Uzboi Vallis
 Uzboi Vallis based on THEMIS day-time image | |
| Coordinates | 29°48′S 37°06′W / 29.8°S 37.1°W / -29.8; -37.1Coordinates: 29°48′S 37°06′W / 29.8°S 37.1°W / -29.8; -37.1 |
|---|---|
| Length | 366.0 |
| Naming | Dry riverbed in Turkmenistan. |
Uzboi Vallis is a valley lying situated within the Margaritifer Sinus quadrangle (MC-19) region on Mars. It is named after the Uzboy dry channel, now in Turkmenistan, which repeatedly served as the main channel of the Amu Darya river. The Uzboi is dotted with seasonal ponds, lakes and brooks.
The valley begins on the northern rim of the Argyre basin, and cuts through several craters, before ending at Holden crater. Surrounding craters include Martynov to the east with a part encircled by the stream, and around the middle on the left is the small Luki crater which likely impacted after the flooding. Adjacent smaller valleys are Nirgal in the middle which it was a smaller river that drained a smaller lake and further north are Runa Vallis and Surinda Valles.
Part of Uzboi Vallis along with nearby craters Colors relate to elevation.
Uzboi Vallis is believed to have been formed by running water. It is believed that layers were formed on the floor of Uzboi Vallis (as shown in the HiRISE image below) when drainage was blocked by the impact that formed Holden Crater to the north. Eventually the lake in the area of Uzboi Vallis went high enough to overtop the rim of Holden.[1] The water then eroded the deposits to expose the layers as they are today. The sediments that make up the layers appear to be coarse in size, suggesting they were probably formed by a rapid flow.[2][3][4][5]
It has been suggested that Uzboi, Ladon, Margaritifer and Ares Valles, although now separated by large craters, once comprised a single outflow channel flowing north into Chryse Planitia.[6][7] The source of this outflow has been suggested as overflow from the Argyre crater, formerly filled to the brim as a lake by channels (Surius, Dzigai, and Palacopus Valles) draining down from the south pole. If real, the full length of this drainage system would be over 8000 km, the longest known drainage path in the solar system. This system has been called the Uzboi-Landon-Morava (ULM) system.
Layers in Uzboi Vallis, as seen by HiRISE. Image located in the Margaritifer Sinus quadrangle.
 | Wikimedia Commons has media related to Uzboi Vallis. |
References
^ http://www.uahirise.org/epo/nuggets/lake-uzboi-vallis.pdf
^ http://hirise.lpl.arizona.edu/PSP_008338_1525
^ http://hirise.lpl.arizona.edu/PSP_003077_1530
^ Grant, J., T. Parker. 2002. Drainage evolution of the Margaritifer Sinus region, Mars. J. Geophysic. Res. 107, doi:10.1029/2001JE001678.
^ Grant, J. et al. 2008. HiRISE imaging of impact megabreccia and sub-meter aqueous strata in Holden Crater, Mars. Geology: 36, 195-198.
^ Grant, J. et al. 2010. A lake in Uzboi Vallis and implications for late Noachian-Early Hesperian climate on Mars. Icarus: 212, 110-122
^ Parker, T.J., Clifford, S.m., and Banerdt, W.B. (2000). Argyre Planitia and the Mars global hydrologic cycle. LPSC XXXI, Abstract 2033.
See also
Eberswalde (crater), a partially buried crater to the north east- Climate of Mars
- Geology of Mars
- Impact crater
- Lakes on Mars
- List of craters on Mars
- Uzboi-Landon-Morava (ULM)
External links
- ESA Mars Express: Crater Holden and Uzboi Vallis
