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Martian landscape. This HiRISE image shows seasonal fans on the surface of Mars. These fans are likely the result of sublimation that exposes darker subsurface material is that later blown about by the wind. A unique optimised version of NASA imagery. Credit: NASA/JPL/UArizona

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Contributor:

J Marshall - Tribaleye Images / Alamy Stock Photo

Image ID:

2K5E6EB

File size:

126.3 MB (15.7 MB Compressed download)

Releases:

Model - no | Property - noDo I need a release?

Dimensions:

10240 x 4310 px | 86.7 x 36.5 cm | 34.1 x 14.4 inches | 300dpi

Date taken:

21 November 2018

Location:

Mars

Photographer:

NASA / digitaleye

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RM2JFX28C–Martian landscape. This HiRISE image shows landforms on the South Polar Residual Cap. These rounded landforms evolve relatively quickly and erode into the surface of the ice cap, approximately 4 to 5 meters (15 feet) per year.Their interesting shapes make for a striking appearance on the surface. It is referred to as a Òresidual capÓ as it relates to ice that has persisted beyond the changing of the seasons.Image is less than 5 km. An optimised and enhanced version of NASA imagery. Credit: NASA/JPL/UArizona

$Martian landscape. This HiRISE image shows landforms on the surface of Mars. Nili Fossae is often on the short-list for potential landing sites for exploration, usually due to the interesting minerals that have been detected here. This observation is to search for possible clays along a fracture in the eastern region of Nili Fossae, which is a large group of concentric grabens located near the Isidis impact basin in the Northern Hemisphere of Mars. Image area is less than 5 km (3 mi) across. A unique optimised version of NASA imagery. Credit: NASA/JPL/UArizona Stock Photo$

RM2K5E3G0–Martian landscape. This HiRISE image shows landforms on the surface of Mars. Nili Fossae is often on the short-list for potential landing sites for exploration, usually due to the interesting minerals that have been detected here. This observation is to search for possible clays along a fracture in the eastern region of Nili Fossae, which is a large group of concentric grabens located near the Isidis impact basin in the Northern Hemisphere of Mars. Image area is less than 5 km (3 mi) across. A unique optimised version of NASA imagery. Credit: NASA/JPL/UArizona

RM2JAPFF6–A Martian shield volcano with a summit caldera.Although there are a few giant shield volcanoes on Mars, there are also many smaller ones. NASA is interested in imaging the vent regions of volcanoes to understand volcanic processes, and search for signs of recent activity. This HiRISE image shows that the summit caldera is mantled by dust and covered by small impact craters, so this volcano hasnÕt been active recently enough to affect current atmospheric trace gases. This image is less than 5km (3mi) across. An optimised and enhanced version of NASA imagery. Credit: NASA/JPL/UArizona

RM2K5E6H4–Martian landscape. This HiRISE image shows the Floor of Saheki Crater, Mars. A unique optimised version of NASA imagery. Credit: NASA/JPL/UArizona

RM2K5E4YH–Martian landscape. This HiRISE image shows landforms on the surface of Mars. Dune Field Activity in Bonestell Crater. A unique optimised version of NASA imagery. Credit: NASA/JPL/UArizona

RM2K5E66F–Martian landscape. This HiRISE image shows pitted material and mounds in Chryse Planitia. The terrain here has many meter-scale pits. A unique optimised version of NASA imagery. Credit: NASA/JPL/UArizona

RM2K5E5XK–Martian landscape. This HiRISE image shows layering in Arabia Terra, Mars. With the use of stereo pairs, it is possible to determine the thickness of the deposits from this image and its counterpart. A unique optimised version of NASA imagery. Credit: NASA/JPL/UArizona

RM2K5E4YP–Martian landscape. This HiRISE image shows terrain on the southwestern portion of an impact crater in Arabia Terra, Mars, featuring dark deposits and outcrops. A unique optimised version of NASA imagery. Credit: NASA/JPL/UArizona

RM2K5E6KH–Martian landscape. This HiRISE image shows landforms on the surface of Mars. These streaks indicate the prevailing direction of the Martian wind. (Note: north is to the right in this image). A unique optimised version of NASA imagery. Credit: NASA/JPL/UArizona

RM2K5E5TR–Martian landscape. This HiRISE image of the surface of Mars shows landforms that NASA scientists call 'Swiss cheese,' There seems to be an overlap of these features by thick lobes of carbon dioxide. A unique optimised version of NASA imagery. Credit: NASA/JPL/UArizona

RM2K5E5N0–Martian landscape. This HiRISE image shows landforms on the surface of Mars. Gullies in Southern Hemisphere Crater. Less than 1 km top to bottom and north is to the left.) A unique optimised version of NASA imagery. Credit: NASA/JPL/UArizona

RM2K5E6N7–Martian landscape. This HiRISE image shows landforms on the surface of Mars. This observation captures exposed bedrock located within a very linear chain of impact craters. (North is to the right.) A unique optimised version of NASA imagery. Credit: NASA/JPL/UArizona

Martian landscape. This HiRISE image shows seasonal fans on the surface of Mars. These fans are likely the result of sublimation that exposes darker subsurface material is that later blown about by the wind. A unique optimised version of NASA imagery. Credit: NASA/JPL/UArizona

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