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Origin of alkylphosphonic acids in the interstellar medium

机译:星际介质中烷基膦酸的起源

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摘要

For decades, the source of phosphorus incorporated into Earth’s first organisms has remained a fundamental, unsolved puzzle. Although contemporary biomolecules incorporate P(+V) in their phosphate moieties, the limited bioavailability of phosphates led to the proposal that more soluble P(+III) compounds served as the initial source of phosphorus. Here, we report via laboratory simulation experiments that the three simplest alkylphosphonic acids, soluble organic phosphorus P(+III) compounds, can be efficiently generated in interstellar, phosphine-doped ices through interaction with galactic cosmic rays. This discovery opens a previously overlooked avenue into the formation of key molecules of astrobiological significance and untangles basic mechanisms of a facile synthesis of phosphorus-containing organics in extraterrestrial ices, which can be incorporated into comets and asteroids before their delivery and detection on Earth such as in the Murchison meteorite.
机译:几十年来,掺入地球第一生物中的磷的来源一直是一个根本未解决的难题。尽管现代生物分子在其磷酸盐部分中掺入了P(+ V),但是磷酸盐的有限生物利用度导致提出了这样的建议,即更可溶的P(+ III)化合物可作为磷的初始来源。在这里,我们通过实验室模拟实验报告说,三种最简单的烷基膦酸,即可溶性有机磷P(+ III)化合物,可以通过与银河系宇宙射线相互作用而有效地在星际,磷化氢掺杂的冰中生成。这一发现为之前具有星空生物学意义的关键分子的形成开辟了一条此前被人们忽视的途径,并揭开了在地外冰中容易合成含磷有机物的基本机制的难题,这些机制可以在彗星和小行星被运送到地球上并在地球上被探测之前被掺入其中,例如在默奇森陨石中。

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