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Psi Scorpii, which is Latinized from ψ Scorpii, is a star in the zodiac constellation of Scorpius. It is white in hue and has an apparent visual magnitude of 4.94, which is bright enough to be faintly visible to the naked eye. Based upon parallax measurements, it is located at a distance of around 162 light years from the Sun. Data collected during the Hipparcos mission suggests it is an astrometric binary, although nothing is known about the companion. The system is drifting closer to the Sun with a radial velocity of −5 km/s.

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rdfs:label
  • Psi Scorpii (en)
  • Psi Scorpii (pt)
  • Пси Скорпиона (ru)
  • Psi Scorpii (sv)
  • HD145570 (uk)
rdfs:comment
  • Psi Scorpii (15 Scorpii) é uma estrela na direção da constelação de Scorpius. Possui uma ascensão reta de 16h 12m 00.00s e uma declinação de −10° 03′ 51.1″. Sua magnitude aparente é igual a 4.93. Considerando sua distância de 165 anos-luz em relação à Terra, sua magnitude absoluta é igual a 1.41. Pertence à classe espectral A3IV. (pt)
  • Psi Scorpii (ψ Scorpii, förkortat Psi Sco, ψ Sco), som är stjärnans Bayerbeteckning, är en stjärna belägen i norra delen av stjärnbilden Skorpionen. Den har en skenbar magnitud på 4,96 och är svagt synlig för blotta ögat. Baserat på parallaxmätningar befinner den sig på ett avstånd av 160 ljusår (ca 48 parsek) från solen. Data som samlats in under Hipparcosuppdraget anger att den är en astrometrisk dubbelstjärna, även om ingenting är känt om följeslagaren. (sv)
  • HD145570 — хімічно пекулярна зоря спектрального класу A2, що має видиму зоряну величину в смузі V приблизно 4,9.Вона розташована на відстані близько 164,8 світлових років від Сонця. (uk)
  • Psi Scorpii, which is Latinized from ψ Scorpii, is a star in the zodiac constellation of Scorpius. It is white in hue and has an apparent visual magnitude of 4.94, which is bright enough to be faintly visible to the naked eye. Based upon parallax measurements, it is located at a distance of around 162 light years from the Sun. Data collected during the Hipparcos mission suggests it is an astrometric binary, although nothing is known about the companion. The system is drifting closer to the Sun with a radial velocity of −5 km/s. (en)
  • Пси Скорпиона (ψ Sco, ψ Scorpii) — звезда в южном зодиакальном созвездии Скорпиона. Обладает видимой звёздной величиной 4,96 и доступна для наблюдения невооружённым глазом. Измерения параллакса привели к оценке расстояния от Солнца до звезды 160 световых лет. По данным, полученным спутником Hipparcos, звезда является астрометрической двойной, но о звезде-компаньоне пока нет дополнительной информации. (ru)
foaf:name
  • ψ Scorpii (en)
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absmag v
  • +1.55 (en)
age myr
appmag v
b-v
  • +0.09 (en)
class
  • A1 V (en)
constell
epoch
  • J2000 (en)
gravity
luminosity
mass
p error
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