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The adapted Modified Gaussian Model: A tool to characterize the composition of magmatic rocks on terrestrial ‘planets’

机译:修改后的改良高斯模型:一种用于表征陆地“行星”上岩浆岩成分的工具

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Here we present an adapted version of the Modified Gaussian Model (MGM), a tool developed to detect and characterize both simple and complex mineralogies in magmatic rocks, and we review the results we obtained over the last years on four different planetary bodies. We first describe the working principle of the adapted MGM technique, with the differences compared to the original version, and the validation process using various laboratory and natural spectra. We then describe the results obtained on the Oman ophiolite (Earth), taken as a planetary spectral analog for magmatic terrains. We finally present spectroscopy-based mineralogical maps and some petrologic implications for key regions of Mars, the Moon and asteroid (4) Vesta.
机译:在这里,我们提出修改后的高斯模型(MGM)的改编版本,该工具开发用于检测和表征岩浆岩中简单和复杂的矿物学,并且我们回顾了过去几年在四个不同行星体上获得的结果。我们首先描述经过修改的MGM技术的工作原理,以及与原始版本相比的差异,以及使用各种实验室光谱和自然光谱进行的验证过程。然后,我们描述在阿曼蛇绿岩(地球)上获得的结果,该结果被用作岩浆地形的行星光谱类似物。最后,我们介绍了基于光谱的矿物学图以及对火星,月球和小行星(4)Vesta关键区域的一些岩石学意义。

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