相关实验视频
Updated: Apr 6, 2026

11:34
Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
11.1K
科特的科学 在67P/Churyumov-Gerasimenko上采用ROLIS降落成像的规律结构
S Mottola1, G Arnold2, H-G Grothues3
1German Aerospace Center (DLR), Institute of Planetary Research, Berlin, Germany. stefano.mottola@dlr.de.
概括
彗星67P
科学领域:
- 彗星科学
- 行星地质学
背景情况:
- 彗星的表面是由它们的活动所塑造的.
- 了解彗星表面的结构可以了解它们的演变.
研究的目的:
- 使用高分辨率图像分析67P/Churyumov-Gerasimenko彗星的表面结构.
- 为了研究形成彗星上层的过程.
主要方法:
- 使用罗塞塔着陆器成像系统 (ROLIS) 在菲拉的下降过程中获取近距离图像.
- 分析表面形态,颗粒大小分布和规律的厚度.
- 侵蚀和动员过程的建模.
主要成果:
- 彗星67P上的阿吉尔基亚现场呈现出光度均的表面,覆盖着 regolith (厘米到米大小的碎片).
- 高分辨率成像显示一个颗粒状的表面没有未解决的沙子大小的颗粒.
- 雷戈石的厚度从0到2米不等;类似石的特征表明动员和侵蚀.
结论:
- 彗星表面活动显著影响了上层结构.
- 由空气落引起的粒子喷是观察到的形成的一个可能的机制.
- 这些发现有助于了解彗星表面的过程和演变.
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