矿物学及其在维斯塔星系的多样性的光谱表征
M C De Sanctis1, E Ammannito, M T Capria
1Istituto di Astrofisica e Planetologia Spaziali, Istituto Nazionale di Astrofisica, Rome, Italy. mariacristina.desanctis@iaps.inaf.it
概括
维斯塔·维斯塔 (Vesta Vesta) 是一个
科学领域:
- 行星科学 行星科学
- 小行星矿物学
- 太空地质化学空间地质化学
背景情况:
- 维斯塔是一个大型小行星,内部有差异化.
- 它的表面成分主要与霍华迪特-尤克里特-二氧化 (HED) 石有关.
- 了解维斯塔的矿物学,可以了解太阳系早期的过程.
研究的目的:
- 使用来自黎明航天器的数据分析小行星维斯塔的矿物学.
- 调查维斯塔表面组成的区域和地方变化.
- 了解维斯塔的地质历史和岩演变.
主要方法:
- 分析了来自"黎明"航天器的可见光谱和红外光谱仪数据.
- 在维斯塔表面的矿物成分的光谱识别.
- 频谱数据与已知的石组成的相关性.
主要成果:
- 维斯塔的矿物学与HED石是一致的.
- 确定了不同的矿物学区域,包括在雷亚西尔维亚盆地中更高的二基因组分和在赤道地区更高的欧基因组分.
- 在火山口墙壁和喷射物上观察到的矿物质层分层的证据.
结论:
- 维斯塔的地由一个上层的eucritic层和一个更深层的diogenitic层组成,受到Rheasilvia冲击的影响.
- 频谱变异性表明,地上存在复杂的基岩和氧积的复杂组合.
- 维斯塔表现出复杂的岩演变,导致了差异化的地和地幔.
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