mercredi 30 décembre 2020

Crater Slopes: The Power of a Repeat Image

 







NASA - Mars Reconnaissance Orbiter (MRO) patch.


Dec. 30, 2020


Map Projected Browse Image


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.

With a repeat image, we can now see any changes of the same crater. And what do you know: all the frost that was once present on the south-facing slopes of the crater are now gone, having sublimated and returned to the Martian atmosphere.

Mars Reconnaissance Orbiter (MRO). Image Credits: NASA/JPL-Caltech

The University of Arizona, Tucson, operates HiRISE, which was built by Ball Aerospace & Technologies Corp., Boulder, Colo. NASA's Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Mars Reconnaissance Orbiter Project for NASA's Science Mission Directorate, Washington. 

Related links:

HiRISE: https://www.uahirise.org/releases/insight/hardware

Mars Reconnaissance Orbiter (MRO): http://www.nasa.gov/mission_pages/MRO/main/index.html

Images, Text, Credits: NASA/JPL-Caltech/University of Arizona.

Greetings, Orbiter.ch