Dark Light

Why does HiRISE take so many repeat images of the same area? Repeat coverage actually serves a special purpose, such as detecting seasonal changes (frost deposition and sublimation) and temporal changes (dust devil tracks and avalanches.) These repeat images also give us a “sneak peek” of future pictures to determine any differences.

Such is the case for this observation which we took in June 2014, and covers a small 1-kilometer sized simple crater located in the Southern hemisphere. In this composite and enhanced image, the crater shows frost on all its south-facing slopes (e.g., the crater’s north wall and southern ejecta). This image was taken in late Martian winter as Mars is heading into spring.


Image: NASA/JPL/University of Arizona https://www.uahirise.org/hipod/ESP_037125_1315
Related Posts

Secondary Craters

This image of a southern mid-latitude crater was intended to investigate the lineated material on the crater floor. At the higher resolution of HiRISE, the image reveals a landscape peppered by small impact craters.

The Saga of Airy-0

Up to now, we’ve never imaged Airy-0, a crater within Airy Crater that formerly was used to define zero longitude on Mars.

An Impact Crater within Nanedi Valles

With this image, we can cross-dating the relative age of the impact with that of the valley system, as well as learning more about the fluvial and morphology characteristics of area.