Astronomy:LHS 1478

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Short description: Red dwarf star in the Serpens constellation
LHS 1478
Observation data
Equinox J2000.0]] (ICRS)
Constellation Cassiopeia[1]
Right ascension  02h 57m 18.25955s[2]
Declination +76° 33′ 11.2535″[2]
Apparent magnitude (V) 13.3[3]
Characteristics
Evolutionary stage main sequence[4]
Spectral type M3V[5]
Astrometry
Radial velocity (Rv)+69.79±0.27[2] km/s
Proper motion (μ) RA: +690.920[2] mas/yr
Dec.: −399.894[2] mas/yr
Parallax (π)54.9036 ± 0.0177[2] mas
Distance59.41 ± 0.02 ly
(18.214 ± 0.006 pc)
Absolute magnitude (MV)+12.1[4]
Details[5]
Mass0.236±0.012 M
Radius0.246±0.008 R
Luminosity0.00715±0.00012 L
Surface gravity (log g)4.87±0.06 cgs
Temperature3381±54 K
Metallicity [Fe/H]−0.13±0.19 dex
Rotation~6.4 d
Rotational velocity (v sin i)<2 km/s
Other designations
G 245-61, LHS 1478, LP 14-53, NLTT 9256[6]
Database references
SIMBADdata
Exoplanet Archivedata

LHS 1478 (also known as TOI-1640) is a M3V-type main sequence star located 59.4 light-years from Earth in the constellation of Cassiopeia.[7] It has a mass of 0.24 solar masses and a radius of 0.25 solar radii. It has an effective temperature of 3381 Kelvin. The star is fairly inactive with no major flaring activity.[5][8]

Planetary system

There is currently only one known exoplanet orbiting around the star named LHS 1478 b. It is a hot super-Earth with a mass of 2.33 Earths and a radius of 1.24 Earths. It has an equilibrium temperature of about ~595 K.[5] James Webb Space Telescope observations disfavor the possibility of a low-albedo bare rock, suggesting that the planet either has an atmosphere or a high albedo.[8]

The LHS 1478 planetary system[5]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b 2.33±0.20 M 0.01848+0.00061
−0.00063
1.9495378(41) 87.452+0.052
−0.048
°
1.242+0.051
−0.049
 R

References

  1. Roman, Nancy G. (1987). "Identification of a constellation from a position". Publications of the Astronomical Society of the Pacific 99 (617): 695. doi:10.1086/132034. Bibcode1987PASP...99..695R  Constellation record for this object at VizieR.
  2. 2.0 2.1 2.2 2.3 2.4 Vallenari, A. et al. (2022). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy & Astrophysics. doi:10.1051/0004-6361/202243940  Gaia DR3 record for this source at VizieR.
  3. Carrión-González, Óscar; Kammerer, Jens; Angerhausen, Daniel; Dannert, Felix; García Muñoz, Antonio; Quanz, Sascha P.; Absil, Olivier; Beichman, Charles A. et al. (2023). "Large Interferometer for Exoplanets (LIFE). X. Detectability of currently known exoplanets and synergies with future IR/O/UV reflected-starlight imaging missions". Astronomy and Astrophysics 678: A96. doi:10.1051/0004-6361/202347027. Bibcode2023A&A...678A..96C. 
  4. 4.0 4.1 Houdebine, Éric R.; Mullan, D. J.; Doyle, J. G.; de la Vieuville, Geoffroy; Butler, C. J.; Paletou, F. (2019). "The Mass-Activity Relationships in M and K Dwarfs. I. Stellar Parameters of Our Sample of M and K Dwarfs". The Astronomical Journal 158 (2): 56. doi:10.3847/1538-3881/ab23fe. Bibcode2019AJ....158...56H. 
  5. 5.0 5.1 5.2 5.3 5.4 Soto, M. G.; Anglada-Escudé, G.; Dreizler, S.; Molaverdikhani, K.; Kemmer, J.; Rodríguez-López, C.; Lillo-Box, J.; Pallé, E. et al. (2021-05-01). "Mass and density of the transiting hot and rocky super-Earth LHS 1478 b (TOI-1640 b)" (in en). Astronomy & Astrophysics 649: A144. doi:10.1051/0004-6361/202140618. ISSN 0004-6361. Bibcode2021A&A...649A.144S. 
  6. "G 245-61". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=G+245-61. 
  7. "★ LHS 1478" (in en). https://www.stellarcatalog.com/stars/lhs-1478. 
  8. 8.0 8.1 August, P. C.; Buchhave, L. A.; Diamond-Lowe, H.; Mendonça, J. M.; Gressier, A.; Rathcke, A. D.; Allen, N. H.; Fortune, M. et al. (2025-03-01). "Hot Rocks Survey I: A possible shallow eclipse for LHS 1478 b" (in en). Astronomy & Astrophysics 695: A171. doi:10.1051/0004-6361/202452611. ISSN 0004-6361. Bibcode2025A&A...695A.171A.