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LHS 288

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Red dwarf star in the constellation Carina
LHS 288
Observation data
Epoch J2000      Equinox J2000
Constellation Carina
Right ascension 10 44 21.320
Declination −61° 12′ 35.44″
Apparent magnitude (V) 13.92
Characteristics
Spectral type M5V (M4)
B−V color index 1.82
V−R color index 1.59
R−I color index 2.02
J−H color index 0.442
J−K color index 0.764
Astrometry
Proper motion (μ) RA: −334 mas/yr
Dec.: 1626 mas/yr
Parallax (π)206.9698 ± 0.0448 mas
Distance15.759 ± 0.003 ly
(4.832 ± 0.001 pc)
Absolute magnitude (MV)15.52
Other designations
L 143-23, RHG95 1673, GJ 3618, LFT 734 LTT 3946, PLX 2511.01, Gaia DR2 5254061535097566848
Database references
SIMBADdata
LHS 288 is located in the constellation Carina.LHS 288 is located in the constellation Carina.LHS 288Location of LHS 288 in the constellation Carina

LHS 288 (Luyten 143-23) is a red dwarf around 15.8 light years from the Sun, the closest in the constellation Carina (near Eta Carinae). It is far too faint to be seen with the unaided eye, with an apparent magnitude of 13.92.

Recent studies suggest it may harbour a planet with a mass as small as 2.4 MJ, but the possibility that it passed over an undetected faint star could not be eliminated.

See also

References

  1. ^ "GJ 3618". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 3 Jun 2017.
  2. ^ "Nearby Stars, Preliminary 3rd Version (Gliese+ 1991)".
  3. Henry, T. J.; Jao, Wei-Chun; Subasavage, John P.; Beaulieu, Thomas D.; Ianna, Philip A.; Costa, Edgardo; Méndez, René A. (2006). "The Solar Neighborhood. XVII. Parallax Results from the CTIOPI 0.9 m Program: 20 New Members of the RECONS 10 Parsec Sample" (PDF). The Astronomical Journal. 132 (6): 2360–2371. arXiv:astro-ph/0608230. Bibcode:2006AJ....132.2360H. doi:10.1086/508233. S2CID 15002841.
  4. Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics. 649: A1. arXiv:2012.01533. Bibcode:2021A&A...649A...1G. doi:10.1051/0004-6361/202039657. S2CID 227254300. (Erratum: doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR.
  5. Bartlett, Jennifer L.; Ianna, P. A.; Begam, M. C. (2007). "Possible Astrometric Perturbation of LHS 288". American Astronomical Society Meeting Abstracts #209. 209: 254.16. Bibcode:2007AAS...20925416B.
calculated using this formula

External links

Known celestial objects within 20 light-years
Primary member type
Celestial objects by systems. Secondary members are listed in small print.
    0–10 ly
Main-sequence
stars
A-type
G-type
M-type
(red dwarfs)
Brown dwarfs
L-type
  • Luhman 16 (6.5029±0.0011 ly)
  • T-type brown dwarf B
Sub-brown dwarfs
and rogue planets
Y-type
10–15 ly
Subgiant stars
F-type
Main-sequence
stars
G-type
  • Tau Ceti (11.9118±0.0074 ly)
  • 4 (8?) planets: (b), (c), (d), e, f, g, h, (i)
K-type
M-type
(red dwarfs)
Degenerate
stars
White dwarfs
Brown dwarfs
T-type
15–20 ly    
Subgiant stars
G-type
Main-sequence
stars
A-type
G-type
K-type
M-type
(red dwarfs)
Degenerate
stars
White dwarfs
Brown dwarfs
L-type
T-type
Y-type
Sub-brown dwarfs
and rogue planets
Y-type
Italic are systems without known trigonometric parallax.
Constellation of Carina
Stars
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Variable
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