
The dark halos around the resulting impact craters are a combination of the light-toned dust being cleared from the impact event and the deposition of the underlying dark toned materials as crater ejecta. The distribution and the pattern of the rayed ejecta suggests that the meteoroid most-likely struck from the south (which is up in the cutout).
HiRISE frequently monitors new impact craters similar to this one; however, this is the first image of this particular impact taken by HiRISE, thanks to a request by the CTX team. Subsequent images will likely follow to monitor if there are any changes to the site from wind-blown activity or dust-deposition over time.
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