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Planum Boreum : ウィキペディア英語版
Planum Boreum

Planum Boreum (Latin: "the northern plain") is the northern polar plain on Mars. It extends northward from roughly 80°N and is centered at . Surrounding the high polar plain is a flat and featureless lowland plain called Vastitas Borealis which extends for approximately 1500 kilometres southwards, dominating the northern hemisphere.〔() and () give Vastitas Borealis starting at 54.7°N and Planum Boreum at 78.5°N. The radius of Mars is approximately 3400 km, so d=\frac\times 2 \pi\ \times 3400\mbox = 1412\mbox
==Ice cap==

Planum Boreum is home to a permanent ice cap consisting mainly of water ice (with a 1 m thick veneer of carbon dioxide ice during the winter). It has a volume of 1.2 million cubic kilometres and covers an area equivalent to about 1.5 times the size of Texas. It has a radius of 600 km. The maximum depth of the cap is 3 km.
The spiral troughs in the ice cap are formed by katabatic winds that entrain surface ice eroded from the equator-facing sides of the troughs, likely aided by solar ablation (sublimation), which is then redeposited on the colder pole-facing slopes. The troughs are roughly perpendicular to the wind direction, which is shifted by the Coriolis effect, leading to the spiral pattern. The troughs gradually migrate towards the pole over time; the central troughs have moved about 65 km in the last 2 million years.〔 Chasma Boreale is a canyon-like feature older than the troughs, and in contrast is aligned parallel to the wind direction.〔
The surface composition of the northern ice cap in middle spring (after a winter's accumulation of seasonal dry ice) has been studied from orbit. The outer edges of the ice cap are contaminated with dust (0.15% by weight) and are mostly water ice. As one moves toward the pole, the surface water ice content decreases and is replaced by dry ice. The purity of the ice also increases. At the pole, the surface seasonal ice consists of essentially pure dry ice with little dust content and 30 parts per million of water ice.〔(【引用サイトリンク】title=Spatial variability and composition of the seasonal north polar cap on Mars )
The Phoenix lander, launched in 2007, arrived at Mars in May 2008 and successfully landed in the Vastitas Borealis region of the planet on May 25, 2008. The north polar cap of Mars has been proposed as a landing site for a human Mars expedition by Landis〔G. Landis, (Polar Landing Site for a First Mars Expedition ) Founding Convention of the Mars Society, August 13–16, 1998, University of Colorado in Boulder, CO〕 and by Charles CockellProject Boreas C. Cockell (editor), (Project Boreas - A Station for the Martian Geographic North Pole ), The British Interplanetary Society (2006)〕

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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