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October 4, 2012
This Dawn framing camera (FC) image of Vesta shows Licinia crater, which is the large crater in the center of the image. Licinia has a fresh, sharp rim that is scalloped in shape. Around the side of Licinia crater there are many streaks of dark and bright material cascading towards the crater’s center. There are also many hummocky slumps of material around the crater’s walls and base. There is a mound of material in the crater’s center, which is surrounded by smooth, darker material. The possibility that such smooth material on Vesta’s surface is impact melt is currently under investigation. Licinia crater is one of the freshest craters in this image. This image is located in Vesta’s Floronia quadrangle, in Vesta’s northern hemisphere. NASA’s Dawn spacecraft obtained this image with its framing camera on Oct. 11, 2011. This image was taken through the camera’s clear filter. The distance to the surface of Vesta is 700 kilometers (435 miles) and the image has a resolution of about 63 meters (207 feet) per pixel. This image was acquired during the HAMO (high-altitude mapping orbit) phase of the mission. The Dawn mission to Vesta and Ceres is managed by NASA’s Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, for NASA’s Science Mission Directorate, Washington D.C. UCLA is responsible for overall Dawn mission science. The Dawn framing cameras have been developed and built under the leadership of the Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany, with significant contributions by DLR German Aerospace Center, Institute of Planetary Research, Berlin, and in coordination with the Institute of Computer and Communication Network Engineering, Braunschweig. The framing camera project is funded by the Max Planck Society, DLR, and NASA/JPL. Image Credit: NASA/ JPL-Caltech/ UCLA/ MPS/ DLR/ IDA

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