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File:Perspective view of chaotic terrain in Mars’ Pyrrhae Regio ESA22328506.jpeg

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English: This image provides a perspective view of chaotic terrain in Mars’ Pyrrhae Regio. Chaotic terrain forms as a shifting subsurface layer of melting ice and sediment causes the surface above to collapse. This view comprises data gathered by ESA’s Mars Express on 3 August 2020 during orbit 20972. The ground resolution is approximately 16 m/pixel and the image is centred at about 322°E/16°S. This view was created using data from the nadir and colour channels of the High Resolution Stereo Camera (HRSC). The nadir channel is aligned perpendicular to the surface of Mars, as if looking straight down at the surface. HRSC stereo imaging was then used to derive the digital elevation model (DTM) upon which this oblique view is based.
Date 19 November 2020 (upload date)
Source Perspective view of chaotic terrain in Mars’ Pyrrhae Regio
Author ESA/DLR/FU Berlin
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Space Science
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Mars Express

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Attribution: ESA/DLR/FU Berlin, CC BY-SA IGO 3.0
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current12:43, 19 November 2020Thumbnail for version as of 12:43, 19 November 20201,920 × 1,080 (679 KB)OptimusPrimeBot (talk | contribs)#Spacemedia - Upload of https://www.esa.int/var/esa/storage/images/esa_multimedia/images/2020/11/perspective_view_of_chaotic_terrain_in_mars_pyrrhae_regio/22328495-1-eng-GB/Perspective_view_of_chaotic_terrain_in_Mars_Pyrrhae_Regio.jpg via Commons:Spacemedia

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