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Tau Aquilae, Latinized from τ Aquilae, is the Bayer designation for a star in the equatorial constellation of Aquila. The apparent visual magnitude of 5.7 indicates it is a faint star that is visible to the naked eye from suburban skies; at least according to the Bortle Dark-Sky Scale. The annual orbital motion of the Earth causes a parallax shift of 5.94 mas, which means the distance to this star is approximately 549 light-years (168 parsecs). The magnitude of the star is diminished by 0.28 from extinction caused by interstellar gas and dust. It is drifting closer to the Sun with a radial velocity of −29 km/s.

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rdf:type
rdfs:label
  • Tau de l'Àguila (ca)
  • Tau Aquilae (in)
  • Tau Aquilae (fr)
  • Tau Aquilae (it)
  • Tau Aquilae (pt)
  • Tau Aquilae (en)
  • Tau Aquilae (sv)
  • 河鼓增七 (zh)
rdfs:comment
  • Tau de l'Àguila (τ Aquilae) és una estrella de la constel·lació de l'Àguila. Tau de l'Àguila és una estrella gegant taronja del tipus K de la magnitud aparent 5,51. Està aproximadament a 527 anys llum de la Terra. (ca)
  • Tau Aquilae est une étoile de la constellation de l'Aigle, située à ∼549 a.l. (∼168 pc) de la Terre. (fr)
  • Tau Aquilae (τ Aql, τ Aquilae) adalah salah satu bintang yang berada di rasi Aquila. Tau Aquilae adalah bintang raksasa jingga tipe K dengan magnitudo 5.51. Bintang ini berada pada jarak 527 tahun cahaya dari Bumi. Pada Almagest, bintang ini disebutkan sebagai quae in medio capite, berarti "yang berada di tengah ekor (sang elang) (in)
  • Tau Aquilae (τ Aql / τ Aquilae) è una stella gigante arancione di magnitudine 5,52 situata nella costellazione dell'Aquila. Dista 527 anni luce dal sistema solare. (it)
  • Tau Aquilae (63 Aquilae) é uma estrela na direção da constelação de Aquila. Possui uma ascensão reta de 20h 04m 08.31s e uma declinação de +07° 16′ 40.6″. Sua magnitude aparente é igual a 5.51. Considerando sua distância de 527 anos-luz em relação à Terra, sua magnitude absoluta é igual a −0.53. Pertence à classe espectral K0III. (pt)
  • Tau Aquilae (τ Aqulilae, förkortat Tau Aql, τ Aql) är en ensam stjärna belägen i den mellersta delen av stjärnbilden Örnen. Den har en skenbar magnitud på 5,68 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 7,1 mas, beräknas den befinna sig på ett avstånd på ca 460 ljusår (ca 142 parsek) från solen. På det beräknade avståndet minskar stjärnans skenbara magnitud med 0,28 enheter genom skymning orsakad av interstellär gas och stoft. (sv)
  • 天鷹座τ,又名BD+06 4416,HD 190327、SAO 125403、HR 7669,是天鷹座的一颗恒星,视星等为5.52,位于銀經48.01,銀緯-12.57,其B1900.0坐标为赤經19h 59m 15.2s,赤緯+6° -12.57′ 44″。 (zh)
  • Tau Aquilae, Latinized from τ Aquilae, is the Bayer designation for a star in the equatorial constellation of Aquila. The apparent visual magnitude of 5.7 indicates it is a faint star that is visible to the naked eye from suburban skies; at least according to the Bortle Dark-Sky Scale. The annual orbital motion of the Earth causes a parallax shift of 5.94 mas, which means the distance to this star is approximately 549 light-years (168 parsecs). The magnitude of the star is diminished by 0.28 from extinction caused by interstellar gas and dust. It is drifting closer to the Sun with a radial velocity of −29 km/s. (en)
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