• "Enhanced Lidov-Kozai migration and the formation of the transiting giant planet WD1856+534b". Monthly Notices of the Royal Astronomical Society.
  • White dwarf WD 1856+534 is located 81 light years away from the Sun. It is a single star of spectral class DC D, that has 52 % of solar mass.
  • Dubbed WD 1856b, the exoplanet is roughly the size of Jupiter — orbiting the white dwarf named WD 1856+534.
  • It has an effective temperature of 4,700 K (4,430 °C; 8,000 °F), corresponding to an age of approximately 5.8 billion years.[2] WD 1856+534 is approximately half as...
  • An artist's impression of the potential Jupiter-size planet WD 1856+534 b and its much smaller host star, a dim white dwarf.
  • View a PDF of the paper titled TTV Constraints on Additional Planets in the WD 1856+534 system, by Sarah Kubiak and 6 other authors.
  • WD 1856+534 b is a gas giant exoplanet that orbits a K-type star. Its mass is 13.8 Jupiters, it takes 1.4 days to complete one orbit of its star, and is 0.0204 AU from its...
  • Gemini/GMOS Transmission Spectroscopy of the Grazing Planet Candidate WD 1856+534 b. 2021 xu sh., diamond-lowe h., macdonald r...
  • TOI-1690 (better known as WD 1856+534) is a white dwarf about 80.737 light-years away in the constellation Draco. It is part of a triple star system called G 229-20.
  • WD 1856+534 b is a gas giant exoplanet that orbits a K-type star. Its mass is 13.8 Jupiters, it takes 1.4 days to complete one orbit of its star, and is 0.0204 AU from its...
  • A transit of the WD1856+534 by an exoplanet candidate (Vanderburg et al. 2020) taken by a single LAST telescope in a test run on 2020 September 14.
  • The WD 1856+534 Exoplanetary System. The WD 1856+534 system contains 1 exoplanet. It is located 80.68 light years away from the solar system.