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Zeta Leonis

Zeta Leonis
Diagram showing star positions and boundaries of the Leo constellation and its surroundings
Cercle rouge 100%.svg

Adhafera is the ζ star in the lion's mane (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Leo
Right ascension 10h 16m 41.41597s
Declination +23° 25′ 02.3221″
Apparent magnitude (V) 3.33
Characteristics
Spectral type F0 III
U−B color index +0.07
B−V color index +0.30
Variable type Suspected
Astrometry
Radial velocity (Rv) -15.6 km/s
Proper motion (μ) RA: +18.39 mas/yr
Dec.: -6.84 mas/yr
Parallax (π) 11.90 ± 0.18mas
Distance 274 ± 4 ly
(84 ± 1 pc)
Details
Mass M
Radius R
Luminosity 85 L
Surface gravity (log g) 3.0 cgs
Temperature 6,792 K
Metallicity [Fe/H] –0.03 dex
Rotational velocity (v sin i) 72.4 km/s
Other designations
Adhafera, Aldhafera, Adhafara, ζ Leo, 36 Leo, HR 4031, BD +24°2209, HD 89025, FK5 384, HIP 50335, SAO 81265, GC 14107, NSV 04804, WDS 10167+2325A.
Database references
SIMBAD data

Zeta Leonis (ζ Leonis, abbreviated Zeta Leo, ζ Leo), also named Adhafera, is a third-magnitude star in the constellation of Leo, the lion. It forms the second star (after Gamma Leonis) in the blade of 'the Sickle', which is an asterism formed from the head of Leo.

ζ Leonis (Latinised to Zeta Leonis) is the star's Bayer designation. It has the traditional name Adhafera (Aldhafera, Adhafara), which comes from the Arabic الضفيرة al-ðafīrah 'the braid/curl', a reference to its position in the lion's mane. In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN) to catalog and standardize proper names for stars. The WGSN's first bulletin of July 2016 included a table of the first two batches of names approved by the WGSN; which included Adhafera for this star.

Adhafera is a giant star with a stellar classification of F0 III. Since 1943, the spectrum of this star has served as one of the stable anchor points by which other stars are classified. Its apparent magnitude is +3.44, making it relatively faint for a star that is visible to the naked eye. Nevertheless, it shines with 85 times the luminosity of the Sun. Adhafera has about three times the Sun's mass and six times the radius of the Sun.Parallax measurements from the Hipparcos satellite yield an estimated distance to Adhafera of 274 light-years (84 parsecs) from the Sun.


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Wikipedia

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