Link (Mars)

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Link
NASA Curiosity rover - Link to a Watery Past (692149main Williams-2pia16188-43).jpg
"Link" rock outcrop on Mars - an ancient streambed [1] [2] [3] viewed by the Curiosity rover (September 2, 2012) (3-D version).
Feature type Rock outcrop
Coordinates 4°35′S137°26′E / 4.59°S 137.44°E / -4.59; 137.44

Link is a rock outcrop on the surface of Aeolis Palus, between Peace Vallis and Aeolis Mons ("Mount Sharp"), in Gale crater on the planet Mars. [1] [2] [3] The outcrop was encountered by the Curiosity rover on the way from Bradbury Landing to Glenelg Intrigue on September 2, 2012 (the 27th sol of the mission), and was named after a significant rock formation (and lake) in the Northwest Territories of Canada. [4] The "approximate" site coordinates are: 4°35′S137°26′E / 4.59°S 137.44°E / -4.59; 137.44 .

Contents

"Goulburn", "Link" and Hottah" rock outcrop - suggest "vigorously" flowing water in an ancient streambed (September 27, 2012). PIA16157-MarsCuriosityRover-GoulburnLinkHottah-20120927.jpg
"Goulburn", "Link" and Hottah" rock outcrop - suggest "vigorously" flowing water in an ancient streambed (September 27, 2012).
The sedimentology of "Link" (left) is strikingly similar to a terrestrial fluvial conglomerate (right). PIA16189 fig1-Curiosity Rover-Rock Outcrops-Mars and Earth.jpg
The sedimentology of "Link" (left) is strikingly similar to a terrestrial fluvial conglomerate (right).

The outcrop is a conglomerate of gravel that has been well-sorted, containing well-rounded, smooth, abraded pebbles. Pebbles and gravel a few millimeters to centimeters across are embedded in amongst a finer, white matrix. This outcrop geology is strikingly similar to some terrestrial fluvial conglomerates. [5] Around the rock are scattered well sorted loose gravel around 1 cm across, which are thought to be weathering out of the outcrop.

The rock has been interpreted as a cemented fluvial sediment, deposited by a "vigorously" flowing stream, probably between ankle and waist deep. This stream is part of an ancient alluvial fan, which descends from the steep terrain at the rim of Gale crater across its floor. [2]

See also

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A pebble is a clast of rock with a particle size of 4–64 mm (0.16–2.52 in) based on the Udden-Wentworth scale of sedimentology. Pebbles are generally considered larger than granules and smaller than cobbles. A rock made predominantly of pebbles is termed a conglomerate. Pebble tools are among the earliest known man-made artifacts, dating from the Palaeolithic period of human history.

<span class="mw-page-title-main">Conglomerate (geology)</span> Sedimentary rock composed of smaller rock fragments

Conglomerate is a sedimentary rock made up of rounded gravel-sized pieces of rock surrounded by finer-grained sediments. The larger fragments within conglomerate are called clasts, while the finer sediment surrounding the clasts is called the matrix. The clasts and matrix are typically cemented by calcium carbonate, iron oxide, silica, or hardened clay.

<span class="mw-page-title-main">Gale (crater)</span> Martian crater

Gale is a crater, and probable dry lake, at 5.4°S 137.8°E in the northwestern part of the Aeolis quadrangle on Mars. It is 154 km (96 mi) in diameter and estimated to be about 3.5–3.8 billion years old. The crater was named after Walter Frederick Gale, an amateur astronomer from Sydney, Australia, who observed Mars in the late 19th century. Mount Sharp is a mountain in the center of Gale and rises 5.5 km (18,000 ft) high. Aeolis Palus is the plain between the northern wall of Gale and the northern foothills of Aeolis Mons. Peace Vallis, a nearby outflow channel, 'flows' down from the hills to the Aeolis Palus below and seems to have been carved by flowing water. Several lines of evidence suggest that a lake existed inside Gale shortly after the formation of the crater.

<span class="mw-page-title-main">Aeolis quadrangle</span> One of a series of 30 quadrangle maps of Mars

The Aeolis quadrangle is one of a series of 30 quadrangle maps of Mars used by the United States Geological Survey (USGS) Astrogeology Research Program. The Aeolis quadrangle is also referred to as MC-23 . The Aeolis quadrangle covers 180° to 225° W and 0° to 30° south on Mars, and contains parts of the regions Elysium Planitia and Terra Cimmeria. A small part of the Medusae Fossae Formation lies in this quadrangle.

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References

  1. 1 2 Brown, Dwayne; Cole, Steve; Webster, Guy; Agle, D.C. (September 27, 2012). "NASA Rover Finds Old Streambed On Martian Surface". NASA . Retrieved September 28, 2012.
  2. 1 2 3 NASA's Curiosity Rover Finds Old Streambed on Mars. NASAtelevision. September 27, 2012. Retrieved September 28, 2012 via YouTube.
  3. 1 2 Chang, Alicia (September 27, 2012). "Mars rover Curiosity finds signs of ancient stream". AP News . Retrieved September 27, 2012.
  4. "Link to a Watery Past". 26 July 2018. Retrieved March 3, 2021.
  5. "Rock Outcrops on Mars and Earth". 26 July 2018. Retrieved March 3, 2021.