OH as a probe of the warm-water cycle in planet-forming disks
Artikel i vetenskaplig tidskrift, 2024
Water is a key ingredient for the emergence of life as we know it. Yet, its destruction and reformation in space remain unprobed in warm gas (T > 300 K). Here we detect with the James Webb Space Telescope the emission of the hydroxyl radical (OH) from d203-506, a planet-forming disk exposed to external far-ultraviolet (FUV) radiation. These observations were made as part of the Early Release Science programme PDRs4All, which is focused on the Orion bar. The observed OH spectrum is compared with the results of quantum dynamical calculations to reveal two essential molecular processes. The highly excited rotational lines of OH in the mid-infrared are telltale signs of H2O destruction by FUV radiation. The OH rovibrational lines in the near-infrared are attributed to chemical excitation by the key reaction O + H-2 -> OH + H, which seeds the formation of water in the gas phase. These results show that under warm and irradiated conditions, water is destroyed and efficiently reformed through gas-phase reactions. We infer that, in this source, the equivalent of Earth oceans' worth of water is destroyed per month and replenished. This warm-water cycle could reprocess some water inherited from cold interstellar clouds and explain the lower deuterium fraction of water in Earth's oceans compared with that found around protostars.
Författare
Marion Zannese
Université Paris-Saclay
Benoit Tabone
Université Paris-Saclay
Emilie Habart
Université Paris-Saclay
Javier R. Goicoechea
CSIC - Instituto de Fisica Fundamental (IFF)
Alexandre Zanchet
CSIC - Instituto de Fisica Fundamental (IFF)
Ewine F. van Dishoeck
Universiteit Leiden
Max-Planck-Gesellschaft
Marc C. van Hemert
Universiteit Leiden
John H Black
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
Alexander G. G. M. Tielens
Universiteit Leiden
University of Maryland
A. Veselinova
Universidad de Salamanca
P. G. Jambrina
Universidad de Salamanca
M. Menendez
Universidad Complutense de Madrid
E. Verdasco
Universidad Complutense de Madrid
F. J. Aoiz
Universidad Complutense de Madrid
L. Gonzalez-Sanchez
Universidad de Salamanca
Boris Trahin
Université Paris-Saclay
Emmanuel Dartois
Université Paris-Saclay
Olivier Berne
Universite Paul Sabatier Toulouse III
Els Peeters
Western University
SETI Institute
Jinhua He
Chinese Academy of Sciences
Universidad de Chile (UCH)
Ameek Sidhu
Western University
Ryan Chown
Western University
Ilane Schroetter
Universite Paul Sabatier Toulouse III
Dries van de Putte
Space Telescope Science Institute (STScI)
Amelie Canin
Universite Paul Sabatier Toulouse III
Felipe Alarcon
University of Michigan
Alain Abergel
Université Paris-Saclay
Edwin A. Bergin
University of Michigan
Jeronimo Bernard-Salas
Innovative Common Laboratory For Space Spectroscopy (INCLASS)
CERGA (Centre d'Etudes et de Recherche de Grasse ACRI)
Christiaan Boersma
NASA Ames Research Center
Emeric Bron
Sorbonne Université
Jan Cami
Western University
SETI Institute
Daniel Dicken
Royal Observatory
Meriem Elyajouri
Université Paris-Saclay
Asuncion Fuente
Centro de Astrobiología (INTA-CSIC)
Karl D. Gordon
Space Telescope Science Institute (STScI)
Universiteit Gent
Lina Issa
Universite Paul Sabatier Toulouse III
Christine Joblin
Universite Paul Sabatier Toulouse III
Olga Kannavou
Université Paris-Saclay
Baria Khan
Western University
David Languignon
Sorbonne Université
Romane Le Gal
Université Grenoble Alpes
Institut de Radioastronomie Millimétrique (IRAM)
Alexandros Maragkoudakis
NASA Ames Research Center
Raphael Meshaka
Université Paris-Saclay
Sorbonne Université
Yoko Okada
Universität zu Köln
Takashi Onaka
Meisei University
University of Tokyo
Sofia Pasquini
Western University
Marc W. Pound
University of Michigan
Massimo Robberto
Space Telescope Science Institute (STScI)
Johns Hopkins University
Markus Roellig
Fraunhofer-Institut für Angewandte Festkörperphysik
Universität zu Köln
Physikalischer Verein
Bethany Schefter
Western University
Thiébaut-Antoine Schirmer
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
Silvia Vicente
Instituto de Astrofísica e Ciências do Espaço (IA)
Mark G. Wolfire
University of Maryland
Nature Astronomy
23973366 (eISSN)
Vol. 8 5 577-586Ämneskategorier
Astronomi, astrofysik och kosmologi
DOI
10.1038/s41550-024-02203-0