A detection of sulfur-bearing cyclic hydrocarbons in space

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Authors: Mitsunori Araki, Miguel Sanz‐Novo, Christian Endres, P. Caselli, V. M. Rivilla, Izaskun Jiménez-Serra, Laura Colzi, Shaoshan Zeng, Andrés Megías, Álvaro López-Gallifa, Antonio Martínez-Henares, David San Andrés
+4 more S. Martín, Miguel A. Requena-Torres, Juan García de la Concepción, Valerio Lattanzi
Cited by: 5
References: 57

Abstract

Abstract Molecules harbouring sulfur are thought to have played a key role in the biological processes of life on Earth, and thus, they are of much interest when found in space. Here we report on the astronomical detection of a six-membered sulfur-bearing cyclic hydrocarbon in the interstellar medium. Observations of the Galactic Centre molecular cloud G+0.693-0.027 reveal the presence of 2,5-cyclohexadien-1-thione, which is a structural isomer of thiophenol ( c -C 6 H 6 S). For the astronomical identification, we first performed precise laboratory measurements of the thiophenol discharge products system. These measurements, conducted in the radio band using a chirped-pulse Fourier transform microwave spectrometer, enabled us to characterize this highly polar molecular species and provided unambiguous fingerprints needed to identify this organosulfur compound in space, which now ranks as the largest interstellar sulfur-bearing molecule. These results herald the discovery of a family of prebiotically relevant sulfur-bearing species, which potentially act as a bridge between the chemical inventory of the interstellar medium and the composition of the minor bodies of the Solar System.

Fields of Study & Subjects

Astrophysics and Star Formation Studies Origins and Evolution of Life Astro and Planetary Science

Publication details

Journal / source
Nature Astronomy
Publisher
Springer Science and Business Media LLC
Volume
10
Issue
3
Pages
401–409
Publication date
23 January 2026
Language
EN