| Literature DB >> 34257894 |
Lucas F Rodríguez-Almeida1, Izaskun Jimenéz-Serra1, Víctor M Rivilla1,2, Jesús Martín-Pintado1, Shaoshan Zeng3, Belén Tercero4, Pablo de Vicente4, Laura Colzi1,2, Fernando Rico-Villas1, Sergio Martín5,6, Miguel A Requena-Torres7,8.
Abstract
The chemical compounds carrying the thiol group (-SH) have been considered essential in recent prebiotic studies regarding the polymerization of amino acids. We have searched for this kind of compounds toward the Galactic Centre quiescent cloud G+0.693-0.027. We report the first detection in the interstellar space of the trans-isomer of monothioformic acid (t-HC(O)SH) with an abundance of ~ 1 × 10-10. Additionally, we provide a solid confirmation of the gauche isomer of ethyl mercaptan (g-C2H5SH) with an abundance of ~ 3 × 10-10, and we also detect methyl mercaptan (CH3SH) with an abundance of ~ 5 × 10-9. Abundance ratios were calculated for the three SH-bearing species and their OH-analogues, revealing similar trends between alcohols and thiols with increasing complexity. Possible chemical routes for the interstellar synthesis of t-HC(O)SH, CH3SH and C2H5SH are discussed, as well as the relevance of these compounds in the synthesis of prebiotic proteins in the primitive Earth.Entities:
Keywords: Astrochemistry; Chemical abundance; Galactic Centre; Interstellar molecules
Year: 2021 PMID: 34257894 PMCID: PMC7611195 DOI: 10.3847/2041-8213/abf7cb
Source DB: PubMed Journal: Astrophys J Lett ISSN: 2041-8205 Impact factor: 7.413