环恒星碳酸盐的"干燥"凝结源
Alice Toppani1, François Robert, Guy Libourel
1Centre de Recherches Pétrographiques et Géochimiques-CNRS UPR 2300, 15 rue Notre Dame des Pauvres, BP 20, Vandoeuvre-les-Nancy, France. toppani2@llnl.gov
Nature
|October 21, 2005
概括
碳酸盐矿物质,以前与水相连,可以在太空中与酸盐一起以非生态方式形成. 这一发现表明,宇宙碳酸盐在热,密集的恒星环境中产生了新的起源.
科学领域:
- 天体化学是天体化学.
- 行星科学 行星科学
- 矿物学是什么?矿物学是什么?
背景情况:
- 碳酸盐矿物质在天体物理环境中被检测到,如原星.
- 无源碳酸盐通常表明与富含二氧化碳的水的水性变化.
- 最近对行星星云和原星的探测挑战了这个指标的相关性.
研究的目的:
- 为了研究天体物理碳酸盐的替代形成途径.
- 探索非平衡凝结在碳酸盐形成中的作用.
- 了解碳酸盐在缺乏液态水的环境中的起源.
主要方法:
- 实验模拟非平衡凝结的情况.
- 在H2O-CO2丰富的蒸气中酸盐气体的凝结.
- 对共同凝结的无形酸盐和碳酸盐的分析.
主要成果:
- 证明了碳酸盐与无形酸盐一起形成的无源性碳酸盐.
- 在非平衡过程中,成功的共冷凝发生了.
- 在没有液态水的情况下,确定了有利于碳酸盐形成的条件.
结论:
- 天体物理碳酸盐可能通过太空中的非平衡凝聚形成.
- 拟议的形成地点包括进化的恒星风和原恒星外流.
- 这为观测到的宇宙碳酸盐提供了另一种解释.
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