WASP-59

WASP-59
Observation data
Epoch J2000      Equinox J2000
Constellation Pegasus
Right ascension 23h 18m 29.5475s[1]
Declination 24° 53′ 21.4364″[1]
Apparent magnitude (V) 12.78
Characteristics
Evolutionary stage Main sequence
Spectral type K5V
Astrometry
Radial velocity (Rv)-56.82[1] km/s
Proper motion (μ) RA: 33.729[1] mas/yr
Dec.: −2.522[1] mas/yr
Parallax (π)8.5968 ± 0.0421 mas[1]
Distance379 ± 2 ly
(116.3 ± 0.6 pc)
Details[2]
Mass0.719±0.035 M
Radius0.613±0.044 R
Temperature4650±150 K
Metallicity [Fe/H]-0.15±0.11 dex
Rotational velocity (v sin i)2.3±1.5 km/s
Age7±Gyr
Other designations
Gaia DR2 2841043011433969152, 2MASS J23182955+2453214[3]
Database references
SIMBADdata

WASP-59 is a K-type main-sequence star about 379 light-years away. The star's age is essentially unconstrained by observations. WASP-59 is slightly depleted in heavy elements, having 70% of the solar abundance of iron.[2] The star produces extremely low levels of ultraviolet light, indicating an absence of flare activity.[4]

A multiplicity survey in 2015 did not detect any stellar companions to WASP-59.[5]

  1. ^ a b c d e f Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
  2. ^ a b Cite error: The named reference Bonomo2017 was invoked but never defined (see the help page).
  3. ^ Cite error: The named reference simbad was invoked but never defined (see the help page).
  4. ^ Shkolnik, Evgenya L. (2013), "An Ultraviolet Investigation of Activity on Exoplanet Host Stars", The Astrophysical Journal, 766 (1): 9, arXiv:1301.6192, Bibcode:2013ApJ...766....9S, doi:10.1088/0004-637X/766/1/9, S2CID 118415788
  5. ^ Wöllert, Maria; Brandner, Wolfgang; Bergfors, Carolina; Henning, Thomas (2015), "A Lucky Imaging search for stellar companions to transiting planet host stars", Astronomy & Astrophysics, 575: A23, arXiv:1507.01938, Bibcode:2015A&A...575A..23W, doi:10.1051/0004-6361/201424091, S2CID 119250579