1 00:00:00,000 --> 00:00:04,000 [music throughout] Narrator: NASA’s TESS mission just discovered its first circumbinary 2 00:00:04,000 --> 00:00:08,000 planet—a world orbiting two stars instead of one. 3 00:00:08,000 --> 00:00:12,000 Named TOI 1338 b, it’s nearly the size of Saturn 4 00:00:12,000 --> 00:00:16,000 and orbits its stars every 95 days. The two stars 5 00:00:16,000 --> 00:00:20,000 orbit each other and consist of a small, cool M dwarf and one much like 6 00:00:20,000 --> 00:00:24,000 the Sun. Together, they form what is called an eclipsing binary, 7 00:00:24,000 --> 00:00:28,000 which means the stars regularly pass in front of each other form our point of view. 8 00:00:28,000 --> 00:00:32,000 TESS hunts for planets in these and other systems by looking 9 00:00:32,000 --> 00:00:36,000 for tiny, regular dips in starlight called transits. TESS saw 10 00:00:36,000 --> 00:00:40,000 TOI 1338 b’s transits of the large star, but spotting them 11 00:00:40,000 --> 00:00:44,000 in the data wasn’t easy. A high school intern examined hundreds of 12 00:00:44,000 --> 00:00:48,000 eclipsing binaries to search for planetary transits, which can look similar to 13 00:00:48,000 --> 00:00:52,000 some of the eclipses. Ultimately, he uncovered transits 14 00:00:52,000 --> 00:00:56,000 caused by the planet. If you could orbit 15 00:00:56,000 --> 00:01:00,000 TOI 1338 b, you’d have a front-row seat to see its suns 16 00:01:00,000 --> 00:01:04,000 eclipse each other every 15 days. But the angle of the planet’s orbit 17 00:01:04,000 --> 00:01:08,000 around the stars changes over time. After 2023, 18 00:01:08,000 --> 00:01:12,000 we won’t see it pass in front of the stars for another 8 years. 19 00:01:12,000 --> 00:01:16,000 TESS will observe hundreds of thousands of eclipsing binaries, so there may be other 20 00:01:16,000 --> 00:01:20,000 planets similar to TOI 1338 b waiting 21 00:01:20,000 --> 00:01:24,000 to be discovered. [music] 22 00:01:24,000 --> 00:01:32,757 [music]