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  • Barrado, David (author)

15NH3 in the atmosphere of a cool brown dwarf

  • Article/chapterEnglish2023

Publisher, publication year, extent ...

  • 2023
  • printrdacarrier

Numbers

  • LIBRIS-ID:oai:DiVA.org:su-227683
  • https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-227683URI
  • https://doi.org/10.1038/s41586-023-06813-yDOI

Supplementary language notes

  • Language:English
  • Summary in:English

Part of subdatabase

Classification

  • Subject category:ref swepub-contenttype
  • Subject category:art swepub-publicationtype

Notes

  • 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. 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. However, the complexity of planet formation requires further tracers, as the unambiguous interpretation of the measured C/O ratio is fraught with complexity. Isotope ratios, such as deuterium to hydrogen and 14N/15N, offer a promising avenue to gain further insight into this formation process, mirroring their use within the Solar System. For exoplanets, only a handful of constraints on 12C/13C exist, pointing to the accretion of 13C-rich ice from beyond the CO iceline of the disks. Here we report on the mid-infrared detection of the 14NH3 and 15NH3 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 14N/15N 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 15N isotope, we expect that 15NH3 will be detectable in several cold, wide-separation exoplanets. 

Subject headings and genre

Added entries (persons, corporate bodies, meetings, titles ...)

  • Mollière, Paul (author)
  • Patapis, Polychronis (author)
  • Min, Michiel (author)
  • Tremblin, Pascal (author)
  • Ardevol Martinez, Francisco (author)
  • Whiteford, Niall (author)
  • Vasist, Malavika (author)
  • Argyriou, Ioannis (author)
  • Samland, Matthias (author)
  • Lagage, Pierre-Olivier (author)
  • Decin, Leen (author)
  • Waters, Rens (author)
  • Henning, Thomas (author)
  • Morales-Calderón, María (author)
  • Guedel, Manuel (author)
  • Vandenbussche, Bart (author)
  • Absil, Olivier (author)
  • Baudoz, Pierre (author)
  • Boccaletti, Anthony (author)
  • Bouwman, Jeroen (author)
  • Cossou, Christophe (author)
  • Coulais, Alain (author)
  • Crouzet, Nicolas (author)
  • Gastaud, René (author)
  • Glasse, Alistair (author)
  • Glauser, Adrian M. (author)
  • Kamp, Inga (author)
  • Kendrew, Sarah (author)
  • Krause, Oliver (author)
  • Lahuis, Fred (author)
  • Mueller, Michael (author)
  • Olofsson, Göran,1944-Stockholms universitet,Institutionen för astronomi(Swepub:su)olofsson (author)
  • Pye, John (author)
  • Rouan, Daniel (author)
  • Royer, Pierre (author)
  • Scheithauer, Silvia (author)
  • Waldmann, Ingo (author)
  • Colina, Luis (author)
  • van Dishoeck, Ewine F. (author)
  • Ray, Tom (author)
  • Östlin, Göran,1968-Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)(Swepub:su)ostlin (author)
  • Wright, Gillian (author)
  • Stockholms universitetInstitutionen för astronomi (creator_code:org_t)

Related titles

  • In:Nature624:7991, s. 263-2660028-08361476-4687

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