WASP-19

Last updated
WASP-19 / Wattle
Observation data
Epoch J2000.0       Equinox J2000.0
Constellation Vela [1]
Right ascension 09h 53m 40.07656s [2]
Declination −45° 39 33.0572 [2]
Apparent magnitude  (V)12.312 ± 0.017 [3]
Characteristics
Spectral type G8V [4]
Apparent magnitude  (B)13.05 [5]
Apparent magnitude  (R)12.12 [5]
Apparent magnitude  (I)11.35 [5]
Apparent magnitude  (J)10.911 ± 0.026 [6]
Apparent magnitude  (H)10.602 ± 0.022 [6]
Apparent magnitude  (K)10.481 ± 0.023 [6]
B−V color index 1.3[ citation needed ]
V−R color index 0.1[ citation needed ]
R−I color index 0.82[ citation needed ]
Variable type planetary transit
Astrometry
Radial velocity (Rv)21.41±0.95 [2] km/s
Proper motion (μ)RA: −35.457 mas/yr [2]
Dec.: 17.378 mas/yr [2]
Parallax (π)3.7516±0.0090  mas [2]
Distance 869 ± 2  ly
(266.6 ± 0.6  pc)
Absolute magnitude  (MV)5.3[ citation needed ]
Details [7]
Mass 0.965+0.091
−0.095
  M
Radius 1.006+0.031
−0.034
  R
Luminosity 0.905+0.071
−0.069
  L
Surface gravity (log g)4.417+0.020
−0.021
  cgs
Temperature 5616+66
−65
  K
Metallicity [Fe/H]0.04+0.25
−0.30
  dex
Rotation 11.76±0.09 d [8]
Rotational velocity (v sin i)4.0 ± 1.0 [9]  km/s
Age 6.4+4.1
−3.5
  Gyr
Other designations
Wattle, TOI-655, TIC 35516889, WASP-19, GSC 08181-01711, 2MASS J09534008-4539330, USNO-B1.0 0443-00193111 [5]
Database references
SIMBAD data
Exoplanet Archive data

WASP-19, formally named Wattle, [10] is a magnitude 12.3 star about 869 light-years (266 parsecs ) away, located in the Vela constellation of the southern hemisphere. [4] This star has been found to host a transiting hot Jupiter-type planet in a tight orbit.

Contents

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. [8]

Nomenclature

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

In August 2022, this planetary system was included among 20 systems to be named by the third NameExoWorlds project. [11] The approved names were proposed by a team from Brandon Park Primary School in Wheelers Hill (Melbourne, Australia), led by scientist Lance Kelly and teacher David Maierhofer [12] and announced in June 2023. WASP-19 is named "Wattle" and its planet is named "Banksia", after the plant genera Wattle (specifically the golden wattle Acacia pycnantha ) and Banksia (specifically the scarlet banksia Banksia coccinea ) respectively. [10]

Planetary system

In December 2009, the SuperWASP project announced that a hot Jupiter type exoplanet, WASP-19b, was orbiting very close to this star and with the shortest orbital period of any transiting exoplanet known at the time. [4]

The WASP-19 planetary system [7]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b / Banksia 1.154+0.078
−0.080
  MJ
0.01652+0.00050
−0.00056
0.78883852(82)0.0126+0.014
−0.0089
79.08+0.34
−0.37
°
1.415+0.044
−0.048
  RJ

References

  1. Roman, Nancy G. (1987). "Identification of a constellation from a position". Publications of the Astronomical Society of the Pacific . 99 (617): 695. Bibcode:1987PASP...99..695R. doi: 10.1086/132034 . Constellation record for this object at VizieR.
  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. 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. 1 2 3 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.
  5. 1 2 3 4 "WASP-19". SIMBAD . Centre de données astronomiques de Strasbourg.
  6. 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
  7. 1 2 Cortés-Zuleta, Pía; Rojo, Patricio; et al. (April 2020). "TraMoS. V. Updated ephemeris and multi-epoch monitoring of the hot Jupiters WASP-18Ab, WASP-19b, and WASP-77Ab". Astronomy & Astrophysics . 636: A98. arXiv: 2001.11112 . Bibcode:2020A&A...636A..98C. doi:10.1051/0004-6361/201936279. S2CID   241596186.
  8. 1 2 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 , Bibcode:2015A&A...577A..90M, doi:10.1051/0004-6361/201525774, S2CID   53324330
  9. 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.
  10. 1 2 "2022 Approved Names". nameexoworlds.iau.org. IAU . Retrieved 7 June 2023.
  11. "List of ExoWorlds 2022". nameexoworlds.iau.org. IAU. 8 August 2022. Retrieved 27 August 2022.
  12. "Facebook". www.facebook.com.

Further reading