LHS 475

LHS 475

Artist's impression of LHS 475 b and its host star
Observation data Epoch J2000      Equinox J2000
Constellation	Octans[1]
Right ascension	19h 20m 54.37612s[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: +342.300 mas/yr[2] Dec.: −1230.297 mas/yr[2]
Parallax (π)	80.1134 ± 0.0206 mas[2]
Distance	40.71 ± 0.01 ly (12.482 ± 0.003 pc)
Details[3]
Mass	0.274±0.015 M☉
Radius	0.2789±0.0014[4] R☉
Luminosity (bolometric)	0.00862±0.00039 L☉
Surface gravity (log g)	4.964±0.046 cgs
Temperature	3289±83 K
Rotation	79.317 d
Other designations
GJ 4102, L 22-69, LFT 1458, LHS 475, LTT 7606, NLTT 47504, PM J19209-8233, TOI-910, TIC 369327947, 2MASS J19205439-8233170[5]
Database references
SIMBAD	data

LHS 475 is a red dwarf star located 40.7 light-years (12.5 parsecs) away from the Solar System in the constellation of Octans. It hosts one known exoplanet.^[6][7]

Planetary system

The exoplanet LHS 475 b was initially found in transit data from TESS, and its confirmation using the NIRSpec instrument of the James Webb Space Telescope, which also observed its transmission spectrum, was published in January 2023.^[7] Another independent confirmation of the planet was published on arXiv in April 2023, and a year later accepted to the Astronomical 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 thin carbon 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 a methane-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 an equilibrium temperature of 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 likely tidally locked.^[4]

Notes

References

• v
• t
• e

Constellation of Octans

• List of stars in Octans
• Octans in Chinese astronomy

Stars

Bayer	α β γ1 γ2 γ3 δ ε ζ η θ ι κ λ μ1 μ2 ν ξ ο π1 π2 ρ σ (Polaris Australis) τ υ φ χ ψ ω
Variable	R BQ CK CW FT
HR	47 512 525 4595 6837 6912 7698 7785 7812 8234 8380 8432 8526 8577 8786 8935 8957 8995
HD	142022 166066 212301
Other	Gliese 877 LHS 475 TOI-4342 W2150AB

Exoplanets	2MASS J2126–8140 HD 142022 Ab HD 212301 b LHS 475 b

Galaxies

NGC	2573 7095 7098
Other	PGC 10922

Category