File:NASA Curiosity rover - Link to a Watery Past (692149main Williams-2pia16188-43).jpg
Summary
In this image from NASA's Curiosity rover, a rock outcrop called Link pops out from a Martian surface that is elsewhere blanketed by reddish-brown dust. The fractured Link outcrop has blocks of exposed, clean surfaces. Rounded gravel fragments, or clasts, up to a couple inches (few centimeters) in size are in a matrix of white material. Many gravel-sized rocks have eroded out of the outcrop onto the surface, particularly in the left portion of the frame. The outcrop characteristics are consistent with a sedimentary conglomerate, or a rock that was formed by the deposition of water and is composed of many smaller rounded rocks cemented together. Water transport is the only process capable of producing the rounded shape of clasts of this size.
Licensing
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File history
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 15:31, 12 January 2017 | 1,276 × 957 (912 KB) | 127.0.0.1 (talk) | In this image from NASA's Curiosity rover, a rock outcrop called Link pops out from a Martian surface that is elsewhere blanketed by reddish-brown dust. The fractured Link outcrop has blocks of exposed, clean surfaces. Rounded gravel fragments, or clasts, up to a couple inches (few centimeters) in size are in a matrix of white material. Many gravel-sized rocks have eroded out of the outcrop onto the surface, particularly in the left portion of the frame. The outcrop characteristics are consistent with a sedimentary conglomerate, or a rock that was formed by the deposition of water and is composed of many smaller rounded rocks cemented together. Water transport is the only process capable of producing the rounded shape of clasts of this size. | |
15:31, 12 January 2017 | 1,276 × 957 (912 KB) | 127.0.0.1 (talk) | In this image from NASA's Curiosity rover, a rock outcrop called Link pops out from a Martian surface that is elsewhere blanketed by reddish-brown dust. The fractured Link outcrop has blocks of exposed, clean surfaces. Rounded gravel fragments, or clasts, up to a couple inches (few centimeters) in size are in a matrix of white material. Many gravel-sized rocks have eroded out of the outcrop onto the surface, particularly in the left portion of the frame. The outcrop characteristics are consistent with a sedimentary conglomerate, or a rock that was formed by the deposition of water and is composed of many smaller rounded rocks cemented together. Water transport is the only process capable of producing the rounded shape of clasts of this size. |
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File usage
The following 25 pages link to this file:
- Adirondack (Mars)
- Barnacle Bill (Martian rock)
- Bathurst Inlet (rock)
- Block Island meteorite
- Bounce Rock
- Composition of Mars
- El Capitan (Mars)
- Geology of Mars
- Goulburn (Mars)
- Heat Shield Rock
- Home Plate (Mars)
- Hottah (Mars)
- Jake Matijevic (rock)
- Last Chance (Mars)
- Link (Mars)
- List of rocks on Mars
- Mackinac Island meteorite
- N165
- Oileán Ruaidh (Mars rock)
- Pot of Gold (Mars)
- Rocknest 3 (rock)
- Shelter Island meteorite
- Tintina (rock)
- Yogi Rock
- Template:MarsRocks