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WASP-64

Coordinates:Sky map02h 44m 09.6098s, −32° 51′ 30.1787″
From Wikipedia, the free encyclopedia
Star in the constellation Canis Major
WASP-64 / Atakoraka
Observation data
Epoch J2000.0      Equinox J2000.0
ConstellationCanis Major
Right ascension06h 44m 27.6052s[1]
Declination−32° 51′ 30.1787″[1]
Apparent magnitude (V)12.29[2]
Characteristics
Evolutionary stagemain-sequence star
Spectral typeG7[2]
Apparent magnitude (J)11.368[1]
Apparent magnitude (G)12.5257[1]
Apparent magnitude (H)11.079[1]
Astrometry
Radial velocity (Rv)35.48 km/s
Proper motion (μ)RA: -19.389[3]mas/yr
Dec.: -1.123[3]mas/yr
Parallax (π)2.6745±0.0218 mas[3]
Distance1,220 ± 10 ly
(374 ± 3 pc)
Details[4]
Mass0.993+0.034
−0.037
 M
Radius1.036+0.046
−0.065
 R
Luminosity0.90±0.15 L
Temperature5400±100[2] K
Metallicity [Fe/H]-0.08±0.11 dex
Rotation15.8±3.7d[5]
Age3.554±1.629[5] Gyr
Other designations
Atakoraka,Gaia DR2 5583523425437258240,GSC 07091-01514,2MASS J06442760-3251302[1]
Database references
SIMBADdata

WASP-64 is a star about 1200 light-years away. It is a G7 classmain-sequence star, orbited by a planet WASP-64b. It is younger than the Sun at 3.6±1.6 billion years,[5] and it has a metal abundance similar to the Sun.[2] The star is rotating rapidly, being spun up by the giant planet in a close orbit.[5]

WASP-64 was namedAtakoraka in 2019 after theAtacora, the largest mountain range inTogo.[6] An imaging survey in 2017 failed to find any stellar companions.[7]

Planetary system

[edit]

Atransitinghot Jupiterexoplanet orbiting WASP-64 was discovered byWASP in 2012.[4] The planetary equilibrium temperature is 1672+59
−63
K,[4] while the measured dayside temperature is hotter at 1989+87
−88
K.[8] Due to the close proximity of the planet to the parent star, orbital decay of WASP-64b, along withHATS-2, may be detectable in the near future.[9] WASP-64b was namedAgouto (afterMount Agou, the highest point of Togo which lies within the Atacora chain) in 2019 by amateur astronomers fromTogo as part of theNameExoWorlds contest.[6]

The WASP-64 planetary system[8]
Companion
(in order from star)
MassSemimajor axis
(AU)
Orbital period
(days)
EccentricityInclinationRadius
b / Agouto0.0272±0.00121.573253+0.000028
−0.000027
089.6±3.2°1.244±0.036 RJ

References

[edit]
  1. ^abcdef"WASP-64".SIMBAD.Centre de données astronomiques de Strasbourg.
  2. ^abcdWASP-64 The planetary system WASP-64 hosts at least one planet
  3. ^abcBrown, 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 atVizieR.
  4. ^abcGillon, M.; Anderson, D. R.; Collier-Cameron, A.; Doyle, A. P.; Fumel, A.; Hellier, C.; Jehin, E.; Lendl, M.; Maxted, P. F. L.; Montalban, J.; Pepe, F.; Pollacco, D.; Queloz, D.; Segransan, D.; Smith, A. M. S.; Smalley, B.; Southworth, J.; Triaud, A. H. M. J.; Udry, S.; West, R. G. (2012), "WASP-64b and WASP-72b: two new transiting highly irradiated giant planets",Astronomy & Astrophysics,552: A82,arXiv:1210.4257,Bibcode:2013A&A...552A..82G,doi:10.1051/0004-6361/201220561,S2CID 53687206
  5. ^abcdGallet, F.; Gallet (2020), "TATOO: Tidal-chronology standalone tool to estimate the age of massive close-in planetary systems",Astronomy & Astrophysics,641: A38,arXiv:2006.07880,Bibcode:2020A&A...641A..38G,doi:10.1051/0004-6361/202038058,S2CID 219687851
  6. ^ab"Togo Approved Names".Name Exoworlds.International Astronomical Union. Retrieved2020-11-12.
  7. ^Evans, D. F.; Southworth, J.; Smalley, B.; Jørgensen, U. G.; Dominik, M.; Andersen, M. I.; Bozza, V.; Bramich, D. M.; Burgdorf, M. J.; Ciceri, S.; d'Ago, G.; Figuera Jaimes, R.; Gu, S.-H.; Hinse, T. C.; Henning, Th.; Hundertmark, M.; Kains, N.; Kerins, E.; Korhonen, H.; Kokotanekova, R.; Kuffmeier, M.; Longa-Peña, P.; Mancini, L.; MacKenzie, J.; Popovas, A.; Rabus, M.; Rahvar, S.; Sajadian, S.; Snodgrass, C.; et al. (2018), "High-resolution Imaging of Transiting Extrasolar Planetary systems (HITEP). II. Lucky Imaging results from 2015 and 2016",Astronomy & Astrophysics,610: A20,arXiv:1709.07476,Bibcode:2018A&A...610A..20E,doi:10.1051/0004-6361/201731855,S2CID 53400492
  8. ^abWong, Ian; Shporer, Avi; Daylan, Tansu; Benneke, Björn; Fetherolf, Tara; Kane, Stephen R.; Ricker, George R.; Vanderspek, Roland; Latham, David W.; Winn, Joshua N.; Jenkins, Jon M.; Boyd, Patricia T.; Glidden, Ana; Goeke, Robert F.; Sha, Lizhou; Ting, Eric B.; Yahalomi, Daniel (2020), "Systematic phase curve study of known transiting systems from year one of the TESS mission",The Astronomical Journal,160 (4): 155,arXiv:2003.06407,Bibcode:2020AJ....160..155W,doi:10.3847/1538-3881/ababad,S2CID 212717799
  9. ^Southworth, John; Dominik, M.; Jørgensen, U. G.; Andersen, M. I.; Bozza, V.; Burgdorf, M. J.; d'Ago, G.; Dib, S.; Figuera Jaimes, R.; Fujii, Y. I.; Gill, S.; Haikala, L. K.; Hinse, T. C.; Hundertmark, M.; Khalouei, E.; Korhonen, H.; Longa-Peña, P.; Mancini, L.; Peixinho, N.; Rabus, M.; Rahvar, S.; Sajadian, S.; Skottfelt, J.; Snodgrass, C.; Spyratos, P.; Tregloan-Reed, J.; Unda-Sanzana, E.; von Essen, C. (2019), "Transit timing variations in the WASP-4 planetary system",Monthly Notices of the Royal Astronomical Society,490 (3):4230–4236,arXiv:1907.08269,doi:10.1093/mnras/stz2602,S2CID 197935338
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