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WASP-159

From Wikipedia, the free encyclopedia
Star in the constellation Caelum
WASP-159
Observation data
Epoch J2000.0      Equinox J2000.0
ConstellationCaelum[1]
Right ascension04h 32m 32.75581s[2]
Declination−38° 58′ 05.9529″[2]
Apparent magnitude (V)12.84±0.24[3]
Characteristics
Evolutionary stagesubgiant[2]
Spectral typeF9[4]
B−Vcolor index−0.21[3]
Astrometry
Radial velocity (Rv)35.16±0.01[4] km/s
Proper motion (μ)RA: −0.586mas/yr[2]
Dec.: +5.347mas/yr[2]
Parallax (π)1.3723±0.0098 mas[2]
Distance2,380 ± 20 ly
(729 ± 5 pc)
Details[4]
Mass1.41±0.12 M
Radius2.11±0.10 R
Luminosity4.674+0.064
−0.053
[2] L
Surface gravity (log g)3.94±0.04 cgs
Temperature6,120±140 K
Metallicity[Fe/H]+0.22±0.12 dex
Rotational velocity (v sin i)5.7±0.4 km/s
Age3.40±0.95 Gyr
Other designations
TOI-1903,TIC 77156657,WASP-159,TYC 7579-251-1[5]
Database references
SIMBADdata
Exoplanet Archivedata

WASP-159 is astar located in the southernconstellationCaelum, the chisel. It has anapparent magnitude of 12.84,[3] making it readily visible intelescopes with an aperture of at least four inches, but not to thenaked eye. The star is located relatively far at a distance of 2,380light-years based on recentparallax measurements from theGaia spacecraft,[2] but it is receding with a heliocentricradial velocity of35.2 km/s.[4]

WASP-159 has astellar classification of F9 indicating that it is a lateF-type star.[4] It appears to be ceasinghydrogen fusion at itscore and evolving towards thered giant branch.[4] It has 1.41 times theSun's mass and 2.11 times theradius of the Sun.[4] It radiates 4.674 times theluminosity of the Sun[2] from itsphotosphere at aneffective temperature of6,120 K,[4] giving it a whitish-yellow hue when viewed in a telescope. WASP-159 is metal enriched with aniron abundance 166% that of theSun, and it is estimated to be 3.4billion years old.[4]

Planetary system

[edit]

In 2019,SuperWASP discovered atransiting exoplanet orbiting the star after spectral and radial velocity observations. WASP-159b is a "bloated"hot Jupiter that takes roughly 3.8days to revolve around its host star in a circularorbit.[4]

TheWASP-159 planetary system[4]
Companion
(in order from star)
MassSemimajor axis
(AU)
Orbital period
(days)
EccentricityInclinationRadius
b0.55±0.08 MJ0.0538±0.00153.8404008+0.0000063
−0.0000064
0.00 (fixed)88.1±1.4°1.38±0.09 RJ

References

[edit]
  1. ^Roman, Nancy G. (1987)."Identification of a constellation from a position".Publications of the Astronomical Society of the Pacific.99 (617): 695.Bibcode:1987PASP...99..695R.doi:10.1086/132034. Constellation record for this object atVizieR.
  2. ^abcdefghVallenari, A.; et al. (Gaia collaboration) (2023)."Gaia Data Release 3. Summary of the content and survey properties".Astronomy and Astrophysics.674: A1.arXiv:2208.00211.Bibcode:2023A&A...674A...1G.doi:10.1051/0004-6361/202243940.S2CID 244398875. Gaia DR3 record for this source atVizieR.
  3. ^abcHøg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P.; Wicenec, A. (1 March 2000). "The Tycho-2 catalogue of the 2.5 million brightest stars".Astronomy and Astrophysics.355:L27–L30.Bibcode:2000A&A...355L..27H.ISSN 0004-6361.
  4. ^abcdefghijkHellier, Coel; Anderson, D. R.; Bouchy, F.; Burdanov, A.; Collier Cameron, A.; Delrez, L.; Gillon, M.; Jehin, E.; Lendl, M.; Nielsen, L. D.; Maxted, P. F. L.; Pepe, F.; Pollacco, D.; Queloz, D.; Ségransan, D.; Smalley, B.; Triaud, A. H. M. J.; Udry, S.; West, R. G. (1 January 2019)."New transiting hot Jupiters discovered by WASP-South, Euler/CORALIE, and TRAPPIST-South".Monthly Notices of the Royal Astronomical Society.482 (1):1379–1391.arXiv:1803.02224.Bibcode:2019MNRAS.482.1379H.doi:10.1093/mnras/sty2741.ISSN 0035-8711.
  5. ^"WASP-159".SIMBAD.Centre de données astronomiques de Strasbourg.
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