Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Aquila |
Right ascension | 19h 12m 40.71201s [2] |
Declination | −07° 56′ 22.2650″ [2] |
Apparent magnitude (V) | 5.362 [3] |
Characteristics | |
Spectral type | B3 V, [4] B3 IV, [5] or B2/3 II [6] |
B−V color index | +0.088 [3] |
Astrometry | |
Radial velocity (Rv) | −23.0±0.7 [7] km/s |
Proper motion (μ) |
RA: +14.040
[2]
mas/
yr Dec.: –6.814 [2] mas/ yr |
Parallax (π) | 3.5374 ± 0.1720 mas [2] |
Distance | 920 ± 40
ly (280 ± 10 pc) |
Absolute magnitude (MV) | −2.02 [8] |
Details | |
Mass | 8.6±0.2 [9] M☉ |
Luminosity (bolometric) | 7,284 [3] L☉ |
Temperature | 18,700 [3] K |
Rotational velocity (v sin i) | 133±6 [4] km/s |
Age | 27.9±4.1 [9] Myr |
Other designations | |
Database references | |
SIMBAD | data |
20 Aquilae, abbreviated 20 Aql, is an irregular variable [11] star in the equatorial constellation of Aquila. 20 Aquilae is its Flamsteed designation. It ranges in magnitude from a peak of 5.33 down to 5.36, which is bright enough for the star to be visible to the naked eye. [12] The estimated distance to this star is around 920 light years, based upon an annual parallax shift of 3.5 mas. [2] The star is moving closer to the Earth with a heliocentric radial velocity of −23 km/s. [7]
There has been some disagreement over the stellar classification of this star. Buscombe (1962) listed a class of B3 IV, [5] which suggests a B-type subgiant star that has exhausted the hydrogen at its core and is expanding off the main sequence. Lesh (1968) [13] and Braganca et al. (2012) [4] matched a B-type main sequence star with a class of B3 V. However, Houk and Swift (1999) found a class of B2/3 II, [6] indicating this is an evolved bright giant.
The star is about 28 [9] million years old with a high rate of spin, showing a projected rotational velocity of 133 km/s. [4] It has 8.6 [9] times the mass of the Sun and is radiating 7,284 times the Sun's luminosity from its photosphere at an effective temperature of 18,700 K. [3]
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Aquila |
Right ascension | 19h 12m 40.71201s [2] |
Declination | −07° 56′ 22.2650″ [2] |
Apparent magnitude (V) | 5.362 [3] |
Characteristics | |
Spectral type | B3 V, [4] B3 IV, [5] or B2/3 II [6] |
B−V color index | +0.088 [3] |
Astrometry | |
Radial velocity (Rv) | −23.0±0.7 [7] km/s |
Proper motion (μ) |
RA: +14.040
[2]
mas/
yr Dec.: –6.814 [2] mas/ yr |
Parallax (π) | 3.5374 ± 0.1720 mas [2] |
Distance | 920 ± 40
ly (280 ± 10 pc) |
Absolute magnitude (MV) | −2.02 [8] |
Details | |
Mass | 8.6±0.2 [9] M☉ |
Luminosity (bolometric) | 7,284 [3] L☉ |
Temperature | 18,700 [3] K |
Rotational velocity (v sin i) | 133±6 [4] km/s |
Age | 27.9±4.1 [9] Myr |
Other designations | |
Database references | |
SIMBAD | data |
20 Aquilae, abbreviated 20 Aql, is an irregular variable [11] star in the equatorial constellation of Aquila. 20 Aquilae is its Flamsteed designation. It ranges in magnitude from a peak of 5.33 down to 5.36, which is bright enough for the star to be visible to the naked eye. [12] The estimated distance to this star is around 920 light years, based upon an annual parallax shift of 3.5 mas. [2] The star is moving closer to the Earth with a heliocentric radial velocity of −23 km/s. [7]
There has been some disagreement over the stellar classification of this star. Buscombe (1962) listed a class of B3 IV, [5] which suggests a B-type subgiant star that has exhausted the hydrogen at its core and is expanding off the main sequence. Lesh (1968) [13] and Braganca et al. (2012) [4] matched a B-type main sequence star with a class of B3 V. However, Houk and Swift (1999) found a class of B2/3 II, [6] indicating this is an evolved bright giant.
The star is about 28 [9] million years old with a high rate of spin, showing a projected rotational velocity of 133 km/s. [4] It has 8.6 [9] times the mass of the Sun and is radiating 7,284 times the Sun's luminosity from its photosphere at an effective temperature of 18,700 K. [3]