Astronomy:WASP-64
| Observation data Equinox J2000.0]] (ICRS) | |
|---|---|
| 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 |
| Distance | 1,220 ± 10 ly (374 ± 3 pc) |
| Details[4] | |
| Mass | 0.993+0.034−0.037 M☉ |
| Radius | 1.036+0.046−0.065 R☉ |
| Luminosity | 0.90±0.15 L☉ |
| Temperature | 5400±100[2] K |
| Metallicity [Fe/H] | -0.08±0.11 dex |
| Rotation | 15.8±3.7 d[5] |
| Age | 3.554±1.629[5] Gyr |
| Other designations | |
| Database references | |
| SIMBAD | data |
WASP-64 is a star about 1200 light-years away. It is a G7 class main-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 named Atakoraka in 2019 after the Atacora, the largest mountain range in Togo.[6] An imaging survey in 2017 failed to find any stellar companions.[7]
Planetary system
A 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 (after Mount Agou, the highest point of Togo which lies within the Atacora chain) in 2019 by amateur astronomers from Togo as part of the NameExoWorlds contest.[6]
| Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
|---|---|---|---|---|---|---|
| b / Agouto | — | 0.0272±0.0012 | 1.573253+0.000028−0.000027 | 0 | 89.6±3.2° | 1.244±0.036 RJ |
References
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 "WASP-64". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=WASP-64.
- ↑ 2.0 2.1 2.2 2.3 WASP-64 The planetary system WASP-64 hosts at least one planet
- ↑ 3.0 3.1 3.2 Brown, A. G. A. (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics 616: A1. doi:10.1051/0004-6361/201833051. Bibcode: 2018A&A...616A...1G. Gaia DR2 record for this source at VizieR.
- ↑ 4.0 4.1 4.2 Gillon, M.; Anderson, D. R.; Collier-Cameron, A.; Doyle, A. P.; Fumel, A.; Hellier, C.; Jehin, E.; Lendl, M. et al. (2012), "WASP-64b and WASP-72b: two new transiting highly irradiated giant planets", Astronomy & Astrophysics 552: A82, doi:10.1051/0004-6361/201220561, Bibcode: 2013A&A...552A..82G
- ↑ 5.0 5.1 5.2 5.3 Gallet, F.; Gallet (2020), "TATOO: Tidal-chronology standalone tool to estimate the age of massive close-in planetary systems", Astronomy & Astrophysics 641: A38, doi:10.1051/0004-6361/202038058, Bibcode: 2020A&A...641A..38G
- ↑ 6.0 6.1 "Togo Approved Names" (in en). International Astronomical Union. http://www.nameexoworlds.iau.org/togo.
- ↑ Evans, D. F.; Southworth, J.; Smalley, B.; Jørgensen, U. G.; Dominik, M.; Andersen, M. I.; Bozza, V.; Bramich, D. M. et al. (2018), "High-resolution Imaging of Transiting Extrasolar Planetary systems (HITEP). II. Lucky Imaging results from 2015 and 2016", Astronomy & Astrophysics 610: A20, doi:10.1051/0004-6361/201731855, Bibcode: 2018A&A...610A..20E
- ↑ 8.0 8.1 Wong, Ian; Shporer, Avi; Daylan, Tansu; Benneke, Björn; Fetherolf, Tara; Kane, Stephen R.; Ricker, George R.; Vanderspek, Roland et al. (2020), "Systematic phase curve study of known transiting systems from year one of the TESS mission", The Astronomical Journal 160 (4): 155, doi:10.3847/1538-3881/ababad, Bibcode: 2020AJ....160..155W
- ↑ Southworth, John; Dominik, M.; Jørgensen, U. G.; Andersen, M. I.; Bozza, V.; Burgdorf, M. J.; d'Ago, G.; Dib, S. et al. (2019), "Transit timing variations in the WASP-4 planetary system", Monthly Notices of the Royal Astronomical Society 490 (3): 4230–4236, doi:10.1093/mnras/stz2602
Coordinates: 
02h 44m 09.6098s, −32° 51′ 30.1787″
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