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Mu Telescopii, Latinized from μ Telescopii is a solitary star in the southern constellation Telescopium. It has an apparent visual magnitude of 6.28, placing it near the limit of naked eye visibility. The object is relatively close at a distance of 118 light years but is receding with a heliocentric radial velocity of 8.6 km/s. It has been observed for infrared excess suggesting the presence of a debris disk but so far, none has been found.

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  • Mu Telescopii (es)
  • Mu Telescopii (en)
  • Mu Telescopii (pt)
  • My Telescopii (sv)
  • 望遠鏡座μ (zh)
rdfs:comment
  • Mu Telescopii (61 Telescopii) é uma estrela na direção da constelação de Telescopium. Possui uma ascensão reta de 19h 30m 34.57s e uma declinação de −55° 06′ 36.1″. Sua magnitude aparente é igual a 6.29. Considerando sua distância de 120 anos-luz em relação à Terra, sua magnitude absoluta é igual a 3.47. Pertence à classe espectral F5V. (pt)
  • My Telescopii ( μ Telescopii, förkortat My Tel, μ Tel) som är stjärnans Bayerbeteckning, är en ensam stjärna belägen i den mellersta delen av stjärnbilden Kikaren. Den har en skenbar magnitud på 6,30 och är nära gränsen för att vara synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 20,2 mas, beräknas den befinna sig på ett avstånd på ca 162 ljusår (ca 50 parsek) från solen. (sv)
  • 望遠鏡座μ,又名CP-55 9100,HD 183028、SAO 246131、HR 7393,是望遠鏡座的一颗恒星,视星等为6.3,位于銀經342.35,銀緯-27.42,其B1900.0坐标为赤經19h 22m 27.9s,赤緯-55° -27.42′ 54″。 (zh)
  • Mu Telescopii (μ Tel)​​ es una estrella en la constelación austral de Telescopium.Tiene magnitud aparente +6,29 y está a 120 años luz de distancia del Sistema Solar. Mu Telescopii es una estrella blanco-amarilla de la secuencia principal de tipo espectral F5V.Las dos componentes del sistema Diadem (α Comae Berenices), ι Pegasi A o ψ Capricorni son estrellas de parecidas características a Mu Telescopii.Esta última tiene una temperatura efectiva de 6503 ± 63 K y su radio es un 45% más grande que el radio solar.​Gira sobre sí misma con una velocidad de rotación proyectada de 11 km/s —límite inferior de la misma—,​ por lo que rota al menos 5 veces más deprisa que el Sol.Aunque presenta un contenido metálico inferior al del Sol, dos estudios determinan diferentes valores de -0,13​ y -0,24​ para (es)
  • Mu Telescopii, Latinized from μ Telescopii is a solitary star in the southern constellation Telescopium. It has an apparent visual magnitude of 6.28, placing it near the limit of naked eye visibility. The object is relatively close at a distance of 118 light years but is receding with a heliocentric radial velocity of 8.6 km/s. It has been observed for infrared excess suggesting the presence of a debris disk but so far, none has been found. (en)
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  • μ Telescopii (en)
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absmag v
  • +3.61 (en)
age gyr
appmag v
b-v
  • +0.45 (en)
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