Omicron Persei

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Template:Short description

ο Persei
Template:Location mark
Location of ο Persei (circled red)
Observation data
Epoch J2000      Equinox J2000
Constellation Perseus
A
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) 3.83[2]
B
Right ascension Template:RA[3]
Declination Template:DEC[3]
Apparent magnitude (V) 6.68[4]
Characteristics
A
Spectral type B1III / B2V[5]
U−B Template:Engvar −0.75[2]
B−V Template:Engvar +0.05[2]
Variable type ellipsoidal[6]
Astrometry
Radial velocity (Rv)+12.20[7] km/s
Absolute magnitude (MV)−4.4[5]
A
Proper motion (μ) RA: +6.091[1] mas/yr
Dec.: −9.732[1] mas/yr
Parallax (π)3.0224±0.3827 mas[1]
Distanceapprox. Template:Rnd ly
(approx. Template:Rnd pc)
Orbit[5]
PrimaryAa
CompanionAb
Period (P)4.4191447 days
Semi-major axis (a)Template:Solar radius
Eccentricity (e)0.0
Inclination (i)Template:Val°
Semi-amplitude (K1)
(primary)
111.8 km/s
Semi-amplitude (K2)
(secondary)
155.0 km/s
Details
Aa
Mass14[8] Template:Solar mass
Radius9.6[5] Template:Solar radius
Surface gravity (log g)3.4[8] cgs
Temperature22,700[8] K
Rotational velocity (v sin i)Template:Val[5] km/s
Ab
Mass10[8] Template:Solar mass
Radius8.9[5] Template:Solar radius
Surface gravity (log g)4.0[8] cgs
Temperature21,000[8] K
Metallicity [Fe/H]{{{metal_fe2}}} dex
Rotational velocity (v sin i)Template:Val[5] km/s
Age15[5] Myr
Other designations
Atik, 38 Persei, ADS 2726 AB, BD+31°642, CCDM J03443+3217AB, GC 4461, GSC 02359-01258, HIP 17448, HR 1131, HD 23180, SAO 56673, WDS J03443+3217AB
Database references
SIMBADdata

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Omicron Persei (ο Persei, abbreviated Omicron Per, ο Per) is a triple star system in the constellation of Perseus. From parallax measurements taken during the Hipparcos mission it is approximately 1,100 light-years (330 parsecs) from the Sun.

The system consists of a spectroscopic binary pair designated Omicron Persei A and a third companion Omicron Persei B.[9] A's two components are themselves designated Omicron Persei Aa (officially named Atik Template:IPAc-en, the traditional name of the system)[10][11] and Ab.

Etymology

File:Omicron Persei.jpg
ο Persei in optical light

ο Persei (Latinised to Omicron Persei) is the system's Bayer designation. The designations of the two constituents as Omicron Persei A and B, and those of A's components - Omicron Persei Aa and Ab - derive from the convention used by the Washington Multiplicity Catalog (WMC) for multiple star systems, and adopted by the International Astronomical Union (IAU).[12]

It bore the traditional name Atik (also Ati, Al Atik), Arabic for "the shoulder". Some sources attribute the name Atik to the nearby, brighter star Zeta Persei.[13][14] In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN)[15] to catalogue and standardize proper names for stars. The WGSN decided to attribute proper names to individual stars rather than entire multiple systems.[16] It approved the name Atik for the component Omicron Persei A on 12 September 2016 and it is now so included in the List of IAU-approved Star Names.[11]

In Chinese, Script error: No such module "Lang". (Script error: No such module "Lang".), meaning Rolled Tongue, refers to an asterism consisting of Omicron Persei, Nu Persei, Epsilon Persei, Xi Persei, Zeta Persei and 40 Persei.[17] Consequently, the Chinese name for Omicron Persei itself is Script error: No such module "Lang". (Script error: No such module "Lang".), "the Fifth Star of Rolled Tongue".[18]

Properties

File:OmicronPerLightCurve.png
A light curve for Omicron Persei A, plotted from TESS data[19]

Omicron Persei A is a spectroscopic binary consisting of a spectral type B1 giant and a type B2 dwarf orbiting each other every 4.4 days. The orbit is near-circular although its inclination is not precisely known. The two stars are separated by approximately Template:Solar radius, the exact value depending on the inclination. The primary is approximately one magnitude brighter than the secondary at visual wavelengths.[5] The binary pair forms a rotating ellipsoidal variable star, which varies in brightness from visual magnitude 3.79 to 3.88 during the orbital period.[20]

Omicron Persei lies just north of the open cluster IC 348, but is not catalogued as a member. Both IC 348 and Omicron Persei belong to the Perseus OB2 association.[21]

Culture

References

Template:Reflist

External links

Template:Stars of Perseus

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  14. Your Sky Object Catalogue: Named Stars
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  17. Template:In lang 中國星座神話, written by 陳久金. Published by 台灣書房出版有限公司, 2005, Template:ISBN.
  18. Template:In lang 香港太空館 - 研究資源 - 亮星中英對照表 Template:Webarchive, Hong Kong Space Museum. Accessed on line November 23, 2010.
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