G Scorpii

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G Scorpii
Location of G Scorpii (circled)
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]
Distance
125.8 ± 0.7 ly
(38.6 ± 0.2 pc)
Absolute magnitude (MV)+0.24[6]
Details
Rotational velocity (v sin i)
<1.0[8] km/s
HR 6630, SAO
 209318
Database references
SIMBADdata

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 below and right (ie. west) of NGC 6441

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