在演化恒星周围的尘埃中检测碳酸盐
F Kemper1, C Jäger, L B F M Waters
1Astronomical Institute "Anton Pannekoek", University of Amsterdam, Kruislaan 403, 1098 SJ Amsterdam, The Netherlands. ciska@science.uva.nl
Nature
|January 18, 2002
概括
在进化的恒星尘埃中发现的碳酸盐挑战了太阳系的起源. 这些外星碳酸盐在没有液态水的情况下形成,这表明非水过程可能会产生它们,影响我们对早期太阳系天体的理解.
科学领域:
- 天体化学是天体化学.
- 行星科学 行星科学
- 太空化学 太空化学
背景情况:
- 地球和火星上的碳酸盐通过水溶液中的酸盐气候变化而形成.
- 小行星和行星间尘埃中的碳酸盐通常归因于母体的水性变化.
- 碳酸盐在太阳系之外的存在一直没有得到证实,直到现在.
研究的目的:
- 研究太阳系外碳酸盐的存在和形成机制.
- 为了确定碳酸盐是否可以在缺乏液态水的环境中形成.
- 重新评估太阳系碳酸盐对早期液态水存在的影响.
主要方法:
- 对围绕进化恒星的尘埃进行分析.
- 碳酸盐矿物质 (石和多洛米特) 的光谱识别.
主要成果:
- 在演化恒星的尘埃中发现石和多洛米特.
- 这些外星碳酸盐在太原的条件下被发现,对于有液态水的大型母体来说太原始了.
- 形成机制很可能是非水性,可能涉及尘埃/冰颗粒或气相凝结的表面过程.
结论:
- 碳酸盐可以通过星际环境中的非水性过程形成.
- 在太阳系天体中碳酸盐的存在可能不仅仅表明过去的液态水.
- 这一发现扩大了对宇宙中碳酸盐形成途径的理解.
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