WASP-20
{{Short description|Star in the constellation Cetus}}
{{Starbox begin}}
{{Starbox observe
| epoch = J2000
| constell = Cetus
| dec = {{DEC|-23|56|08.6028}}
}}
{{Starbox character
}}
{{Starbox astrometry
| radial_v = {{val|1.26|0.85}}
| prop_mo_ra = 1.352
| prop_mo_dec = -14.739
| parallax = 3.4699
| p_error = 0.7095
| absmag_v =
| absmag_bol =
}}
{{Starbox detail
| mass = {{val|1.200|0.041}}
| radius = {{val|1.392|0.044}}
| luminosity =
| gravity =
| temperature = {{val|5940|100}}
| metal_fe = {{val|−0.008|0.060}}
| rotation =
| rotational_velocity = {{val|4.75|0.51}}
| age_gyr = {{val|7.0|2.0|1.0}}
}}
{{Starbox catalog
| names = {{odlist | 2MASS=J00203853-2356086 | CD=-24 102 | GSC=06413-00439 | TIC=211438925 | TOI=194 | TYC=6413-439-1 | WASP=20}}
}}
{{Starbox reference
| Simbad = CD-24+102
| NSTED = WASP-20
}}
{{Starbox end}}
WASP-20, also known as CD-24 102, is a binary star system in the equatorial constellation Cetus, located at a distance of about {{convert|940|ly|pc|lk=on|abbr=off}} from the Sun. The primary star is an F-type main sequence star and hosts one confirmed exoplanet, WASP-20b.{{Cite web |title=WASP-20 {{!}} NASA Exoplanet Archive |url=https://exoplanetarchive.ipac.caltech.edu/overview/wasp%2020%20b#overview}}
Stellar properties
Planetary system
WASP-20b is a transiting hot Jupiter discovered in 2014. WASP-20b orbits WASP-20 in less than five Earth days very close to its star (0.06 AU) in a circular (near-zero eccentricity) orbit. The orbit is inclined by 85.56 ± 0.22° relative to the plane of the sky and is thus edge-on, as necessary for a transit to be observed.
{{Orbitbox planet begin
| name = WASP-20
}}
{{Orbitbox planet
| exoplanet = b
| mass = {{val|0.311|0.019|0.018}}
| radius = {{val|1.462|0.059}}
| semimajor = {{val|0.05999|0.00069|0.00068}}
| period = {{val|4.8996284|(33)}}
| eccentricity = <0.039
| inclination = {{val|85.56|0.22}}
}}
{{Orbitbox end}}
See also
References
{{reflist|refs=
{{cite simbad |title=CD-24 102 |access-date=16 April 2024}}
{{Cite Gaia DR3|2359978293137038720}}
{{cite journal |last1=Anderson |first1=D. R. |last2=Collier Cameron |first2=A. |display-authors=etal |date=March 2015 |title=WASP-20b and WASP-28b: a hot Saturn and a hot Jupiter in near-aligned orbits around solar-type stars |journal=Astronomy & Astrophysics |volume=575 |issue= |pages=A61 |doi=10.1051/0004-6361/201423591 |arxiv=1402.1482 |bibcode=2015A&A...575A..61A}}
{{cite journal |last1=Evans |first1=Daniel F. |last2=Southworth |first2=John |last3=Smalley |first3=Barry |date=December 2016 |title=WASP-20 Is a Close Visual Binary with a Transiting Hot Jupiter |journal=The Astrophysical Journal Letters |volume=833 |issue=2 |pages=L19 |doi=10.3847/2041-8213/833/2/L19 |doi-access=free |arxiv=1611.08735 |bibcode=2016ApJ...833L..19E}}
{{cite journal |last1=Bonomo |first1=A. S. |last2=Desidera |first2=S. |display-authors=etal |date=June 2017 |title=The GAPS Programme with HARPS-N at TNG. XIV. Investigating giant planet migration history via improved eccentricity and mass determination for 231 transiting planets |journal=Astronomy & Astrophysics |volume=602 |issue= |pages=A107 |doi=10.1051/0004-6361/201629882 |arxiv=1704.00373 |bibcode=2017A&A...602A.107B}}
{{Cite constellation|WASP-20}}
}}
{{Cetus}}
Category:F-type main-sequence stars