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乌斯钵-拉冬-摩拉瓦谷

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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

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另请参阅

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参考资料

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  1. ^ Baker, V. 1982. The Channels of Mars. University of Texas Press. Austin, TX
  2. ^ 2.0 2.1 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.