Gamma Lupi

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Gamma Lupi
Diagram showing star positions and boundaries of the Lupus constellation and its surroundings
Cercle rouge 100%.svg

Location of γ Lupi (circled)
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Lupus
Right ascension 15h 35m 08.44835s[1]
Declination –41° 10′ 00.3247″[1]
Apparent magnitude (V) 2.77[2]
Characteristics
Spectral type B2 IV[3]
U−B color index –0.82[4]
B−V color index –0.20[4]
Astrometry
Radial velocity (Rv) +2.3[5] km/s
Proper motion (μ) RA: −15.62[1] mas/yr
Dec.: −25.43[1] mas/yr
Parallax (π) 7.75 ± 0.50[1] mas
Distance 420 ± 30 ly
(129 ± 8 pc)
Absolute magnitude (MV) –2.4[2]
Orbit[6]
Period (P) 190.0 yr
Semi-major axis (a) 0.655"
Eccentricity (e) 0.51
Inclination (i) 95.0°
Longitude of the node (Ω) 94.6°
Periastron epoch (T) 1885.0
Argument of periastron (ω)
(secondary)
311.5°
Details
γ Lup A
Mass 9.5 ± 0.2[3] M
Luminosity 5,000[2] L
Surface gravity (log g) 3.96[2] cgs
Temperature 20,900[2] K
Rotational velocity (v sin i) 270[7] km/s
Age 18.6 ± 2.4[3] Myr
Other designations
Gam Lup, CD −40° 9760, HD 138690, HIP 76297, HR 5776, SAO 225938.[8]

Gamma Lupi (γ Lupi, γ Lup) is a 3rd-magnitude, B-type blue giant star in the constellation of Lupus. It is also known in ancient Chinese astronomy as 騎官一 or "the 1st (star) of the Cavalry Officer". With a telescope, Gamma Lupi can be resolved into a binary star system in close orbit. This is known as the Gamma Lupi AB system, often abbreviated as γ Lupi AB or γ Lup AB. Gamma Lupi A is itself a spectroscopic binary with a period of 2.8081[9] days.

This star is a proper motion member of the Upper-Centaurus Lupus sub-group in the Scorpius-Centaurus OB association, the nearest such co-moving association of massive stars to the Sun.[2]

See also

References

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