Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Sagittarius |
Right ascension | 18h 01m 23.12190s [1] |
Declination | −17° 09′ 24.7302″ [1] |
Apparent magnitude (V) | 6.27 [2] |
Characteristics | |
Spectral type | K2 III [3] |
B−V color index | 1.763±0.010 [4] |
Astrometry | |
Radial velocity (Rv) | −22.0±4.3 [2] km/s |
Proper motion (μ) |
RA: −0.86
[1]
mas/
yr Dec.: −7.15 [1] mas/ yr |
Parallax (π) | 1.24 ± 0.44 mas [1] |
Distance | approx. 2,600
ly (approx. 800 pc) |
Details | |
Mass | 10.6±1.9 [5] M☉ |
Luminosity | 6,816.79 [6] L☉ |
Temperature | 3,778 [6] K |
Age | 25.1±3.8 [5] Myr |
Other designations | |
Database references | |
SIMBAD | data |
6 Sagittarii is a massive, orange-hued
star in the southern
zodiac
constellation of
Sagittarius. With an
apparent visual magnitude of 6.27,
[2] it is just below the nominal brightness limit for visibility with the typical naked eye under ideal viewing conditions. The distance can be estimated from the annual
parallax shift of 1.24±0.44
mas
[1] as roughly 2,600
light years away. It is moving closer to the Sun with a heliocentric
radial velocity of −22 km/s.
[2] 6 Sagittarii has a
peculiar velocity of 31.8+9.9
−14.1 km/s, which may indicate it is a
runaway star.
[5]
This is an evolved giant star with a stellar classification of K2 III. [3] It is only 25 [5] million years old and has around ten times the mass of the Sun. [5] The star is radiating about 6,817 times the Sun's luminosity from its photosphere at an effective temperature of 3,778 K. [6] It appears to be a source of extended infrared excess, but this emission may be due to intervening cirrus. [8]
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Sagittarius |
Right ascension | 18h 01m 23.12190s [1] |
Declination | −17° 09′ 24.7302″ [1] |
Apparent magnitude (V) | 6.27 [2] |
Characteristics | |
Spectral type | K2 III [3] |
B−V color index | 1.763±0.010 [4] |
Astrometry | |
Radial velocity (Rv) | −22.0±4.3 [2] km/s |
Proper motion (μ) |
RA: −0.86
[1]
mas/
yr Dec.: −7.15 [1] mas/ yr |
Parallax (π) | 1.24 ± 0.44 mas [1] |
Distance | approx. 2,600
ly (approx. 800 pc) |
Details | |
Mass | 10.6±1.9 [5] M☉ |
Luminosity | 6,816.79 [6] L☉ |
Temperature | 3,778 [6] K |
Age | 25.1±3.8 [5] Myr |
Other designations | |
Database references | |
SIMBAD | data |
6 Sagittarii is a massive, orange-hued
star in the southern
zodiac
constellation of
Sagittarius. With an
apparent visual magnitude of 6.27,
[2] it is just below the nominal brightness limit for visibility with the typical naked eye under ideal viewing conditions. The distance can be estimated from the annual
parallax shift of 1.24±0.44
mas
[1] as roughly 2,600
light years away. It is moving closer to the Sun with a heliocentric
radial velocity of −22 km/s.
[2] 6 Sagittarii has a
peculiar velocity of 31.8+9.9
−14.1 km/s, which may indicate it is a
runaway star.
[5]
This is an evolved giant star with a stellar classification of K2 III. [3] It is only 25 [5] million years old and has around ten times the mass of the Sun. [5] The star is radiating about 6,817 times the Sun's luminosity from its photosphere at an effective temperature of 3,778 K. [6] It appears to be a source of extended infrared excess, but this emission may be due to intervening cirrus. [8]