Location of HAT-P-36 (circled) within Canes Venatici | |
Observation data Epoch J2000.0 Equinox J2000.0 | |
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Constellation | Canes Venatici[1] |
Right ascension | 12h 33m 03.9061s[2] |
Declination | +44° 54′ 55.196″[2] |
Apparent magnitude (V) | 12.26 |
Characteristics | |
Spectral type | G |
Astrometry | |
Radial velocity (Rv) | −16.434 km/s |
Proper motion (μ) | RA: −11.622(8) mas/yr[2] Dec.: 8.138(10) mas/yr[2] |
Parallax (π) | 3.4055 ± 0.0110 mas[2] |
Distance | 958 ± 3 ly (293.6 ± 0.9 pc) |
Details | |
Mass | 1.022 ± 0.049 M☉ |
Radius | 1.096 ± 0.056 R☉ |
Temperature | 5580 ± 100.0 K |
Metallicity [Fe/H] | 0.26 ± 0.08 dex |
Age | 6.6 ± 1.8 Gyr |
Other designations | |
Database references | |
SIMBAD | data |
HAT-P-36, also referred to as Tuiren[4] is a 12th magnitude G-type main-sequence star estimated to be approximately 958 light-years away from Earth[2] in the constellation Canes Venatici. HAT-P-36 is too faint to be seen with the naked eye, but it is possible to view it with binoculars or a small telescope. In 2012 a hot Jupiter-type exoplanet was discovered orbiting HAT-P-36 with an orbital period of about 1.3 Earth days.[5] In December 2019, HAT-P-36 was named Tuiren and its planetary companion, HAT-P-36b, was named Bran as a result of Ireland's contribution to the 2019 NameExoWorlds campaign.[6] Bran has a mass approximately 1.8 times that of Jupiter and a radius 1.2 times larger.
Roman1987
was invoked but never defined (see the help page).Gaia DR3
was invoked but never defined (see the help page).Simbad
was invoked but never defined (see the help page).