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WASP-19 is a magnitude 12.3 star located in the Vela constellation of the southern hemisphere.[8] This star has been found to host a transiting hot Jupiter-type planet in tight orbit.

WASP-19
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Vela[1]
Right ascension 09h 53m 40.0765s[2]
Declination −45° 39′ 33.056″[2]
Apparent magnitude (V) 12.312 ± 0.017[3]
Characteristics
Spectral type G8V
Apparent magnitude (B) 13.58
Apparent magnitude (R) 12.17
Apparent magnitude (I) 11.35
Apparent magnitude (J) 10.911 ± 0.026[4]
Apparent magnitude (H) 10.602 ± 0.022[4]
Apparent magnitude (K) 10.481 ± 0.023[4]
B−V color index 1.3
V−R color index 0.1
R−I color index 0.82
Variable type planetary transit
Astrometry
Proper motion (μ) RA: −35.407±0.041[2] mas/yr
Dec.: 17.288±0.040[2] mas/yr
Parallax (π)3.6981 ± 0.0236 mas[2]
Distance882 ± 6 ly
(270 ± 2 pc)
Absolute magnitude (MV)5.3
Details[5]
Mass0.97±0.02[6] M☉
Radius0.885+0.086
−0.084 R☉
Luminosity0.71 L☉
Surface gravity (log g)4.45 ± 0.05[7] cgs
Temperature5568 ± 71[7] K
Metallicity [Fe/H]0.15 ± 0.07[7] dex
Rotation11.76±0.09 d
Rotational velocity (v sin i)4.0 ± 1.0[7] km/s
Age9.95±2.49 Gyr
Other designations
GSC 08181-01711, USNO-B1.0 0443-00193111, 2MASS J09534008-4539330, Gaia DR2 5411736896952029568
Database references
SIMBADdata
Extrasolar Planets
Encyclopaedia		data

The WASP-19 is older than Sun, has fraction of heavy elements above solar abundance, and is rotating rapidly, being spun up by the tides raised by the giant planet on the close orbit.[5]


Planetary system


In December 2009 SuperWASP project announced that a hot Jupiter type extrasolar planet, WASP-19b, was orbiting very close to this star and with the shortest orbital period so far detected.[8]

In August 2022, this planetary system was included among 20 systems to be named by the third NameExoWorlds project.[9]

The WASP-19 planetary system[10][6]
Companion
(in order from star)		 Mass Semimajor axis
(AU)		 Orbital period
(days)		 Eccentricity Inclination Radius
b 1.168±0.023 MJ 0.01634 ± 0.00019 0.7888396 ± 0.00000010 0 78.76 ± 0.13° 1.18±0.12 RJ

See also



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. Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
  3. Maxted, P. F. L.; et al. (2011). "UBV(RI)C photometry of transiting planet hosting stars". Monthly Notices of the Royal Astronomical Society. 418 (2): 1039–1042. arXiv:1108.0349. Bibcode:2011MNRAS.418.1039M. doi:10.1111/j.1365-2966.2011.19554.x. S2CID 117056033.
  4. 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: 1163–1183. doi:10.1086/498708. ISSN 0004-6256. Vizier catalog entry
  5. Maxted, P. F. L.; Serenelli, A. M.; Southworth, J. (2015), "A comparison of gyrochronological and isochronal age estimates for transiting exoplanet host stars", Astronomy & Astrophysics, 577: A90, arXiv:1503.09111, doi:10.1051/0004-6361/201525774, S2CID 53324330
  6. Dragomir, Diana; Kane, Stephen R.; Pilyavsky, Genady; Mahadevan, Suvrath; Ciardi, David R.; Zachary Gazak, J.; Gelino, Dawn M.; Payne, Alan; Rabus, Markus; Ramirez, Solange V.; von Braun, Kaspar; Wright, Jason T.; Wyatt, Pamela (2011). "Terms Photometry of Known Transiting Exoplanets". The Astronomical Journal. 142 (4): 115. arXiv:1108.2308. Bibcode:2011AJ....142..115D. doi:10.1088/0004-6256/142/4/115. S2CID 118606598.
  7. Torres, Guillermo; et al. (2012). "Improved Spectroscopic Parameters for Transiting Planet Hosts". The Astrophysical Journal. 757 (2). 161. arXiv:1208.1268. Bibcode:2012ApJ...757..161T. doi:10.1088/0004-637X/757/2/161. S2CID 16580774.
  8. Hebb, L.; et al. (2010). "WASP-19b: The Shortest Period Transiting Exoplanet Yet Discovered". The Astrophysical Journal. 708 (1): 224–231. arXiv:1001.0403. Bibcode:2010ApJ...708..224H. doi:10.1088/0004-637X/708/1/224. S2CID 119189785.
  9. "List of ExoWorlds 2022". nameexoworlds.iau.org. IAU. 8 August 2022. Retrieved 27 August 2022.
  10. Mancini, L.; et al. (2013). "Physical properties, transmission and emission spectra of the WASP-19 planetary system from multi-colour photometry". Monthly Notices of the Royal Astronomical Society. 436 (1): 2–18. arXiv:1306.6384. Bibcode:2013MNRAS.436....2M. doi:10.1093/mnras/stt1394. S2CID 55455709.

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На других языках

- [en] WASP-19

[ru] WASP-19

WASP-19 — звезда в созвездии Парусов на расстоянии около 815 световых лет от Солнца. Вокруг звезды обращается, как минимум, одна планета.


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