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.
[4] An imaging survey in 2015 found no detectable stellar companions,[7] although a spectroscopic survey in 2016 yielded a suspected red dwarf companion with a temperature of 3800±1100 K.[8] In 2011 a transiting hot Jupiter planet b was detected.
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