HD 15082

HD 15082

A light curve for V807 Andromedae (HD 15082), plotted from TESS data. The deep minima are caused by the planet transits.
Observation data
Epoch J2000      Equinox J2000
Constellation Andromeda
Right ascension 02h 26m 51.0583s
Declination +37° 33′ 01.736″
Apparent magnitude (V) 8.3
Characteristics
Evolutionary stage main sequence
Spectral type kA5hA8mF4
B−V color index 0.27
Variable type δ Sct+planetary transit
Astrometry
Radial velocity (Rv)−2.70±0.33 km/s
Proper motion (μ) RA: −0.977(35) mas/yr
Dec.: −8.895(34) mas/yr
Parallax (π)8.2238±0.0327 mas
Distance397 ± 2 ly
(121.6 ± 0.5 pc)
Absolute magnitude (MV)+2.85
Details
Mass1.495±0.031 M
Radius1.444±0.034 R
Luminosity6.6 L
Surface gravity (log g)4.3±0.2 cgs
Temperature7,430±100 K
Metallicity [Fe/H]0.1±0.2 dex
Rotational velocity (v sin i)86 km/s
Age100 Myr
Other designations
V807 And, BD+36 489, HD 15082, HIP 11397, SAO 55561, TOI-1599, TIC 129979528, WASP-33, 2MASS J02265106+3733017
Database references
SIMBADdata
Exoplanet Archivedata

HD 15082 (also known as WASP-33) is a star located 397 light years away in the northern constellation of Andromeda. The star is a Delta Scuti variable and a planetary transit variable. A hot Jupiter type extrasolar planet, named WASP-33b or HD 15082b, orbits this star with an orbital period of 1.22 days. It is the first Delta Scuti variable known to host a planet.