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Wikipedia

WASP-35

WASP-35 is a G-type main-sequence star about 660 light-years away. The star's age cannot be well constrained, but it is probably older than the Sun. WASP-35 is similar in concentration of heavy elements compared to the Sun. The star has no detectable starspot activity. An imaging survey in 2015 found no detectable stellar companions, although a spectroscopic survey in 2016 yielded a suspected red dwarf companion with a temperature of 3800±1100 K.

Planetary system In 2011 a transiting hot Jupiter planet, WASP-35b, was detected. The planet's equilibrium temperature is 1450±20 K.

References

Tags

  • Durchmusterung objects
  • Eridanus (constellation)
  • Exoplanet stubs
  • G-type main-sequence stars
  • Main-sequence-star stubs
  • Planetary systems with one confirmed planet
  • Planetary transit variables
  • TESS Objects of Interest
  • Wide Angle Search for Planets