Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Perseus |
Right ascension | 03h 32m 08.60842s[1] |
Declination | +48° 01′ 24.5285″[1] |
Apparent magnitude (V) | 5.45 - 5.53[2] |
Characteristics | |
Spectral type | B8 III[3] |
U−B color index | −0.61[3] |
B−V color index | −0.17[3] |
Variable type | SX Arietis[2] |
Astrometry | |
Radial velocity (Rv) | 2.6±0.9[4] km/s |
Proper motion (μ) | RA: 18.314±0.149[1] mas/yr Dec.: −28.723±0.144[1] mas/yr |
Parallax (π) | 5.6378 ± 0.1539 mas[1] |
Distance | 580 ± 20 ly (177 ± 5 pc) |
Absolute magnitude (MV) | −0.982[5] |
Details | |
Mass | 6.46[5] M☉ |
Radius | 3.55[5] R☉ |
Luminosity | 708[5] L☉ |
Surface gravity (log g) | 4.15[5] cgs |
Temperature | 16,000[5] K |
Metallicity [Fe/H] | +0.92[6] dex |
Rotation | 2.49246±0.00035 d[7] |
Rotational velocity (v sin i) | 35[8] km/s |
Age | 12±6[9] Myr |
Other designations | |
Database references | |
SIMBAD | data |
HD 21699, also known as HR 1063 and V396 Persei, is a star about 580 light years from the Earth, in the constellation Perseus.[1] It is a 5th magnitude star, so it will be faintly visible to the naked eye of an observer far from city lights. This is a variable star, whose brightness varies slightly from 5.45 to 5.53 during its 2.4761 day rotation period.[2] It has a remarkable dipole magnetic field which is displaced from the star's center by 0.4 stellar radii, the poles of which appear close to each other on the stellar surface.[11] HD 21699 is a member of the Alpha Persei Cluster.[12]
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