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S Apodis (HD 133444) is an R Coronae Borealis variable star located in the far southern constellation Apus. These are extremely hydrogen-deficient supergiants thought to have arisen as the result of the merger of two white dwarfs; fewer than 100 have been discovered as of 2012. Located around 13,000 light-years distant, it shines with a luminosity approximately 960 times that of the Sun and has a surface temperature of 3916 K.

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  • S Apodis
  • S Apodis
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  • S Apodis (HD 133444) is an R Coronae Borealis variable star located in the far southern constellation Apus. These are extremely hydrogen-deficient supergiants thought to have arisen as the result of the merger of two white dwarfs; fewer than 100 have been discovered as of 2012. Located around 13,000 light-years distant, it shines with a luminosity approximately 960 times that of the Sun and has a surface temperature of 3916 K.
  • S Apodis är en eruptiv variabel av RCB-typ (RCB) i stjärnbilden Paradisfågeln. Stjärnan har magnitud +9,6 och når i förmörkelsefasen ner till +15,2.
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  • S Apodis (HD 133444) is an R Coronae Borealis variable star located in the far southern constellation Apus. These are extremely hydrogen-deficient supergiants thought to have arisen as the result of the merger of two white dwarfs; fewer than 100 have been discovered as of 2012. Located around 13,000 light-years distant, it shines with a luminosity approximately 960 times that of the Sun and has a surface temperature of 3916 K.
  • S Apodis är en eruptiv variabel av RCB-typ (RCB) i stjärnbilden Paradisfågeln. Stjärnan har magnitud +9,6 och når i förmörkelsefasen ner till +15,2.
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  • C
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  • J2000
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