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Scattering And Absorption of Light in Planetary Regoliths
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冥王星和哈伦的表面组成

W M Grundy1, R P Binzel2, B J Buratti3

  • 1Lowell Observatory, Flagstaff, AZ 86001, USA. w.grundy@lowell.edu.

Science (New York, N.Y.)
|March 19, 2016
PubMed
概括
此摘要是机器生成的。

新视野号绘制了冥王星和哈伦的地图, 揭示了冥王星上复杂的冰分布和多种表面颜色. 在撞击坑附近, 查伦显示出更简单的颜色图案,

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科学领域:

  • 星球科学
  • 天文地质学
  • 表面构成分析

背景情况:

  • 新地平线任务提供了前所未有的近距离数据.
  • 了解这些柯伊伯带天体的表面组成和地质对于行星科学至关重要.

研究的目的:

  • 绘制和分析冥王星和哈伦的颜色和红外光谱.
  • 了解影响地表冰和地质特征的分布和过程

主要方法:

  • 使用新地平线航天器的成像和光谱绘图能力.
  • 分析了冥王星和黑龙的相遇半球的可见色彩和近红外光谱.

主要成果:

  • 冥王星表面表现出甲,一氧化碳和冰的复杂分布,受升温,凝结和冰川流动的影响.
  • 在冥王星上观察到明显的区域色彩变化,
  • 哈伦呈现出更简单的色彩图案,中性低度和红色的北极区域,以及在撞击坑附近的局部氨吸收.

结论:

  • 冥王星的各种表面特征和冰的分布是由季节性和地质过程塑造的.
  • 哈伦的表面成分,特别是氨的存在, 提供了洞察它的地质活动和历史.