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HD 156411 is a 7th magnitude G-type main-sequence star located approximately 186 light years away in the southern constellation Ara. This star is larger, hotter, brighter, and more massive than the Sun. Its metal content is three-fourths as much as the Sun. The star is around 4.3 billion years old and is spinning with a projected rotational velocity of 1.8 km/s. Naef and associates (2010) noted the star appears to be slightly evolved, and thus may be in the process of leaving the main sequence. In 2009, a gas giant planet was found in orbit around the star.

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  • HD 156411 (en)
  • HD 156411 (it)
  • HD 156411 (ja)
  • HD 156411 (pt)
  • HD 156411 (sv)
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  • HD 156411 è stella situata nella costellazione dell'Altare a circa 179 anni luce di distanza dal Sole. Avendo una magnitudine apparente di 6,67, non è visibile ad occhio nudo ma si può osservare facilmente con un binocolo. Nel 2009 è stato scoperto un pianeta extrasolare che le orbita attorno, . (it)
  • HD 156411は、地球からさいだん座の方向に約190光年離れた位置にある7等級の恒星である。 (ja)
  • Inquill eller HD 156411 är en ensam stjärna belägen i den norra delen av stjärnbilden Altaret. Den har en skenbar magnitud av ca 6,67 och kräver åtminstone en handkikare för att kunna observeras. Baserat på parallax enligt Gaia Data Release 2 på ca 17,6 mas, beräknas den befinna sig på ett avstånd på ca 186 ljusår (ca 57 parsek) från solen. Den rör sig närmare solen med en heliocentrisk radialhastighet på ca -39 km/s. (sv)
  • HD 156411 is a 7th magnitude G-type main-sequence star located approximately 186 light years away in the southern constellation Ara. This star is larger, hotter, brighter, and more massive than the Sun. Its metal content is three-fourths as much as the Sun. The star is around 4.3 billion years old and is spinning with a projected rotational velocity of 1.8 km/s. Naef and associates (2010) noted the star appears to be slightly evolved, and thus may be in the process of leaving the main sequence. In 2009, a gas giant planet was found in orbit around the star. (en)
  • HD 156411 é uma estrela na constelação de Ara. Tem uma magnitude aparente de 6,67, sendo invisível a olho nu. Medições de paralaxe mostram que está a uma distância de 179 anos-luz (55 parsecs) da Terra, com uma margem de erro de 5 anos-luz. Em 2009 foi descoberto um planeta extrassolar gigante gasoso ao redor de HD 156411. Tem uma massa mínima de 0,74 massas de Júpiter, e orbita a estrela a uma distância média de 1,88 UA a cada 842,2 dias. (pt)
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