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LHS 475

Coordinates:Sky map19h20m54.38s,−82° 33′ 16.17″
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LHS 475

Artist's impression of LHS 475 b and its host star
Observation data
EpochJ2000EquinoxJ2000
Constellation Octans[1]
Right ascension 19h20m54.37612s[2]
Declination −82° 33′ 16.1679″[2]
Apparent magnitude(V) 12.69[3]
Characteristics
Evolutionary stage Main sequence
Spectral type M3.5V[4]
Apparent magnitude(V) 12.69±0.03[3]
Apparent magnitude(G) 11.413±0.003[2]
Apparent magnitude(J) 8.555±0.030[3]
Apparent magnitude(H) 8.004±0.038[3]
Apparent magnitude(K) 7.686±0.042[3]
Astrometry
Radial velocity(Rv)−10.59±0.24[2]km/s
Proper motion(μ)RA:+342.300mas/yr[2]
Dec.:−1230.297mas/yr[2]
Parallax(π)80.1134 ± 0.0206mas[2]
Distance40.71 ± 0.01ly
(12.482 ± 0.003pc)
Details[3]
Mass0.274±0.015M
Radius0.2789±0.0014[4]R
Luminosity (bolometric)0.00862±0.00039L
Surface gravity(logg)4.964±0.046cgs
Temperature3289±83K
Rotation79.317d
Other designations
GJ4102,L22-69,LFT1458,LHS475,LTT7606,NLTT47504,PMJ19209-8233,TOI-910,TIC369327947,2MASSJ19205439-8233170[5]
Database references
SIMBADdata

LHS 475is ared dwarfstar located 40.7light-years(12.5parsecs) away from theSolar Systemin the constellation ofOctans.It hosts one knownexoplanet.[6][7]

Planetary system

[edit]
Transmission spectrum of LHS 475 b from NIRSpec

The exoplanetLHS 475 bwas initially found intransitdata fromTESS,and its confirmation using theNIRSpecinstrument of theJames Webb Space Telescope,which also observed itstransmission spectrum,was published in January 2023.[7]Another independent confirmation of the planet was published onarXivin April 2023, and a year later accepted to theAstronomical Journal.[3]

The JWST data is consistent with a featureless spectrum, as would be expected of a planet with no atmosphere, but is also consistent with some types of atmosphere, such as a thincarbon dioxide-dominated atmosphere like that of Mars, or an atmosphere obscured by a thick cloud deck such as that of Venus.[4]Other atmospheric compositions, such as amethane-dominated atmosphere, are ruled out by this spectrum.[6]

LHS 475 b is close in size to Earth, at 99% its diameter, but is much hotter, with anequilibrium temperatureof 586 K (313 °C; 595 °F). Assuming the planet has little to no atmosphere, its dayside temperature is estimated at 748 K (475 °C; 887 °F). The planet completes an orbit around its star in just two days and is likelytidally locked.[4]

The LHS 475 planetary system[4][3]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b 0.914±0.187[note 1]M🜨 0.02037(37) 2.0291010(17) 0 87.38±0.19° 0.991±0.050R🜨

Notes

[edit]
  1. ^The mass of this planet has not been measured; this value is an estimate.

References

[edit]
  1. ^"Finding the constellation which contains given sky coordinates".djm.cc.2 August 2008.
  2. ^abcdefVallenari, A.; et al. (Gaia collaboration) (2023)."GaiaData Release 3. Summary of the content and survey properties ".Astronomy and Astrophysics.674:A1.arXiv:2208.00211.Bibcode:2023A&A...674A...1G.doi:10.1051/0004-6361/202243940.S2CID244398875. Gaia DR3 record for this sourceatVizieR.
  3. ^abcdefghMent, Kristo; Charbonneau, David; et al. (May 2024)."LHS 475 b: A Potential Venus Analog Orbiting a Nearby M Dwarf".The Astronomical Journal.167(5): 197.arXiv:2304.01920.Bibcode:2024AJ....167..197M.doi:10.3847/1538-3881/ad1b58.
  4. ^abcdeLustig-Yaeger, J.; Fu, G.; et al. (January 2023). "A JWST transmission spectrum of the nearby Earth-sized exoplanet LHS 475 b".Nature Astronomy.7(11): 1317–1328.arXiv:2301.04191.Bibcode:2023NatAs...7.1317L.doi:10.1038/s41550-023-02064-z.S2CID261439142.
  5. ^"LHS 475".SIMBAD.Centre de données astronomiques de Strasbourg.Retrieved12 January2023.
  6. ^ab"NASA's Webb Confirms Its First Exoplanet".NASA.11 January 2023.Retrieved12 January2023.
  7. ^abChow, Denise (11 January 2023)."James Webb Telescope finds its first exoplanet - The planet is almost the same size as Earth, according to a research team led by astronomers at the Johns Hopkins University Applied Physics Laboratory".NBC News.Retrieved12 January2023.