Observation data Epoch J2000.0 Equinox J2000.0 ( ICRS) | |
---|---|
Constellation | Antlia |
Right ascension | 09h 37m 00.2073s [1] |
Declination | −25° 17′ 48.335″ [1] |
Apparent magnitude (V) | 5.68±0.01 [2] |
Characteristics | |
Evolutionary stage | RGB [3] |
Spectral type | K0 III [4] |
B−V color index | +1.12 [5] |
Astrometry | |
Radial velocity (Rv) | 30±2 [6] km/s |
Proper motion (μ) |
RA: −63.114
mas/
yr
[1] Dec.: +36.255 mas/ yr [1] |
Parallax (π) | 11.4429 ± 0.0711 mas [1] |
Distance | 285 ± 2
ly (87.4 ± 0.5 pc) |
Absolute magnitude (MV) | +0.78 [7] |
Details | |
Mass | 1.6+0.6 −0.9 [8] M☉ |
Radius | 10.6 [9] R☉ |
Luminosity | 52.7 ± 0.5 [10] L☉ |
Surface gravity (log g) | 2.40 ± 0.37 [11] cgs |
Temperature | 4,610±110 [8] K |
Metallicity [Fe/H] | +0.05 [12] dex |
Age | 2.67+0.28 −0.56 [3] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
HD 83332 (HR 3830) is a solitary, [15] orange hued star located in the southern constellation Antlia. It has an apparent magnitude of 5.68, [2] making it faintly visible to the naked eye if viewed under ideal conditions. The star is located 285 light years [1] away based on its annual parallax shift, but is drifting away with a radial velocity of 30 km/s. [6]
HD 83332 has a classification of K0 III, [4] which suggests it is an evolved giant star, as stellar models place it on the red giant branch. [3] At present it has 1.6 [8] times the mass of the Sun and at an age of 2.7 billion years, [3] has expanded to a radius of 10.6 R☉. It radiates at 52.7 times the luminosity of the Sun [10] from its enlarged photosphere at an effective temperature of 4,610 K. [8] HD 83332 has a solar metallicity, 112% that of the Sun to be exact, and is a member of the thin disk. [12]
Observation data Epoch J2000.0 Equinox J2000.0 ( ICRS) | |
---|---|
Constellation | Antlia |
Right ascension | 09h 37m 00.2073s [1] |
Declination | −25° 17′ 48.335″ [1] |
Apparent magnitude (V) | 5.68±0.01 [2] |
Characteristics | |
Evolutionary stage | RGB [3] |
Spectral type | K0 III [4] |
B−V color index | +1.12 [5] |
Astrometry | |
Radial velocity (Rv) | 30±2 [6] km/s |
Proper motion (μ) |
RA: −63.114
mas/
yr
[1] Dec.: +36.255 mas/ yr [1] |
Parallax (π) | 11.4429 ± 0.0711 mas [1] |
Distance | 285 ± 2
ly (87.4 ± 0.5 pc) |
Absolute magnitude (MV) | +0.78 [7] |
Details | |
Mass | 1.6+0.6 −0.9 [8] M☉ |
Radius | 10.6 [9] R☉ |
Luminosity | 52.7 ± 0.5 [10] L☉ |
Surface gravity (log g) | 2.40 ± 0.37 [11] cgs |
Temperature | 4,610±110 [8] K |
Metallicity [Fe/H] | +0.05 [12] dex |
Age | 2.67+0.28 −0.56 [3] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
HD 83332 (HR 3830) is a solitary, [15] orange hued star located in the southern constellation Antlia. It has an apparent magnitude of 5.68, [2] making it faintly visible to the naked eye if viewed under ideal conditions. The star is located 285 light years [1] away based on its annual parallax shift, but is drifting away with a radial velocity of 30 km/s. [6]
HD 83332 has a classification of K0 III, [4] which suggests it is an evolved giant star, as stellar models place it on the red giant branch. [3] At present it has 1.6 [8] times the mass of the Sun and at an age of 2.7 billion years, [3] has expanded to a radius of 10.6 R☉. It radiates at 52.7 times the luminosity of the Sun [10] from its enlarged photosphere at an effective temperature of 4,610 K. [8] HD 83332 has a solar metallicity, 112% that of the Sun to be exact, and is a member of the thin disk. [12]