HD 83446

HD 83446
Observation data
Epoch J2000      Equinox J2000
Constellation Vela
Right ascension 09h 36m 49.53851s
Declination −49° 21 18.0873
Apparent magnitude (V) 4.34
Characteristics
Evolutionary stage main sequence
Spectral type A7 V
B−V color index 0.173±0.005
Variable type δ Sct
Astrometry
Radial velocity (Rv)+17.8±0.5 km/s
Proper motion (μ) RA: −130.55 mas/yr
Dec.: +42.98 mas/yr
Parallax (π)30.4562±0.1933 mas
Distance107.1 ± 0.7 ly
(32.8 ± 0.2 pc)
Absolute magnitude (MV)1.79
Details
Mass1.8+0.11
−0.09
 M
Luminosity15.99 L
Surface gravity (log g)4.3±0.14 cgs
Temperature8,331±283 K
Rotational velocity (v sin i)155 km/s
Age453+256
−278
 Myr
Other designations
M Vel, CD−48°4836, FK5 2768, HD 83446, HIP 47175, HR 3836, SAO 221344
Database references
SIMBADdata

HD 83446 is a probable astrometric binary star system in the constellation Vela. It is visible to the naked eye with an apparent visual magnitude of 4.34. Based upon an annual parallax shift of 30.5 mas, it is located 107.1 light years from the Sun. The system is moving further away with a heliocentric radial velocity of +18 km/s.

The visible component is an A-type main-sequence star with a stellar classification of A7 V. Observations with the BRITE constellation led to this star's identification as a Delta Scuti variable with pulsation frequencies of 31.0806 and 34.2098 cycles per day, corresponding to periods of 46.3 and 42.1 minutes, respectively. It has a high rate of spin with a projected rotational velocity of 155 km/s, which is giving the star an oblate shape with an equatorial bulge that is 6% larger than the polar radius. The star is roughly 453 million years old with 1.8 times the mass of the Sun. It is radiating 16 times the Sun's luminosity from its photosphere at an effective temperature of 8,331 K.