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HD 13189는 삼각형자리에 있는 항성으로, 겉보기 등급은 +8이다. 13189는 오렌지색 거성으로 지구에서 603광년 떨어져 있다. 질량은 태양의 4.5배로 주계열성이었을 때 B 분광형이었을 것으로 추측된다. 절대 등급은 +1이다. 이 별은 행성 또는 갈색 왜성으로 추정되는 동반 천체를 거느리고 있다.
, HD 13189 är en ensam stjärna belägen i den … HD 13189 är en ensam stjärna belägen i den mellersta delen av stjärnbilden Triangeln. Den har en skenbar magnitud av ca 7,57 och kräver åtminstone en stark handkikare eller ett mindre teleskop för att kunna observeras. Baserat på parallax enligt Gaia Data Release 2 på ca 1,98 mas, beräknas den befinna sig på ett avstånd på ca 1 650 ljusår (ca 500 parsek) från solen. Den rör sig bort från solen med en heliocentrisk radialhastighet på ca +25 km/s.iocentrisk radialhastighet på ca +25 km/s.
, HD 13189 is an 8th magnitude star in Trian … HD 13189 is an 8th magnitude star in Triangulum constellation. In 2005, a planetary companion or brown dwarf was announced in orbit around this star. At the time, the parallax estimate was 0.54±0.93 mas, which would suggest a distance of 6,040 ly (1,850 pc) with a high margin of error. In 2007, van Leeuwen published a revised parallax measurement of 1.78±0.73 mas, which corresponds to a distance of 1,830 ly (560 pc) with a smaller but still significant margin of error. In 2022 the Gaia spacecraft measured a parallax of 2.0450±0.0240 mas which is a distance of 1,590 ly (489 pc) with an error of only 20 ly (6 pc). It has a spectral classification of K1II-III, making it a giant star that has evolved away from the main sequence. The mass is 1.2 times the Sun's, while measurements of the star's radius give estimates of 38 R☉. The atmosphere of the star displays short period radial velocity variations with a primary period of 4.89 days. This behavior is typical for giant K-type stars such as this and it is not the result of a close-orbit planetary companion.sult of a close-orbit planetary companion.
, HD 13189 — звезда в созвездии Треугольник на расстоянии около 603 световых лет от Солнечной системы. Вокруг звезды обращается, как минимум, одна планета .
, HD 13189 ist ein Riesenstern der Spektralk … HD 13189 ist ein Riesenstern der Spektralklasse K2. Er besitzt eine scheinbare Helligkeit von 7,57 mag. Die Masse von HD 13189 beträgt etwa zwei bis sieben Sonnenmassen. Astronomen der Friedrich-Schiller-Universität Jena veröffentlichten im Jahr 2005 ihre an der Thüringer Landessternwarte gemachte Entdeckung eines Objektes, das um diesen Stern kreist und bei dem es sich um einen Braunen Zwerg oder Exoplaneten handeln könnte.nen Zwerg oder Exoplaneten handeln könnte.
, HD 13189是一個位於三角座的8等恆星。
, HD 13189 est une étoile de la constellatio … HD 13189 est une étoile de la constellation boréale du Triangle. Sa magnitude apparente est égale à 7,56. Elle est distante d'environ ∼1 650 a.l. (∼506 pc) de la Terre. Il s'agit d'une étoile géante de type spectral K2. Sa masse vaut deux à sept masses solaires. Les astronomes de l'Université d'Iéna ont publié en 2005 leur découverte à l'observatoire Karl-Schwarzschild d'un objet qui est en rotation autour de cette étoile et qu'il pourrait s'agir d'une naine brune ou d'une exoplanète.gir d'une naine brune ou d'une exoplanète.
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HD 13189 est une étoile de la constellatio … HD 13189 est une étoile de la constellation boréale du Triangle. Sa magnitude apparente est égale à 7,56. Elle est distante d'environ ∼1 650 a.l. (∼506 pc) de la Terre. Il s'agit d'une étoile géante de type spectral K2. Sa masse vaut deux à sept masses solaires. Les astronomes de l'Université d'Iéna ont publié en 2005 leur découverte à l'observatoire Karl-Schwarzschild d'un objet qui est en rotation autour de cette étoile et qu'il pourrait s'agir d'une naine brune ou d'une exoplanète.gir d'une naine brune ou d'une exoplanète.
, HD 13189 ist ein Riesenstern der Spektralk … HD 13189 ist ein Riesenstern der Spektralklasse K2. Er besitzt eine scheinbare Helligkeit von 7,57 mag. Die Masse von HD 13189 beträgt etwa zwei bis sieben Sonnenmassen. Astronomen der Friedrich-Schiller-Universität Jena veröffentlichten im Jahr 2005 ihre an der Thüringer Landessternwarte gemachte Entdeckung eines Objektes, das um diesen Stern kreist und bei dem es sich um einen Braunen Zwerg oder Exoplaneten handeln könnte.nen Zwerg oder Exoplaneten handeln könnte.
, HD 13189는 삼각형자리에 있는 항성으로, 겉보기 등급은 +8이다. 13189는 오렌지색 거성으로 지구에서 603광년 떨어져 있다. 질량은 태양의 4.5배로 주계열성이었을 때 B 분광형이었을 것으로 추측된다. 절대 등급은 +1이다. 이 별은 행성 또는 갈색 왜성으로 추정되는 동반 천체를 거느리고 있다.
, HD 13189 är en ensam stjärna belägen i den … HD 13189 är en ensam stjärna belägen i den mellersta delen av stjärnbilden Triangeln. Den har en skenbar magnitud av ca 7,57 och kräver åtminstone en stark handkikare eller ett mindre teleskop för att kunna observeras. Baserat på parallax enligt Gaia Data Release 2 på ca 1,98 mas, beräknas den befinna sig på ett avstånd på ca 1 650 ljusår (ca 500 parsek) från solen. Den rör sig bort från solen med en heliocentrisk radialhastighet på ca +25 km/s.iocentrisk radialhastighet på ca +25 km/s.
, HD 13189 — звезда в созвездии Треугольник на расстоянии около 603 световых лет от Солнечной системы. Вокруг звезды обращается, как минимум, одна планета .
, HD 13189 is an 8th magnitude star in Trian … HD 13189 is an 8th magnitude star in Triangulum constellation. In 2005, a planetary companion or brown dwarf was announced in orbit around this star. At the time, the parallax estimate was 0.54±0.93 mas, which would suggest a distance of 6,040 ly (1,850 pc) with a high margin of error. In 2007, van Leeuwen published a revised parallax measurement of 1.78±0.73 mas, which corresponds to a distance of 1,830 ly (560 pc) with a smaller but still significant margin of error. In 2022 the Gaia spacecraft measured a parallax of 2.0450±0.0240 mas which is a distance of 1,590 ly (489 pc) with an error of only 20 ly (6 pc).89 pc) with an error of only 20 ly (6 pc).
, HD 13189是一個位於三角座的8等恆星。
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HD 13189
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