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Sigma Leonis

Star in the constellation Leo From Wikipedia, the free encyclopedia

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Sigma Leonis, Latinized from σ Leonis, is a blue-white hued star in the zodiac constellation Leo that is visible to the naked eye with an apparent visual magnitude of 4.0.[3] Its annual parallax shift of 15.24 mas as seen from Earth implies a distance around 210 light years from the Sun. It is moving closer to the Sun with a radial velocity of –5 km/s.[7]

Quick Facts Observation data Epoch J2000 Equinox J2000, Constellation ...

Chini et al. (2012) list this as a single-lined spectroscopic binary system.[5] The visible component has a stellar classification of B9.5 Vs,[5] indicating it is a B-type main-sequence star. It is a suspected magnetic Ap star that shows an abundance anomaly with the element silicon.[14] Sigma Leonis has an estimated 2.76 times the mass of the Sun[8] and 3.07 times the Sun's radius.[9] It is about 293 million years old[8] with a projected rotational velocity of 70 km/s.[12] The star is radiating 133 times the Sun's luminosity from its photosphere[1] at an effective temperature of 11,000 K.[9]

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Name

In Chinese, 太微右垣 (Tài Wēi Yòu Yuán), meaning Right Wall of Supreme Palace Enclosure, refers to an asterism consisting of σ Leonis, β Virginis, ι Leonis, θ Leonis and δ Leonis.[15] Consequently, the Chinese name for σ Leonis itself is 太微右垣二 (Tài Wēi Yòu Yuán èr, English: the Second Star of Right Wall of Supreme Palace Enclosure.),[16] representing 西上將 (Xīshǎngjiāng), meaning The First Western General.[17] 西上將 (Xīshǎngjiāng), spelled Shang Tseang by R.H. Allen, means "the Higher General".[18]

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References

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