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Wikipedia

WASP-75

WASP-75 is an F-type main-sequence star about 980 light-years away. The star is much younger than the Sun at approximately 2.9 billion years. WASP-75 is similar to the Sun in its concentration of heavy elements.

Planetary system In 2013, a transiting hot Jupiter planet b was detected on a tight, circular orbit, and the planet was confirmed in 2018. Its equilibrium temperature is 1,688 K.

References

Tags

  • Aquarius (constellation)
  • Durchmusterung objects
  • F-type main-sequence stars
  • Main-sequence-star stubs
  • Planetary systems with one confirmed planet
  • Planetary transit variables
  • Wide Angle Search for Planets