File:Phlegra Montes ESA240696.tiff
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editDescriptionPhlegra Montes ESA240696.tiff |
English: Phlegra Montes is a range of gently curving mountains and ridges on Mars. Flow patterns attributable to water are widely visible across the image. Linear flow patterns can be seen inside the valley (Box 1). Nearly every mountain is surrounded by an apron of rocky debris (Box 2). Over time, this debris appears to have moved down the mountainside and looks similar to the debris found covering glaciers here on Earth. Lobe-shaped structures seen inside impact craters in the region (Box 3) are known as concentric crater fill and are perhaps another indication of subsurface water ice. The High-Resolution Stereo Camera on ESA’s Mars Express collected the data for these images on 1 June 2011 during orbit 9465. |
Date | |
Source | http://www.esa.int/spaceinimages/Images/2011/12/Phlegra_Montes |
Author | European Space Agency |
Permission (Reusing this file) |
ESA/DLR/FU Berlin (G. Neukum),CC BY-SA 3.0 IGO |
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Title InfoField | Phlegra Montes |
Mission InfoField | Mars Express |
Activity InfoField | Space Science |
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editThis file is licensed under the Creative Commons Attribution-ShareAlike 3.0 IGO license.
Attribution: ESA/DLR/FU Berlin (G. Neukum)
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 12:11, 24 May 2017 | 7,000 × 3,654 (23.14 MB) | Fæ (talk | contribs) | European Space Agency, Id 240696, http://www.esa.int/spaceinimages/Images/2011/12/Phlegra_Montes, User:Fæ/Project_list/ESA |
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Image title | DB-TIFF |
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height | 3,654 |
width | 7,000 |
Width | 7,000 px |
Height | 3,654 px |
Compression scheme | LZW |
Pixel composition | Black and white (Black is 0) |
Orientation | Normal |
Number of components | 1 |
Number of rows per strip | 37 |
Horizontal resolution | 72 dpi |
Vertical resolution | 72 dpi |
Software used | Adobe Photoshop CS4 Windows |
File change date and time | 16:54, 11 November 2011 |
Color space | Uncalibrated |