WASP-12
{{Short description|Star in the constellation Auriga}}
{{Starbox begin
| name = WASP-12
}}
{{Starbox observe
| epoch = J2000.0
| constell = Auriga
| appmag_v = {{val|11.560|0.068}}
}}
{{Starbox character
| class = G0V or F{{cn|date=December 2020}}
| appmag_1_passband = B
| appmag_1 = {{val|12.138|0.019}}
| appmag_2_passband = R
| appmag_3_passband = J
| appmag_3 = {{val|10.477|0.021}}
| appmag_4_passband = H
| appmag_4 = {{val|10.228|0.022}}
| appmag_5_passband = K
| appmag_5 = {{val|10.188|0.020}}
| variable =
}}
{{Starbox astrometry
| radial_v =
| prop_mo_ra = {{val|−1.519|(19)}}
| prop_mo_dec = {{val|−6.761|(15)}}
| parallax = 2.4213
| p_error = 0.0166
| absmag_v =
}}
{{Starbox detail
| age =
| mass = {{Val|1.434|0.11|0.09}}
| radius = {{Val|1.657|0.046|0.044}}
| rotation =
| luminosity = {{Val|4.05|0.54|0.53}}
| temperature = {{val|6360|130|140}}
| metal = {{val|+0.33|0.14|0.17}}
}}
{{Starbox catalog
| names = TYC 1891-1178-1, 2MASS J06303279+2940202, UCAC2 42216354, Gaia DR2 3435282862461427072
}}
{{Starbox reference
| Simbad = WASP-12
| EPE = WASP-12
}}
{{Starbox end}}
WASP-12 is a magnitude 11 yellow dwarf star located approximately 1347 light-years away in the constellation Auriga.{{cite web
| url=http://simbad.u-strasbg.fr/simbad/sim-id?Ident=WASP-12
| title =SIMBAD query result: WASP-12 -- Star
| publisher=Centre de Données astronomiques de Strasbourg
| access-date=2009-04-24 }} WASP-12 has a mass and radius similar to the Sun and is known for being orbited by a planet that is extremely hot and has a retrograde orbit around WASP-12. WASP-12 forms a triple star system with two red dwarf companions. Both of them have spectral types of M3V and are only 38% and 37% as massive as the Sun, respectively.{{cite journal|bibcode=2014ApJ...788....2B|doi=10.1088/0004-637X/788/1/2|arxiv=1307.6857|title=WASP-12b AND HAT-P-8b ARE MEMBERS OF TRIPLE STAR SYSTEMS|journal=The Astrophysical Journal|volume=788|issue=1|pages=2|year=2014|last1=Bechter|first1=Eric B.|last2=Crepp|first2=Justin R.|last3=Ngo|first3=Henry|last4=Knutson|first4=Heather A.|last5=Batygin|first5=Konstantin|last6=Hinkley|first6=Sasha|last7=Muirhead|first7=Philip S.|last8=Johnson|first8=John Asher|last9=Howard|first9=Andrew W.|last10=Montet|first10=Benjamin T.|last11=Matthews|first11=Christopher T.|last12=Morton|first12=Timothy D.|s2cid=36306243}}
Planetary system
In 2008, the extrasolar planet WASP-12b was discovered orbiting WASP-12 by the transit method. Its high carbon-to-oxygen ratio indicates that rocky planets might have formed in the star system, and it may be a carbon planet.{{Cite journal |first1=Nikku |last1=Madhusudhan |last2=Harrington |date=December 8, 2010 |first2=Joseph |pages=64–7 |last3=Stevenson |first3=Kevin B. |last4=Nymeyer |first4=Sarah |last5=Campo |first5=Christopher J. |last6=Wheatley |first6=Peter J. |last7=Deming |first7=Drake |last8=Blecic |first8=Jasmina |last9=Hardy |first9=Ryan A. |last10=Lust |first10=Nate B. |last11=Anderson |first11=David R. |last12=Collier-Cameron |first12=Andrew |last13=Britt |first13=Christopher B. T. |last14=Bowman |first14=William C. |last15=Hebb |first15=Leslie |last16=Hellier |first16=Coel |last17=Maxted |first17=Pierre F. L. |last18=Pollacco |first18=Don |last19=West |first19=Richard G. |title=A high C/O ratio and weak thermal inversion in the atmosphere of exoplanet WASP-12b |volume=469 |journal=Nature |doi=10.1038/nature09602 |arxiv=1012.1603 |bibcode = 2011Natur.469...64M |issue=7328 |pmid=21150901|s2cid=4415171 |display-authors=8 }}. It is subject to intensive photo-evaporation, and may be completely destroyed within one billion years from now.[https://www.aanda.org/articles/aa/full_html/2011/05/aa16356-10/T2.html D. Ehrenreich and J.-M. Désert, "Mass-loss rates for transiting exoplanets", 2011]
In 2015, no indications of additional planets were found in the WASP-12 system.{{cite journal|arxiv=1512.00464|last1=Collins|first1=Karen A.|last2=Kielkopf|first2=John F.|last3=Stassun|first3=Keivan G.|title=TRANSIT TIMING VARIATION MEASUREMENTS OF WASP-12b AND QATAR-1b: NO EVIDENCE OF ADDITIONAL PLANETS|journal=The Astronomical Journal|year=2015|volume=153|issue=2|page=78|doi=10.3847/1538-3881/153/2/78|s2cid=55191644 |doi-access=free }}
File:WASP-12b a Hot, Carbon-Rich Planet.jpg
File:WASP-12b.jpg
File:WASP-12b (NASA).jpg|Artist's conception of WASP-12 & WASP-12b
{{OrbitboxPlanet begin}}
{{OrbitboxPlanet
| exoplanet = b
| mass = {{val|1.41|0.1}}
| period = {{val|1.091423|0.000003}}
| semimajor = {{val|0.0229|0.0008}}
| eccentricity = {{val|0.049|0.015}}
| inclination = {{val|86.0|3.0}}{{cite encyclopedia |author=Staff |title=Planet WASP-12 b |url=https://exoplanet.eu/catalog/wasp_12_b--459/ |date=2015 |encyclopedia=Extrasolar Planets Encyclopaedia |access-date=4 August 2017 }}
| radius = {{val|1.736|0.092}}
}}
{{Orbitbox end}}
See also
References
External links
- [http://www.perseus.gr/Astro-Photometry-WASP-12-20110114.htm WASP-12b in transit (lightcurve)]
- {{cite web
| url=http://media4.obspm.fr/exoplanets/base/etoile.php?nom=WASP-12
| title=WASP-12
| work=Exoplanets
| access-date=2009-05-06
| archive-date=2009-11-25
| archive-url=https://web.archive.org/web/20091125030722/http://media4.obspm.fr/exoplanets/base/etoile.php?nom=WASP-12
| url-status=dead
}}
{{Sky|06|30|32.794|+|29|40|20.29|871}}
{{Stars of Auriga}}
{{DEFAULTSORT:WASP-12}}
Category:G-type main-sequence stars
Category:Planetary systems with one confirmed planet