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彗星67P/Churyumov-Gerasimenko中的分子表明形成温度低
M Rubin1, K Altwegg2, H Balsiger3
1Physikalisches Institut, University of Bern, Sidlerstrasse 5, CH-3012 Bern, Switzerland. martin.rubin@space.unibe.ch.
概括
在彗星67P/Churyumov-Gerasimenko中检测到分子 (N2),对行星形成至关重要. 这一发现表明彗星颗粒是在极低的温度下形成的,低于30克尔文.
科学领域:
- 宇宙化学的宇宙化学
- 星球科学 星球科学
- 彗星科学是一门彗星科学.
背景情况:
- 分子 (N2) 是早期太阳系中重要的源.
- 在气体巨星和像冥王星和顿这样的冰体中,N2是丰富的.
- 彗星样本中显著缺少N2,这给太阳系形成模型带来了一个难题.
研究的目的:
- 在木星家族彗星中直接测量分子 (N2).
- 为了研究彗星中N2的丰富性和来源.
- 了解太阳系早期的粒度形成条件.
主要方法:
- 在现场测量分子 (N2) 使用罗塞塔轨道仪离子和中性分析光谱仪 (ROSINA) 质谱仪.
- 对彗星昏迷中的一氧化碳 (CO) 相对于N2丰度的分析.
- 测量N2/CO比率与太阳前太阳值的比较.
主要成果:
- 在彗星67P/Churyumov-Gerasimenko中直接检测到分子 (N2).
- 测量了5.70 ± 0.66 × 10 ((-3) 的N2 / CO比率.
- 这表明与原太阳星云相比,N2耗尽了大约25.4±8.9倍.
结论:
- 彗星的N2丰富度明显低于从原太阳组成中预期的.
- 观察到的枯竭表明彗星颗粒是在非常寒冷的条件下 (<30克尔文) 形成的.
- 这为太阳系形成期间的热史和化学过程提供了洞察力.
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