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WASP-29

WASP-29
Observation data
Epoch J2000      Equinox J2000
Constellation Phoenix
Right ascension 23h 51m 31.08391s[1]
Declination −39° 54′ 24.2582″[1]
Apparent magnitude (V) 11.33[2]
Characteristics
WASP-29A
Evolutionary stage main sequence star
Spectral type K4V[3]
B−V color index 0.82
J−H color index 0.478
J−K color index 0.570
WASP-29B
Spectral type M3V[3]
Astrometry
Radial velocity (Rv)24.31±0.20[1] km/s
Proper motion (μ) RA: −56.767(14) mas/yr[1]
Dec.: −88.988(13) mas/yr[1]
Parallax (π)11.4349 ± 0.0151 mas[1]
Distance285.2 ± 0.4 ly
(87.5 ± 0.1 pc)
Position (relative to WASP-29A)[3]
ComponentWASP-29B
Epoch of observation2021
Angular distance125.2″
Projected separation10994 AU
Details[4]
WASP-29A
Mass0.825±0.033 M☉
Radius0.808±0.044 R☉
Surface gravity (log g)4.5±0.2 cgs
Temperature4800±150 K
Metallicity [Fe/H]0.11±0.14 dex
Rotational velocity (v sin i)1.50±0.60 km/s
Age14+0
−7 Gyr
WASP-29B
Mass0.38[3] M☉
Other designations
CD−40 15273, TOI-192, TIC 183537452, WASP-29, TYC 8015-1020-1, 2MASS J23513108-3954241, DENIS J235131.0-395423[2]
WASP-29A: Gaia DR3 6534414719318886144
WASP-29B: Gaia DR3 6534426740931264896
Database references
SIMBADdata

WASP-29 is a binary star system 285 light-years (87 parsecs) away in the constellation of Phoenix. The primary star is a K-type main-sequence star. Its comoving companion, a red dwarf star, was discovered in 2021.[3] The star system kinematically belongs to the thin disk of the Milky Way.[5] The primary is an old star with small starspot activity and low x-ray flux.[6]

  1. ^ a b c d e Cite error: The named reference GaiaDR3 was invoked but never defined (see the help page).
  2. ^ a b Cite error: The named reference SIMBAD was invoked but never defined (see the help page).
  3. ^ a b c d e Cite error: The named reference Fontanive2021 was invoked but never defined (see the help page).
  4. ^ Cite error: The named reference Bonomo2017 was invoked but never defined (see the help page).
  5. ^ Cite error: The named reference Hellier2010 was invoked but never defined (see the help page).
  6. ^ Dos Santos, L. A.; Bourrier, V.; Ehrenreich, D.; Sanz-Forcada, J.; López-Morales, M.; Sing, D. K.; García Muñoz, A.; Henry, G. W.; Lavvas, P.; Lecavelier Des Etangs, A.; Mikal-Evans, T.; Vidal-Madjar, A.; Wakeford, H. R. (2021), "HST PanCET program: Non-detection of atmospheric escape in the warm Saturn-sized planet WASP-29 B", Astronomy & Astrophysics, 649: A40, arXiv:2103.15688, Bibcode:2021A&A...649A..40D, doi:10.1051/0004-6361/202140491, S2CID 232417342

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