PASADENA, Calif. -- These Dawn FC (framing camera) images show
part of the rim of the south polar basin, which is dominated by a large
scarp (eg. cliff) that runs vertically across the center of the images.
The piled-up material at the scarp’s base is likely due to landsliding.
There is also some hummocky (eg. wavy/ undulating) terrain to the left
of the scarp. The left image is an albedo image, which is taken directly
through the clear filter of the FC. Such an image shows the albedo (eg.
brightness/ darkness) of the surface. The right image uses the same
albedo image as its base but then a color-coded height representation of
the topography is overlain onto it. The topography is calculated from a
set of images that were observed from different viewing directions,
called stereo images. The various colors correspond to the height of the
area that they color. For example, white and red areas on the right are
the highest regions and the blue areas on the left are the lowest. The
change in color-coded height on the scarp from red to green illustrates
its dramatic topographic profile. The blue color-coded hummocky terrain
is located on the base of the south polar basin, which is the lowest
region in this image.
NASA’s Dawn spacecraft obtained the albedo
image with its framing camera on August 11, 2011. This image was taken
through the camera’s clear filter. The distance to the surface of Vesta
is 2740 km the image has a resolution of about 250 meters per pixel. The
images are projected using a lambert-azimuthal map projection.
.
Image Credit: NASA/ JPL-Caltech/ UCLA/ MPS/ DLR/ IDA
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