相关实验视频
Updated: Jul 12, 2026

11:34
Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
概括
火星的卫星博斯比以前认为的更大,更暗,白度非常低. 新的分析表明,它很可能被火星捕获,而不是与行星一起形成.
科学领域:
- 行星科学 行星科学
- 天文学 天文学
- 太阳系研究 太阳系研究
背景情况:
- 博斯是火星的两个卫星之一.
- 之前对博星的大小和表面特性的估计是基于有限的数据.
- 了解博斯的特征是了解火星历史的关键.
研究的目的:
- 重新评估福博斯的尺寸和表面特性.
- 为了确定Phobos的起源.
主要方法:
- 分析一个特定的Mariner 7图像 (7F91框架).
- 从图像中测量了Phobos的四肢形状.
- 视觉几何色度的计算.
主要成果:
- 博的四肢轮尺寸为18×22公里,表明它的尺寸比以前认为的要大.
- 波斯有一个较暗的表面,视觉几何色度为0.065.5.
- 这个白度低于任何其他已知的太阳系天体的白度.
结论:
- 福博斯比以前估计的要大,更暗.
- 低的白度和大小表明,福博斯可能没有在火星周围的现场形成.
- 很可能,福博斯在以后的时间被火星捕获.
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