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奥利文在维斯塔表面的一个意想不到的位置
E Ammannito1, M C De Sanctis, E Palomba
1Istituto di Astrofisica e Planetologia Spaziali, INAF, 00133 Rome, Italy.
Nature
|November 8, 2013
概括
在小行星维斯塔上发现了Olivine.
科学领域:
- 行星科学 行星科学
- 天文地质学 天文地质学
- 矿物学是一门学科.
背景情况:
- 橄是地球等差异化天体上一个关键的地幔矿物.
- 小行星维斯塔是一个独特的差异化原行星,其石 (HED) 提供了其组成的线索.
- 之前在维斯塔星球上检测到的橄素是不确定的.
研究的目的:
- 确认奥利文在维斯塔的表面存在并确定其分布.
- 调查维斯塔岛上表面橄石的起源和地质背景.
主要方法:
- 维斯塔表面的遥感观测 (光谱和颜色数据).
- 对石组成 (霍华德石,欧克里特石,二氧化石) 的分析进行比较.
主要成果:
- 确认Olivine在维斯塔表面的局部存在.
- 意想不到的是,橄石是在北半球发现的,而不是在南极深处的盆地.
- 富含橄素的材料 (>50%的橄素) 与霍华德石混合,而不是二氧化石,在坑和喷射物中暴露.
结论:
- 维斯塔的表面橄石与撞击盆地中发现的预期地幔材料 (二原石) 不相关.
- 与霍华达石的分布和关联表明,维斯塔的地幔和表面有一个复杂的地质历史.
- 需要进一步的研究,以了解这种表面olivine. emplacement机制.
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