GJ 3929

GJ 3929

Artist's impression and size comparison of the two planets in the GJ 3929 system with Earth
Observation data
Epoch J2000      Equinox J2000
Constellation Corona Borealis[note 1]
Right ascension 15h 58m 18.8s[1]
Declination +35° 24′ 24.3″[1]
Apparent magnitude (V) 12.67[2]
Characteristics
Spectral type M3.5V[1]
Astrometry
Radial velocity (Rv)10.14[2] km/s
Proper motion (μ) RA: −143.277±0.066 mas/yr[2]
Dec.: 318.219±0.082 mas/yr[2]
Parallax (π)63.1727 ± 0.038 mas[1]
Distance51.58±0.02 ly
(15.822±0.006 pc)[3]
Absolute magnitude (MV)11
Details[3]
Mass0.313+0.027
−0.022
 M
Radius0.32±0.01 R
Luminosity0.0109+0.0005
−0.0004
 L
Surface gravity (log g)4.89±0.05 cgs
Temperature3,384±88 K
Metallicity [Fe/H]−0.02±0.12 dex
Rotation122±13 d[4]
Rotational velocity (v sin i)<2 km/s
Age2.2 – 11.2[note 2] Gyr
Other designations
TOI-2013, TIC 188589164, 2MASS J15581883+3524236, Gaia DR3 1372215976327300480,[3] G 180-18[5]
Database references
SIMBADdata

GJ 3929, also known as Gliese 3929 and TOI-2013, is a red dwarf star located 51.6 light-years from Earth, in the constellation Corona Borealis.[5][note 3] With an apparent magnitude of 12,[5] it is not visible to the naked eye. In 2022, two exoplanets were detected orbiting the star.[4]

  1. ^ a b c d e f "G 180-18". SIMBAD. Retrieved January 4, 2023.
  2. ^ a b c Cite error: The named reference :6 was invoked but never defined (see the help page).
  3. ^ a b c Cite error: The named reference :2 was invoked but never defined (see the help page).
  4. ^ a b Kemmer, J.; Dreizler, S.; Kossakowski, D.; Stock, S.; Quirrenbach, A.; Caballero, J. A.; Amado, P. J.; Collins, K. A.; Espinoza, N.; Herrero, E.; Jenkins, J. M.; Latham, D. W.; Lillo-Box, J.; Narita, N.; Pallé, E. (2022-03-01). "Discovery and mass measurement of the hot, transiting, Earth-sized planet, GJ 3929 b". Astronomy & Astrophysics. 659: A17. arXiv:2202.00970. Bibcode:2022A&A...659A..17K. doi:10.1051/0004-6361/202142653. ISSN 0004-6361.
  5. ^ a b c "★ Gliese 3929". Stellar Catalog. Retrieved 2024-01-01.


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