A light curve for V807 Andromedae (HD 15082), plotted from TESS data.[1] The deep minima are caused by the planet transits. | |
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Andromeda |
Right ascension | 02h 26m 51.0583s[2] |
Declination | +37° 33′ 01.736″[2] |
Apparent magnitude (V) | 8.3[3] |
Characteristics | |
Spectral type | A5[4] |
B−V color index | 0.27[5] |
Variable type | δ Sct[3]+Planetary transit variable |
Astrometry | |
Radial velocity (Rv) | −9.20±2.8[6] km/s |
Proper motion (μ) | RA: −0.977(35) mas/yr[2] Dec.: −8.895(34) mas/yr[2] |
Parallax (π) | 8.2238 ± 0.0327 mas[2] |
Distance | 397 ± 2 ly (121.6 ± 0.5 pc) |
Details | |
Mass | 1.55 ± 0.04[7] M☉ |
Radius | 1.51[8] R☉ |
Surface gravity (log g) | 4.3 ± 0.2[3] cgs |
Temperature | 7,400 ± 200[3] K |
Metallicity [Fe/H] | 0.1 ± 0.2[7] dex |
Rotational velocity (v sin i) | 86[3] km/s |
Age | 100[9] Myr |
Other designations | |
Database references | |
SIMBAD | data |
HD 15082 (also known as WASP-33) is a star located roughly 397 light years away[2] in the northern constellation of Andromeda.[10] The star is a Delta Scuti variable[11] 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.[12]
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