Saiph

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Saiph
Location of Saiph (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Orion
Right ascension 05h 47m 45.38884s[1]
Declination −09° 40′ 10.5777″[1]
Apparent magnitude (V) 2.09[2]
Characteristics
Spectral type B0.5 Ia[3]
U−B color index −1.02[2]
B−V color index −0.18[2]
Variable type Suspected[4]
Distance
650 ± 30 ly
(198 ± 9 pc)
Absolute magnitude (MV)−6.1[6]
Details
Myr
HR 2004, SAO 132542.[9]
Database references
SIMBADdata

Saiph

apparent visual magnitude of 2.1.[2] The luminosity of this star changes slightly, varying by 0.04 magnitudes.[4]

Nomenclature

Kappa Orionis is the star's

giant. This name was originally applied to Eta Orionis.[10] In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN)[11] to catalog and standardize proper names for stars. The WGSN's first bulletin of July 2016[12] included a table of the first two batches of names approved by the WGSN; which included Saiph for this star. It is now so entered in the IAU Catalog of Star Names.[13]

In the 17th-century catalogue of stars in the Calendarium of Al Achsasi al Mouakket, this star was designated Rekbah al Jauza al Yemeniat, which was translated into Latin as Genu Dextrum Gigantis "right knee of the giant".[14]

Properties

Saiph is a

spectrum yields a mass 15.50 ± 1.25 times and luminosity 56,881 times that of the Sun.[7] Analysis of the spectra and age of the members of the Orion OB1 association yields a mass 28 times that of the Sun (from an original mass 31.8 times that of the Sun) and an age of 6.2 million years.[15] Large stars such as Saiph (and many other stars in Orion) are destined to collapse on themselves and explode as supernovae.[16]

In non-Western astronomy and culture

In

Chinese name for Saiph is 參宿六 (Shēn Sù liù, English: the Sixth Star of Three Stars).[18]

The Wardaman people of northern Australia regard Saiph as the Guman digging stick, used to make a canyon by Black-headed Python.[19]

References


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