File:Stereoscopic view of the Nereidum Mountain Range on Mars (50300921913).jpg
![File:Stereoscopic view of the Nereidum Mountain Range on Mars (50300921913).jpg](https://upload.wikimedia.org/wikipedia/commons/thumb/4/4c/Stereoscopic_view_of_the_Nereidum_Mountain_Range_on_Mars_%2850300921913%29.jpg/800px-Stereoscopic_view_of_the_Nereidum_Mountain_Range_on_Mars_%2850300921913%29.jpg?20201203145355)
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Summary
[edit]DescriptionStereoscopic view of the Nereidum Mountain Range on Mars (50300921913).jpg |
A stereoscopic image of a region in the Nereidum Mountain Range in the southern hemisphere of Mars generated from data captured by the High Resolution Stereo Camera (HRSC) on ESA's Mars Express orbiter in 2015. The image, derived from data acquired by the nadir channel and the stereo channels of the HRSC camera provides a three-dimensional experience when viewed using red-green or red-blue glasses. Evidence of geological processes that have shaped the region north of the large Argyre impact basin can be seen in the image. Branch-like structures of valleys were carved into the slopes either by the melting snow and ice or runoff from rain in the early period of Mars’ evolution when the planet had abundant water resources. Inside the craters in the image, one can see deposits, in some cases concentric, probably created by the sublimation of ice that used to cover the region in the past. Scientists believe water ice might still be present in the region deep under the surface. Mass wasting deposits clearly visible in the canyons captured in this image are also a result of glacial processes that had taken place in the area in the past. The dark streak on the left-hand side of the image represents dune fields created by the effects of wind as it transports sand grains over large distances on the surface of Mars. On the north-facing slope of the ridge between the northern part of the dune field and the large filled crater towards the south, one can clearly see recently created alcoves and gullies. These structures are often linked to the melting of ground ice and could also point to still existing water ice deposits in the subsurface. Credits: ESA/DLR/FU Berlin, CC BY-SA 3.0 IGO |
Date | |
Source | Stereoscopic view of the Nereidum Mountain Range on Mars |
Author | European Space Agency |
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This image was originally posted to Flickr by europeanspaceagency at https://flickr.com/photos/37472264@N04/50300921913. It was reviewed on 3 December 2020 by FlickreviewR 2 and was confirmed to be licensed under the terms of the cc-by-sa-2.0. |
3 December 2020
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current | 14:53, 3 December 2020 | ![]() | 8,169 × 3,914 (26.39 MB) | Eyes Roger (talk | contribs) | Transferred from Flickr via #flickr2commons |
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This file contains additional information such as Exif metadata which may have been added by the digital camera, scanner, or software program used to create or digitize it. If the file has been modified from its original state, some details such as the timestamp may not fully reflect those of the original file. The timestamp is only as accurate as the clock in the camera, and it may be completely wrong.
Author | Björn Schreiner - FU Berlin |
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Orientation | Normal |
Horizontal resolution | 72 dpi |
Vertical resolution | 72 dpi |
Software used | Adobe Photoshop CS6 (Windows) |
File change date and time | 21:08, 12 April 2016 |
Y and C positioning | Centered |
Exif version | 2.32 |
Date and time of digitizing | 17:21, 12 April 2016 |
Meaning of each component |
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Supported Flashpix version | 1 |
Color space | Uncalibrated |
Bits per component |
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Height | 3,914 px |
Width | 8,169 px |
Pixel composition | RGB |
Number of components | 3 |
Date metadata was last modified | 23:08, 12 April 2016 |
Unique ID of original document | xmp.did:298AA4E8BE00E6118188CF7CC3C0B95E |