乌斯钵-拉冬-摩拉瓦谷

乌斯钵-拉冬-摩拉瓦 (Uzboi-Landon-Morava) 溢道系统是一长串的河床和洼地，可能曾携带着水流穿过了火星大部分的地区。它启源于流入阿耳古瑞区中阿耳古瑞盆地的河道。积蓄在阿耳古瑞盆地中的大水，据说随后漫溢而出向北奔流，一路穿过乌斯钵谷，进入拉冬盆地，再穿越摩拉瓦谷，最后抵达珍珠湾盆底^[1]^[2]^[3]。其中部分水流可能冲刷蚀刻了阿瑞斯谷 ^[4]^[5]^[6]^[7]^[8] 。总之，该流域的总溢流面积可能约为 11 X 10⁶公里²或约火星9% 的表面^[9]^[2]。

下面的图片显示了曾经被水注满的阿耳古瑞盆地。此外，更广阔的视图显示了水流穿越的距离，从阿耳古瑞盆地以南一直到珍珠高地。

图集

显示了阿耳古瑞区地理环境的激光测高图。
阿耳古瑞平原及其他地区边界激光测高图
乌斯钵谷、拉冬谷以及附近其它特征位置图

另请参阅

参考资料

[1]
Baker, V. 1982. The Channels of Mars. University of Texas Press. Austin, TX
[2]
Phillips, R., et al. 2001. Ancient geodynamics and global-scale hydrology on Mars. Science: 291, 2587_2591.
[3]
Saunders, S. 1979. Geologic map of the Margaritifer Sinus quadrangle of Mars, U.S. Geological Survey Misc. Invest. Ser. Map I-1144, scale 1:5M.
[4]
Carr, M. 1979. Formation of Martian flood features by the release of water from confined aquifers. J. Geophys. Res. 84, 2995-3007.
[5]
Carr, M., G. Clow. 1981. Martian channels and valleys: their characteristics, distribution, and age. Icarus: 48 (1), 91-117.
[6]
Grant, J., T. Parker. 2002. Drainage evolution of the Margaritifer Sinus region, Mars. J. Geophys. Res. 107, doi:10.1029/2001JE001678.
[7]
Grant., J. et al. 2009. Geologic map of MTM-20012 and -25012 quadrangles, Margaritifer Terra region of Mars, U.S. Geol. Sur, Scientific Investigations Map 3041, scale 1:1,000,000.
[8]
Rotto, S., K. Tanaka. 1995. Geologic/Geomorphic map of the Chryse Planitia region of Mars, U.S. Geol. Surv. Invest. Ser. Map I-2441, scale 1:5M.
[9]
Banerdt, W. 2000. Surface drainage patterns on Mars from MOLA tpoography, Eos Trans. AGU, 81, 48, Fall Meet. Suppl. Abstract P52C-04.

[1] [1]
Baker, V. 1982. The Channels of Mars. University of Texas Press. Austin, TX

[#1-2] [2]
Phillips, R., et al. 2001. Ancient geodynamics and global-scale hydrology on Mars. Science: 291, 2587_2591.

[3] [3]
Saunders, S. 1979. Geologic map of the Margaritifer Sinus quadrangle of Mars, U.S. Geological Survey Misc. Invest. Ser. Map I-1144, scale 1:5M.

[4] [4]
Carr, M. 1979. Formation of Martian flood features by the release of water from confined aquifers. J. Geophys. Res. 84, 2995-3007.

[5] [5]
Carr, M., G. Clow. 1981. Martian channels and valleys: their characteristics, distribution, and age. Icarus: 48 (1), 91-117.

[6] [6]
Grant, J., T. Parker. 2002. Drainage evolution of the Margaritifer Sinus region, Mars. J. Geophys. Res. 107, doi:10.1029/2001JE001678.

[7] [7]
Grant., J. et al. 2009. Geologic map of MTM-20012 and -25012 quadrangles, Margaritifer Terra region of Mars, U.S. Geol. Sur, Scientific Investigations Map 3041, scale 1:1,000,000.

[8] [8]
Rotto, S., K. Tanaka. 1995. Geologic/Geomorphic map of the Chryse Planitia region of Mars, U.S. Geol. Surv. Invest. Ser. Map I-2441, scale 1:5M.

[9] [9]
Banerdt, W. 2000. Surface drainage patterns on Mars from MOLA tpoography, Eos Trans. AGU, 81, 48, Fall Meet. Suppl. Abstract P52C-04.

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