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HD 145377 is a star in the southern constellation Scorpius. It has an apparent visual magnitude of 8.10 and can be viewed with a small telescope. The star is located at a distance of 175 light years from the Sun based on parallax, and it is drifting further away with a radial velocity of +11.6. The absolute magnitude of this star is 4.31, indicating it would be visible to the naked eye if it were at a distance of 10 parsecs.

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  • HD 145377 (en)
  • HD 145377 (fr)
  • HD 145377 (pl)
  • HD 145377 (pt)
  • HD 145377 (ru)
  • HD 145377 (sv)
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  • HD 145377 är en ensam stjärna belägen i den mellersta delen av stjärnbilden Skorpionen. Den har en skenbar magnitud av ca 8,10 och kräver åtminstone en stark handkikare eller ett mindre teleskop för att kunna observeras. Baserat på parallax enligt Gaia Data Release 2 på ca 18,7 mas, beräknas den befinna sig på ett avstånd på ca 175 ljusår (ca 54 parsek) från solen. Den rör sig bort från solen med en heliocentrisk radialhastighet på ca 12 km/s. (sv)
  • HD 145377 – gwiazda typu widmowego G położona w gwiazdozbiorze Skorpiona w odległości około 188 lat świetlnych. Ma jedną znaną planetę HD 145377 b, która krąży wokół niej w średniej odległości 0,45 ± 0,004 j.a. (pl)
  • HD 145377 — звезда в созвездии Скорпиона на расстоянии около 188 световых лет от нас. Вокруг звезды обращается, как минимум, одна планета. (ru)
  • HD 145377 is a star in the southern constellation Scorpius. It has an apparent visual magnitude of 8.10 and can be viewed with a small telescope. The star is located at a distance of 175 light years from the Sun based on parallax, and it is drifting further away with a radial velocity of +11.6. The absolute magnitude of this star is 4.31, indicating it would be visible to the naked eye if it were at a distance of 10 parsecs. (en)
  • HD 145377 est un système planétaire situé à une distance de ∼175 a.l. (∼53,7 pc) du Soleil, dans la constellation zodiacale du Scorpion. Du point de vue observationnel, il s'agit d'un système binaire spectroscopique à raies simples sans éclipses. L'étoile centrale, HD 145377 a, est l'objet primaire du système. Il s'agit d'une étoile naine (classe de luminosité V) jaune (classe spectrale G3) Un seul corps secondaire est connu à ce jour (novembre 2017) dans le système, à savoir la planète HD 145377 b. (fr)
  • HD 145377 é uma estrela na constelação de Scorpius. Tem uma magnitude aparente visual de 8,12, portanto não é visível a olho nu. Com base em sua paralaxe medida pela sonda Gaia, está localizada a aproximadamente 176 anos-luz (53,8 parsecs) da Terra. (pt)
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  • Gyr (en)
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