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Star in the constellation Mensa From Wikipedia, the free encyclopedia
HD 35184 is a solitary star in the southern circumpolar constellation Mensa. It has an apparent magnitude of 6.50, which the maximum naked eye visibility. Located 375 light years away, it is receding with a heliocentric radial velocity of 13.6 km/s.
Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Mensa |
Right ascension | 05h 15m 24.8374s[1] |
Declination | −73° 35′ 18.5123″[1] |
Apparent magnitude (V) | 6.50±0.01[2] |
Characteristics | |
Spectral type | A6 V[3] |
B−V color index | +0.15[4] |
Astrometry | |
Radial velocity (Rv) | 13.6±0.6[5] km/s |
Proper motion (μ) | RA: −22.228 mas/yr[1] Dec.: +5.616 mas/yr[1] |
Parallax (π) | 8.7050 ± 0.0209 mas[1] |
Distance | 374.7 ± 0.9 ly (114.9 ± 0.3 pc) |
Absolute magnitude (MV) | +1.26[4] |
Details | |
Mass | 2.15±0.04[6] M☉ |
Radius | 2.8±0.1[7] R☉ |
Luminosity | 24.5[8] L☉ |
Surface gravity (log g) | 3.82+0.09 −0.07[7] cgs |
Temperature | 8,034[8] K |
Metallicity [Fe/H] | −0.01[9] dex |
Rotational velocity (v sin i) | 92.4±2.9[10] km/s |
Age | 674[9] Myr |
Other designations | |
Database references | |
SIMBAD | data |
HD 35184 has a stellar classification of A6 V, indicating that it is an ordinary A-type main-sequence star. At present it has 2.15 times the mass of the Sun[6] and 2.8 times the radius of the Sun.[7] It shines at 24.5 L☉ from its photosphere at an effective temperature of 8,034 K,[8] giving it a white hue. HD 35184 is 674 million years old – 79.6% through its main sequence lifetime[6] – and spins with a projected rotational velocity of 92 km/s−1.[10]
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