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Propionamide (C2H5CONH2): The largest peptide-like molecule in space

  • Juan Li*
  • , Junzhi Wang*
  • , Xing Lu
  • , Vadim Ilyushin
  • , Roman A. Motiyenko
  • , Qian Gou
  • , Eugene A. Alekseev
  • , Donghui Quan
  • , Laurent Margulès
  • , Feng Gao
  • , Frank J. Lovas
  • , Yajun Wu
  • , Edwin Bergin
  • , Shanghuo Li
  • , Zhiqiang Shen
  • , Fujun Du
  • , Meng Li
  • , Siqi Zheng
  • , Xingwu Zheng
  • *Corresponding author for this work
  • CAS - Shanghai Astronomical Observatory
  • Chinese Academy of Sciences
  • National Institutes of Natural Sciences - National Astronomical Observatory of Japan
  • NASU - Institute of Radio Astronomy
  • V. N. Karazin Kharkiv National University
  • Laboratoire de Physique des Lasers, Atomes et Molécules (PhLam)
  • Chongqing University
  • CAS - National Astronomical Observatories
  • Eastern Kentucky University
  • University of Hamburg
  • Max Planck Institute for Extraterrestrial Physics
  • National Institute of Standards and Technology
  • University of Michigan, Ann Arbor
  • Korea Astronomy and Space Science Institute
  • CAS - Purple Mountain Observatory
  • University of Science and Technology of China
  • University of Chinese Academy of Sciences
  • Nanjing University

Research output: Contribution to journalArticlepeer-review

17 Citations (Scopus)

Abstract

Peptide bonds, as the molecular bridges that connect amino acids, are crucial to the formation of proteins. Searches and studies of molecules with embedded peptide-like bonds are thus important for the understanding of protein formation in space. Here we report the first tentative detection of propionamide (C2H5CONH2), the largest peptidelike molecule detected in space toward Sagittarius B2(N1) at a position called N1E that is slightly offset from the continuum peak. New laboratory measurements of the propionamide spectrum were carried out in the 9-461 GHz range, which provide good opportunity to check directly for the transition frequencies of detected interstellar lines of propionamide. Our observing result indicates that propionamide emission comes from the warm, compact cores in Sagittarius B2, in which massive protostellars are forming. The column density of propionamide toward Sgr B2(N1E) was derived to be 1.5 × 1016 cm-2, which is three-fifths of that of acetamide, and one-nineteenth of that of formamide. This detection suggests that large peptide-like molecules can form and survive during star-forming process and may form more complex molecules in the interstellar medium (ISM). The detection of propionamide bodes well for the presence of polypeptides, as well as other complex prebiotic molecules in the ISM.

Original languageEnglish
Article number4
JournalAstrophysical Journal
Volume919
Issue number1
DOIs
Publication statusPublished - 20 Sept 2021

Keywords

  • Data behind figures
  • Machine-readable tables

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