概括
1987年查伦阴影的红外观测揭示了不同的光谱特征. 哈伦 (Charon) 是一个名字.
科学领域:
- 行星科学 行星科学
- 天文学 天文学
- 频谱学是一种光谱学.
背景情况:
- 冥王星及其卫星哈伦是外太阳系的关键物体.
- 了解它们的表面组成对于行星形成模型至关重要.
研究的目的:
- 为了确定与冥王星相对的哈伦的表面组成.
- 为了调查查伦上存在特定冰的存在.
主要方法:
- 红外光谱 (1.5-2.35微米) 在1987年3月3日的查伦-冥王星隐形期间.
- 从事件期间的光谱流中减去事件之前/之后的光谱流.
主要成果:
- 获得了冥王星和沙龙的个别光谱特征.
- 与冥王星相比,哈伦的表面显示甲耗尽.
- 哈伦在2.0微米时出现了光谱黑色,表明了强烈的水冰吸收.
结论:
- 光谱数据表明,查伦表面存在水冰.
- 甲冰在夏龙星上比在冥王星上少.
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