Apparent Brightness and Topography Images of Eusebia Crater

• Click the image above for a larger view
• Full-Res JPEG (3100 x 1600) (297.4 kB)
• Full-Res TIFF (3100 x 1600) (14.9 MB)

Caption:

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. Eusebia crater is the large crater roughly in the center of the images. Tuccia crater is the much smaller crater centered on the top left edge of the images. It is clear in the topography image that the bottom side of Eusebia crater is quite shallow. This may be due to mass movement or slumping of material into the crater. The bowl shape of Tuccia crater is seen in the topography image and the bright rays surrounding it are clear in the apparent brightness image. There is a large ridge running horizontally across the bottom of the images. Such ridges are common in Vesta's southern hemisphere.

These images are located in Vesta's Tuccia quadrangle, in Vesta's southern hemisphere. NASA's Dawn spacecraft obtained the apparent brightness 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 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-azimuthal map projected.

Background Info:

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.

More information about Dawn is online at http://www.nasa.gov/dawn and http://dawn.jpl.nasa.gov .

Cataloging Keywords: