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V424 Lacertae (V424 Lac) is a red supergiant variable star in the constellation Lacerta. It is a member of the Lacerta OB1 stellar association. The MK spectral type of V424 Lac has been determined to be K5, but it has also been classified as M0. It was discovered to be slightly variable using analysis of Hipparcos photometry. The total range is less than a tenth of a magnitude. Multiple short periods are detected, as well as slow variations with a period of 1,100 or 1,601 days. Although listed in the General Catalogue of Variable Stars as a slow irregular variable, it has been considered to be either a semiregular variable or long secondary period variable.

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rdf:type
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  • V424 Lacertae (es)
  • HD 216946 (it)
  • V424 Lacertae (en)
  • HD 216946 (zh)
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  • HD 216946 è una stella supergigante rossa della costellazione della Lucertola, situata nella parte centrale della costellazione, a poco più di un minuto in Ascensione Retta dalla costellazione di Andromeda. È una stella variabile, nota come V0424 Lac, originariamente descritta come di incerta attribuzione, con oscillazioni di magnitudine da 4,92 a 5,03, con ampiezza media di 0,06 magnitudini; uno studio del 2007 l'ha classificata più stabilmente come variabile LSP, cioè come stella variabile di lungo periodo, quantificato per adesso a 1601 giorni. (it)
  • HD 216946,又名BD+48 3887,SAO 52516、HR 8726,是一颗恒星,视星等为4.95,位于銀經104.59,銀緯-9,其B1900.0坐标为赤經22h 52m 2.8s,赤緯+49° -9′ 59″。 (zh)
  • V424 Lacertae (V424 Lac / HD 216946 / HR 8726)​ es una estrella variable en la constelación de Lacerta. De magnitud aparente media +5,00, visualmente se localiza muy cerca del límite con Andrómeda.Es una estrella lejana cuya distancia es mal conocida; su posible pertenencia a la Asociación estelar Lac OB1 permite estimar su distancia en unos 1700 años luz.​ (es)
  • V424 Lacertae (V424 Lac) is a red supergiant variable star in the constellation Lacerta. It is a member of the Lacerta OB1 stellar association. The MK spectral type of V424 Lac has been determined to be K5, but it has also been classified as M0. It was discovered to be slightly variable using analysis of Hipparcos photometry. The total range is less than a tenth of a magnitude. Multiple short periods are detected, as well as slow variations with a period of 1,100 or 1,601 days. Although listed in the General Catalogue of Variable Stars as a slow irregular variable, it has been considered to be either a semiregular variable or long secondary period variable. (en)
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  • V424 Lacertae (en)
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  • http://commons.wikimedia.org/wiki/Special:FilePath/Red_circle.svg
  • http://commons.wikimedia.org/wiki/Special:FilePath/Lacerta_constellation_map.svg
  • http://commons.wikimedia.org/wiki/Special:FilePath/V424LacLightCurve.png
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  • −4.27 (en)
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