早期的太阳系. 在太阳系内部,水的早期积累来自类似碳酸的碳酸源
Adam R Sarafian1, Sune G Nielsen2, Horst R Marschall3
1Department of Geology and Geophysics, Woods Hole Oceanographic Institution, Woods Hole, MA 02543, USA. asarafian@whoi.edu.
概括
像维斯塔这样的富含水的小行星为早期地球提供了必需的挥发性物质. 这一发现表明,地球是地球.
科学领域:
- 行星科学 行星科学
- 天体生物学 天体生物学
- 地质化学 地质化学
背景情况:
- 了解太阳系内部水积累的起源和时间对于行星形成理论至关重要.
- 交付水的时间影响了地球上早期生命出现的模型.
研究的目的:
- 为了研究来自小行星4 Vesta. eucrite石石中阿帕的同位素组成.
- 为了确定维斯塔是否代表着与地球挥发性库存相关的古老的水库.
主要方法:
- 在现场测量同位素组成.
- 在岩石中的阿帕矿物样本的分析.
主要成果:
- 维斯塔的同样具有与碳酸的同位素构成相同.
- 源自维斯塔的欧克里特石石拥有古老的气储库.
- 维斯塔与地球之间存在,碳和的同位素相似性.
结论:
- 挥发性物质,包括水,可能早在地球上被积累.
- 这挑战了挥发性资产在晚期积累阶段完全获得的概念.
- 维斯塔作为一个潜在的模拟早期挥发性传送到陆地行星.
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