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V385 Andromedae is a variable star in the constellation Andromeda, about 360 parsecs (1,200 ly) away. It is a red giant over a hundred times larger than the sun. It has an apparent magnitude around 6.4, just about visible to the naked eye in ideal conditions. V385 Andromedae was identified as a long-period variable in 1999 from analysis of Hipparcos photometry. It was classified as a slow irregular variable, but analysis of its light curve identified a possible 36 day period. It varies by about 0.1 magnitudes.

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  • V385 Andromedae (it)
  • 안드로메다자리 V385 (ko)
  • V385 Андромеды (ru)
  • V385 Andromedae (en)
rdfs:comment
  • V385 Andromedae è una stella gigante brillante rossa di magnitudine 6,42 situata nella costellazione di Andromeda. Dista 1250 anni luce dal sistema solare. (it)
  • V385 Andromedae is a variable star in the constellation Andromeda, about 360 parsecs (1,200 ly) away. It is a red giant over a hundred times larger than the sun. It has an apparent magnitude around 6.4, just about visible to the naked eye in ideal conditions. V385 Andromedae was identified as a long-period variable in 1999 from analysis of Hipparcos photometry. It was classified as a slow irregular variable, but analysis of its light curve identified a possible 36 day period. It varies by about 0.1 magnitudes. (en)
  • 안드로메다자리 V385(영어: V385 Andromedae)는 안드로메다자리에 있는 M형 주계열성 불규칙 변광성이다. (ko)
  • V385 Андромеды (лат. V385 Andromedae), HD 220524 — двойная звезда в созвездии Андромеды на расстоянии приблизительно 1174 световых лет (около 360 парсеков) от Солнца. Видимая звёздная величина звезды — от +6,47m до +6,36m. (ru)
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  • V385 Andromedae (en)
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  • http://commons.wikimedia.org/wiki/Special:FilePath/Red_circle.svg
  • http://commons.wikimedia.org/wiki/Special:FilePath/Andromeda_constellation_map.svg
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appmag v
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  • +1.66 (en)
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  • M0 (en)
constell
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  • J2000 (en)
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has abstract
  • V385 Andromedae è una stella gigante brillante rossa di magnitudine 6,42 situata nella costellazione di Andromeda. Dista 1250 anni luce dal sistema solare. (it)
  • V385 Andromedae is a variable star in the constellation Andromeda, about 360 parsecs (1,200 ly) away. It is a red giant over a hundred times larger than the sun. It has an apparent magnitude around 6.4, just about visible to the naked eye in ideal conditions. V385 Andromedae was identified as a long-period variable in 1999 from analysis of Hipparcos photometry. It was classified as a slow irregular variable, but analysis of its light curve identified a possible 36 day period. It varies by about 0.1 magnitudes. (en)
  • 안드로메다자리 V385(영어: V385 Andromedae)는 안드로메다자리에 있는 M형 주계열성 불규칙 변광성이다. (ko)
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