G Scorpii
Appearance
Observation data Epoch J2000 Equinox J2000 | ||
---|---|---|
Constellation | Scorpius | |
Right ascension | 17h 49m 51.48081s[1] | |
Declination | −37° 02′ 35.8975″[1] | |
Apparent magnitude (V) | 3.21[2] | |
Characteristics | ||
Evolutionary stage | horizontal branch[3] | |
Spectral type | K2 III[4] | |
U−B color index | +1.19[2] | |
B−V color index | +1.17[2] | |
Absolute magnitude (MV) | +0.24[6] | |
Details Rotational velocity (v sin i) <1.0[8] km/s | | |
HR 6630, SAO 209318 | ||
Database references | ||
SIMBAD | data |
G Scorpii (abbreviated G Sco), also named Fuyue, is a giant star in the constellation of Scorpius. It has an apparent magnitude of +3.19. It is approximately 126 light-years from the Sun.
Nomenclature
G Scorpii is the star's Bayer designation. It was formerly situated in the constellation of Telescopium where it was designated γ Telescopii, Latinised to Gamma Telescopii.[9] It was resited in Scorpius and redesignated G Scorpii by Benjamin Apthorp Gould.[10]
In 2016, the IAU organized a
Working Group on Star Names (WGSN)[11] to catalog and standardize proper names for stars. The WGSN approved the name Fuyue for this star on 30 June 2017 and it is now so included in the List of IAU-approved Star Names.[12]
G Scorpii bore the
traditional name Fuyue (simplified Chinese: 傅说; traditional Chinese: 傅說) in ancient China. Fu Yue was a former slave that became a high-ranking minister to Shang dynasty ruler Wu Ding
.
Properties
G Scorpii is an orange
Evolutionary models show that G Scorpii has probably left the
red giant branch and is now fusing helium in its core. This makes it a red clump star, at the cool end of the horizontal branch.[3]
Just 5
At magnitude 3.2, G Scorpii is around 40 times brighter than the entire globular cluster.References
- ^ S2CID 18759600.
- ^ Bibcode:1966CoLPL...4...99J.
- ^ S2CID 102486794.
- S2CID 119476992.
- Bibcode:1953GCRV..C......0W.
- S2CID 12136256.
- S2CID 204907220.
- S2CID 54046583.
- ^ Ian Ridpath, "Telescopium", Star Tales, retrieved 2020-05-23.
- ISBN 978-0-939923-78-6.
- ^ IAU Working Group on Star Names (WGSN), retrieved 22 May 2016.
- ^ Naming Stars, IAU.org, retrieved 16 December 2017.
- ISBN 3540296921. The radius (R*) is given by:
- ISBN 978-1139851541.