A new technique developed in part by Planetary Science Institute Senior Scientist Nader Haghighipour has allowed astronomers to quickly detect a transiting circumbinary planet orbiting around two suns, according to a new Astronomical Journal paper on which Haghighipour is an author.
Circumbinary planets are planetary bodies that rotate around two stars. Although for years, they were merely a matter of science fiction, thanks to the successful operation of NASA’s Kepler and Transiting Exoplanet Survey Satellite (TESS) telescopes, an all-sky survey mission designed to discover thousands of exoplanets around nearby bright stars, a team of astronomers, including Haghighipour, have detected 14 such bodies.
“Detecting circumbinary planets is much more complicated than detecting planets orbiting single stars. The most promising technique for detecting circumbinary planets is transit photometry, which measures drops in starlight caused by those planets whose orbits are oriented in space such that they periodically pass between their stars and the telescope. In this technique, the measurements of the decrease in the intensity of the light of a star is used to infer the existence of a planet,” Haghighipour said. “To determine the orbit of the planet, precisely, at least three transit events are required. This becomes complicated when a planet orbits a double-star system because transits will not happen with the same interval over the same star. The planet may transit one star and then transit the other before transiting the first star again, and so on.”