Article (Scientific journals)
15NH3 in the atmosphere of a cool brown dwarf
Barrado, David; Mollière, Paul; Patapis, Polychronis et al.
2023In Nature, 624, p. 263-266
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Abstract :
[en] Brown dwarfs serve as ideal laboratories for studying the atmospheres of giant exoplanets on wide orbits, as the governing physical and chemical processes within them are nearly identical<SUP>1,2</SUP>. Understanding the formation of gas-giant planets is challenging, often involving the endeavour to link atmospheric abundance ratios, such as the carbon-to-oxygen (C/O) ratio, to formation scenarios<SUP>3</SUP>. However, the complexity of planet formation requires further tracers, as the unambiguous interpretation of the measured C/O ratio is fraught with complexity<SUP>4</SUP>. Isotope ratios, such as deuterium to hydrogen and <SUP>14</SUP>N/<SUP>15</SUP>N, offer a promising avenue to gain further insight into this formation process, mirroring their use within the Solar System<SUP>5-7</SUP>. For exoplanets, only a handful of constraints on <SUP>12</SUP>C/<SUP>13</SUP>C exist, pointing to the accretion of <SUP>13</SUP>C-rich ice from beyond the CO iceline of the disks<SUP>8,9</SUP>. Here we report on the mid-infrared detection of the <SUP>14</SUP>NH<SUB>3</SUB> and <SUP>15</SUP>NH<SUB>3</SUB> isotopologues in the atmosphere of a cool brown dwarf with an effective temperature of 380 K in a spectrum taken with the Mid-Infrared Instrument (MIRI) of JWST. As expected, our results reveal a <SUP>14</SUP>N/<SUP>15</SUP>N value consistent with star-like formation by gravitational collapse, demonstrating that this ratio can be accurately constrained. Because young stars and their planets should be more strongly enriched in the <SUP>15</SUP>N isotope<SUP>10</SUP>, we expect that <SUP>15</SUP>NH<SUB>3</SUB> will be detectable in several cold, wide-separation exoplanets.
Research center :
STAR - Space sciences, Technologies and Astrophysics Research - ULiège [BE]
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Barrado, David ;  Center for Astrobiology, Madrid
Mollière, Paul ;  Max-Planck-Institute for Astronomy, Heidelberg
Patapis, Polychronis ;  Institute of Particle Physics and Astrophysics, ETH Zurich, Zürich, Switzerland
Min, Michiel;  Netherlands Institute for Space Research
Tremblin, Pascal;  Université Paris-Saclay, UVSQ, CNRS, CEA, Gif-sur-Yvette, France
Ardevol Martinez, Francisco;  Netherlands Institute for Space Research, -, University of Edinburgh, School of Geosciences, University of Edinburgh, Centre for Astrobiology
Whiteford, Niall;  American Museum of Natural History, New York
Vasist, Malavika Vijayendra ;  Université de Liège - ULiège > Unités de recherche interfacultaires > Space sciences, Technologies and Astrophysics Research (STAR)
Argyriou, Ioannis;  Katholieke University of Leuven, Astronomical Institute
Samland, Matthias;  Max-Planck-Institute for Astronomy, Heidelberg
Lagage, Pierre-Olivier;  CEA Saclay, Service d'Astrophysique
Decin, Leen;  Katholieke University of Leuven, Astronomical Institute
Waters, Rens;  Netherlands Institute for Space Research, Radboud University Nijmegen, Department of Astronomy and Physics
Henning, Thomas;  Max-Planck-Institute for Astronomy, Heidelberg
Morales-Calderón, María;  Center for Astrobiology, Madrid
Guedel, Manuel;  Max-Planck-Institute for Astronomy, Heidelberg, -, University of Vienna, Department of Astronomy
Vandenbussche, Bart;  Katholieke University of Leuven, Astronomical Institute
Absil, Olivier  ;  Université de Liège - ULiège > Département d'astrophysique, géophysique et océanographie (AGO)
Baudoz, Pierre;  LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de Paris Cité, Meudon, France
Boccaletti, Anthony;  LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de Paris Cité, Meudon, France
Bouwman, Jeroen;  Max-Planck-Institute for Astronomy, Heidelberg
Cossou, Christophe;  Université Paris-Saclay, CEA, IRFU, Gif-sur-Yvette, France
Coulais, Alain;  CEA Saclay, Service d'Astrophysique, -
Crouzet, Nicolas;  Leiden Observatory
Gastaud, René;  Université Paris-Saclay, CEA, IRFU, Gif-sur-Yvette, France
Glasse, Alistair;  Royal Observatory Edinburgh
Glauser, Adrian M.;  Institute of Particle Physics and Astrophysics, ETH Zurich, Zürich, Switzerland
Kamp, Inga;  Kapteyn Institute of Astronomy, University of Groningen, Groningen, The Netherlands
Kendrew, Sarah;  Space Telescope Science Institute, ESA Office, Baltimore, Maryland
Krause, Oliver;  Max-Planck-Institute for Astronomy, Heidelberg
Lahuis, Fred;  Netherlands Institute for Space Research
Mueller, Michael;  Kapteyn Institute of Astronomy, University of Groningen, Groningen, The Netherlands
Olofsson, Göran;  AlbaNova University Center
Pye, John;  School of Physics &, Astronomy, Space Research Centre, Space Park Leicester, University of Leicester, Leicester, UK
Rouan, Daniel;  LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de Paris Cité, Meudon, France
Royer, Pierre;  Katholieke University of Leuven, Astronomical Institute
Scheithauer, Silvia;  Max-Planck-Institute for Astronomy, Heidelberg
Waldmann, Ingo;  University College London, Department of Physics and Astronomy
Colina, Luis;  Center for Astrobiology, Madrid
van Dishoeck, Ewine F.;  Leiden Observatory
Ray, Tom;  Dublin Institute for Advanced Studies, School of Cosmic Physics
Östlin, Göran;  Stockholm University, Department of Astronomy
Wright, Gillian;  Royal Observatory Edinburgh
More authors (33 more) Less
 These authors have contributed equally to this work.
Language :
English
Title :
15NH3 in the atmosphere of a cool brown dwarf
Publication date :
06 November 2023
Journal title :
Nature
ISSN :
0028-0836
eISSN :
1476-4687
Publisher :
Nature Publishing Group, London, Gb
Volume :
624
Pages :
263-266
Peer reviewed :
Peer Reviewed verified by ORBi
Available on ORBi :
since 25 January 2024

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