Gliese 229

Gliese 229

Gliese 229 A and B
Observation data
Epoch J2000      Equinox J2000
Constellation Lepus
Right ascension 06h 10m 34.61494s[1]
Declination −21° 51′ 52.6564″[1]
Apparent magnitude (V) 8.14
Characteristics
Evolutionary stage Main sequence / Brown dwarf
Spectral type M1Ve / T7[2]
U−B color index +1.222[2]
B−V color index +1.478[2]
Variable type Flare star
Astrometry
Radial velocity (Rv)4.23±0.12[1] km/s
Proper motion (μ) RA: −135.692(11) mas/yr[1]
Dec.: −719.178(17) mas/yr[1]
Parallax (π)173.5740 ± 0.0170 mas[1]
Distance18.791 ± 0.002 ly
(5.7612 ± 0.0006 pc)
Absolute magnitude (MV)9.326[3]
Absolute bolometric
magnitude
 (Mbol)
7.96[4]
Orbit[3][5]
CompanionGliese 229 B
Period (P)216.925+10.604
−10.352
yr
Semi-major axis (a)28.933+1.008
−1.000
 AU
Eccentricity (e)0.853±0.002
Inclination (i)5.497+0.153
−0.162
°
Longitude of the node (Ω)145.946+0.306
−0.294
°
Periastron epoch (T)2466912+97
−63
Argument of periastron (ω)
(secondary)
358.285+0.836
−0.846
°
Semi-amplitude (K1)
(primary)
0.081674+0.001688
−0.001680
km/s
Details
A
Mass0.579[3] M
Radius0.69[6] R
Luminosity (bolometric)0.0430[3] L
Luminosity (visual, LV)0.0158[nb 1] L
Temperature3,700[4] K
Rotation27.3±0.2 d[7]
Rotational velocity (v sin i)1[8] km/s
B
Mass60.423+2.339
−2.379
[5] MJup
Radius1.105±0.025[9] RJup
Luminosity (bolometric)~0.000011 L
Surface gravity (log g)4.93+0.02
−0.03
[9] cgs
Temperature869+5
−7
[9] K
Other designations
NSV 2863, BD−21°1377, GJ 229, HD 42581, HIP 29295, SAO 171334, LHS 1827, TYC 5945-765-1
Database references
SIMBADA
B
Gliese 229 is located in the constellation Lepus
Gliese 229 is located in the constellation Lepus
Gliese 229
Location of Gliese 229 in the constellation Lepus

Gliese 229 (also written as Gl 229 or GJ 229) is a binary system composed of a red dwarf and the second brown dwarf seen by astronomers, 18.8 light years away in the constellation Lepus. The primary component has 58% of the mass of the Sun,[3] 69% of the Sun's radius,[6] and a very low projected rotation velocity of 1 km/s at the stellar equator.[8]

The star is known to be a low activity flare star, which means it undergoes random increases in luminosity because of magnetic activity at the surface. The spectrum shows emission lines of calcium in the H and K bands. The emission of X-rays has been detected from the corona of this star.[10] These may be caused by magnetic loops interacting with the gas of the star's outer atmosphere. No large-scale star spot activity has been detected.[2]

The space velocity components of this star are U = +12, V = –11 and W = –12 km/s.[11] The orbit of this star through the Milky Way galaxy has an eccentricity of 0.07 and an orbital inclination of 0.005.[2]

  1. ^ a b c d e Cite error: The named reference GaiaDR3 was invoked but never defined (see the help page).
  2. ^ a b c d e Cite error: The named reference mnras214 was invoked but never defined (see the help page).
  3. ^ a b c d e Cite error: The named reference Brandt2021 was invoked but never defined (see the help page).
  4. ^ a b Cite error: The named reference Morales+2008 was invoked but never defined (see the help page).
  5. ^ a b Cite error: The named reference Feng2022 was invoked but never defined (see the help page).
  6. ^ a b Cite error: The named reference apjss71 was invoked but never defined (see the help page).
  7. ^ Cite error: The named reference DíezAlonso2019 was invoked but never defined (see the help page).
  8. ^ a b Cite error: The named reference aaa467 was invoked but never defined (see the help page).
  9. ^ a b c Cite error: The named reference Howe2022 was invoked but never defined (see the help page).
  10. ^ Cite error: The named reference Schmitt was invoked but never defined (see the help page).
  11. ^ Cite error: The named reference Gliese1969 was invoked but never defined (see the help page).


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