在彗星C/1995 O1 (Hale-Bopp) 中确定HDO/H2O比率
R Meier1, T C Owen, H E Matthews
1University of Hawaii, Institute for Astronomy, 2680 Woodlawn Drive, Honolulu, HI 96822, USA.
概括
黑尔-波普彗星中的化水 (HDO) 用詹姆斯·克莱克麦克斯韦尔望远镜测量. 它的高D/H比表明彗星不是地球海洋的唯一来源.
科学领域:
- 天文学和天体物理学
- 行星科学 行星科学
- 彗星科学 彗星科学
背景情况:
- 彗星是冰的物体,可能为早期的地球提供了水.
- 测量彗星水中的与 (D/H) 比率,可以了解彗星水的起源.
研究的目的:
- 为了检测和量化彗星C/1995 O1 (海尔波普) 水中的D/H比.
- 为了比较彗星D/H比率与陆地水和前太阳值,以评估彗星对地球海洋的贡献.
主要方法:
- 使用詹姆斯·克莱克麦克斯韦尔望远镜检测化水 (HDO).
- 用光谱分析来确定D/H比.
主要成果:
- 在海尔-波普彗星中成功检测到化水 (HDO).
- 黑尔-波普的水中的D/H比被确定为 (3.3 ± 0.8) x 10−4.4.
- 这个比率与P/哈雷彗星和C/1996 B2 (Hyakutake) 的测量结果一致.
结论:
- 哈雷波普彗星中的D/H比率明显高于陆地水的D/H比率.
- 彗星D/H比值是原太阳H2值的10倍以上.
- 彗星本身无法解释地球海洋的起源.
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