在无形彗星冰中形成的克拉特酸盐水合物在真空中的类似物
D Blake1, L Allamandola, S Sandford
1Planetary Biology Branch, Ames Research Center, Moffett Field, CA 94035, USA.
概括
克拉特酸盐水合物在彗星冰中通过冰的变暖过程中的固态重组而形成. 这一发现解释了彗星中的异常气体释放和挥发性保留,这对于理解太阳系形成至关重要.
科学领域:
- 太空化学 太空化学
- 行星科学 行星科学
- 天体生物学 天体生物学
背景情况:
- 彗星冰中的克拉特酸水合物被假定可以解释不寻常的气体释放和挥发性保留.
- 在低压环境 (星际云,太阳星云,彗星冰) 中,酸盐水合物的形成机制尚不清楚.
研究的目的:
- 为了研究低压条件下的无形冰中酸盐水合物的形成.
- 阐明有关彗星冰的酸盐水合物形成所涉及的固态过程.
主要方法:
- 使用改造的电子显微镜进行实验.
- 在真空 (in vacuo) 中对蒸汽沉积的无形冰进行受控加热.
主要成果:
- 观察到,在无形冰的变暖过程中,通过固态重排形成了克拉特酸盐水合物.
- 这些重新排列导致相位分离和微孔纹理的发展.
结论:
- 固态重组在低压天体物理环境中为酸盐水合物形成提供了可行的机制.
- 观察到的现象为彗星的异常行为提供了解释,包括气体释放和挥发性保留.
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