火性石表明,在早期的太阳星云中,-26具有异质性
Evgenii Krestianinov1, Yuri Amelin2,3,4, Qing-Zhu Yin5
1Research School of Earth Sciences, Australian National University, Canberra, 2601, Australia. evgenii.krestianinov@anu.edu.au.
Nature communications
|August 29, 2023
概括
早期的太阳系材料显示-26 (Al) 同位素的分布不均. 这一发现影响了行星形成和早期融化过程的模型.
科学领域:
- 太空化学 太空化学
- 行星科学 行星科学
- 同位素地球化学 同位素地球化学
背景情况:
- 短命的放射性核酸-26 (Al) 对于早期的行星变暖和约会至关重要.
- 了解太阳系早期26Al的分布是行星形成模型的关键.
研究的目的:
- 调查太阳系早期26Al的初始分布.
- 为了确定26Al在太阳星云中是否均或异质分布.
主要方法:
- 精确的-207 - -206 (Pb-Pb) 同位素约会的Erg Chech 002亚.
- 分析现有的Al-26Mg数据与新的年龄确定结合.
主要成果:
- 精确的Pb-Pb同位素年龄为4565.56±0.12百万年,被确定为Erg Chech 002.
- 在Erg Chech 002的原始材料中,初始26/27的Al比率明显高于其他Achondrites.
- 数据表明太阳系早期的26Al的空间异质性是3~4倍.
结论:
- 26Al的异质分布表明,恒星材料中含有新合成的放射性核素的添加较晚.
- 这种异质性影响了早期的行星融化,需要对太阳星云模型进行改进.
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