相关实验视频
Updated: May 28, 2026

11:34
Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
小行星21 Lutetia的图像:来自太阳系早期的小行星遗留物
1Max-Planck-Institut für Sonnensystemforschung, Max-Planck-Strasse 2, 37191 Katlenburg-Lindau, Germany. sierks@mps.mpg.de
概括
小行星21 Lutetia表现出复杂的地质和高密度,表明它是一个原始的小行星. 这一发现与较小的小行星形成鲜明对比,这些小行星可能是碎片或废墟堆.
科学领域:
- 行星科学 行星科学
- 小行星研究研究.
- 地质地质地质地质地质地
背景情况:
- 之前的任务显示,较小的小行星通常是碎片或碎片堆.
- 与较小的天体相比,21号小行星Lutetia的性质仍然不太了解.
研究的目的:
- 为了研究小行星21 Lutetia的地质特征和密度.
- 为了确定21 Lutetia是否与较小的小行星相比,代表了不同的小行星类.
主要方法:
- 来自罗塞塔航天器上的光学,光谱和红外远程成像系统 (OSIRIS) 摄像机的图像分析.
主要成果:
- 卢提亚表现出复杂的地质,包括厚厚的岩层和北极地区的山体滑坡.
- 测量密度为3.4±0.3g/cm3,是小行星中记录的最高密度之一.
- 表面的特征表明一个古老的年龄.
结论:
- 复杂的地质,古老的表面和高密度强烈地表明21 Lutetia是一个原始的小行星.
- 卢提亚的特征使其与以前研究的较小,碎片化小行星有所区别.
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