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Evolved magma on Mars

机译:火星上的岩浆演化

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Earth is distinguished from the other terrestrial planets by its continents, which are largely made of low-density rocks termed felsic - that is, rich in silica and the mineral feldspar. These rocks are formed from magma through extensive melting and subsequent recrystallization, and are abundant on Earth. In contrast, the surface of Mars is dominated by denser, iron-rich basaltic rocks~1 that have experienced little magmatic evolution, similar to the rocks beneath Earth’s oceans. However, writing in Nature Geoscience, Wray et al.~2 and Carter and Poulet~3 present spectral satellite data that reveal the presence of feldspar-rich rocks throughout the ancient southern highlands of Mars. These rocks signal a whole new suite of magmatic processes on Mars, and may help scientists understand the origin of the felsic rocks and soils that have been identified at the Curiosity rover’s landing site in Gale Crater~(4-6) (Fig. 1).
机译:地球与其他陆地行星的不同之处在于,它们的大陆主要由被称为长英质的低密度岩石构成,岩石中富含二氧化硅和矿物长石。这些岩石是由岩浆经过广泛的熔化和随后的再结晶作用形成的,并且在地球上非常丰富。相比之下,火星的表面以致密,富含铁的玄武岩为主[1],几乎没有岩浆演化,类似于地球海洋下方的岩石。然而,Wray等人〜2和Carter和Poulet〜3在《自然地球科学》中撰文提出了光谱卫星数据,揭示了整个火星南部南部高地中富含长石的岩石的存在。这些岩石标志着火星上出现了全新的岩浆过程,并可能有助于科学家了解在大风火山口(4-6)的好奇号火星登陆场发现的长英质岩石和土壤的起源(图1)。 。

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