Lambda Tauri

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Names in other languages

  • caLambda del Taure
  • uzSigir lyambdasi
  • Русскийлямбда Тельца
  • astLambda Tauri
  • DeutschLambda Tauri
  • EnglishLambda Tauri35 Tauri, 35 Tau, λ Tauri, λ Tau, lam Tau, SAO 93719, SRS 30150, PPM 119535, ROT 590, Elthor, HR 1239, HGAM 314, HD 25204, HIP 18724, HIC 18724, GC 4805, PLX 883, ALS 17279, GCRV 2290
  • EnglishLambda Tauri
  • EnglishLambda Tauri
  • EspañolLambda Tauri35 Tauri
  • FrançaisLambda Tauri35 Tauri, HR 1239
  • gaLambda Tauri
  • glLambda Tauri
  • ItalianoLambda Tauri
  • NederlandsLambda Tauri
  • Polskilambda TauriElthor
  • PortuguêsLambda Tauri
  • PortuguêsLambda Tauri
  • skLambda Tauri
  • SvenskaLambda Tauri
  • فارسیلاندا گاو
  • ΕλληνικάΛ ΤαύρουΛάμδα Ταύρου
  • 日本語おうし座ラムダ星おうし座λ星, おうし座λ, おうし座35番星
  • 한국어황소자리 람다
  • mulElthor* lam Tau, V* lam Tau
  • 中文毕宿八HD 25204, 金牛座λ
  • 简体中文毕宿八
  • 繁體中文畢宿八
  • 中文畢宿八

Article bodies are English and are not machine-translated. A name in another language is not a translation of the article.

Lambda Tauri (Latinized from λ Tauri), formally named Bibing, is a triple star system in the constellation Taurus. In 1848, the light from this system was found to vary periodically and it was determined to be an eclipsing binary system—the third such discovered. The components of this system have a combined apparent visual magnitude of +3.37 at its brightest, making it one of the brighter members of the constellation. Based upon parallax measurements from the Hipparcos mission, the distance to this system is approximately .

Lambda Tauri (Latinized from λ Tauri), formally named Bibing, is a triple star system in the constellation Taurus. In 1848, the light from this system was found to vary periodically and it was determined to be an eclipsing binary system—the third such discovered. The components of this system have a combined apparent visual magnitude of +3.37 at its brightest, making it one of the brighter members of the constellation. Based upon parallax measurements from the Hipparcos mission, the distance to this system is approximately . ==References==

Text derived from https://en.wikipedia.org/w/index.php?oldid=1374742723 under CC BY-SA 4.0; modifications have been made.