This articlecontains too many images for its overall length. Relevant discussion may be found on thetalk page. Please helpimprove this article by removingindiscriminate collections of images or by adjusting images that aresandwiching text in accordance with Wikipedia'sManual of Style.(November 2024) (Learn how and when to remove this message)

Aureum Chaos

Map showing location of Aureum Chaos (shown on the far left) along withArsinoes Chaos (far left),Iani Chaos, Margaritifer Chaos, and other nearby features
Coordinates	4°24′S27°00′W / 4.4°S 27°W /-4.4; -27
Length	368 km
Discoverer	Mariner 9

Aureum Chaos is a rough, collapsed region (chaos terrain) in theMargaritifer Sinus quadrangle (MC-19) portion of the planetMars at approximately 4.4° south latitude and 27° west longitude, it is also in the west ofMargaritifer Terra. It is 368 km across and was named after a classical albedo feature name.^[1]

The classic name came from one of the first maps of Mars drawn bySchiaparelli who has been called the "Father of Mars." He called a feature "Aurea Cherso, which translates to the golden peninsula—an ancient name for Malaya.^[2] Aureum is the Latin word forgold. In chemistry, the symbol for gold is Au from gold's Latin name.

In many places, the canyons of Aureum Chaos are about 1 km deep—a little more than half the depth of theGrand Canyon. But, Aureum Chaos covers an area about the size of the state ofAlabama, almost 20 times larger than theGrand Canyon National Park.

Aureum Chaos is a major canyon system and collapsed area. Large outflow channels on Mars are believed to be caused by catastrophic discharges of ground water.^[3] Many of the channels begin in chaotic terrain, where the ground has apparently collapsed. In the collapsed section, blocks of undisturbed material can be seen. The OMEGA experiment onMars Express discovered clay minerals (phyllosilicates) in a variety places in Aureum Chaos.Clay minerals need water to form, so the area may once have contained large amounts of water.^[4] Scientists are interested in determining what parts of Mars contained water because evidence of past or present life may be found there. Aureum Chaos is one more piece of evidence that Mars once had great amounts of water.

• 
  Huge canyons in Aureum Chaos, as seen byTHEMIS. Gullies are rare at this latitude.
• 
  Aureum Chaos, as seen from Themis.

• 
  THEMIS image of wide view of following HiRISE images. Black box shows location of HiRISE images. Image is part of the Aureum Chaos. Click on image for details.
• 
  Aureum Chaos, as seen by HiRISE, under theHiWish program.
• 
  Close up view of previous image, as seen by HiRISE under HiWish program. Small round dots are boulders.
• 
  Light toned butte on floor of crater, light toned butte, as seen by HiRISE. Arrows show outcrops of light toned material (probably sulfate-rich and once covering the whole floor).
• 
  Light toned butte, as seen by HiRISE, under HiWish program.
• 
  Close up of top of light toned butte, as seen by HiRISE under HiWish program.

• 
  Light-toned mass in Aureum Chaos, as seen by HiRISE under HiWish program Light-toned materials often form on Mars with the aid of water.
• 
  Layered features, as seen by HiRISE under HiWish program Light-toned materials often form on Mars with the aid of water. Gray material in image is probably dark, basalt sand.
• 
  Layered features, as seen by HiRISE under HiWish program Light-toned materials often form on Mars with the aid of water. Gray material in image is probably dark, basalt sand.

• List of areas of chaos terrain on Mars

• Media related toAureum Chaos at Wikimedia Commons
• The mesas of Aureum Chaos with Mars Express
• NASA Astronomy Picture of the Day: Layers in Aureum Chaos (4 April 2008)

• Margaritifer Sinus quadrangle
• Chaotic terrains on Mars

• Pages using gadget WikiMiniAtlas
• Articles with short description
• Short description matches Wikidata
• Pages with too many photos
• Coordinates on Wikidata
• Commons category link from Wikidata