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作为火星土壤模拟材料的含铁硫酸盐蒙脱石的反射光谱学。

Reflectance spectroscopy of ferric sulfate-bearing montmorillonites as Mars soil analog materials.

作者信息

Bishop J L, Pieters C M, Burns R G, Edwards J O, Mancinelli R L, Fröschl H

机构信息

Department of Chemistry and Geological Sciences, Brown University, Providence, Rhode Island 02912, USA.

出版信息

Icarus. 1995 Sep;117(1):101-19. doi: 10.1006/icar.1995.1145.

Abstract

Spectroscopic analyses have shown that smectites enhanced in the laboratory with additional ferric species exhibit important similarities to those of the soils on Mars. Ferrihydrite in these chemically treated smectites has features in the visible to near-infrared region that resemble the energies and band strengths of features in reflectance spectra observed for several bright regions on Mars. New samples have been prepared with sulfate as well, because S was found by Viking to be a major component in the surface material on Mars. A suite of ferrihydrite-bearing and ferric sulfate-bearing montmorillonites, prepared with variable Fe3+ and S concentrations and variable pH conditions, has been analyzed using reflectance spectroscopy in the visible and infrared regions, Mössbauer spectroscopy at room temperature and 4 K, differential thermal analysis, and X-ray diffraction. These analyses support the formation of ferrihydrite of variable crystallinity in the ferrihydrite-bearing montmorillonites and a combination of schwertmannite and ferrihydrite in the ferric sulfate-bearing montmorillonites. Small quantities of poorly crystalline or nanophase forms of other ferric materials may also be present in these samples. The chemical formation conditions of the ferrihydrite-bearing and ferric sulfate-bearing montmorillonites influence the character of the low temperature Mössbauer sextets and the visible reflectance spectra. An absorption minimum is observed at 0.88-0.89 micrometers in spectra of the ferric sulfate-bearing samples, and at 0.89-0.92 micrometers in spectra of the ferrihydrate-bearing montmorillonites. Mössbauer spectra of the ferric sulfate-bearing montmorillonites indicate variable concentrations of ferrihydrite and schwertmannite in the interlaminar spaces and along grain surfaces. Dehydration under reduced atmospheric pressure conditions induces a greater effect on the adsorbed and interlayer water in ferrihydrite-bearing montmorillonite than on the water in ferric sulfate-bearing montmorillonite. Reflectance spectra of ferric sulfate-bearing montmorillonite include a strong 3-micrometers band that is more resistant to dry atmospheric conditions than the 3-micrometers band in spectra of similarly prepared ferrihydrite-bearing montmorillonites.

摘要

光谱分析表明,在实验室中用额外的铁物种增强的蒙脱石与火星土壤的蒙脱石表现出重要的相似性。这些经过化学处理的蒙脱石中的水铁矿在可见光到近红外区域的特征类似于在火星上几个明亮区域观测到的反射光谱特征的能量和谱带强度。还制备了含硫酸盐的新样品,因为“海盗号”探测器发现硫是火星表面物质的主要成分。使用可见光和红外区域的反射光谱、室温及4K下的穆斯堡尔光谱、差热分析和X射线衍射,对一系列含有不同Fe3+和S浓度以及不同pH条件制备的含铁水合物和硫酸铁的蒙脱石进行了分析。这些分析支持了在含铁水合物的蒙脱石中形成了结晶度可变的水铁矿,以及在含硫酸铁的蒙脱石中形成了施韦特曼石和水铁矿的组合。这些样品中也可能存在少量结晶性差或纳米相形式的其他铁材料。含铁水合物和硫酸铁的蒙脱石的化学形成条件影响低温穆斯堡尔六重峰的特征和可见光反射光谱。在含硫酸铁的样品光谱中,在0.88 - 0.89微米处观察到一个吸收最小值,在含铁水合物的蒙脱石光谱中,在0.89 - 0.92微米处观察到一个吸收最小值。含硫酸铁的蒙脱石的穆斯堡尔光谱表明,层间空间和颗粒表面的水铁矿和施韦特曼石浓度不同。在减压条件下脱水对含铁水合物的蒙脱石中吸附水和层间水的影响比对含硫酸铁的蒙脱石中的水的影响更大。含硫酸铁的蒙脱石的反射光谱包括一个强的3微米谱带,与类似制备的含铁水合物的蒙脱石光谱中的3微米谱带相比,它对干燥大气条件更具抗性。

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