Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Perseus |
Right ascension | 02h 43m 02.83826s[1] |
Declination | +55° 06′ 21.6700″[1] |
Apparent magnitude (V) | 5.76[2] |
Characteristics | |
Evolutionary stage | main sequence[3] |
Spectral type | B7 III(p?) (Hg?)[4] |
B−V color index | −0.110±0.003[2] |
Astrometry | |
Radial velocity (Rv) | −0.7±1.0[2] km/s |
Proper motion (μ) | RA: +34.859[1] mas/yr Dec.: −21.955[1] mas/yr |
Parallax (π) | 7.8022 ± 0.0874 mas[1] |
Distance | 418 ± 5 ly (128 ± 1 pc) |
Absolute magnitude (MV) | 0.16[2] |
Details | |
Mass | 3.77±0.06[3] M☉ |
Radius | 3.2[5] R☉ |
Luminosity | 210.4+21.9 −19.9[3] L☉ |
Surface gravity (log g) | 4.19[6] cgs |
Temperature | 14,550[6] K |
Metallicity [Fe/H] | +0.09[6] dex |
Rotation | 25–70 d[7] |
Rotational velocity (v sin i) | 4.50[8] km/s |
Age | 50.9±12.2[9] Myr |
Other designations | |
Database references | |
SIMBAD | data |
11 Persei is a single[11][8] star in the constellation of Perseus, located about 418 light years away from the Sun. It is visible to the naked eye as a dim, blue-white hued star with an apparent visual magnitude of 5.76.[2]
This is a chemically peculiar mercury-manganese star.[12][6] Cowley (1972) found a stellar classification of B7 III(p?) (Hg?),[4] while Hube (1970) had B8 IV,[13] and Appenzeller (1967) showed B6 V.[14] Stellar models indicate this is a young B-type main sequence star[3] with an estimated age of around 51[9] million years. It has a low rotation rate, showing a projected rotational velocity of 4.50 km/s.[8] The star has 3.8[3] times the mass of the Sun and is radiating 210[3] times the Sun's luminosity from its photosphere at an effective temperature of 14,550 K.[6]
GaiaDR2
was invoked but never defined (see the help page).Anderson2012
was invoked but never defined (see the help page).zorec2012
was invoked but never defined (see the help page).Cowley1972
was invoked but never defined (see the help page).PasinettiFracassini2001
was invoked but never defined (see the help page).Ghazaryan2016
was invoked but never defined (see the help page).Wahlgren2012
was invoked but never defined (see the help page).Hubrig2001
was invoked but never defined (see the help page).Tetzlaff2011
was invoked but never defined (see the help page).Simbad
was invoked but never defined (see the help page).Eggleton2008
was invoked but never defined (see the help page).Adelman2010
was invoked but never defined (see the help page).Hube1970
was invoked but never defined (see the help page).Appenzeller1967
was invoked but never defined (see the help page).