在彗星9P/Tempel 1表面露出水冰沉积物
J M Sunshine1, M F A'Hearn, O Groussin
1Science Applications International Corporation (SAIC), Chantilly, VA 20151, USA. sunshinej@saic.com
概括
彗星9P/Tempel 1上固体水冰的直接检测是深度冲击任务实现的. 这些通过近红外光谱识别的表面冰沉积物表明松散的聚合物,并指向彗星外气的地下来源.
科学领域:
- 彗星科学 彗星科学
- 天文地质学 天文地质学
- 频谱学是一种光谱学.
背景情况:
- 彗星是冰冷的天体,可以提供关于太阳系早期的见解.
- 了解彗星的组成对于行星科学至关重要.
- 以前的研究表明彗星上存在水冰,但直接地表检测仍然具有挑战性.
研究的目的:
- 直接检测和描述彗星9P/Tempel 1表面的固体水冰沉积物.
- 分析彗星上的异常表面积的光谱特性.
- 研究表面水冰对彗星活动的起源和影响.
主要方法:
- 通过深度冲击任务获得的近红外光谱的分析.
- 模拟1.5和2.0微米的光谱吸收以确定水冰.
- 描述水冰颗粒的大小和分布.
主要成果:
- 在彗星9P/Tempel 1上,在三个不同的表面区域直接检测到固体水冰.
- 光谱分析证实了水冰的存在,吸收在1.5和2.0微米.
- 水冰颗粒被建模为10-50微米直径的聚合物,大于撞击喷射物.
结论:
- 表面沉积物很可能是水冰的松散聚合物.
- 观察到的表面冰面积不足以解释彗星的总体排气.
- 地下区域可能是彗星排气的主要来源.
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