H'/> Meter-scale thermal contraction crack polygons on the nucleus of comet 67P/Churyumov-Gerasimenko
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Meter-scale thermal contraction crack polygons on the nucleus of comet 67P/Churyumov-Gerasimenko

机译:彗星67p / churyumov-gerasimenko核尺度热收缩裂纹多边形

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Highlights?Polygonal morphologies with a mean size of 3.0?m are reported on the nucleus of comet 67P.?Polygons are consistent with thermal contraction crack polygons known on Earth and Mars.?They imply a consolidated sintered layer of water ice, located a few cm below the surface.?Polygons are young surface morphologies and could be as young as a few orbital periods.AbstractWe report on the detection and characterization of more than 6300 polygons on the surface of the nucleus of comet 67P/Churyumov-Gerasimenko, using images acquired by the OSIRIS camera onboard Rosetta between August 2014 and March 2015. They are found in consolidated terrains and grouped in localized networks. They are present at all latitudes (from North to South) and longitudes (head, neck, and body), sometimes on pit walls or following lineaments. About 1.5% of the observed surface is cover
机译:<![cdata [ 亮点 彗星67p核上的平均尺寸为平均尺寸的多边形形态。 多边形与热收缩裂缝一致地球和火星已知的多边形。 它们意味着综合烧结的水冰层,位于表面下方的几厘米。 多边形是年轻表面形态,可以像几个轨道时期那样年轻。 抽象< / ce:section-title> 我们报告更多的检测和表征更多在2014年8月和2015年3月之间使用Osiris相机船上的奥西里斯相机船上获取的图像超过了6300个多边形。它们在综合地形中找到并在本地化网络中分组。它们存在于所有纬度(从北到南部)和纵向(头部,颈部和身体),有时在坑墙或以下谱系上。约1.5%的观察表面是覆盖的

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