石和近地小行星之间的组成差异
P Vernazza1, R P Binzel, C A Thomas
1Research and Scientific Support Department, European Space Agency, Keplerlaan 1, 2201 AZ Noordwijk, The Netherlands. pierre.vernazza@esa.int
Nature
|August 16, 2008
概括
大多数近地小行星与罕见的LL石石具有相同的光谱特性,这表明它们有着令人惊的起源. 佛罗拉小行星家族可能是主要来源,可能受到Yarkovsky效应对运输的影响.
科学领域:
- 行星科学 行星科学
- 天文学 天文学
- 太空化学 太空化学
背景情况:
- 了解近地小行星 (NEAs) 和潜在的危险小行星 (PHAs) 对于科学和实际原因至关重要.
- 预计小行星的组成将与地球上常见的石类型相似.
研究的目的:
- 为了研究NEAs和PHAs的光谱特性.
- 为了确定地球附近的小行星的起源和组成.
- 为了确定NEAs在小行星带内的潜在来源区域.
主要方法:
- 接近地球的小行星的光谱分析.
- 将NEA的光谱特性与已知的石类别进行比较.
- 识别具有相似光谱特征的小行星家族.
主要成果:
- 大多数NEAs,包括PHAs,表现出类似于LL石石的光谱特性.
- 弗洛拉小行星家族的光谱属性相似,表明它可能是NEAs的来源.
- 由于LL类冠状炎的NEA的发病率令人惊,因为它们的罕见性 (约. 8% 的石落下).
结论:
- 接近地球的小行星主要来源于Flora家族,其光谱与LL合体有相似之处.
- 令人惊的LL地铁样NEAs的丰富性可以通过依赖大小的传输机制来解释,例如Yarkovsky效应.
- 需要进一步的研究才能充分了解从主带到地球附近的小行星运输动态.
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