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ZTF J1813+4251 is a binary star system including a sun-like star and white dwarf, co-orbiting every 51 minutes, about 3,000 light years away in the constellation of Hercules. It is considered a cataclysmic variable with the white dwarf pulling outer layers of hydrogen from the star onto itself. It has the shortest orbital period of all hydrogen-rich cataclysmic variable stars known. It is predicted that the orbital period will reach a minimum of 18 minutes within 75 million years as the system evolves.

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  • ZTF J1813+4251 (en)
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  • ZTF J1813+4251 is a binary star system including a sun-like star and white dwarf, co-orbiting every 51 minutes, about 3,000 light years away in the constellation of Hercules. It is considered a cataclysmic variable with the white dwarf pulling outer layers of hydrogen from the star onto itself. It has the shortest orbital period of all hydrogen-rich cataclysmic variable stars known. It is predicted that the orbital period will reach a minimum of 18 minutes within 75 million years as the system evolves. (en)
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  • ZTF J1813+4251 (en)
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  • http://commons.wikimedia.org/wiki/Special:FilePath/Accretion_Disk_Binary_System.jpg
  • http://commons.wikimedia.org/wiki/Special:FilePath/ZTFJ18134251LightCurve.png
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  • White Dwarf (en)
  • Donor (en)
constell
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  • J2016.0 (en)
equinox
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  • −2.656 (en)
prop mo ra
  • −12.317 (en)
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  • ZTF J1813+4251 is a binary star system including a sun-like star and white dwarf, co-orbiting every 51 minutes, about 3,000 light years away in the constellation of Hercules. It is considered a cataclysmic variable with the white dwarf pulling outer layers of hydrogen from the star onto itself. It has the shortest orbital period of all hydrogen-rich cataclysmic variable stars known. It is predicted that the orbital period will reach a minimum of 18 minutes within 75 million years as the system evolves. It was identified in 2022 by Kevin Burdge of MIT using a computer algorithm that searched over 1,000 images from the Zwicky Transient Facility, identifying stars that had brightness variability periods around one hour. (en)
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