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Star in the constellation Sagittarius From Wikipedia, the free encyclopedia
Xi1 Sagittarii (ξ1 Sagittarii) is a solitary,[11] blue-white hued star in the zodiac constellation of Sagittarius. It is visible to the naked eye with an apparent visual magnitude of +5.06.[2] Based upon a small annual parallax shift of 1.58 mas as seen from Earth,[1] this system is located roughly 2,100 light years from the Sun.
Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Sagittarius |
Right ascension | 18h 57m 20.47670s[1] |
Declination | −20° 39′ 22.8539″[1] |
Apparent magnitude (V) | +5.06[2] |
Characteristics | |
Spectral type | B9/A0 Ib[3] |
U−B color index | −0.14[2] |
B−V color index | +0.12[2] |
Astrometry | |
Proper motion (μ) | RA: −1.46[1] mas/yr Dec.: −5.75[1] mas/yr |
Parallax (π) | 1.58 ± 0.26 mas[1] |
Distance | approx. 2,100 ly (approx. 600 pc) |
Absolute magnitude (MV) | −3.92[4] |
Details | |
Mass | 7.8±0.1[5] M☉ |
Radius | 15[6] R☉ |
Luminosity | 2,753[7] L☉ |
Surface gravity (log g) | 2.3[8] cgs |
Temperature | 9,400[8] K |
Metallicity [Fe/H] | −0.20[8] dex |
Rotational velocity (v sin i) | 10[9] km/s |
Age | 39.8±4.9[5] Myr |
Other designations | |
Database references | |
SIMBAD | data |
This is a massive supergiant star[6] with a stellar classification of B9/A0 Ib.[3] With an estimated 7.8[5] times the mass of the Sun and an age of about 40[5] million years it has depleted the hydrogen at its core, causing it to expand to about 15 times the Sun's radius.[6] It is radiating 2,753[7] times the Sun's luminosity from its photosphere at an effective temperature of about 9,400 K.[8]
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