Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Andromeda |
Right ascension | 23h 07m 45.38355s [1] |
Declination | +49° 17′ 44.7904″ [1] |
Apparent magnitude (V) | 5.68 [2] |
Characteristics | |
Spectral type | F5 V [3] |
B−V color index | 0.449±0.003 [2] |
Astrometry | |
Radial velocity (Rv) | −2.6±0.3 [2] km/s |
Proper motion (μ) |
RA: 151.592(34)
[1]
mas/
yr Dec.: 131.723(31) [1] mas/ yr |
Parallax (π) | 29.0956 ± 0.0408 mas [1] |
Distance | 112.1 ± 0.2
ly (34.37 ± 0.05 pc) |
Absolute magnitude (MV) | 3.00 [2] |
Details [4] | |
Mass | 1.386+0.010 −0.009 M☉ |
Luminosity | 5.62 [2] L☉ |
Surface gravity (log g) | 4.12±0.02 cgs |
Temperature | 6,605±61 K |
Metallicity [Fe/H] | −0.09±0.05 dex |
Rotational velocity (v sin i) | 9.7 [5] km/s |
Age | 2.28+0.12 −0.25 Gyr |
Other designations | |
Database references | |
SIMBAD | data |
5 Andromedae is a single, [7] yellow-white hued star in the northern constellation of Andromeda. Its designation comes from a catalogue of stars by English astronomer John Flamsteed, published in 1712. The star is faintly visible to the naked eye, having an apparent visual magnitude of 5.68. [2] Based upon an annual parallax shift of 29.12 [1] mas as seen from Earth, it is located 112 light years away. 5 Andromedae is moving closer to the Sun with a radial velocity of −2.6 km/s. [2] It has a relatively high proper motion, advancing across the celestial sphere at the rate of 0.201 arc seconds per year. [8]
This is an ordinary F-type main-sequence star with a stellar classification of F5 V. [3] It is estimated to be 2.3 [4] billion years old and is spinning with a projected rotational velocity of 9.7 km/s. [5] The star has 1.39 times the mass of the Sun. It is radiating 5.6 [2] times the Sun's luminosity from its photosphere at an effective temperature of about 6,605 K. [4]
Within Andromeda it is the second of a northerly chain asterism – 7, 8, 11 are further south-westward, with 3 Andromedae in the other direction.
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Andromeda |
Right ascension | 23h 07m 45.38355s [1] |
Declination | +49° 17′ 44.7904″ [1] |
Apparent magnitude (V) | 5.68 [2] |
Characteristics | |
Spectral type | F5 V [3] |
B−V color index | 0.449±0.003 [2] |
Astrometry | |
Radial velocity (Rv) | −2.6±0.3 [2] km/s |
Proper motion (μ) |
RA: 151.592(34)
[1]
mas/
yr Dec.: 131.723(31) [1] mas/ yr |
Parallax (π) | 29.0956 ± 0.0408 mas [1] |
Distance | 112.1 ± 0.2
ly (34.37 ± 0.05 pc) |
Absolute magnitude (MV) | 3.00 [2] |
Details [4] | |
Mass | 1.386+0.010 −0.009 M☉ |
Luminosity | 5.62 [2] L☉ |
Surface gravity (log g) | 4.12±0.02 cgs |
Temperature | 6,605±61 K |
Metallicity [Fe/H] | −0.09±0.05 dex |
Rotational velocity (v sin i) | 9.7 [5] km/s |
Age | 2.28+0.12 −0.25 Gyr |
Other designations | |
Database references | |
SIMBAD | data |
5 Andromedae is a single, [7] yellow-white hued star in the northern constellation of Andromeda. Its designation comes from a catalogue of stars by English astronomer John Flamsteed, published in 1712. The star is faintly visible to the naked eye, having an apparent visual magnitude of 5.68. [2] Based upon an annual parallax shift of 29.12 [1] mas as seen from Earth, it is located 112 light years away. 5 Andromedae is moving closer to the Sun with a radial velocity of −2.6 km/s. [2] It has a relatively high proper motion, advancing across the celestial sphere at the rate of 0.201 arc seconds per year. [8]
This is an ordinary F-type main-sequence star with a stellar classification of F5 V. [3] It is estimated to be 2.3 [4] billion years old and is spinning with a projected rotational velocity of 9.7 km/s. [5] The star has 1.39 times the mass of the Sun. It is radiating 5.6 [2] times the Sun's luminosity from its photosphere at an effective temperature of about 6,605 K. [4]
Within Andromeda it is the second of a northerly chain asterism – 7, 8, 11 are further south-westward, with 3 Andromedae in the other direction.