WASP-64

WASP-64 is a single star about 1200 light-years away. It is a G7 class main-sequence star, orbited by a planet WASP-64b. The age of WASP-64 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
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Canis Major
Right ascension 06h 44m 27.6052s[1]
Declination −32° 51 30.1787[1]
Apparent magnitude (V) 12.29[2]
Characteristics
Evolutionary stage main-sequence star
Spectral type G7[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[3] mas
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±3.7 d[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 was named Atakoraka in 2019.[6] An imaging survey in 2017 has failed to find any stellar companions to WASP-64.[7]

Planetary system

The transiting hot Jupiter exoplanet orbiting WASP-64 was discovered by WASP 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 with HATS-2, may be detectable in the near future.[9]

WASP-64b was named "Agouto" in 2019 by amateur astronomers from Togo as part of the NameExoWorlds contest.[6]

The WASP-64 planetary system[8]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b 0.0272±0.0012 1.573253+0.000028
0.000027
0 89.6±3.2° 1.244±0.036 RJ

References

  1. "WASP-64". SIMBAD. Centre de données astronomiques de Strasbourg.
  2. WASP-64 The planetary system WASP-64 hosts at least one planet
  3. 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.
  4. Gillon, 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, arXiv:1210.4257, doi:10.1051/0004-6361/201220561, S2CID 53687206
  5. Gallet, 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, doi:10.1051/0004-6361/202038058, S2CID 219687851
  6. "Togo Approved Names". Name Exoworlds. International Astronomical Union. Retrieved 2020-11-12.
  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, doi:10.1051/0004-6361/201731855, S2CID 53400492
  8. Wong, 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, 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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