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Image of the Mare Australe Quadrangle (MC-30). The region includes the South Polar ice cap. The central part is mainly a permanent residual ice cap su
Image of the Mare Australe Quadrangle (MC-30). The region includes the South Polar ice cap. The central part is mainly a permanent residual ice cap surrounded by layered and troughed terrain which is, in turn, encircled by heavily cratered terrain.
Star burst Channels caused by escaping gas, as seen by HiRISE. Star burst channels, also called spiders, may be about 500 meters in diameter and 1 met
Star burst Channels caused by escaping gas, as seen by HiRISE. Star burst channels, also called spiders, may be about 500 meters in diameter and 1 meter deep.
Spider on the second Martian day of spring, as seen by HiRISE
Spider on the second Martian day of spring, as seen by HiRISE
Some spider 14 Martian days later, as seen by HiRISE. Notice increased dark fans caused by outgassing of carbon dioxide and dark material.
Some spider 14 Martian days later, as seen by HiRISE. Notice increased dark fans caused by outgassing of carbon dioxide and dark material.
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Image of the Mare Boreum Quadrangle (MC-1). The region includes the North Polar ice cap, Korolov crater and Chasma Boreale.
Image of the Mare Boreum Quadrangle (MC-1). The region includes the North Polar ice cap, Korolov crater and Chasma Boreale.
Layers exposed in northern ice cap, as seen by HiRISE under HiWish program
Layers exposed in northern ice cap, as seen by HiRISE under HiWish program
Layers exposed in northern ice cap, as seen by HiRISE under HiWish program
Layers exposed in northern ice cap, as seen by HiRISE under HiWish program
Close view of layers exposed in northern ice cap, as seen by HiRISE under HiWish program
Close view of layers exposed in northern ice cap, as seen by HiRISE under HiWish program