Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Cepheus |
Right ascension | 2h 9m 25.30805s [1] |
Declination | +81° 17′ 45.3964″ [1] |
Apparent magnitude (V) | 6.05 [2] |
Characteristics | |
Spectral type | A1.5V [3] |
U−B color index | 0.06 [4] |
B−V color index | 0.11 [4] |
Astrometry | |
Radial velocity (Rv) | −9.0±3.0 [5] km/s |
Proper motion (μ) |
RA: −34.605
[1]
mas/
yr Dec.: 6.674 [1] mas/ yr |
Parallax (π) | 14.1120 ± 0.0500 mas [1] |
Distance | 231.1 ± 0.8
ly (70.9 ± 0.3 pc) |
Absolute magnitude (MV) | +1.81 [6] |
Details | |
Mass | 1.81 [7] M☉ |
Radius | 1.92 [8] R☉ |
Luminosity | 16 [6] L☉ |
Surface gravity (log g) | 4.30 [7] cgs |
Temperature | 8,528 [7] K |
Rotational velocity (v sin i) | 130 [9] km/s |
Age | 254 [7] Myr |
Other designations | |
Database references | |
SIMBAD | data |
HD 12467 is a single [11] star in the northern circumpolar constellation of Cepheus. It has a white hue and is barely visible to the naked eye with an apparent visual magnitude of 6.05. [2] The distance to this object is 231 light years based on parallax, [1] but it is drifting closer with a heliocentric radial velocity of −9 km/s. [5]
This object is an ordinary A-type main-sequence star with a stellar classification of A1.5V, [3] which indicates it is generating energy through core hydrogen fusion. It is 254 [7] million years old with a relatively high projected rotational velocity of 130 km/s. [9] The star has 1.8 [7] times the mass of the Sun and 1.9 [8] times the Sun's radius. It is radiating 16 [6] times the luminosity of the Sun from its photosphere at an effective temperature of 8,528 K. [7]
The star displays an infrared excess with a signature that suggests it has two debris disks. The inner disk is orbiting 7.4 AU from the host star with a mean temperature of 200 K, while the outer disk is 50 K at a separation of 119 AU. [8]
Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Cepheus |
Right ascension | 2h 9m 25.30805s [1] |
Declination | +81° 17′ 45.3964″ [1] |
Apparent magnitude (V) | 6.05 [2] |
Characteristics | |
Spectral type | A1.5V [3] |
U−B color index | 0.06 [4] |
B−V color index | 0.11 [4] |
Astrometry | |
Radial velocity (Rv) | −9.0±3.0 [5] km/s |
Proper motion (μ) |
RA: −34.605
[1]
mas/
yr Dec.: 6.674 [1] mas/ yr |
Parallax (π) | 14.1120 ± 0.0500 mas [1] |
Distance | 231.1 ± 0.8
ly (70.9 ± 0.3 pc) |
Absolute magnitude (MV) | +1.81 [6] |
Details | |
Mass | 1.81 [7] M☉ |
Radius | 1.92 [8] R☉ |
Luminosity | 16 [6] L☉ |
Surface gravity (log g) | 4.30 [7] cgs |
Temperature | 8,528 [7] K |
Rotational velocity (v sin i) | 130 [9] km/s |
Age | 254 [7] Myr |
Other designations | |
Database references | |
SIMBAD | data |
HD 12467 is a single [11] star in the northern circumpolar constellation of Cepheus. It has a white hue and is barely visible to the naked eye with an apparent visual magnitude of 6.05. [2] The distance to this object is 231 light years based on parallax, [1] but it is drifting closer with a heliocentric radial velocity of −9 km/s. [5]
This object is an ordinary A-type main-sequence star with a stellar classification of A1.5V, [3] which indicates it is generating energy through core hydrogen fusion. It is 254 [7] million years old with a relatively high projected rotational velocity of 130 km/s. [9] The star has 1.8 [7] times the mass of the Sun and 1.9 [8] times the Sun's radius. It is radiating 16 [6] times the luminosity of the Sun from its photosphere at an effective temperature of 8,528 K. [7]
The star displays an infrared excess with a signature that suggests it has two debris disks. The inner disk is orbiting 7.4 AU from the host star with a mean temperature of 200 K, while the outer disk is 50 K at a separation of 119 AU. [8]