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Eta Leonis
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Eta Leonis
Location of η Leo (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Leo
Right ascension 10h 07m 19.9519s[1]
Declination +16° 45′ 45.592″[1]
Apparent magnitude (V) 3.486[2]
Characteristics
Evolutionary stage Blue supergiant (blue loop)[3]
Spectral type A0 Ib[2]
U−B color index −0.206[2]
B−V color index −0.026[2]
Astrometry
Radial velocity (Rv)1.40[4] km/s
Proper motion (μ) RA: −2.80[1] mas/yr
Dec.: −1.82[1] mas/yr
Parallax (π)2.57±0.16 mas[1]
Distance1,270 ± 80 ly
(390 ± 20 pc)
Absolute magnitude (MV)−5.54[3]
Details
Mass10[5] M
Radius47[3] R
Luminosity19,000[5] L
Surface gravity (log g)2.00[5] cgs
Temperature9,600[2] K
Metallicity−0.04[3]
Rotational velocity (v sin i)2[2] km/s
Age25[5] Myr
Other designations
η Leo, 30 Leonis, HR 3975, BD+17°2171, HD 87737, FK5 379, HIP 49583, SAO 98955, GC 13899
Database references
SIMBADdata

Eta Leonis (η Leo, η Leonis) is a third-magnitude blue supergiant star in the constellation Leo, about 1,270 light years away.

Nomenclature

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With Regulus, γ Leonis (Algieba), and ζ Leonis (Adhafera), it formed the Arabic lunar mansion Al Jabhah, the forehead (of the lion).[6] Some sources apply the name Al Jabhah to this star specifically,[7] though the name Algieba for γ Leonis has the same etymology.[8]

Properties

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Eta Leonis is a blue supergiant with the stellar classification A0Ib. Since 1943, the spectrum of this star has served as one of the stable anchor points by which other stars are classified.[9] Though its apparent magnitude is 3.5, making it a relatively dim star to the naked eye, it is nearly 20,000 times more luminous than the Sun, with an absolute magnitude of -5.60. The Hipparcos astrometric data has estimated the distance of Eta Leonis to be roughly 390 parsecs from Earth, or 1,270 light years away. It is believed to be in a blue loop phase.[3]

Eta Leonis is apparently a multiple star system, but the number of components and their separation is uncertain.[10]

References

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