Astronomers report finding 27 potential “circumbinary” planets—worlds that orbit two stars—more than doubling the number of such candidates previously identified. While about 18 circumbinary planets had been known, more than 6,000 exoplanets are known to orbit single stars. The new candidates are located roughly 650 to 18,000 light-years from Earth. The work focuses on star systems where the two stars eclipse each other, producing precisely timed changes. Researchers use a method called “apsidal precession” to detect a wobble in these eclipsing binaries that could indicate an additional third body. After accounting for other explanations tied to the stars’ rotation and gravitational effects, the team finds 36 systems among 1,590 where the behavior suggests something else is present; 27 of those objects could have planet-like masses. The study uses data from NASA’s Transiting Exoplanet Survey Satellite (TESS), launched in 2018. The team notes that further observations—particularly spectroscopic measurements of the objects’ light—are needed to confirm whether each candidate is truly a planet rather than a brown dwarf or a star.