彗星9P/Tempel 1中的母挥发物:撞击前后
Michael J Mumma1, Michael A DiSanti, Karen Magee-Sauer
1Solar System Exploration Division, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA. michael.j.mumma@nasa.gov
概括
泰尔1彗星1号彗星
科学领域:
- 行星科学 行星科学
- 彗星科学 彗星科学
- 天体化学是天体化学.
背景情况:
- 木星家族彗星提供了对太阳系早期的洞察力.
- 彗星的挥发性组成可以揭示起源和进化途径.
研究的目的:
- 要量化彗星Tempel 1中的母挥发物丰度.
- 为了将Tempel 1的组成与奥尔特云彗星进行比较.
- 为了调查彗星冰的起源.
主要方法:
- 高分散红外光谱 (2.85.0微米).
- 对八种母挥发性物质进行量化:H2O,C2H6,HCN,CO,CH3OH,H2CO,C2H2和CH4.
主要成果:
- 在撞击后,乙的丰度显著增加.
- 甲醇和化的丰度在撞击后保持不变.
- 坦佩尔1号的喷射物与奥尔特云彗星有相似之处,但甲醇和乙含量较低.
结论:
- 坦佩尔1号和奥特云彗星中的挥发性冰可能在原行星盘中具有共同的起源.
- 冲击事件改变了Tempel 1的波动性概况.
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