彗星C/1999S4 (LINEAR) 中NH3的自旋温度
H Kawakita1, J Watanabe, H Ando
1Gunma Astronomical Observatory, 6860-86 Nakayama, Takayama, Agatsuma, Gunma 377-0702, Japan. kawakita@astron.pref.gunma.jp
概括
彗星C/1999S4 (LINEAR) 中氨的正正比比表明它的冰形成在土星和天王星之间. 这提供了关于太阳星云的线索.
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:
- 彗星的组成提供了对早期太阳系的洞察.
- 氨是彗星中的关键挥发物,起源于太阳星云.
- 氨的正正比 (OPR) 是其形成温度的敏感标记.
研究的目的:
- 为了确定彗星C/1999S4 (LINEAR) 中的NH2的正正比 (OPR).
- 推断彗星氨冰的形成温度和位置.
- 了解太阳星云中的彗星冰的热史和起源.
主要方法:
- 使用Subaru望远镜获得彗星C/1999S4 (LINEAR) 的高分散光学光谱.
- 使用光激发模型分析了NH2排放线.
- 计算了正正对比 (OPR) 并推导出氨的旋转温度.
主要成果:
- 高信号噪声比频谱产生了精确的NH2排放线.
- 确定NH2的正整比 (OPR) 为3.33 ± 0.07.
- 氨的衍生自旋温度为28±2凯尔文.
结论:
- NH2 OPR反映了原始氨OPR,表示形成条件.
- 衍生自旋温度表明彗星氨冰在土星和天王星之间形成.
- 这一发现限制了早期太阳星云中分子形成和凝聚的位置.
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