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在67P/Churyumov-Gerasimenko彗星的昏迷中大量的分子氧
A Bieler1,2, K Altwegg2,3, H Balsiger2
1Department of Climate and Space Science and Engineering, University of Michigan, 2455 Hayward Street, Ann Arbor, Michigan 48109, USA.
Nature
|October 30, 2015
概括
在彗星67P/Churyumov-Gerasimenko中检测到分子氧气 (O2)
科学领域:
- 彗星科学
- 天体化学
- 星球科学
背景情况:
- 彗星昏迷主要由H2O,CO和CO2组成.
- 存在其他分子,如硫化合物和碳化合物.
- 分子氧 (O2) 在其他冰体上被检测到,但在彗星中没有.
研究的目的:
- 在67P/Churyumov-Gerasimenko彗星中发现分子氧气 (O2).
- 测量相对于H2O的O2的丰度.
- 研究彗星核中的O2的分布和起源.
主要方法:
- 在67P/Churyumov-Gerasimenko彗星中测量中性气体组成.
- 分析相对于H2O的O2丰度.
- 评估O2/H2O比率的同otropy和依赖于日心距离.
主要成果:
- 在67P/Churyumov-Gerasimenko彗星的昏迷中检测到分子氧气 (O2).
- 与H2O相比,局部O2度在1%至10%之间,平均值为3.80±0.85%.
- 发现O2/H2O比为同位素且独立于日心距离.
结论:
- 氧气的存在表明它在彗星形成过程中被纳入了彗星核.
- 这一发现挑战了当前的太阳系形成模型.
- 需要进一步的研究来了解允许O2的条件.
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