Centro de Astrobiología, INTA-CSIC, Torrejón de Ardoz, 28850 Madrid, Spain; MALTA-Consolider Team and QUIMAPRES, Departamento de Química Física I, Facultad de Química, Universidad Complutense, 28040 Madrid, Spain.
Spectrochim Acta A Mol Biomol Spectrosc. 2013 Dec;116:26-30. doi: 10.1016/j.saa.2013.06.121. Epub 2013 Jul 9.
We have carried out a systematic study of abiotic precipitation at different temperatures of several Mg and Ca carbonates (calcite, nesquehonite, hydrocalcite) present in carbonaceous chondrites. This study highlights the capability of Raman spectroscopy as a primary tool for performing full mineralogical analysis. The precipitation reaction and the structure of the resulting carbonates were monitored and identified with Raman spectroscopy. Raman spectroscopy enabled us to confirm that the precipitation reaction is very fast (minutes) when Ca(II) is present in the solution, whereas for Mg(II) such reactions developed at rather slow rates (weeks). We also observed that both the composition and the reaction mechanisms depended on temperature, which might help to clarify several issues in the fields of planetology and geology, because of the environmental implications of these carbonates on both terrestrial and extraterrestrial objects.
我们对几种存在于碳质球粒陨石中的镁和钙碳酸盐(方解石、水菱镁矿、水羟钙石)在不同温度下的非生物沉淀进行了系统研究。这项研究强调了拉曼光谱作为进行全矿物分析的主要工具的能力。沉淀反应和生成的碳酸盐结构通过拉曼光谱进行监测和识别。拉曼光谱使我们能够确认,当溶液中存在 Ca(II) 时,沉淀反应非常快(分钟),而对于 Mg(II),这种反应的发展速度较慢(周)。我们还观察到,组成和反应机制都取决于温度,这可能有助于澄清行星学和地质学领域的几个问题,因为这些碳酸盐对地球和外星物体都有环境影响。