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首页> 外文期刊>Journal of geophysical research. Planets >The rock abrasion record at Gale Crater: Mars Science Laboratory results from Bradbury Landing to Rocknest
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The rock abrasion record at Gale Crater: Mars Science Laboratory results from Bradbury Landing to Rocknest

机译:大风火山口:火星科学实验室的岩石磨损记录,从布拉德伯里着陆到洛克内斯特

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摘要

Ventifacts, rocks abraded by wind-borne particles, are found in Gale Crater, Mars. In the eastward drive from "Bradbury Landing" to "Rocknest," they account for about half of the float and outcrop seen by Curiosity's cameras. Many are faceted and exhibit abrasion textures found at a range of scales, from submillimeter lineations to centimeter-scale facets, scallops, flutes, and grooves. The drive path geometry in the first 100 sols of the mission emphasized the identification of abrasion facets and textures formed by westerly flow. This upwind direction is inconsistent with predictions based on models and the orientation of regional dunes, suggesting that these ventifact features formed from very rare high-speed winds. The absence of active sand and evidence for deflation in the area indicates that most of the ventifacts are fossil features experiencing little abrasion today.
机译:在火星的大风陨石坑中发现了被风吹散的颗粒磨蚀的岩石。在从“布拉德伯里着陆点”向“洛克内斯特”向东行驶的过程中,它们约占好奇号相机所看到的浮标和露头的一半。许多表面都是刻面的,并且在从亚毫米线条到厘米尺度的刻面,扇贝,凹槽和凹槽的各种比例尺上都显示出磨损纹理。任务的前100个溶胶中的驱动路径几何形状强调了对由西风流形成的磨损面和纹理的识别。这种上风方向与基于模型和区域沙丘方向的预测不一致,表明这些极小的特征是由非常罕见的高速风形成的。该地区缺少活性砂和放气迹象,表明大多数通风是化石特征,如今几乎没有磨损。

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