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Scattering And Absorption of Light in Planetary Regoliths
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彗星67P的轨道水冰循环
Gianrico Filacchione1, Fabrizio Capaccioni2, Mauro Ciarniello2
1INAF-IAPS, Institute for Space Astrophysics and Planetology, Rome, Italy. gianrico.filacchione@inaf.it.
Nature
|February 7, 2020
概括
彗星67P/Churyumov-Gerasimenko在其表面和昏迷中呈现相反的季节性颜色变化. 有机丰富的尘埃使昏迷变红,而暴露的冰在周日经过时使核表面变蓝.
科学领域:
- 星球科学
- 彗星科学
- 天体化学
背景情况:
- 彗星活动是由太阳加热驱动的,导致气体释放和尘埃喷射.
- 彗星的昏迷和核特性在整个轨道上动态演变.
- 粉尘颗粒的颜色因其组成 (有机,酸盐,水冰) 和颗粒大小而异.
研究的目的:
- 观测和分析67P/Churyumov-Gerasimenko彗星表面的季节性颜色周期.
- 研究太阳能变热,尘埃组成和观察到的颜色变化之间的关系.
主要方法:
- 对67P/Churyumov-Gerasimenko彗星的观测结果的光谱分析.
- 通过周日通道监测昏迷和核表面的颜色变化.
主要成果:
- 在和核中观察到两种相反的季节性颜色周期.
- 由于亚微米有机物质和无形碳颗粒的丰富而引起的红.
- 由于原始的冰层暴露, 核表面呈现出更蓝的色调.
结论:
- 彗星尘埃的组成和粒径大大影响着彗星的颜色.
- 季节性变化揭示了除尘,冰层升温和表面演变之间的动态相互作用.
- 远离太阳,表面脱水和尘埃重新沉积会减少水冰的丰富性和昏迷的红色.
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