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Apparent brightness and topography images of Occia crater

Apparent brightness and topography images of Occia crater

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July 16, 2012

The left-hand image is a Dawn FC (framing camera) image, which shows the apparent brightness of Vesta’s surface. The right-hand image is based on this apparent brightness image, which has had a color-coded height representation of the topography overlain onto it. The topography is calculated from a set of images that were observed from different viewing directions, which allows stereo reconstruction. The various colors correspond to the height of the area. The white and red areas in the topography image are the highest areas and the blue areas are the lowest areas. Occia crater is the crater with dark material in the top left corner of the image. The dark material associated with Occia is not evenly spread around the crater; it is concentrated into two areas. In these areas it is both inside and outside of Occia’s rim. The topography image gives a possible explanation for why the dark material is unevenly located around Occia. The areas with the dark material generally have a lower relief (colored dark blue) than the areas without dark material. Perhaps the dark material is concentrated in these low relief areas because it is easier for it to slump into areas of lower topography.

These images are located in Vesta’s Gegania quadrangle, in Vesta’s southern hemisphere. NASA’s Dawn spacecraft obtained the apparent brightness image with its framing camera on Oct. 28, 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 70 meters (230 feet) per pixel. This image was acquired during the HAMO (high-altitude mapping orbit) phase of the mission. These images are lambert-azimuthalmap projected.

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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