证据表明火星上存在极快的岩海洋结晶和地形成
Laura C Bouvier1, Maria M Costa1, James N Connelly1
1Centre for Star and Planet Formation and Natural History Museum of Denmark, University of Copenhagen, Copenhagen, Denmark.
Nature
|June 29, 2018
概括
最古老的火星石可以追溯到44.76亿年前, 这种早期的地形成表明,在太阳系形成后不久,行星的分化和岩海洋的结晶
科学领域:
- 星球科学
- 地质化学
- 宇宙化学
背景情况:
- 在陆地行星上原始地形成的时间对于理解行星进化至关重要.
- 的U-Pb年代和Hf同位素分析使其成为研究早期地历史的理想选择.
- 之前的研究表明,火星地在4430万年前的早期形成是基于石中的.
研究的目的:
- 准确地测定来自NWA 7034火星 regolith 石的古老石年龄.
- 确定这些古老的石的Hf同位素组成和源储量.
- 限制原始地形成的时间和火星的早期行星分化.
主要方法:
- 高精度- (U-Pb) 的同位素测年.
- 卢-哈芬 (Lu-Hf) 的同位素分析,以确定源储体特征.
- 从NWA 7034火星规律裂中分析石.
主要成果:
- 七个石在4476.3±0.9和4429.7±1.0百万年前产生了U-Pb,代表了火星上最古老的材料.
- 所有分析的石均表现出非放射性初始Hf同位素组成,表明它们来自于4,547亿年前形成的丰富的地.
- 数据表明原始地存在于45.47亿年前,并在大约1亿年后重新形成.
结论:
- 火星的原始地在45.47亿年前形成,
- 这个地的快速形成意味着火星的积聚,核心形成和岩海洋结晶是在太阳系形成的2000万年内完成的.
- 这些发现支持火星早期极快行星分化和地幔翻转的模型.
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