柯伊伯带对象 (50000) Quaoar上的水晶冰
1Institute for Astronomy, 2680 Woodlawn Drive, Honolulu, Hawaii 96822, USA. jewitt@hawaii.edu
Nature
|December 14, 2004
概括
柯伊伯带天体Quaoar显示了水晶冰和氨水合物的迹象,表明最近重新浮出水面. 这表明原始太阳系天体上有活跃的动态过程.
科学领域:
- 行星科学 行星科学
- 天文学 天文学
- 太阳系探索 太阳系探索
背景情况:
- 柯伊伯带是海王星之外的一个区域,是太阳系原始材料的所在地.
- 大多数柯伊伯带天体 (KBO) 太弱,无法进行详细的组成分析.
- 柯伊伯带的表面温度极低 (大约为2°C). 50 千克) 的时间.
研究的目的:
- 为了研究大型柯伊伯带天体 (50000) Quaoar的表面组成.
- 了解柯伊伯带冰的保存和潜在变化.
主要方法:
- 在近红外观测 (50000) Quaoar.
- 谱分析用于识别表面材料.
主要成果:
- 在Quaoar的表面检测到晶体水冰.
- 氨水合物的鉴定.
- 有证据表明,冰已经被加热到至少110K.
结论:
- 水晶冰和氨水合物的存在表明,Quaoar最近重新浮出水面.
- 可能的复苏机制包括冲击暴露或冷火山活动.
- 这些发现表明,尽管温度低,KBO上仍存在活跃的地质过程.
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