File:ESP 055307 2215 (42691611070).jpg
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DescriptionESP 055307 2215 (42691611070).jpg |
Pitted Cones: Possible Methane Sources? — This observation shows relatively bright mounds scattered throughout darker and diverse surfaces in Chryse Planitia. These mounds are hundreds of meters in size. The largest of the mounds shows a central pit, similar to the collapsed craters found at the summit of some volcanoes on Earth. The origins of these pitted mounds or cratered cones are uncertain. They could be the result of the interaction of lava and water, or perhaps formed from the eruption of hot mud originating from beneath the surface. NASA/JPL/University of Arizona (302 km above the surface) Source: www.uahirise.org/ESP_055307_2215 |
Date | |
Source | ESP_055307_2215 |
Author | UAHiRISE (NASA) |
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Public domainPublic domainfalsefalse |
This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.) | ||
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current | 10:20, 16 May 2019 | 2,560 × 1,920 (7.29 MB) | Meisam (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.
Orientation | Normal |
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Horizontal resolution | 72 dpi |
Vertical resolution | 72 dpi |
Software used | Adobe Photoshop CC (Macintosh) |
File change date and time | 15:00, 10 August 2018 |
Color space | sRGB |
Date and time of digitizing | 08:51, 15 September 2009 |
Date metadata was last modified | 08:00, 10 August 2018 |
Unique ID of original document | uuid:183BB7C606F9DD11BA66D1AD63D425C6 |