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Sigma Sagittarii

Sigma Sagittarii
Diagram showing star positions and boundaries of the Sagittarius constellation and its surroundings
Cercle rouge 100%.svg

Location of σ Sagittarii (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Sagittarius
Right ascension 18h 55m 15.92650s
Declination –26° 17′ 48.2068″
Apparent magnitude (V) 2.05
Characteristics
Spectral type B2.5 V
U−B color index –0.761
B−V color index –0.204
Astrometry
Radial velocity (Rv) –11.2 km/s
Proper motion (μ) RA: +15.14 mas/yr
Dec.: –53.43 mas/yr
Parallax (π) 14.32 ± 0.29mas
Distance 228 ± 5 ly
(70 ± 1 pc)
Details
Mass 7.8 ± 0.2 M
Radius 4.5 R
Luminosity 3,300 L
Temperature 18,890 K
Rotational velocity (v sin i) 165 km/s
Age 31.4 ± 0.4 Myr
Other designations
Nunki, Sadira, σ Sagittarii, σ Sgr, Sigma Sgr, 34 Sagittarii, CCDM J18552-2618A, CPD-27  5241, FK5 706, GC 25941, HD 175191, HIP 92855, HR 7121, IDS 18491-2625 A, PPM 269078, SAO 187448, WDS J18553-2618Aa,Ab.
Database references
SIMBAD data

Sigma Sagittarii (σ Sagittarii, abbreviated Sigma Sgr, σ Sgr), also named Nunki, is the second brightest star in the constellation of Sagittarius. It has an apparent magnitude of +2.05, making it readily visible to the naked eye. The distance to this star, determined using parallax measurements from the Hipparcos astrometry satellite, yields an estimated value of 228 light-years (70 parsecs) from the Sun.

Sigma Sagittarii has a spectrum matching a stellar classification of B2.5 V, which indicates this is a B-type main sequence star. Its total luminosity is 3300 times that of the Sun while it has a surface temperature of 18,890 K. X-ray emission has been detected from this star, which has an estimated X-ray luminosity of 1.2 × 1028 erg s−1.

It has a 10th magnitude optical companion located 5.2 arcminutes away.

Because it is close to the ecliptic, it can be occulted by the Moon and very rarely by planets. The last occultation by a planet took place on November 17, 1981, when it was occulted by Venus. Furthermore, this is the brightest star that can be principally occulted by an exterior planet between 5000 BC and 5000 AD. However, only Mars can do this, and only rarely; the last time was on September 3, 423.

σ Sagittarii (Latinised to Sigma Sagittarii) is the star's Bayer designation.


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Wikipedia

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