来自冰喷射的升华作为探测彗星星际挥发性物质含量的探测器
G A Blake1, C Qi, M R Hogerheijde
1Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena 91125, USA. gab@gps.caltech.edu
Nature
|March 27, 1999
概括
哈雷-波普彗星的彗星
科学领域:
- 天文学和天体物理学
- 行星科学 行星科学
- 天体化学是天体化学.
背景情况:
- 彗星提供了对早期太阳系和分子云转化为行星系统的洞察力.
- 之前的研究平均了大面积的挥发性成分,混合了核和彗星化学过程.
研究的目的:
- 以高分辨率研究海尔波普彗星中挥发物质的组成.
- 通过分析分子丰度比率来确定彗星材料的起源.
主要方法:
- 高分辨率观察哈雷波普彗星中HNC,DCN和HDO分子的辐射.
- 在小尺度 (1-3弧秒) 上分析分子丰度比率.
主要成果:
- 在核附近确定了弧形结构 (冰喷气).
- 在小尺度上观察到的分子丰度比率与较大的尺度有显著差异.
- 这些比率与星际云和年轻恒星物体中发现的比率相匹配.
结论:
- 从核中喷射出来的冰颗粒的升华提供了对不变的挥发性物质的访问.
- 黑尔-波普彗星中含有相当大一部分 (15-40%的质量) 未经处理的星际物质.
- 这表明早期的太阳星云中包含了大量的原始星际物质.
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