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WASP-12

Coordinates:Sky map06h 30m 32.794s, +29° 40′ 20.29″
From Wikipedia, the free encyclopedia
Star in the constellation Auriga
WASP-12
Observation data
Epoch J2000.0      Equinox J2000.0
ConstellationAuriga[1]
Right ascension06h 30m 32.7966s[2]
Declination+29° 40′ 20.264″[2]
Apparent magnitude (V)11.560±0.068[3]
Characteristics
Spectral typeG0V or F[citation needed]
Apparent magnitude (B)12.138±0.019[3]
Apparent magnitude (R)~11.6[4]
Apparent magnitude (J)10.477±0.021[5]
Apparent magnitude (H)10.228±0.022[5]
Apparent magnitude (K)10.188±0.020[5]
Astrometry
Proper motion (μ)RA: −1.519(19)mas/yr[2]
Dec.: −6.761(15)mas/yr[2]
Parallax (π)2.4213±0.0166 mas[2]
Distance1,347 ± 9 ly
(413 ± 3 pc)
Details
Mass1.434+0.11
−0.09
[6] M
Radius1.657+0.046
−0.044
[6] R
Luminosity4.05+0.54
−0.53
[6] L
Temperature6360+130
−140
[6] K
Metallicity+0.33+0.14
−0.17
[6]
Other designations
TYC 1891-1178-1,2MASS J06303279+2940202, UCAC2 42216354, Gaia DR2 3435282862461427072[4]
Database references
SIMBADdata

WASP-12 is amagnitude 11yellow dwarfstar located approximately 1347light-years away[2] in theconstellationAuriga.[4] WASP-12 has amass andradius similar to theSun and is known for being orbited by a planet that is extremely hot and has aretrograde orbit around WASP-12. WASP-12 forms a triple star system with twored dwarf companions. Both of them have spectral types of M3V and are only 38% and 37% as massive as the Sun, respectively.[7]

Planetary system

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In 2008, theextrasolar planetWASP-12b was discovered orbiting WASP-12 by thetransit method.[8] Its high carbon-to-oxygen ratio indicates that rocky planets might have formed in the star system, and it may be acarbon planet.[9] It is subject to intensive photo-evaporation, and may be completely destroyed within one billion years from now.[10]

In 2015, no indications of additional planets were found in the WASP-12 system.[6]

  • Artist's conception of WASP-12 & WASP-12b
    Artist's conception of WASP-12 &WASP-12b
The WASP-12 planetary system
Companion
(in order from star)
MassSemimajor axis
(AU)
Orbital period
(days)
EccentricityInclinationRadius
b1.41±0.1 MJ0.0229±0.00081.091423±0.0000030.049±0.01586.0±3.0[11]°1.736±0.092[11] RJ

See also

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References

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  1. ^Roman, Nancy G. (1987)."Identification of a Constellation From a Position".Publications of the Astronomical Society of the Pacific.99 (617):695–699.Bibcode:1987PASP...99..695R.doi:10.1086/132034.Vizier query form
  2. ^abcdeVallenari, 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. ^abHenden, A. A.; et al. (2016). "VizieR Online Data Catalog: AAVSO Photometric All Sky Survey (APASS) DR9 (Henden+, 2016)".VizieR On-line Data Catalog: II/336. Originally Published in: 2015AAS...22533616H.2336.Bibcode:2016yCat.2336....0H.Vizier catalog entry
  4. ^abc"SIMBAD query result: WASP-12 -- Star". Centre de Données astronomiques de Strasbourg. Retrieved2009-04-24.
  5. ^abcSkrutskie, Michael F.; Cutri, Roc M.; Stiening, Rae; Weinberg, Martin D.; Schneider, Stephen E.; Carpenter, John M.; Beichman, Charles A.; Capps, Richard W.; Chester, Thomas; Elias, Jonathan H.; Huchra, John P.; Liebert, James W.; Lonsdale, Carol J.; Monet, David G.; Price, Stephan; Seitzer, Patrick; Jarrett, Thomas H.; Kirkpatrick, J. Davy; Gizis, John E.; Howard, Elizabeth V.; Evans, Tracey E.; Fowler, John W.; Fullmer, Linda; Hurt, Robert L.; Light, Robert M.; Kopan, Eugene L.; Marsh, Kenneth A.; McCallon, Howard L.; Tam, Robert; Van Dyk, Schuyler D.; Wheelock, Sherry L. (1 February 2006)."The Two Micron All Sky Survey (2MASS)".The Astronomical Journal.131 (2):1163–1183.Bibcode:2006AJ....131.1163S.doi:10.1086/498708.ISSN 0004-6256.S2CID 18913331.Vizier catalog entry
  6. ^abcdefCollins, Karen A.; Kielkopf, John F.; Stassun, Keivan G. (2015)."TRANSIT TIMING VARIATION MEASUREMENTS OF WASP-12b AND QATAR-1b: NO EVIDENCE OF ADDITIONAL PLANETS".The Astronomical Journal.153 (2): 78.arXiv:1512.00464.doi:10.3847/1538-3881/153/2/78.S2CID 55191644.
  7. ^Bechter, Eric B.; Crepp, Justin R.; Ngo, Henry; Knutson, Heather A.; Batygin, Konstantin; Hinkley, Sasha; Muirhead, Philip S.; Johnson, John Asher; Howard, Andrew W.; Montet, Benjamin T.; Matthews, Christopher T.; Morton, Timothy D. (2014). "WASP-12b AND HAT-P-8b ARE MEMBERS OF TRIPLE STAR SYSTEMS".The Astrophysical Journal.788 (1): 2.arXiv:1307.6857.Bibcode:2014ApJ...788....2B.doi:10.1088/0004-637X/788/1/2.S2CID 36306243.
  8. ^Hebb, L.; et al. (2009-03-10)."WASP-12b: The Hottest Transiting Extrasolar Planet Yet Discovered".The Astrophysical Journal.693 (2):1920–1928.arXiv:0812.3240.Bibcode:2009ApJ...693.1920H.doi:10.1088/0004-637X/693/2/1920.
  9. ^Madhusudhan, Nikku; Harrington, Joseph; Stevenson, Kevin B.; Nymeyer, Sarah; Campo, Christopher J.; Wheatley, Peter J.; Deming, Drake; Blecic, Jasmina; et al. (December 8, 2010). "A high C/O ratio and weak thermal inversion in the atmosphere of exoplanet WASP-12b".Nature.469 (7328):64–7.arXiv:1012.1603.Bibcode:2011Natur.469...64M.doi:10.1038/nature09602.PMID 21150901.S2CID 4415171..
  10. ^D. Ehrenreich and J.-M. Désert, "Mass-loss rates for transiting exoplanets", 2011
  11. ^abStaff (2015)."Planet WASP-12 b".Extrasolar Planets Encyclopaedia. Retrieved4 August 2017.

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