater interior. On the crater floor and on some of the planes there are clusters of small pits and pits surrounded by light material. Dawn took this image on Oct. 6, 2015, from an altitude of 915 miles (1,470 kilometers). It has a resolution of 450 feet (140 meters) per pixel. The image is located at 36 degrees north latitude, 43 degrees east longitude. Detailed maps of the polar regions allow researchers to study the craters in this area and compare them to those covering other parts of Ceres. Variations in shape and complexity can point to different surface compositions. In addition, the bottoms of some craters located close to the poles receive no sunlight throughout Ceres' orbit around the sun. Scientists want to investigate whether surface ice can be found there. Dawn's mission is managed by JPL for NASA's Science Mission Directorate in Washington. Dawn is a project of the directorate's Discovery Program, managed by NASA's Marshall Space Flight Center in Huntsville, Alabama. UCLA is responsible for overall Dawn mission science. Orbital ATK, Inc., in Dulles, Virginia, designed and built the spacecraft. The German Aerospace Center, the Max Planck Institute for Solar System Research, the Italian Space Agency and the Italian National Astrophysical Institute are international partners on the mission team. For a complete list of acknowledgments, see http://dawn.jpl.nasa.gov/mission. For more information about the Dawn mission, visit http://dawn.jpl.nasa.gov.
Date	6 October 2015
Source	http://photojournal.jpl.nasa.gov/jpeg/PIA20127.jpg
Author	NASA/JPL-Caltech/UCLA/MPS/DLR/IDA

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