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Theta Volantis, Latinized from θ Volantis, is a solitary star in the southern constellation of Volans. Based upon parallax measurements, is approximately 240 light years from the Sun. It has an apparent visual magnitude of 5.19, which is bright enough to be faintly visible to the naked eye. The star has two optical companions: a magnitude 15.0 star at an angular separation of 22.10″ along a position angle of 58°, and a magnitude 10.64 star at an angular separation of 41.3″ along a position angle of 105° (both as of 2000).

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  • Theta Volantis, Latinized from θ Volantis, is a solitary star in the southern constellation of Volans. Based upon parallax measurements, is approximately 240 light years from the Sun. It has an apparent visual magnitude of 5.19, which is bright enough to be faintly visible to the naked eye. Theta Volantis is an A-type main sequence star with a stellar classification of A0 V and a mass around 2.3 times that of the Sun. It is a young star with an estimated age of a few hundred million years, and is spinning rapidly with a projected rotational velocity of 98 km/s. Theta Volantis shines 37 times as brightly as the Sun, with an effective temperature of 8,753 K in its outer atmosphere. The star has two optical companions: a magnitude 15.0 star at an angular separation of 22.10″ along a position angle of 58°, and a magnitude 10.64 star at an angular separation of 41.3″ along a position angle of 105° (both as of 2000). (en)
  • Theta Volantis (θ Vol) – biała gwiazda ciągu głównego typu widmowego A, znajdująca się w gwiazdozbiorze Ryby Latającej. Jej obserwowana wielkość gwiazdowa wynosi +5,19m. Oddalona jest o około 239 lat świetlnych od Słońca. (pl)
  • Theta Volantis (θ Vol, θ Volantis) é uma estrela na constelação de Volans. Tem uma magnitude aparente visual de 5,20, sendo visível a olho nu em locais com pouca poluição luminosa. Com base em medições de paralaxe, está localizada a aproximadamente 237 anos-luz (72,7 parsecs) da Terra. É uma estrela de classe A da sequência principal com um tipo espectral de A0 V e temperatura efetiva de 10 083 K. Forma uma estrela dupla óptica com uma estrela de magnitude aparente 15 a uma separação de 21,4 segundos de arco na esfera celeste, que é uma fonte de raios X com uma luminosidade de 2,143×1022 W. Essa estrela não está relacionada fisicamente com Theta Volantis. (pt)
  • Theta Volantis (θ Volantis, förkortat Theta Vol, θ Vol) som är stjärnans Bayerbeteckning, är en enkel stjärna belägen i den östra delen av stjärnbilden Flygfisken. Den har en skenbar magnitud på 5,19 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 13,6 mas, beräknas den befinna sig på ett avstånd på ca 240 ljusår (ca 74 parsek) från solen. (sv)
  • 飛魚座θ,又名CP-69 946,HD 74405、SAO 256535、HR 3460,是飛魚座的一颗恒星,视星等为5.2,位于銀經284.68,銀緯-17.12,其B1900.0坐标为赤經8h 38m 43.1s,赤緯-70° -17.12′ 47″。 (zh)
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  • +0.01 (en)
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  • A0 V (en)
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  • Theta Volantis (θ Vol) – biała gwiazda ciągu głównego typu widmowego A, znajdująca się w gwiazdozbiorze Ryby Latającej. Jej obserwowana wielkość gwiazdowa wynosi +5,19m. Oddalona jest o około 239 lat świetlnych od Słońca. (pl)
  • Theta Volantis (θ Vol, θ Volantis) é uma estrela na constelação de Volans. Tem uma magnitude aparente visual de 5,20, sendo visível a olho nu em locais com pouca poluição luminosa. Com base em medições de paralaxe, está localizada a aproximadamente 237 anos-luz (72,7 parsecs) da Terra. É uma estrela de classe A da sequência principal com um tipo espectral de A0 V e temperatura efetiva de 10 083 K. Forma uma estrela dupla óptica com uma estrela de magnitude aparente 15 a uma separação de 21,4 segundos de arco na esfera celeste, que é uma fonte de raios X com uma luminosidade de 2,143×1022 W. Essa estrela não está relacionada fisicamente com Theta Volantis. (pt)
  • Theta Volantis (θ Volantis, förkortat Theta Vol, θ Vol) som är stjärnans Bayerbeteckning, är en enkel stjärna belägen i den östra delen av stjärnbilden Flygfisken. Den har en skenbar magnitud på 5,19 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 13,6 mas, beräknas den befinna sig på ett avstånd på ca 240 ljusår (ca 74 parsek) från solen. (sv)
  • 飛魚座θ,又名CP-69 946,HD 74405、SAO 256535、HR 3460,是飛魚座的一颗恒星,视星等为5.2,位于銀經284.68,銀緯-17.12,其B1900.0坐标为赤經8h 38m 43.1s,赤緯-70° -17.12′ 47″。 (zh)
  • Theta Volantis, Latinized from θ Volantis, is a solitary star in the southern constellation of Volans. Based upon parallax measurements, is approximately 240 light years from the Sun. It has an apparent visual magnitude of 5.19, which is bright enough to be faintly visible to the naked eye. The star has two optical companions: a magnitude 15.0 star at an angular separation of 22.10″ along a position angle of 58°, and a magnitude 10.64 star at an angular separation of 41.3″ along a position angle of 105° (both as of 2000). (en)
rdfs:label
  • Theta Volantis (pl)
  • Theta Volantis (pt)
  • Theta Volantis (en)
  • Theta Volantis (sv)
  • 飛魚座θ (zh)
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  • θ Volantis (en)
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