2023Natur.624..263B


Query : 2023Natur.624..263B

2023Natur.624..263B - Nature, 624, 263-266 (2023/December-0)

15NH3 in the atmosphere of a cool brown dwarf.

BARRADO D., MOLLIERE P., PATAPIS P., MIN M., TREMBLIN P., ARDEVOL MARTINEZ F., WHITEFORD N., VASIST M., ARGYRIOU I., SAMLAND M., LAGAGE P.-O., DECIN L., WATERS R., HENNING T., MORALES-CALDERON M., GUEDEL M., VANDENBUSSCHE B., ABSIL O., BAUDOZ P., BOCCALETTI A., BOUWMAN J., COSSOU C., COULAIS A., CROUZET N., GASTAUD R., GLASSE A., GLAUSER A.M., KAMP I., KENDREW S., KRAUSE O., LAHUIS F., MUELLER M., OLOFSSON G., PYE J., ROUAN D., ROYER P., SCHEITHAUER S., WALDMANN I., COLINA L., VAN DISHOECK E.F., RAY T., OSTLIN G. and WRIGHT G.

Abstract (from CDS):

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.


Abstract Copyright: 2023 The Author(s), under exclusive licence to Springer Nature Limited

Journal keyword(s):

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 WISE J182831.08+265037.7 BD* 18 28 30.30897 +26 50 36.0751           Y0 76 0

Query : 2023Natur.624..263B

Basic data :
WISE J182831.08+265037.7 -- Brown Dwarf
Other object types:
otypes_help
MIR (WISEA,WISEP,...), BD* (2012AJ), * (CNS5)
ICRS coord. (ep=J2000) :
18 28 30.30897 +26 50 36.0751 (Middle-IR) [ ] C 2021ApJS..253....7K
FK4 coord. (ep=B1950 eq=1950) :
18 26 26.27259 +26 48 27.8749 [ ]
Gal coord. (ep=J2000) :
055.07309817 +16.57241759 [ ]
Proper motions mas/yr :
1016.5 169.3 [0.8 0.8 90] C 2021ApJS..253....7K
Parallaxes (mas):
100.3 [2.0] C 2021ApJS..253....7K
Spectral type:
Y0 C 2011ApJS..197...19K
Fluxes (3) :
J 23.48 [0.23] C 2014ApJ...796...39T
H 22.73 [0.13] D 2017ApJ...842..118L
K 23.48 [0.36] D 2017ApJ...842..118L
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Identifiers (5) :
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CNS5 4565 WISEP J182831.08+265037.8 EQ J1828+2650
WISEA J182831.08+265037.6 WISE J182831.08+265037.7

References (76 between 1850 and 2026) (Total 76)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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Distance : 3    Plx : 4    PM : 4    SpT : 1   

   


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