These images are located in Vesta's Rheasilvia quadrangle, near asteroid Vesta's south pole. NASA's Dawn spacecraft obtained the apparent brightness image with its framing camera on Oct. 22, 2011.
Add image to your album
Email this page Post this page to your Facebook wall Tweet this page

Apparent Brightness and Topography Images of Severina Crater

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. Severina crater is the large crater in the left of the images. The topography image shows that Severina crater is a deep crater because the color-coding changes from red or yellow at Severina's rim to blue at its base. The topography image also highlights the ridges and grooves in the right side of the image.

These images are located in Vesta's Rheasilvia quadrangle, near Vesta's south pole. NASA's Dawn spacecraft obtained the apparent brightness image with its framing camera on Oct. 22, 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.

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 the Dawn mission is online at http://www.nasa.gov/dawn and http://dawn.jpl.nasa.gov.

Image details

ID#:
PIA15486

Date added:
2012-03-15

Target:
Vesta

Mission:
Dawn

Spacecraft:
Dawn

Instruments:
Framing Camera

Size:
3450 x 1900 pixels (width x height)

Rating:



Views:
1,855

Full-Res TIFF:
PIA15486.tif (19.67 MB)

Full-Res JPG:
PIA15486.jpg (0.43 MB)

Image credit:
NASA/JPL-Caltech/UCLA/MPS/DLR/IDA