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WASP-159

From Wikipedia, the free encyclopedia
WASP-159
Observation data
Epoch J2000      Equinox J2000
Constellation Caelum
Right ascension 04h 32m 32.7558s[1]
Declination −38° 58′ 05.953″[1]
Apparent magnitude (V) 12.84±0.24[2]
Characteristics
Spectral type F9IV[3]
B−V color index −0.21[2]
Astrometry
Radial velocity (Rv)+35.16±0.01[3] km/s
Proper motion (μ) RA: −0.586(10) mas/yr[1]
Dec.: 5.347(14) mas/yr[1]
Parallax (π)1.3723 ± 0.0098 mas[1]
Distance2,380 ± 20 ly
(729 ± 5 pc)
Details[3]
Mass1.41±0.12 M
Radius2.11±0.10 R
Luminosity4.78+0.23
−0.21
[4] 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
Gaia DR2 4864759888238232320
Database references
SIMBADdata
Exoplanet Archivedata

WASP-159 is a faint star located in the southern constellation Caelum. With an apparent magnitude of 12.84, a powerful telescope is needed to see the star. The star is located 2,380 light-years (730 parsecs) based on parallax, but is drifting away with a heliocentric radial velocity of +35.16 km/s.

Properties

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WASP-159 is a F-type subgiant with 1.41 times the Sun's mass, and double the Sun's radius. It radiates at 4.78 times the Sun's luminosity from its photosphere at an effective temperature of 6,120 K. WASP-159 is about 3 billion years old, and is metal-rich like many other planetary hosts.

Planetary system

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In 2019, SuperWASP discovered an inflated "hot Jupiter" orbiting the star.[3]

The WASP-159 planetary system[3]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b 0.55±0.08 MJ 0.06±0.00 3.84±0.00 0 88.1±1.4° 1.38±0.09 RJ

References

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  1. ^ a b c d Vallenari, 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 at VizieR.
  2. ^ a b Høg, 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.
  3. ^ a b c d e Hellier, 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.
  4. ^ Stassun, Keivan G.; Oelkers, Ryan J.; Paegert, Martin; Torres, Guillermo; Pepper, Joshua; De Lee, Nathan; Collins, Kevin; Latham, David W.; Muirhead, Philip S.; Chittidi, Jay; Rojas-Ayala, Bárbara; Fleming, Scott W.; Rose, Mark E.; Tenenbaum, Peter; Ting, Eric B.; Kane, Stephen R.; Barclay, Thomas; Bean, Jacob L.; Brassuer, C. E.; Charbonneau, David; Ge, Jian; Lissauer, Jack J.; Mann, Andrew W.; McLean, Brian; Mullally, Susan; Narita, Norio; Plavchan, Peter; Ricker, George R.; Sasselov, Dimitar; Seager, S.; Sharma, Sanjib; Shiao, Bernie; Sozzetti, Alessandro; Stello, Dennis; Vanderspek, Roland; Wallace, Geoff; Winn, Joshua N. (October 2019). "The Revised TESS Input Catalog and Candidate Target List". The Astronomical Journal. 158 (4): 138. arXiv:1905.10694. Bibcode:2019AJ....158..138S. doi:10.3847/1538-3881/ab3467. hdl:1721.1/124721. ISSN 0004-6256. S2CID 166227927.