太阳系I小行星和彗星中小型天体中的火性过程
Giovanni Leone1,2, Hiroyuki K M Tanaka2,3,4
1Instituto de Investigación en Astronomía y Ciencias Planetarias, Universidad de Atacama, Chile.
iScience
|August 3, 2023
概括
在小型太阳系天体中,火性过程是常见的,由放射性同位素和冲击的热量驱动. 像奥利文这样的矿物质可能起源于星云过程或星际空间,而不仅仅来自火热活动.
科学领域:
- 行星科学 行星科学
- 太空化学 太空化学
- 地质物理学 地质物理学
背景情况:
- 在小型太阳系天体 (SBSS) 中,火热过程很普遍,由各种热源提供燃料.
- 长寿命的放射性同位素继续加热地球和恒星等活体天体.
研究的目的:
- 调查太阳系中广泛存在的矿物质,如橄和火素的起源.
- 在SBSS中区分岩性过程和其他矿物形成来源.
主要方法:
- 分析行星和SBSS中的矿物分布.
- 考虑太阳系内的热史和运输机制.
主要成果:
- 在SBSS中广泛存在的橄素和火氧素可能不仅仅是火性过程的结果.
- 星云过程或星际卷入是这些矿物质的可信的替代来源.
- 太阳系中的温度梯度有利于原太阳附近的橄酸.
结论:
- 岩性活动是重要的,但不是SBSS中关键矿物质的唯一来源.
- 星际运输为矿物质存在提供了一个令人信服的解释,可能绕过早期星云流.
- 了解矿物质起源对于重建太阳系的形成和演变至关重要.
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