Alpha Equulei

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α Equulei
Location of α Equulei (circled)
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation
Equuleus
Right ascension 21h 15m 49.43192s[1]
Declination +05° 14′ 52.2430″[1]
Apparent magnitude (V) +3.919[2](4.49/4.96)
Characteristics
Spectral type G7III + kA3hA4mA9[3]
U−B color index +0.284[2]
B−V color index +0.529[2]
Distance
190 ± 2 ly
(58.3 ± 0.7 pc)
Absolute magnitude (MV)+0.17 (0.71 + 1.18)[3]
Semi-amplitude
(K1)
(primary)
16.34 ± 0.07 km/s
Semi-amplitude (K2)
(secondary)
17.9 ± 0.3 km/s
Details
A
Myr
FK5 800, GC
 29735
Database references
SIMBADdata

Alpha Equulei (α Equulei, abbreviated Alpha Equ, α Equ), officially named Kitalpha

proper-motion star only 190 light-years
away.

Nomenclature

α Equulei (Latinised to Alpha Equulei) is the star's Bayer designation.

It bore the traditional name Kitalpha (rarely Kitel Phard or Kitalphar), a contraction of the

Working Group on Star Names (WGSN)[7] to catalogue and standardize proper names for stars. The WGSN approved the name Kitalpha for this star on 21 August 2016 and it is now so entered in the IAU Catalog of Star Names.[6]

In

Chinese name for Alpha Equulei itself is 虛宿二 (Xū Sù èr, English: the Second Star of Emptiness).[9]

Properties

The overall appearance of α Equulei is a

spectroscopic binary
consisting of two individual stars.

The primary star is a G7 giant about fifty times more luminous than the Sun. It has an effective temperature of 5,100 K and a radius of 9.2 times greater than the Sun.

The secondary is an

A-type dwarf about 26 times as luminous as the sun. It has an effective temperature of 8,150 K and a radius 2.6 times greater than the sun. It is a chemically peculiar Am star.[3]

The two stars revolve in a circular orbit every 98.8 days. Their respective orbital velocities allow their masses to be calculated at 2.3 M and 2.0 M, respectively.[3]

References