Peter 229

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Double star
Gliese 229
left: Discovery of GJ 229 B at the Palomar Observatory right: image from the Hubble Space Telescope (NASA)
left: Discovery of GJ 229 B at the Palomar Observatory
right: image from the Hubble Space Telescope (NASA)
Observation
dates equinoxJ2000.0 , epoch : J2000.0
AladinLite
Constellation Hare
Right ascension 06 h 10 m 34.6 s
declination −21 ° 51 ′ 52.7 ″
Apparent brightness  8.12 likes
Known exoplanets

2

Position of the attendant   ( JD 2450398)
Angular distance 7 ", 674 ± 0", 007
Position angle 163 °, 91 ± 0 °, 10
Astrometry
parallax (173.70 ± 0.05) mas
distance  (18.77 ± 0.01) ly
(5.76 ± 0.01 pc )
Individual data
Names A ; B.
Observation data:
Apparent brightness A. 8.13 mag
B.
Typing:
Spectral class A. M1 V
B. T6.5
B − V color index A. (1.19)
U − B color index A. (1.48)
Physical Properties:
Absolute vis.
Brightness
M vis
A. +9.3 mag
B.
Dimensions A. (0.563 ± 0.042) M
B. 0.03 M
radius A. (0.547 ± 0.044) R
B.
Luminosity A. 0.03 L
B.
Effective temperature A. 3560 K
B. ~ 850 K
Other names
and catalog entries
Bonn survey BD -21 ° 1377
Henry Draper Catalog HD 42581 [1]
SAO catalog SAO 171334 [2]
Tycho catalog TYC 5945-765-1 [3]
Hipparcos catalog HIP 29295 [4]
Further designations: LHS 1827, GJ 229

Gliese 229 (Gl 229, GJ 229) is a star in the constellation Rabbit . It is a double system 18.8  light years away.

Gliese 229 A is a red dwarf of the spectral type M1, while Gliese 229 B is a brown dwarf of the spectral class T6 with 20 to 50 times the mass of Jupiter and a surface temperature of around 850 Kelvin. The distance between the two components is approximately 50  astronomical units .

Gliese 229 B is the first unequivocally proven brown dwarf (Nakajima et al., 1995).

In 2014, an exoplanet was discovered around Gliese 229 A (Gliese 229 A b) and another in 2020.

Size and temperature comparison between the sun , Gliese 229 A + B, Teide 1 and Jupiter

table

Gliese 229 companion
Planet
(order
from the star)
Discovered Mass
( earth masses )
Major semiaxis of
the railway
( AU )
Rotation time
( days )
eccentricity
Gliese 229 A c 2020 7.93   +2.39−3.44 0.339   +0.024−0.029 122.0 ± 0.4 0.29   +0.06−0.26
Gliese 229 A b 2014 10.02   +3.35−6.10 0.896   +0.069−0.073 523.2   +13.0−7.0 0.17   +0.07−0.17

Web links

Commons : Gliese 229  - Collection of images, videos and audio files

Individual evidence

  1. a b c d e f HD 42581. In: SIMBAD . Center de Données astronomiques de Strasbourg , accessed December 6, 2018 .
  2. HD 42581 B. In: SIMBAD. Center de Données astronomiques de Strasbourg, accessed December 6, 2018 .
  3. a b P. E. Kervella, F. Arenou, F. Mignard, F. Thévenin: Stellar and substellar companions of nearby stars from Gaia DR2. Binarity from proper motion anomaly . In: Astronomy & Astrophysics . 623, p. A72. arxiv : 1811.08902 . bibcode : 2019A & A ... 623A..72K . doi : 10.1051 / 0004-6361 / 201834371 .
  4. ^ GJ 229 B. In: Extrasolar Planets Encyclopaedia . Retrieved December 6, 2018 .
  5. a b c M. Tuomi et al .: Bayesian search for low-mass planets around nearby M dwarfs - estimates for occurrence rate based on global detectability statistics . In: MNRAS . 441, No. 2, pp. 1545-1569. arxiv : 1403.0430 . bibcode : 2014MNRAS.441.1545T . doi : 10.1093 / mnras / stu358 .
  6. T. Nakajima, T. Tsuji, Y. Takeda: Physical Properties of Gliese 229B Based on Newly Determined Carbon and Oxygen Abundances of Gliese 229A . In: The Astronomical Journal . 150, No. 2. arxiv : 1506.03178 . bibcode : 2015AJ .... 150 ... 53N . doi : 10.1088 / 0004-6256 / 150/2/53 .
  7. ^ T. Nakajima et al .: Discovery of a cool brown dwarf . In: Nature . 378, No. 6556, 1995, pp. 463-465. bibcode : 1995Natur.378..463N . doi : 10.1038 / 378463a0 .
  8. a b Fabo Feng et al .: Search for Nearby Earth Analogs II. detection of five new planets, eight planet candidates, and confirmation of three planets around within nearby M dwarfs ∗ . In: The Astrophysical Journal Supplement Series . 246, No. 1, August. arxiv : 2001.02577 . bibcode : 2020ApJS..246 ... 11F . doi : 10.3847 / 1538-4365 / ab5e7c .