相关实验视频
Updated: Jul 11, 2026

11:34
Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
用维京登陆器摄像头对恐惧症的多色观测:证据表明一种碳状体构成
概括
这就是Phobosos.
科学领域:
- 行星科学 行星科学
- 天文地质学 天文地质学
- 频谱学是一种光谱学.
背景情况:
- 火星的一个卫星 - - 博斯 (Phobos) 的表面构成尚未完全理解.
- 之前的研究为Phobos提供了有限的光谱数据.
研究的目的:
- 为了确定Phobos在0.4至1.1微米光谱区域的反射率.
- 将Phobos的光谱属性与实验室样本进行比较,以推断其起源.
主要方法:
- 来自维京着陆器摄像头图像的反射率数据的分析.
- 观察到的光谱数据与碳酸和玄武岩的实验室光谱的比较.
主要成果:
- 波斯表现出0.4至1.1微米之间的平面反射率曲线.
- 确定了福博斯的几何色度为0.05 +/- 0.01.
- 观测到的光谱与碳状地质结合,而不是玄武岩.
结论:
- 福博斯的光谱特征与碳状地质材料相一致.
- 这些发现表明,福博斯可能是一个被捕获的小行星,而不是火星的天然卫星.
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