Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Pegasus |
Right ascension | 22h 21m 19.33896s [1] |
Declination | 28° 19′ 49.8786″ [1] |
Apparent magnitude (V) | 4.81 [2] (4.83 + 8.86) [3] |
Characteristics | |
Spectral type | B9III [4] |
U−B color index | −0.19 [2] |
B−V color index | +0.00 [2] |
Astrometry | |
Radial velocity (Rv) | +11.40 [5] km/s |
Proper motion (μ) |
RA: +17.426
[1]
mas/
yr Dec.: +7.122 [1] mas/ yr |
Parallax (π) | 5.7814 ± 0.3196 mas [1] |
Distance | 560 ± 30
ly (173 ± 10 pc) |
Absolute magnitude (MV) | −1.82 [6] |
Details | |
32 Peg Aa | |
Luminosity | 541 [6] L☉ |
Temperature | 11,403 [7] K |
Rotational velocity (v sin i) | 60 [8] km/s |
Other designations | |
Database references | |
SIMBAD | data |
32 Pegasi is a binary star [10] system in the northern constellation of Pegasus. It is visible to the naked eye as a faint, blue-white hued point of light with an apparent visual magnitude of 4.81 [2] The system is located approximately 560 light years away from the Sun based on parallax, and is drifting further away with a radial velocity of +11.4 km/s. [5]
The brighter member of this system, designated component Aa, has visual magnitude 4.83 with a stellar classification of B9III, [4] matching a late B-type star with the luminosity class of a giant. It is spinning with a projected rotational velocity of 60 km/s, [8] and is radiating 541 [6] times the luminosity of the Sun from its photosphere at an effective temperature of 11,403 K. [7]
The fainter secondary, component Ab, is of magnitude 8.86 with an angular separation of 0.50 ″ along a position angle of 288° from the primary, as of 2005. Visual companions include component B, at a 70.7″ separation from the primary and magnitude 10.73; C, at a separation from B of 3.2″ and magnitude 12.4; as well as D (separation from A of 42.8″ and magnitude 11.9) and E (separation from A of 58.3" and magnitude 11.9). [3]
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Pegasus |
Right ascension | 22h 21m 19.33896s [1] |
Declination | 28° 19′ 49.8786″ [1] |
Apparent magnitude (V) | 4.81 [2] (4.83 + 8.86) [3] |
Characteristics | |
Spectral type | B9III [4] |
U−B color index | −0.19 [2] |
B−V color index | +0.00 [2] |
Astrometry | |
Radial velocity (Rv) | +11.40 [5] km/s |
Proper motion (μ) |
RA: +17.426
[1]
mas/
yr Dec.: +7.122 [1] mas/ yr |
Parallax (π) | 5.7814 ± 0.3196 mas [1] |
Distance | 560 ± 30
ly (173 ± 10 pc) |
Absolute magnitude (MV) | −1.82 [6] |
Details | |
32 Peg Aa | |
Luminosity | 541 [6] L☉ |
Temperature | 11,403 [7] K |
Rotational velocity (v sin i) | 60 [8] km/s |
Other designations | |
Database references | |
SIMBAD | data |
32 Pegasi is a binary star [10] system in the northern constellation of Pegasus. It is visible to the naked eye as a faint, blue-white hued point of light with an apparent visual magnitude of 4.81 [2] The system is located approximately 560 light years away from the Sun based on parallax, and is drifting further away with a radial velocity of +11.4 km/s. [5]
The brighter member of this system, designated component Aa, has visual magnitude 4.83 with a stellar classification of B9III, [4] matching a late B-type star with the luminosity class of a giant. It is spinning with a projected rotational velocity of 60 km/s, [8] and is radiating 541 [6] times the luminosity of the Sun from its photosphere at an effective temperature of 11,403 K. [7]
The fainter secondary, component Ab, is of magnitude 8.86 with an angular separation of 0.50 ″ along a position angle of 288° from the primary, as of 2005. Visual companions include component B, at a 70.7″ separation from the primary and magnitude 10.73; C, at a separation from B of 3.2″ and magnitude 12.4; as well as D (separation from A of 42.8″ and magnitude 11.9) and E (separation from A of 58.3" and magnitude 11.9). [3]