WASP-12

Last updated
WASP-12
Observation data
Epoch J2000.0       Equinox J2000.0
Constellation Auriga [1]
Right ascension 06h 30m 32.7966s [2]
Declination +29° 40 20.264 [2]
Apparent magnitude  (V)11.560±0.068 [3]
Characteristics
Spectral type G0V 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]
Distance 1,347 ± 9  ly
(413 ± 3  pc)
Details
Mass 1.434+0.11
−0.09
[6]   M
Radius 1.657+0.046
−0.044
[6]   R
Luminosity 4.05+0.54
−0.53
[6]   L
Temperature 6360+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
SIMBAD data

WASP-12 is a magnitude 11 yellow dwarf star located approximately 1347 light-years away [2] in the constellation Auriga. [4] 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. [7]

Contents

Planetary system

In 2008, the extrasolar planet WASP-12b was discovered orbiting WASP-12 by the transit method. [8] Its high carbon-to-oxygen ratio indicates that rocky planets might have formed in the star system, and it may be a carbon 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 except for WASP-12b. [6]

The WASP-12 planetary system
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b 1.41±0.1  MJ 0.0229±0.00081.091423±0.0000030.049±0.01586.0±3.0 [11] ° 1.736±0.092 [11]   RJ

See also

Related Research Articles

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<span class="mw-page-title-main">Kepler-7</span> G-type star located in the constellation Lyra

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<span class="mw-page-title-main">HD 15082</span> Star in the constellation Andromeda

HD 15082 is a star located roughly 397 light years away in the northern constellation of Andromeda. The star is a Delta Scuti variable and a planetary transit variable. A hot Jupiter type extrasolar planet, named WASP-33b or HD 15082b, orbits this star with an orbital period of 1.22 days. It is the first Delta Scuti variable known to host a planet.

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<span class="mw-page-title-main">Kepler-25</span> Yellow-white hued star in the constellation Lyra

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<span class="mw-page-title-main">K2-25</span>

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References

  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. 1 2 3 4 5 6 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.
  3. 1 2 Henden, 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. 1 2 3 "SIMBAD query result: WASP-12 -- Star". Centre de Données astronomiques de Strasbourg. Retrieved 2009-04-24.
  5. 1 2 3 Skrutskie, 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. 1 2 3 4 5 6 Collins, 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. 1 2 Staff (2015). "Planet WASP-12 b". Extrasolar Planets Encyclopaedia . Retrieved 4 August 2017.