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11 Canis Minoris is a single star in the equatorial constellation of Canis Minor, located around 313 light years away from the Sun. It is visible to the naked eye as a faint, white-hued star with an apparent visual magnitude of 5.25. This object is moving away from the Earth with a heliocentric radial velocity of +28 km/s, having come to within 157 light-years some 2.35 million years ago.

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  • 11 Canis Minoris (en)
  • 11 Canis Minoris (it)
  • 11 Canis Minoris (sv)
  • 11 Малого Пса (ru)
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  • 11 Canis Minoris (11 CMi / 11 Canis Minoris) è una stella bianca nella sequenza principale di magnitudine 5,25 situata nella costellazione del Cane Minore. Dista 312 anni luce dal sistema solare. (it)
  • 11 Canis Minoris, som är stjärnans Flamsteed-beteckning, är en ensam stjärna, belägen i den norra delen av stjärnbilden Lilla hunden. Den har en skenbar magnitud av ca 5,25 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallax enligt Gaia Data Release 2 på ca 10,4 mas, beräknas den befinna sig på ett avstånd på ca 313 ljusår (ca 96 parsek) från solen. Den rör sig bort från solen med en heliocentrisk radialhastighet på ca 28 km/s och var inom 157 ljusårs avstånd från solen för 2,35 miljoner år sedan. (sv)
  • 11 Малого Пса — звезда в созвездии Малого Пса. 11 Малого Пса — белая звезда главной последовательности спектрального класса А с видимым блеском +5.25. Звезда удалена от Земли на расстоянии 312 световых лет. Невооружённым глазом звезда видна только зорким людям при хорошей видимости, или в бинокль. (ru)
  • 11 Canis Minoris is a single star in the equatorial constellation of Canis Minor, located around 313 light years away from the Sun. It is visible to the naked eye as a faint, white-hued star with an apparent visual magnitude of 5.25. This object is moving away from the Earth with a heliocentric radial velocity of +28 km/s, having come to within 157 light-years some 2.35 million years ago. (en)
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absmag v
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  • A1Vnn (en)
constell
epoch
  • J2000.0 (en)
gravity
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parallax
prop mo dec
  • −25.275 (en)
prop mo ra
  • −29.902 (en)
radius
has abstract
  • 11 Canis Minoris is a single star in the equatorial constellation of Canis Minor, located around 313 light years away from the Sun. It is visible to the naked eye as a faint, white-hued star with an apparent visual magnitude of 5.25. This object is moving away from the Earth with a heliocentric radial velocity of +28 km/s, having come to within 157 light-years some 2.35 million years ago. This is an A-type main-sequence star with a stellar classification of A1Vnn, where the 'n' notation indicates (very) "nebulous" lines due to rapid rotation. However, Gray and Garrison (1987) found a class of A0.5 IVnn, which would instead match an evolving subgiant star. It is a suspected variable star of unknown type. This object is 149 million years old with 2.23 times the mass of the Sun and about 2.5 times the Sun's radius. It is radiating 65 times the Sun's luminosity from its photosphere at an effective temperature of 9,972 K. (en)
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