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WASP-19

Coordinates:Sky map09h 53m 40.07s, −45° 39′ 33.06″
From Wikipedia, the free encyclopedia
Star in the constellation Vela
WASP-19 / Wattle
Observation data
Epoch J2000.0      Equinox J2000.0
ConstellationVela[1]
Right ascension09h 53m 40.07656s[2]
Declination−45° 39′ 33.0572″[2]
Apparent magnitude (V)12.312 ± 0.017[3]
Characteristics
Spectral typeG8V
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−Vcolor index1.3
V−Rcolor index0.1
R−Icolor index0.82
Variable typeplanetary transit
Astrometry
Radial velocity (Rv)21.41±0.95[2] km/s
Proper motion (μ)RA: −35.457mas/yr[2]
Dec.: 17.378mas/yr[2]
Parallax (π)3.7516±0.0090 mas[2]
Distance869 ± 2 ly
(266.6 ± 0.6 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±0.09d
Rotational velocity (v sin i)4.0 ± 1.0[7] km/s
Age9.95±2.49 Gyr
Other designations
Wattle,TOI-655,WASP-19,GSC 08181-01711,2MASS J09534008-4539330,USNO-B1.0 0443-00193111
Database references
SIMBADdata

WASP-19, formally namedWattle,[8] is amagnitude 12.3star about 869light-years (266parsecs) away, located in theVelaconstellation of thesouthern hemisphere.[9] This star has been found to host a transitinghot Jupiter-type planet in tight orbit.

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

Nomenclature

[edit]

The designationWASP-19 indicates that this was the 19th star found to have a planet by theWide Angle Search for Planets.

In August 2022, this planetary system was included among 20 systems to be named by the thirdNameExoWorlds project.[10] The approved names were proposed by a team from Brandon Park Primary School inWheelers Hill (Melbourne,Australia), led by scientist Lance Kelly and teacher David Maierhofer[11] and announced in June 2023. WASP-19 is named "Wattle" and its planet is named "Banksia", after the plant generaWattle (specifically the golden wattleAcacia pycnantha) andBanksia (specifically the scarlet banksiaBanksia coccinea) respectively.[8]

Planetary system

[edit]

In December 2009, theSuperWASP project announced that ahot Jupiter typeexoplanet,WASP-19b, was orbiting very close to this star and with the shortest orbital period of any transiting exoplanet known at the time.[9]

The WASP-19 planetary system[12][6]
Companion
(in order from star)
MassSemimajor axis
(AU)
Orbital period
(days)
EccentricityInclinationRadius
b / Banksia1.168±0.023 MJ0.01634 ± 0.000190.7888396 ± 0.00000010078.76 ± 0.13°1.18±0.12 RJ

See also

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References

[edit]
  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. ^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. ^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
  5. ^abMaxted, 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,Bibcode:2015A&A...577A..90M,doi:10.1051/0004-6361/201525774,S2CID 53324330
  6. ^abDragomir, 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. ^abcdTorres, 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. ^ab"2022 Approved Names".nameexoworlds.iau.org.IAU. Retrieved7 June 2023.
  9. ^abHebb, 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.
  10. ^"List of ExoWorlds 2022".nameexoworlds.iau.org.IAU. 8 August 2022. Retrieved27 August 2022.
  11. ^"Facebook".www.facebook.com.
  12. ^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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