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彗星67P/Churyumov-Gerasimenko的表面变化表明它在过去更为活跃
M Ramy El-Maarry1,2, O Groussin3, N Thomas4
1Physikalisches Institut, Universität Bern, 3012 Bern, Switzerland. mohamed.el-maarry@lasp.colorado.edu.
概括
罗塞塔航天器的数据显示,彗星67P/Churyumov-Gerasimenko因太阳辐射而发生局部变化. 这些微小的表面变化表明彗星的早期形成的主要地形.
科学领域:
- 彗星科学
- 行星地质学
- 太空探索
背景情况:
- 罗塞塔号在67P/Churyumov-Gerasimenko彗星的轨道上运行了大约两年.
- 观察主要集中在表面特征和子尺度监测上.
研究的目的:
- 在2014年12月至2016年6月期间观察到的67P/Churyumov-Gerasimenko彗星的局部表面变化.
- 了解推动这些变化的过程及其对彗星景观演变的影响.
主要方法:
- 通过罗塞塔航天器进行现场表面监测.
- 分析高分辨率图像和数据以识别和量化表面变化.
- 观察到的变化归因于彗星的气候变化,侵蚀和短暂的太阳驱动事件.
主要成果:
- 在彗星67P/Churyumov-Gerasimenko上观察到许多局部的表面变化.
- 这些变化归因于彗星的气候变化,侵蚀和太阳辐射带来的短暂事件.
- 尽管有局部变化,但整体变化规模并没有大大改变彗星的主要地形.
结论:
- 最近变化的规模有限表明67P/Churyumov-Gerasimenko彗星的主要地形是在其当前轨道配置的早期建立的.
- 这些地形的形成可能早于目前的轨道,可能与CO或CO2冰或无形冰等更大的挥发物质库存有关.
- 构成或物理异质性是由局部变化的建议,但景观演变主要是古老的.
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