WASP-11/HAT-P-10 Latitude and Longitude:
Sky map 03h 09m 28.55s, +30° 40′ 24.9″
From Wikipedia, the free encyclopedia
WASP-11/HAT-P-10
Observation data
Epoch J2000.0       Equinox J2000.0
Constellation Aries
Right ascension 03h 09m 28.5434s [1]
Declination +30° 40′ 24.863″ [1]
Apparent magnitude (V) 11.57 ± 0.15 [2]
Characteristics
Spectral type K3V [3]
Apparent magnitude (B) 12.58 ± 0.30 [2]
Apparent magnitude (V) 11.57 ± 0.15 [2]
Apparent magnitude (J) 10.015 ± 0.020 [4]
Apparent magnitude (H) 9.560 ± 0.019 [4]
Apparent magnitude (K) 9.421 ± 0.017 [4]
Variable type planetary transit [5]
Astrometry
Proper motion (μ) RA: 3.334(68)  mas/ yr [1]
Dec.: −44.433(53)  mas/ yr [1]
Parallax (π)7.6997 ± 0.0579  mas [1]
Distance424 ± 3  ly
(129.9 ± 1.0  pc)
Details [6]>
WASP-11 A
Mass0.77 ± 0.02 [7]  M☉
Radius0.74 ± 0.01 [7]  R☉
Luminosity0.28 ± 0.002 [7]  L☉
Surface gravity (log g)4.58 ± 0.02 [7]  cgs
Temperature4,884±16 [7]  K
Metallicity [Fe/H]0.25 ± 0.07 [8]  dex
Rotational velocity (v sin i)1.9 ± 0.9 [8] km/s
Age8.7 ± 3.5 [7]  Gyr
WASP-11 B
Mass0.34  M☉
Temperature3,494±37 [9]  K
Other designations
HAT-P-10, Gaia DR3 123376685084303360, WASP-11, TYC 2340-1714-1, GSC 02340-01714, 2MASS J03092855+3040249 [2]
Database references
SIMBAD data

WASP-11/HAT-P-10 is a binary star. It is a primary main-sequence orange dwarf star. Secondary is M-dwarf with a projected separation of 42  AU. [9] The system is located about 424 light-years away [1] in the constellation Aries. [2] [10]

Planetary system

A semi-Jovian planet, WASP-11b/HAT-P-10b (WASP-11 A b/HAT-P-10 A b), was detected around the primary star independently by the Hungarian Automated Telescope Network and the Wide Angle Search for Planets teams, both of which used the transit method. [3] [5]

The WASP-11/HAT-P-10 planetary system [11]
Companion
(in order from star) 		Mass Semimajor axis
( AU) 		Orbital period
( days) 		Eccentricity Inclination Radius
b 0.532+0.020
−0.021  MJ 		0.04376+0.00071
−0.00067 		3.7224793±0.0000007 <0.03 89.03±0.34 ° 0.990±0.022  RJ

See also

References

  1. ^ a b c d e 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.
  2. ^ a b c d e "SIMBAD query result: NAME HAT P-10 -- Star". Centre de Données astronomiques de Strasbourg. Retrieved 2009-05-05.
  3. ^ a b West, R. G.; et al. (2009). "The sub-Jupiter mass transiting exoplanet WASP-11b". Astronomy and Astrophysics. 502 (1): 395–400. arXiv: 0809.4597. Bibcode: 2009A&A...502..395W. doi: 10.1051/0004-6361/200810973. S2CID  18189916.
  4. ^ a b c 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
  5. ^ a b Bakos, G. Á.; et al. (2009). "HAT-P-10b: A Light and Moderately Hot Jupiter Transiting A K Dwarf". The Astrophysical Journal. 696 (2): 1950–1955. arXiv: 0809.4295. Bibcode: 2009ApJ...696.1950B. doi: 10.1088/0004-637X/696/2/1950. S2CID  12146075.
  6. ^ Quarles, Billy; Li, Gongjie; Kostov, Veselin; Haghighipour, Nader (2020), "Orbital Stability of Circumstellar Planets in Binary Systems", The Astronomical Journal, 159 (3): 80, arXiv: 1912.11019, Bibcode: 2020AJ....159...80Q, doi: 10.3847/1538-3881/ab64fa, S2CID  209444271
  7. ^ a b c d e f Bonfanti, A.; et al. (2015). "Revising the ages of planet-hosting stars". Astronomy and Astrophysics. 575 (18). A18. arXiv: 1411.4302. Bibcode: 2015A&A...575A..18B. doi: 10.1051/0004-6361/201424951. S2CID  54555839.
  8. ^ a b 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.
  9. ^ a b Piskorz, Danielle; Knutson, Heather A.; Ngo, Henry; Muirhead, Philip S.; Batygin, Konstantin; Crepp, Justin R.; Hinkley, Sasha; Morton, Timothy D. (2015), "Friends of Hot Jupiters. III. An Infrared Spectroscopic Search for Low-Mass Stellar Companions", The Astrophysical Journal, 814 (2): 148, arXiv: 1510.08062, Bibcode: 2015ApJ...814..148P, doi: 10.1088/0004-637X/814/2/148, S2CID  11525988
  10. ^ Mayor, M; Marmier, M; Lovis, C; Udry, S; Ségransan, D; Pepe, F; Benz, W; Bertaux, J. -L; Bouchy, F; Dumusque, X; Lo Curto, G; Mordasini, C; Queloz, D; Santos, N. C (2011). "The HARPS search for southern extra-solar planets XXXIV. Occurrence, mass distribution and orbital properties of super-Earths and Neptune-mass planets". arXiv: 1109.2497 [ astro-ph.EP].
  11. ^ Bonomo, A. S.; et al. (2017). "The GAPS Programme with HARPS-N at TNG. XIV. Investigating giant planet migration history via improved eccentricity and mass determination for 231 transiting planets". Astronomy and Astrophysics. 602. A107. arXiv: 1704.00373. Bibcode: 2017A&A...602A.107B. doi: 10.1051/0004-6361/201629882. S2CID  118923163.

External links



Stub icon

This main-sequence-star-related article is a stub. You can help Wikipedia by expanding it.

Retrieved from " https://en.wikipedia.org/?title=WASP-11/HAT-P-10&oldid=1187069936"