Zeta Andromedae
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Zeta Andromedae, also named Shimu,[9] is a binary star system in the northern constellation Andromeda. It is visible to the naked eye with an apparent visual magnitude that varies from Template:Val over the course of its 17.7 day orbit.[2] Based on parallax measurements, it is located at a distance of approximately 181 light-years from the Sun. The system is drifting closer with a heliocentric radial velocity of −24.4 km/s.[5]
Naming
The star's location is in the northern constellation Andromeda, in which it is the second-most southerly of the stars in this often drawn characteristic shape representing the mythical princess asterism, after η Andromedae.
Zeta Andromedae (Zeta And, ζ Andromedae, ζ And) is the star's Bayer designation. It also has the Flamsteed designation 34 Andromedae and multiple other designations in stellar catalogues.
In Chinese, Script error: No such module "Lang". (Script error: No such module "Lang".), meaning Legs (asterism), refers to an asterism consisting of ζ Andromedae, η Andromedae, 65 Piscium, ε Andromedae, δ Andromedae, π Andromedae, ν Andromedae, μ Andromedae, β Andromedae, σ Piscium, τ Piscium, 91 Piscium, υ Piscium, φ Piscium, χ Piscium and ψ1 Piscium. Consequently, the Chinese name for ζ Andromedae itself is Script error: No such module "Lang". (Script error: No such module "Lang"., Template:Langx).[10]
An older Chinese name is Tian Shi Mu, The Eye of the Celestial Pig. Based on this, the IAU Working Group on Star Names approved the name Shimu for this star on 16 March 2025 and it is now so entered in the IAU Catalog of Star Names.[9]
System
The system is a spectroscopic binary whose Template:Abbreviation is classified as an orange K-type giant with a mean apparent magnitude of +4.08. Due to brightness changes caused by the ellipsoidal shape of that object, the system is also an RS Canum Venaticorum-type variable star. It is a magnetically active star with a brightness that varies from magnitude +3.92 to +4.14 over a period of 17.77 days, and its spectrum shows strong and variable Ca II H and K lines. The orbital period of the binary is 17.77 days.[3]
The primary component of this binary system, Zeta Andromedae Aa, is one of the few stars who has been resolved using Doppler imaging and long-baseline infrared interferometry. With resolved images astronomers can recover additional information about this star.
| Parameter | Value |
|---|---|
| Oblateness | 1.060±0.011 |
| Polar radius | Template:Val |
| Axis InclinationTemplate:Efn | Template:Val |
| Pole angleTemplate:Efn | Template:Val |
Resolved images also allowed observation of starspots (the analogue to sunspots), on this star, and their asymmetric distribution showed that the magnetic field of the star is generated by a mechanism different from the solar dynamo.[12] A Sun-like differential rotation of the star was observed instead.[3]
Visual companions
The WDS notes three visual companions to the eclipsing binary (Aa and Ab, forming binary A).[4] The parallax of the D star has been measured by Gaia proving its distance to be much greater than Zeta Andromedae, probably a distant red giant.[13] The closest companion, B, is likewise a background object.[14] The companion C at Template:Val shares a common proper motion and a similar parallax.[15]
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Template:Componentbox component Template:Componentbox component Template:Componentbox component Template:Componentbox end |
Notes
References
External links
- Zeta Andromedae Template:Webarchive at Alcyone Software's Star Data Pages
- Image ζ Andromedae
- Rachael Roettenbacher, "How the face of a distant star reveals our place in the cosmos," Aeon Magazine [retrieved July 27, 2016]
Template:Stars of Andromeda Template:Sky
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- Pages with script errors
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- K-type giants
- K-type main-sequence stars
- Spectroscopic binaries
- RS Canum Venaticorum variables
- Rotating ellipsoidal variables
- Multiple stars
- Andromeda (constellation)
- Bayer objects
- Bright Star Catalogue objects
- Durchmusterung objects
- Flamsteed objects
- Henry Draper Catalogue objects
- Hipparcos objects
- Stars with proper names
- Pages with reference errors