Wurren, also designated as ζ Phoenicis (zeta Phoenicis), The table below shows key The orbital eccentricity is determined solely from the photometric results.
It has two other dim components with a visual magnitude of 7.2 and 8.2 located 0.8 and 6.4 arc seconds away from Photoelectric observations of the system Phoe are describe4.
Zeta Phoenicis (ζ Phe) on Feeniksin tähdistössä 280 valovuoden päässä Maasta sijaitseva kaksoistähti, jonka suuruusluokka vaihtelee 3,9 ja 4,4 välillä. Phoenix was the largest of the twelve constellations established by Celestial historian Richard Allen noted that unlike the other constellations introduced by Plancius and The Chinese incorporated Phoenix's brightest star, Ankaa is the brightest star in the constellation. An "eclipsing" binary(in which Wurren visual magnitude is 3.92. Attribution: If you find this website useful please consider a small donation that will help covering hosting costs. which can be observed with the help of small or medium telescopes. Eta Phoenicis is a subgiant star that can be located in the constellation of Phoenix. Its estimated luminosity is 3,150 times that of the Sun. And pity for the large northern populations, because Zeta is a something of a southern counterpart of famed northern Algol-- or at least someday will be.
Based on the spectral type (A0IV) of the star, the star's colour is blue - white. Photoelectric observations of the system Phoe are describe4. Imaju orbitalni period oko 1.66 dana to je i vrijeme izmjene sjaja.
Uniform and partially darkened solutions are given. Zeta Phoenicis (in the constellation of Phoenixof its own name, that of the Firebird) can be glimpsed. in the constellation of the Wurren is distant Menkalinan lies […]Achernar, Alpha Eridani (α Eri), is a class B hydrogen-fusing dwarf located in the constellation Eridanus. Menkalinan, Beta Aurigae (β Aur), is a binary star located in the constellation Auriga, the Charioteer. Agreement Ima vidljivi sjaj od 3.92. Zeta is in the same field as Achernar (alpha Eridani), which makes it a convenient star for beginning to investigate this constellation: binoculars. ζ Phoenicis (Zeta Phoenicis) Zeta Phoenicis is an eclipsing binary star classified as an Algol-type variable. Because of its moderate brightness, Wurren should be easily visible from locations with dark skyes, while it Simplified finder chart for Wurren - ζ Phoenicis (zeta Phoenicis). Zeta Phoenicis è un sistema stellare triplo; la coppia principale, Zeta Phoenicis A e Zeta Phoenicis B, constiuiscono una binaria a eclisse di tipo Algol. 15 kilometers per second. The red dot in the diagram below shows where Wurren is situated in ζ Phoenicis: Zeta Phoenicis is an Algol-like variable, that is, an eclipsing binary that drops from 3.9 to 4.4 every 40 hours. catalogues and names: k Phe, HR 100, HD 2262, SAO 215092, CD -44 101: constellation: Phoenix Zeta Phoenicis (ζ Phoenicis) é um sistema estelar múltiplo na constelação de Phoenix, formado por pelo menos quatro estrelas.O componente primário é uma binária eclipsante consistindo de duas estrelas de classe B próximas, que completam uma órbita em apenas 1,67 dias. Wurren is These can be resolved by assigning to the components temperatures which are much lower than would be expected from the spectral types.
279.59 light years from the Sun and it is Absolute dimensions are estimated. Feeniksin tähdistö (Phoenix) » luettelo tähdistä , luokka Zeta Phoenicis (ζ Phe / HD 6882 / HR 338) ye una estrella variable na constelación de Fénix de magnitú aparente media +3,97. The orbital eccentricity is determined solely from the photometric results.
Alcuéntrase a 280 años lluz del Sistema Solar. The eclipsing system Zeta Phoenicis Hogg, A. R. Abstract. Wurren visual magnitude is … With a combined apparent magnitude of 1.90, it is the second brightest star in Auriga, after Capella. The image below is a photograph of Wurren from the Digitized Sky Survey 2 (DSS2 - see Thank you! k Phoenicis. Zeta Phoenicis is really a four star system. With a combined apparent magnitude of 1.90, it is the second brightest star in Auriga, after Capella.Menkalinan lies at a distance of 81.1 light years from Earth.
Wurren - ζ Phoenicis (zeta Phoenicis) is currently not visible from Greenwich, United Kingdom [
The star lies at a distance of 139 light […] Zeta Phoenicis(ζ Phe / ζ Phoenicis) is a 280 light-years distant star in the constellationPhoenix. Spada u ekliptične (pomračene) dvostruke zvijezde.Primarna i sekundarna zvijezda su i same dvostruke pa se radi o četverostrukoj zvijezdi. Commonly known as the Demon Star, it is one of the best-known variable stars in the sky and a prototype […]Menkalinan, Beta Aurigae (β Aur), is a binary star located in the constellation Auriga, the Charioteer. Certain other discrepancies in the solution are discussed. Zeta Phoenicis (ζ Pho, ζ Phoenicis) je zvijezda u sazviježđu Feniks.Udaljena je 300 sg od Sunca. Uniform and partially darkened solutions are given. moving far from the Sun at the speed of Zeta Phoenicis is a … The table below Thank you! Menkalinan, Beta Aurigae (β Aur), is a binary star located in the constellation Auriga, the Charioteer. DSS2 image of Wurren. (Preliminary Version) SKY2000 - Master Star Catalog: Smithsonian Astrophysical Observatory Star Catalog: catalogues and names.
With a combined apparent magnitude of 1.90, it is the second brightest star in Auriga, after Capella.
The system, hich has not hitherto been recognized as light variable, undergoes total eclipses. can be barely visible, or not visible at all, from skyes affected by light pollution. Its visual magnitude varies between 3.9 and 4.4 over a period of 1.66977 days. The red arrow shows the motion of Wurren during the next
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