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Beta Piscis Austrini, Latinized from β Piscis Austrini, is catalogued as a binary star system in the southern constellation of Piscis Austrinus. It is visible to the naked eye with an apparent visual magnitude of +4.29. Based upon an annual parallax shift of 22.84 mas as seen from the Earth, the star is located 143 light years from the Sun. These coordinates are a source of X-ray emission with a luminosity of 88.5×1020 W, which is most likely coming from a source other than the A-type stars. With Delta and Zeta it constituted Tien Kang ("heavenly rope") in China.

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rdfs:label
  • Beta Piscis Austrini (es)
  • Beta Piscis Austrini (en)
  • Beta Piscis Austrini (fr)
  • Beta Piscis Austrini (in)
  • 남쪽물고기자리 베타 (ko)
  • Beta Piscis Austrini (pt)
  • Бета Южной Рыбы (ru)
  • Beta Piscis Austrini (sv)
  • 败臼增一 (zh)
rdfs:comment
  • Beta Piscis Austrini adalah salah satu bintang pada rasi Piscis Austrinus. Bintang ini memiliki magnitudo 4.29 dan berada pada jarak 148 tahun cahaya dari Bumi. (in)
  • Бета Южной Рыбы (Beta PsA, β Piscis Austrini, β PsA) — звезда в созвездии Южной Рыбы. Видимая звёздная величина +4.29 (видна невооружённым глазом). Удалена приблизительно на 148 световых лет от Земли. С Дельтой и Дзетой она образует китайский астеризм Tien Kang («небесный канат»). (ru)
  • Beta Piscis Austrini (β Piscis Austrini, förkortat Beta PsA, β PsA) som är stjärnans Bayerbeteckning, är en dubbelstjärna belägen i den mellersta delen av stjärnbilden Södra fisken. Den har en kombinerad skenbar magnitud på 4,29 och är synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 22,8 mas, beräknas den befinna sig på ett avstånd på ca 143 ljusår (ca 44 parsek) från solen. (sv)
  • Beta Piscis Austrini (Tien Kang, 17 Piscis Austrini) é uma estrela na direção da Piscis Austrinus. Possui uma ascensão reta de 22h 31m 30.29s e uma declinação de −32° 20′ 45.7″. Sua magnitude aparente é igual a 4.29. Considerando sua distância de 148 anos-luz em relação à Terra, sua magnitude absoluta é igual a 1.00. Pertence à classe espectral A1V. (pt)
  • 敗臼增一 （南魚座β）在星表上是南天星座，南魚座內的一對聯星。它的視星等為肉眼可見的4.29等。依據從地球觀察得到的年周視差22.84mas，這顆恆星與太陽的距離是143光年。它的座標位置是X射線的發射源，亮度為88.5×1020 W，但這應該不是來自這顆A-型恆星，可能還有其它發射源。 Oblak（1978年）曾將其視為一顆三合星，但隨後就將其列為聯星。它的星等為4.29，主星A，是一顆白色的A型主序星，類型為 A1V。估計質量是2.3太陽質量，半徑是2.1太陽半徑。有效溫度是9,638K，來自光球層的發光強度是太陽亮度的37倍。紅外過量的證據顯示它有岩屑盤，估計其軌道距離主星12AU，溫度為188K。伴星B的星等為7.8，恆星分類為A2V，與主星距離30.3角秒。 敗臼增一相對於太陽以每秒14.4公里的速度在銀河系中移動。它投射的銀河軌道讓它在距離銀河中心23,900至28,300光年的軌道上運動。 在中國，它與敗臼一（天鶴座γ）、敗臼二、敗臼三和組成星官敗臼。 (zh)
  • Beta Piscis Austrini, Latinized from β Piscis Austrini, is catalogued as a binary star system in the southern constellation of Piscis Austrinus. It is visible to the naked eye with an apparent visual magnitude of +4.29. Based upon an annual parallax shift of 22.84 mas as seen from the Earth, the star is located 143 light years from the Sun. These coordinates are a source of X-ray emission with a luminosity of 88.5×1020 W, which is most likely coming from a source other than the A-type stars. With Delta and Zeta it constituted Tien Kang ("heavenly rope") in China. (en)
  • Beta Piscis Austrini (β PsA / 17 Piscis Austrini / HD 213398)​ es una estrella de magnitud aparente +4,29. Pese a su denominación de Bayer «Beta» es solo la cuarta estrella más brillante en la constelación de Piscis Austrinus, después de Fomalhaut (α Piscis Austrini), ε Piscis Austrini y δ Piscis Austrini.Junto a esta última y , era conocida en China como Tien Kang, «la cuerda celestial».​ (es)
  • Beta Piscis Austrini (β Piscis Austrini / β PsA) est une étoile binaire de la constellation australe du Poisson austral. Elle est visible à l'œil nu avec une magnitude apparente visuelle de +4,29. Sur la base d'une parallaxe annuelle de 22,84 mas, le système est situé à 143 années-lumière du Soleil. Ces coordonnées sont une source d'émission de rayons X avec une luminosité de 88,5 × 1020 W, qui provient très probablement d'une source autre que les étoiles de type A. Avec et , elle constituait Tien Kang ("corde céleste") en Chine. (fr)
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