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R Capricorni (R Cap) is a star in the constellation of Capricornus. It has an apparent visual magnitude which varies between 9.4 and 14.9. A mira variable and ageing red giant, it is in the asymptotic giant branch stage of its lifespan. R Capricorni is too far from earth for its parallax to be measured effectively; Guandalini and Cristallo calculated the luminosity of Mira variables based on their periods. Using a period of 345.13 days, they calculated the absolute magnitude of R Capricorni to be -4.58. The R Capricorni is losing mass at rate of 2.8*10−6M☉/year.

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  • R Capricorni (en)
  • R Capricorni (sv)
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  • R Capricorni (R Cap) is a star in the constellation of Capricornus. It has an apparent visual magnitude which varies between 9.4 and 14.9. A mira variable and ageing red giant, it is in the asymptotic giant branch stage of its lifespan. R Capricorni is too far from earth for its parallax to be measured effectively; Guandalini and Cristallo calculated the luminosity of Mira variables based on their periods. Using a period of 345.13 days, they calculated the absolute magnitude of R Capricorni to be -4.58. The R Capricorni is losing mass at rate of 2.8*10−6M☉/year. (en)
  • R Capricorni är en pulserande variabel av Mira Ceti-typ i stjärnbilden Stenbocken. Stjärnan var den första i Stenbockens stjärnbild som fick en variabelbeteckning. Stjärnan varierar mellan visuell magnitud +8,9 och 14,9 med en period av 343 dygn. (sv)
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  • R Capricorni (en)
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  • http://commons.wikimedia.org/wiki/Special:FilePath/RCapLightCurve.png
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  • Cev (en)
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  • J2000.0 (en)
prop mo dec
  • −6 (en)
prop mo ra
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  • R Capricorni (R Cap) is a star in the constellation of Capricornus. It has an apparent visual magnitude which varies between 9.4 and 14.9. A mira variable and ageing red giant, it is in the asymptotic giant branch stage of its lifespan. R Capricorni is too far from earth for its parallax to be measured effectively; Guandalini and Cristallo calculated the luminosity of Mira variables based on their periods. Using a period of 345.13 days, they calculated the absolute magnitude of R Capricorni to be -4.58. The R Capricorni is losing mass at rate of 2.8*10−6M☉/year. (en)
  • R Capricorni är en pulserande variabel av Mira Ceti-typ i stjärnbilden Stenbocken. Stjärnan var den första i Stenbockens stjärnbild som fick en variabelbeteckning. Stjärnan varierar mellan visuell magnitud +8,9 och 14,9 med en period av 343 dygn. (sv)
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