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Psi Phoenicis (ψ Phoenicis) is a star in the constellation Phoenix. Its apparent magnitude varies from 4.3 to 4.5 with a period of about 30 days and it is approximately 342 light years away based on parallax. Psi Phoenicis is considered a single star, and has no known companions. It has been considered a possible spectroscopic binary, including in the Hipparcos Catalogue, which stems from spectroscopic observations in 1919 which showed a possibly variable radial velocity. More recent data, however, showed the velocity to be constant.

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  • Psi Phoenicis (es)
  • Psi Phoenicis (en)
  • Psi Phoenicis (pt)
  • Psi Phoenicis (sv)
  • 鳳凰座ψ (zh)
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  • Psi Phoenicis är en halvregelbunden variabel av SR-typ i stjärnbilden Fenix. Stjärnan varierar mellan visuell magnitud +4,3 och 4,5 med en period av 30 dygn. (sv)
  • 鳳凰座ψ,又名CD-46 552,HD 11695、SAO 215696、HR 555,是鳳凰座的一颗恒星,视星等为4.41,位于銀經274.35,銀緯-67.22,其B1900.0坐标为赤經1h 49m 38.2s,赤緯-46° -67.22′ 32″。 (zh)
  • Psi Phoenicis (ψ Phe / HD 11695 / HR 555)​ es una estrella en la constelación de Fénix. Se encuentra a unos 321 años luz del Sistema Solar. Psi Phoenicis es una gigante roja de tipo espectral M4III​con una temperatura superficial de 3415 ± 87 K.De magnitud aparente media +4,44, es una de las pocas gigantes rojas que se pueden observar a simple vista, al igual que γ Phoenicis, algo más brillante y en esta misma constelación.La medida de su diámetro angular —considerando el — es de 8,7 ± 0,3 milisegundos de arco.​Este valor corresponde a un diámetro estelar 85 veces más grande que el del Sol, igual a 0,40 UA, aproximadamente la distancia existente entre Mercurio y el Sol.Gira sobre sí misma con una velocidad de rotación proyectada entre 2,5 y 3,9 km/s.​Su luminosidad es 882 veces superior a (es)
  • Psi Phoenicis (ψ Phoenicis) is a star in the constellation Phoenix. Its apparent magnitude varies from 4.3 to 4.5 with a period of about 30 days and it is approximately 342 light years away based on parallax. Psi Phoenicis is considered a single star, and has no known companions. It has been considered a possible spectroscopic binary, including in the Hipparcos Catalogue, which stems from spectroscopic observations in 1919 which showed a possibly variable radial velocity. More recent data, however, showed the velocity to be constant. (en)
  • Psi Phoenicis (ψ Phoenicis) é uma estrela na constelação de Phoenix. Possui uma magnitude aparente visual média de 4,4, sendo visível a olho nu em locais sem muita poluição luminosa. De acordo com medições de paralaxe pela sonda Gaia, encontra-se a uma distância de aproximadamente 335 anos-luz (103 parsecs) da Terra. Sua magnitude absoluta visual é de −0,7. (pt)
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  • ψ Phoenicis (en)
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  • http://commons.wikimedia.org/wiki/Special:FilePath/Red_circle.svg
  • http://commons.wikimedia.org/wiki/Special:FilePath/Phoenix_constellation_map.svg
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