Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Vela |
HD 92449 | |
Right ascension | 10h 39m 18.3925s [1] |
Declination | −55° 36′ 11.765″ [1] |
Apparent magnitude (V) | 4.29 [2] |
HD 92463 | |
Right ascension | 10h 39m 24.2778s [3] |
Declination | −55° 36′ 25.642″ [3] |
Characteristics | |
Spectral type | G5 IIa [4] + B8 V [5] |
B−V color index | 1.025±0.003 [2] |
Astrometry | |
HD 92449 | |
Radial velocity (Rv) | +20.1±0.7 [6] km/s |
Proper motion (μ) |
RA: −19.032(91)
mas/
yr
[1] Dec.: 5.032(90) mas/ yr [1] |
Parallax (π) | 4.1595 ± 0.0940 mas [1] |
Distance | 780 ± 20
ly (240 ± 5 pc) |
Absolute magnitude (MV) | −2.76 [2] |
HD 92463 | |
Proper motion (μ) |
RA: −18.941(40)
mas/
yr
[3] Dec.: 5.386(42) mas/ yr [3] |
Parallax (π) | 4.2647 ± 0.0405 mas [3] |
Distance | 765 ± 7
ly (234 ± 2 pc) |
Details | |
Luminosity | 1370.29 [7] L☉ |
Temperature | 5,100 [7] K |
Other designations | |
A: CD−54 3915, HD 92449, HIP 52154, SAO 238309 | |
B: CD−54 3675, HD 92463, SAO 238313 | |
Database references | |
SIMBAD | HD 92449 |
HD 92463 |
HR 4180 is a double star with components HD 92449 and HD 92463 in the southern constellation of Vela. They are probably members of a binary star system. [8] HR 4180 can be viewed with the naked eye, having an apparent visual magnitude of 4.29. [2] Based upon the annual parallax shift of the two stars it is located approximately 780 light years from the Sun. [1] [3] The system is moving further from the Earth with a heliocentric radial velocity of +20 km/s. [6]
The primary component of this system, HD 92449, is a bright giant with a stellar classification of G5 IIa. [4] The star radiates 1,370 times the Sun's luminosity from its photosphere at an effective temperature of 5,100 K. [7] It shares a common proper motion with the magnitude 6.06 [9] star HD 92463, [10] and the pair likely form a binary system. [8] This secondary component is a B-type main-sequence star with a class of B8 V. [5] As of 2000, it had an angular separation of 51.70 ″ along a position angle of 105° from the primary. [9]
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Vela |
HD 92449 | |
Right ascension | 10h 39m 18.3925s [1] |
Declination | −55° 36′ 11.765″ [1] |
Apparent magnitude (V) | 4.29 [2] |
HD 92463 | |
Right ascension | 10h 39m 24.2778s [3] |
Declination | −55° 36′ 25.642″ [3] |
Characteristics | |
Spectral type | G5 IIa [4] + B8 V [5] |
B−V color index | 1.025±0.003 [2] |
Astrometry | |
HD 92449 | |
Radial velocity (Rv) | +20.1±0.7 [6] km/s |
Proper motion (μ) |
RA: −19.032(91)
mas/
yr
[1] Dec.: 5.032(90) mas/ yr [1] |
Parallax (π) | 4.1595 ± 0.0940 mas [1] |
Distance | 780 ± 20
ly (240 ± 5 pc) |
Absolute magnitude (MV) | −2.76 [2] |
HD 92463 | |
Proper motion (μ) |
RA: −18.941(40)
mas/
yr
[3] Dec.: 5.386(42) mas/ yr [3] |
Parallax (π) | 4.2647 ± 0.0405 mas [3] |
Distance | 765 ± 7
ly (234 ± 2 pc) |
Details | |
Luminosity | 1370.29 [7] L☉ |
Temperature | 5,100 [7] K |
Other designations | |
A: CD−54 3915, HD 92449, HIP 52154, SAO 238309 | |
B: CD−54 3675, HD 92463, SAO 238313 | |
Database references | |
SIMBAD | HD 92449 |
HD 92463 |
HR 4180 is a double star with components HD 92449 and HD 92463 in the southern constellation of Vela. They are probably members of a binary star system. [8] HR 4180 can be viewed with the naked eye, having an apparent visual magnitude of 4.29. [2] Based upon the annual parallax shift of the two stars it is located approximately 780 light years from the Sun. [1] [3] The system is moving further from the Earth with a heliocentric radial velocity of +20 km/s. [6]
The primary component of this system, HD 92449, is a bright giant with a stellar classification of G5 IIa. [4] The star radiates 1,370 times the Sun's luminosity from its photosphere at an effective temperature of 5,100 K. [7] It shares a common proper motion with the magnitude 6.06 [9] star HD 92463, [10] and the pair likely form a binary system. [8] This secondary component is a B-type main-sequence star with a class of B8 V. [5] As of 2000, it had an angular separation of 51.70 ″ along a position angle of 105° from the primary. [9]