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星际介质中烷基膦酸的起源。

Origin of alkylphosphonic acids in the interstellar medium.

作者信息

Turner Andrew M, Abplanalp Matthew J, Bergantini Alexandre, Frigge Robert, Zhu Cheng, Sun Bing-Jian, Hsiao Chun-Ta, Chang Agnes H H, Meinert Cornelia, Kaiser Ralf I

机构信息

Department of Chemistry, University of Hawaii at Manoa, Honolulu, HI 96822, USA.

W.M. Keck Laboratory in Astrochemistry, University of Hawaii at Manoa, Honolulu, HI 96822, USA.

出版信息

Sci Adv. 2019 Aug 7;5(8):eaaw4307. doi: 10.1126/sciadv.aaw4307. eCollection 2019 Aug.

Abstract

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.

摘要

几十年来,地球上第一批生物所吸收磷的来源一直是一个基本的未解之谜。尽管当代生物分子在其磷酸基团中结合了五价磷(P(+V)),但磷酸盐有限的生物可利用性使得人们提出,更易溶解的三价磷(P(+III))化合物是磷的初始来源。在此,我们通过实验室模拟实验报告,三种最简单的烷基膦酸,即可溶性有机磷三价磷化合物,能够通过与银河宇宙射线相互作用,在星际掺有磷化氢的冰中高效生成。这一发现开辟了一条此前被忽视的途径,通向具有天体生物学意义的关键分子的形成,并解开了在外星冰中简便合成含磷有机物的基本机制,这些含磷有机物在被彗星和小行星携带并在地球上被发现(如默奇森陨石)之前就可以被纳入其中。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/d164/6685711/b56e410981f5/aaw4307-F1.jpg

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