奥索尼亚桌山

**奥索尼亚桌山**
	火星全球探勘者号拍摄的奥索尼亚桌山，这座受侵蚀的桌山分布有很多的河道。
坐标	30.3°S 262.3°W
直径	103公里（64英里）

奥索尼亚桌山（Ausonia Mensa）是位于火星希腊区南纬30.3度、西经262.3度处的一座桌山，它直径约103公里，名称取自火星古典反照率特征[1]。“桌山”一词用于指带有陡峭绝壁的平顶台地[2]，奥索尼亚桌山分布有许多小水道，有些地貌看起来像冲积扇，这些通道提供了大量证明水曾在火星上流动的证据[3][4]。从火星航天器上拍摄的照片中能看到弯曲的通道，这些图像可追溯到20世纪70年代初，当时使用的是水手9号轨道飞行器[5][6][7][8]。

HiWish计划下高分辨率成像科学设备显示的奥索尼亚桌山中的河道。

另请查阅

高分辨率成像科学设备
HiWish计划
火星全球探勘者号（MGS）
谷网 (火星)

参引资料

"奥索尼亚桌山". Gazetteer of Planetary Nomenclature. USGS Astrogeology Research Program.
International Astronomical Union (IAU) Working Group for Planetary System Nomenclature (WGPSN). . Gazetteer of Planetary Nomenclature. US Geological Survey. [21 January 2021]. （原始内容存档于2013-12-10）.
Baker, V., et al. 2015. "Fluvial geomorphology on Earth-like planetary surfaces: a review". Geomorphology. 245, 149–182.
Carr, M. 1996. in Water on Mars. Oxford Univ. Press.
Baker, V. 1982. The Channels of Mars. Univ. of Tex. Press, Austin, TX
Baker, V., R. Strom, R., V. Gulick, J. Kargel, G. Komatsu, V. Kale. 1991. "Ancient oceans, ice sheets and the hydrological cycle on Mars". Nature 352, 589–594.
Carr, M. 1979. "Formation of Martian flood features by release of water from confined aquifers". J. Geophys. Res. 84, 2995–300.
Komar, P. 1979. "Comparisons of the hydraulics of water flows in Martian outflow channels with flows of similar scale on Earth". Icarus 37, 156–181.

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[1] "奥索尼亚桌山". Gazetteer of Planetary Nomenclature. USGS Astrogeology Research Program.

[2] International Astronomical Union (IAU) Working Group for Planetary System Nomenclature (WGPSN). . Gazetteer of Planetary Nomenclature. US Geological Survey. [21 January 2021]. （原始内容存档于2013-12-10）.

[3] Baker, V., et al. 2015. "Fluvial geomorphology on Earth-like planetary surfaces: a review". Geomorphology. 245, 149–182.

[4] Carr, M. 1996. in Water on Mars. Oxford Univ. Press.

[5] Baker, V. 1982. The Channels of Mars. Univ. of Tex. Press, Austin, TX

[6] Baker, V., R. Strom, R., V. Gulick, J. Kargel, G. Komatsu, V. Kale. 1991. "Ancient oceans, ice sheets and the hydrological cycle on Mars". Nature 352, 589–594.

[7] Carr, M. 1979. "Formation of Martian flood features by release of water from confined aquifers". J. Geophys. Res. 84, 2995–300.

[8] Komar, P. 1979. "Comparisons of the hydraulics of water flows in Martian outflow channels with flows of similar scale on Earth". Icarus 37, 156–181.