Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Sagittarius |
Right ascension | 19h 09m 45.83293s[1] |
Declination | –21° 01′ 25.0103″[1] |
Apparent magnitude (V) | +2.89[2] |
Characteristics | |
Spectral type | F2 II[2] |
U−B color index | +0.22[3] |
B−V color index | +0.35[3] |
Astrometry | |
Radial velocity (Rv) | –9.8[4] km/s |
Proper motion (μ) | RA: –1.36[1] mas/yr Dec.: –36.45[1] mas/yr |
Parallax (π) | 6.2410 ± 0.2868 mas[5] |
Distance | 520 ± 20 ly (160 ± 7 pc) |
Absolute magnitude (MV) | −3.08[6] |
Details | |
Mass | 5.9 ± 0.3[2] M☉ |
Surface gravity (log g) | 2.21 ± 0.05[2] cgs |
Temperature | 6,590 ± 50[2] K |
Rotational velocity (v sin i) | 30[7] km/s |
Age | 67[2] Myr |
Other designations | |
Database references | |
SIMBAD | data |
Pi Sagittarii (π Sagittarii, abbreviated Pi Sgr, π Sgr) is a triple star system in the zodiac constellation of Sagittarius. It has an apparent visual magnitude of +2.89,[2] bright enough to be readily seen with the naked eye. Based upon parallax measurements, it is roughly 510 light-years (160 parsecs) from the Sun.[1]
The three components are designated Pi Sagittarii A (officially named Albaldah /ælˈbɔːldə/, from the traditional name of the entire system),[9] B and C.[8]
aaa474_2_653
was invoked but never defined (see the help page).mnras402_2_1369
was invoked but never defined (see the help page).aass34_1
was invoked but never defined (see the help page).gcrv1953
was invoked but never defined (see the help page).Anderson2012
was invoked but never defined (see the help page).csrv
was invoked but never defined (see the help page).SIMBAD
was invoked but never defined (see the help page).