PASADENA, Calif. -- These Dawn FC (framing camera) images show
two different resolution views of the ejecta blanket of Vesta’s “snowman
craters.” The snowman-like pattern of these craters is clearly seen in
the center of the left hand image. However, the ejecta blanket
surrounding these craters is much less obvious in the lower resolution,
left hand image. The ejecta blanket is much clearer in the higher
resolution right hand image: it is visible as an area of Vesta’s surface
which is significantly smoother than the neighboring regions. The
ejecta blanket thins towards the top left of this image and consequently
Vesta’s surface begins to appear rougher. Some older impacts are seen
through the ejecta blanket and the clusters of small, fresh craters on
the ejecta blanket are likely secondary impacts. These secondary craters
probably formed due to large debris being thrown out of the “snowmen
craters” during their formation. The smaller debris which were thrown
out formed the ejecta blanket.
NASA’s Dawn spacecraft obtained
these images with its framing camera on August 20 and September 20,
2011. These images were taken through the camera’s clear filter. The
distance to the surface of Vesta is 2740 km and 673 km and the images
have a resolution of about 260 meters and 66 meters per pixel
respectively.
Image Credit: NASA/ JPL-Caltech/ UCLA/ MPS/ DLR/ IDA
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