Gamma Lyrae

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Gamma Lyrae
Location of γ Lyrae
Observation data
Epoch J2000      Equinox J2000
Constellation Lyra
Right ascension 18h 58m 56.62241s[1]
Declination +32° 41′ 22.4003″[1]
Apparent magnitude (V) 3.261[2]
Characteristics
Spectral type B9 III[3]
U−B color index –0.125[2]
B−V color index –0.047[2]
Distance
620 ± 30 ly
(190 ± 10 pc)
Absolute magnitude (MV)−3.14[5]
Details
Rotational velocity (v sin i)
71–72[7] km/s
HR 7178, SAO 67663[8]
Database references
SIMBADdata

Gamma Lyrae,

interstellar dust.[6]

Nomenclature

γ Lyrae (Latinised to Gamma Lyrae) is the star's Bayer designation.

It bore the traditional names Sulafat (Sulaphat), from the

Working Group on Star Names (WGSN)[12] to catalogue and standardize proper names for stars. The WGSN approved the name Sulafat for this star on 21 August 2016 and it is now so entered in the IAU Catalog of Star Names.[10]

In

Chinese name
for Gamma Lyrae itself is 漸台三 (Jiāntāisān, English: the Third Star of Clepsydra Terrace).

Properties

This is a

In 1909, Canadian astronomer

absorption lines of the components. He found that a period of 25.6 days matched his measurements.[18] It was reported as a spectroscopic binary as recently as 2001,[19] but is now believed to be a single star[20][21] with a high rate of rotation for stars of this type.[19]

References

External links