Kepler-1658 is an F-type star located in the constellation Cygnus, [1] approximately 2,629 light-years (806 parsecs ) away. [2] . It has 1.45 times the solar mass and 2.89 times the solar radius. [2] According to a study in 2025, it might have two stellar companions. [3]
In 2009, a hot Jupiter planet candidate (KOI-4.01) was identified around Kepler-1658 by the Kepler space telescope via the transit method. Initially ruled out as a false alarm, the existence of the planet was established in 2019 (Kepler-1658b). [4] [5] Analysis of the Transiting Exoplanet Survey Satellite (TESS) data in 2022 showed that it is gradually spiraling into its star, with its orbit decaying. [6] However, based on the relevant data, in 2025 it was demonstrated that Kepler-1658b is very likely a false positive system. [3] In reality, all the data that supported the detection of a planet with physical orbital decay could just as well be explained via the assertion of the system as a triple star system, where the primary observed star has a companion system that consists of an eclipsing binary with a period of 3.8 days. This explanation can thoroughly account for all the system discrepancies when asserting a planet while providing a consistent explanation for all historical data.