Kepler-1704b is a super-Jupiter on a highly eccentric orbit around the star Kepler-1704.
The planet's distance from its star varies from 0.16 to 3.9 AU.
It is a failed hot Jupiter, having been scattered from its birth orbit to orbit with a periastron just above the tidal circularization distance.
[1] The high planetary mass makes Kepler-1704b a super-Jupiter.
Kepler-1704b goes on a highly eccentric 2.7 year-long (988.88 days) orbit around its star as well as transiting.