Determination of Martian meteorite lithologies and mineralogies using vibrational spectroscopy

1997 ◽  
Vol 102 (E11) ◽  
pp. 25593-25603 ◽  
Author(s):  
Victoria E. Hamilton ◽  
Philip R. Christensen ◽  
Harry Y. McSween
Minerals ◽  
2021 ◽  
Vol 11 (2) ◽  
pp. 176
Author(s):  
Ryoichi Nakada ◽  
Gaku Tanabe ◽  
Iori Kajitani ◽  
Tomohiro Usui ◽  
Masashi Shidare ◽  
...  

The aqueous environment of ancient Mars is of significant interest because of evidence suggesting the presence of a large body of liquid water on the surface at ~4 Ga, which differs significantly from the modern dry and oxic Martian environment. In this study, we examined the Fe-bearing minerals in the 4 Ga Martian meteorite, Alan Hills (ALH) 84001, to reveal the ancient aqueous environment present during the formation of this meteorite. Extended X-ray absorption fine structure (EXAFS) analysis was conducted to determine the Fe species in ALH carbonate and silica glass with a high spatial resolution (~1–2 μm). The μ-EXAFS analysis of ALH carbonate showed that the Fe species in the carbonate were dominated by a magnesite-siderite solid solution. Our analysis suggests the presence of smectite group clay in the carbonate, which is consistent with the results of previous thermochemical modeling. We also found serpentine in the silica glass, indicating the decrease of water after the formation of carbonate, at least locally. The possible allochthonous origin of the hematite in the carbonate suggests a patchy redox environment on the ancient Martian surface.


1993 ◽  
Vol 115 (10) ◽  
pp. 4264-4270 ◽  
Author(s):  
Mohammed Ouali ◽  
Richard Letellier ◽  
Jian Sheng Sun ◽  
Alain Akhebat ◽  
Frederic Adnet ◽  
...  

2018 ◽  
Vol 115 (17) ◽  
pp. E3888-E3894 ◽  
Author(s):  
Deheng Yang ◽  
Yadong Li ◽  
Xinyi Liu ◽  
Yue Cao ◽  
Yi Gao ◽  
...  

The facet-specific interaction between molecules and crystalline catalysts, such as titanium dioxides (TiO2), has attracted much attention due to possible facet-dependent reactivity. Using surface-sensitive sum-frequency vibrational spectroscopy, we have studied how methanol interacts with different common facets of crystalline TiO2, including rutile(110), (001), (100), and anatase(101), under ambient temperature and pressure. We found that methanol adsorbs predominantly in the molecular form on all of the four surfaces, while spontaneous dissociation into methoxy occurs preferentially when these surfaces become defective. Extraction of Fermi resonance coupling between stretch and bending modes of the methyl group in analyzing adsorbed methanol spectra allows determination of the methanol adsorption isotherm. The isotherms obtained for the four surfaces are nearly the same, yielding two adsorbed Gibbs free energies associated with two different adsorption configurations singled out by ab initio calculations. They are (i) ∼−20 kJ/mol for methanol with its oxygen attached to a low-coordinated surface titanium, and (ii) ∼−5 kJ/mol for methanol hydrogen-bonded to a surface oxygen and a neighboring methanol molecule. Despite similar adsorption energetics, the Fermi resonance coupling strength for adsorbed methanol appears to depend sensitively on the surface facet and coverage.


2006 ◽  
Vol 124 (17) ◽  
pp. 174302 ◽  
Author(s):  
Joseph C. Bopp ◽  
Eric G. Diken ◽  
Jeffrey M. Headrick ◽  
Joseph R. Roscioli ◽  
Mark A. Johnson ◽  
...  

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