Difference between revisions of "Xanthe Terra"
m (→Location) |
m (→Major features) |
||
| Line 17: | Line 17: | ||
[[File:Ganges Chasma.jpg||thumb|300px|left| File:Ganges Chasma]] | [[File:Ganges Chasma.jpg||thumb|300px|left| File:Ganges Chasma]] | ||
| − | <gallery | + | <gallery> |
File:Nanedivalles.gif|Wide view of Nanedi Vallis, as seen by Viking Orbiter 1 | File:Nanedivalles.gif|Wide view of Nanedi Vallis, as seen by Viking Orbiter 1 | ||
File:Nanedivallesmoc2.gif|Close view of Nanedi Vallis, as seen by the Mars Orbiter Camera (MOC) on Mars Global Surveyor Arrow shows small channel. | File:Nanedivallesmoc2.gif|Close view of Nanedi Vallis, as seen by the Mars Orbiter Camera (MOC) on Mars Global Surveyor Arrow shows small channel. | ||
| Line 26: | Line 26: | ||
Images from Mars Express, Mars Global Surveyor, and the Mars Reconnaissance Orbiter have revealed ancient river valleys and deltas. The deltas show many thin layers just as deltas on Earth. Scientists speculate that features in Xanthe Terra show evidence of precipitation on early Mars.<ref>http://www.spaceref.com/news/viewpr.html?pid=26527</ref> | Images from Mars Express, Mars Global Surveyor, and the Mars Reconnaissance Orbiter have revealed ancient river valleys and deltas. The deltas show many thin layers just as deltas on Earth. Scientists speculate that features in Xanthe Terra show evidence of precipitation on early Mars.<ref>http://www.spaceref.com/news/viewpr.html?pid=26527</ref> | ||
| − | <gallery class="center" widths="190px" heights="180px" > | + | <gallery class="center" widths="190px" heights="180px"> |
Image:Alluvial Fans in Mojave Crater.jpg|Alluvial Fans in Mojave Crater, as seen by HiRISE. High ground is on the right. Branched network of channels runs from higher ground (crater rim) to lower ground. | Image:Alluvial Fans in Mojave Crater.jpg|Alluvial Fans in Mojave Crater, as seen by HiRISE. High ground is on the right. Branched network of channels runs from higher ground (crater rim) to lower ground. | ||
</gallery> | </gallery> | ||
Revision as of 10:16, 12 April 2018
MOLA map showing boundaries of Xanthe Terra and other regions
Location
Xanthe Terra is a large area on Mars, centered just north of the Martian equator. Its coordinates are 3 N and 312E, and its diameter is 1867.65 km. Parts of Xanthe are in four different quadrangles: Lunae Palus, Coprates, Margaritifer Sinus, and Oxia Palus.
Its name means "golden-yellow land." “Xanthe” comes from a Greek word meaning yellow. This word is found in other words such as xanthophyll, a plant pigment often seen in leaves in the fall.
Major features
Many interesting features are found in this small region including, Ravi Vallis, Aromatum Chaos, Ophir, Ganges Chasma, Nanedi Valles, Shalbatana Vallis, Orson Welles Crater, Mutch Crater, and Da Vinci. A Viking 1 orbiter picture of Ravi Vallis and Aromatum Chaos was highly suggestive that huge floods came out of the ground in chaos regions and formed large outflow channels. Orson Welles Crater was named after Orson Welles who did the 1938 radio broadcast of “The War of the Worlds.” Mutch Crater was named after Thomas Mutch who wrote “The Geology of Mars” in 1977. Mars Global Surveyor’s MOC found a 660 foot (200 m) wide channel on the floor of Nanedi Vallis that is thought to from a continued flow that caused new downcutting.
Wide view of Nanedi Vallis, as seen by Viking Orbiter 1
Close view of Nanedi Vallis, as seen by the Mars Orbiter Camera (MOC) on Mars Global Surveyor Arrow shows small channel.
Images from Mars Express, Mars Global Surveyor, and the Mars Reconnaissance Orbiter have revealed ancient river valleys and deltas. The deltas show many thin layers just as deltas on Earth. Scientists speculate that features in Xanthe Terra show evidence of precipitation on early Mars.[1]
Alluvial Fans in Mojave Crater, as seen by HiRISE. High ground is on the right. Branched network of channels runs from higher ground (crater rim) to lower ground.
