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HD 133131 is a binary star in the constellation of Libra. It is roughly 168 light-years (51.5 parsecs) away from the Sun. It consists of two G-type main-sequence stars; neither are bright enough to be seen with the naked eye. Both components, HD 133131 A and B, are very similar to the Sun but are far older, about 6 billion years old. They also have low metallicities (50% of solar abundance), and HD 133131 A is additionally depleted in heavy elements compared to HD 133131 B, indicating a possibly past planetary engulfment event for HD 133131 B.

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  • HD 133131 (en)
  • HD 133131 (fr)
  • HD 133131 (it)
  • HD 133131 (ja)
  • HD 133131 (pt)
  • HD 133131 (sv)
  • HD 133131 (ru)
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  • HD 133131 is a binary star in the constellation of Libra. It is roughly 168 light-years (51.5 parsecs) away from the Sun. It consists of two G-type main-sequence stars; neither are bright enough to be seen with the naked eye. Both components, HD 133131 A and B, are very similar to the Sun but are far older, about 6 billion years old. They also have low metallicities (50% of solar abundance), and HD 133131 A is additionally depleted in heavy elements compared to HD 133131 B, indicating a possibly past planetary engulfment event for HD 133131 B. (en)
  • HD 133131 est un système stellaire et planétaire constitué de deux étoiles de et trois planètes, situé dans la constellation zodiacale de la Balance. L'étoile principale est entourée par deux planètes tandis que la seconde étoile abrite la troisième. (fr)
  • HD 133131は、地球から約140光年離れた位置にある連星系である。太陽によく似た2つのG型主系列星から成る。 (ja)
  • HD 133131 também conhecido como HIP 73674, é um sistema estelar binário localizado a uma distância de aproximadamente 163 anos-luz de distância da Terra. Esse sistema foi descoberto em 1972, na Universidade do Chile pelos astrônomos Jurgen Stock e Herbert Wroblewski, tem uma idade estimada de 9.5 bilhões de anos e é formado por duas estrelas gêmeas, ou seja, de mesmo tipo espectral, e que são também do mesmo tipo espectral que o Sol, G2V. Essas duas estrelas estão separadas por um distância de 360 UA. (pt)
  • HD 133131 är en dubbelstjärna belägen i den södra delen av stjärnbilden Vinkelhaken. Den har en skenbar magnitud av ca 8,40 och kräver åtminstone en stark handkikare eller ett mindre teleskop för att kunna observeras. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 19,4 mas, beräknas den befinna sig på ett avstånd på ca 168 ljusår (ca 52 parsek) från solen. Den rör sig närmare solen med en heliocentrisk radialhastighet på ca -16 km/s. (sv)
  • HD 133131 — двойная звезда в созвездии Весов. Другие обозначения — CPD−27° 5116, HIP 73674. Находится на расстоянии 153 световых лет (47 парсек) от Солнца. Это первая двойная звёздная система, в которой планеты обнаружены и у основной звезды, и у звезды-компаньона. Планеты у звезды HD 133131 A искали с помощью спектрографа MIKE телескопа Магеллан и спектрографа PFS телескопа Магеллан II (телескоп Клея). С помощью спектрографа PFS также искали планеты у звезды HD 133131 B. (ru)
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  • HD 133131 A (en)
  • HD 133131 B (en)
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age gyr
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  • G2 + G2 (en)
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  • HD 133131 A (en)
  • HD 133131 B (en)
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  • c (en)
  • b (en)
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