Endurance Crater
   HOME

TheInfoList



OR:

Endurance is an impact crater lying situated within the
Margaritifer Sinus quadrangle The Margaritifer Sinus quadrangle is one of a series of 30 quadrangle maps of Mars used by the United States Geological Survey (USGS) Astrogeology Research Program. The Margaritifer Sinus quadrangle is also referred to as MC-19 (Mars Chart-19) ...
(MC-19) region of the planet
Mars Mars is the fourth planet from the Sun and the second-smallest planet in the Solar System, only being larger than Mercury (planet), Mercury. In the English language, Mars is named for the Mars (mythology), Roman god of war. Mars is a terr ...
. This crater was visited by the ''Opportunity'' rover from May until December 2004. Mission scientists named the crater after the ship '' Endurance'' that sailed to the
Antarctic The Antarctic ( or , American English also or ; commonly ) is a polar region around Earth's South Pole, opposite the Arctic region around the North Pole. The Antarctic comprises the continent of Antarctica, the Kerguelen Plateau and other ...
through the Weddell Sea during the ill-fated 1914-1917 Imperial Trans-Antarctic Expedition, considered to be the last expedition of the
Heroic Age of Antarctic Exploration The Heroic Age of Antarctic Exploration was an era in the exploration of the continent of Antarctica which began at the end of the 19th century, and ended after the First World War; the Shackleton–Rowett Expedition of 1921–1922 is often cit ...
organized by
Ernest Shackleton Sir Ernest Henry Shackleton (15 February 1874 – 5 January 1922) was an Anglo-Irish Antarctic explorer who led three British expeditions to the Antarctic. He was one of the principal figures of the period known as the Heroic Age of ...
. The rover entered the crater interior on its 134th mission Timekeeping on Mars, sol (June 15), and exited on the 315th sol (December 14). During this time it traversed various obstacles, steep inclines, and overcame large wheel slippage when driving over fine sand. __TOC__


Exploration by ''Opportunity''

After arriving at the crater, ''Opportunity'' performed a surveying, survey of the crater to plan the further steps in exploring the Geology of Mars, local geology. A site dubbed "Karatepe" was chosen to enter the crater and investigate the layering of the bedrock. The picture to the right shows changes in the color of the bedrock layers. The layer "A" is closer to the rover and higher than the layers "B" to "E". Texture and geochemistry, rock chemistry also differed with depth. Thus scientists infer that the age of these layers is following a similar pattern, with the higher layers being younger than the lower layers.NASA http://apod.nasa.gov/apod/ap041115.html ''Opportunity'' then went farther down into the crater to investigate the sand dunes. Various rock outcrops were investigated while the rover descended. It was decided not to drive into the dunes, for fear the rover might get stuck permanently. Instead, ''Opportunity'' did some work on some rocks surrounding the dunes before heading back up to the rim of the crater. On the way, it encountered a boulder, nicknamed 'Wopmay', that provided inconclusive evidence that rocks near the bottom of the crater were affected by water before and after the crater formed. The rover then headed off to Burns Cliff. Burns Cliff, named for the late mineralogist Roger Burns of Massachusetts Institute of Technology, MIT, was studied closely by ''Opportunity''. High amounts of slippage prevented the rover from using its robotic arm, however high resolution imaging was conducted with the Pancam. It shows layers of sediment that might indicate deposition by a liquid. The layers in the cliff would later be followed south of the crater to identify it as a geologic formation, in this case the "Burns Formation". These names are not official until made so by the International Astronomical Union. Burns Cliff was the final science stop inside Endurance. The rover had some trouble making it out, noticing slippage, but prevailed. Leaving Endurance it headed for its heat shield where it would find the Heat Shield Rock, Meridiani Planum meteorite, which happened to be the first meteorite discovered on another planet.


Wet history

''Opportunity'' spent about half a year exploring Endurance. During that time, data collected by the rover supplanted and greatly expanded on the Extraterrestrial liquid water#Evidence of past surface water, history of water at Meridiani Planum, in addition to the confirmation that there had been liquid water here in ancient times. Endurance provided mission scientists with a cross-section of the bedrock on this part of Mars, showing that liquid water hadn't flowed across the surface just once, but was of an episodic nature, and wasn't permanently present, with floods periodically washing over the landscape, and then drying up again. Interpretation of the materials (such as sulfates) in Endurance's evaporite outcrops led mission scientists to believe that this shallow sea was probably rather acidic in nature, but couldn't rule out that life may have been present at some point.


See also

* Exploration of Mars * Geography of Mars * List of craters on Mars *Opportunity mission timeline, ''Opportunity'' mission timeline


References


Further reading

*


External links


The official Mars Exploration Rover Mission website
* Various papers on the geology encountered at Endurance Crater and the processes involved: [ftp://ftp.lpi.usra.edu/pub/outgoing/lpsc2006/full451.pdf] [ftp://ftp.lpi.usra.edu/pub/outgoing/lpsc2006/full604.pdf]
The sedimentary rocks of Sinus Meridiani: Five key observations from data acquired by the Mars Global Surveyor and Mars Odyssey orbiters
- proposes a theory on crater exhumation in the region
Endurance crater
and the surrounding plains of Meridiani Planum (panoramic image) {{DEFAULTSORT:Endurance (Crater) Impact craters on Mars Margaritifer Sinus quadrangle