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SDSS J143317.78+101123.3 (shortened to SDSS J1433+1011, more simply J1433) is a binary system composed of a white dwarf and a brown dwarf. The brown dwarf is about 57 Jupiter masses and has transitioned from a stellar object to a brown dwarf due to losing mass to the white dwarf. As of 2016, this was the only known binary of this type.

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  • SDSS J143317.78+101123 (fr)
  • SDSS J143317.78+101123.3 (en)
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  • SDSS J143317.78+101123.3 (shortened to SDSS J1433+1011, more simply J1433) is a binary system composed of a white dwarf and a brown dwarf. The brown dwarf is about 57 Jupiter masses and has transitioned from a stellar object to a brown dwarf due to losing mass to the white dwarf. As of 2016, this was the only known binary of this type. (en)
  • SDSS J143317.78+101123 (abrégé en SDSS J1433+1011 voire simplement J1433) est un système binaire constitué d'une naine blanche et d'une naine brune. (fr)
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  • SDSS J143317.78+101123.3.3 (en)
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  • J1433 (en)
  • J1433b (en)
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  • en-UK (en)
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  • J2000 (en)
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  • SDSS J143317.78+101122.8b (en)
  • J1433, PM J14332+1011, SDSS J143317.78+101122.8, Gaia EDR3 1176468611268115200, Gaia DR2 1176468611268115200 (en)
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  • −53.117 (en)
prop mo ra
  • −12.782 (en)
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  • SDSS J143317.78+101123.3 (shortened to SDSS J1433+1011, more simply J1433) is a binary system composed of a white dwarf and a brown dwarf. The brown dwarf is about 57 Jupiter masses and has transitioned from a stellar object to a brown dwarf due to losing mass to the white dwarf. As of 2016, this was the only known binary of this type. (en)
  • SDSS J143317.78+101123 (abrégé en SDSS J1433+1011 voire simplement J1433) est un système binaire constitué d'une naine blanche et d'une naine brune. (fr)
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