1 00:00:00,000 --> 00:00:04,000 [music] Tom Barclay: For the longest time, space seemed 2 00:00:04,000 --> 00:00:08,000 like a big, nearly empty place, and we were really only familiar 3 00:00:08,000 --> 00:00:12,000 with our home, Earth. But as we learned more, 4 00:00:12,000 --> 00:00:16,000 we realized there was actually a lot out there, including planets 5 00:00:16,000 --> 00:00:20,000 orbiting the Sun, and even other stars. 6 00:00:20,000 --> 00:00:24,000 To get to these more distant worlds, though, it helps to start thinking of space 7 00:00:24,000 --> 00:00:28,000 as a bunch of nested bubbles. Our first bubble 8 00:00:28,000 --> 00:00:32,000 is the magnetosphere—Earth’s invisible magnetic field that 9 00:00:32,000 --> 00:00:36,000 protects us from high-energy particles and radiation from the Sun, 10 00:00:36,000 --> 00:00:40,000 allowing life as we know it to develop and thrive. The next bubble, 11 00:00:40,000 --> 00:00:44,000 just past the solar system, is the Heliosphere-- 12 00:00:44,000 --> 00:00:48,000 the edge of the Sun’s influence, where the particles and fields 13 00:00:48,000 --> 00:00:52,000 of interstellar space take over. The two Voyager 14 00:00:52,000 --> 00:00:56,000 spacecraft have left this bubble and are our first interstellar 15 00:00:56,000 --> 00:01:00,000 spacecraft! It took Voyager 1 35 years, and it took 16 00:01:00,000 --> 00:01:04,000 Voyager 2 41 years to travel this far. 17 00:01:04,000 --> 00:01:08,000 The next stop is our nearest stars. The Alpha Centauri 18 00:01:08,000 --> 00:01:12,000 system, at just over 4 light-years away, is close by cosmic standards, 19 00:01:12,000 --> 00:01:16,000 but it would take either Voyager about 75,000 years to get 20 00:01:16,000 --> 00:01:20,000 there at current speeds. We clearly need to use other tools 21 00:01:20,000 --> 00:01:24,000 to look for worlds that far away. Enter Kepler, 22 00:01:24,000 --> 00:01:28,000 a space telescope that radically changed our understanding 23 00:01:28,000 --> 00:01:32,000 of planets outside our solar system—also known as exoplanets. 24 00:01:32,000 --> 00:01:36,000 In finding thousands of new planets, Kepler showed 25 00:01:36,000 --> 00:01:40,000 that there are more planets in our galaxy than there are stars! 26 00:01:40,000 --> 00:01:44,000 But Kepler looked at only a small fraction of the sky, and many [on screen: the Kepler search region, which is approximately 3,000 light-years long] 27 00:01:44,000 --> 00:01:48,000 of the planets it discovered are too far away to study in much further detail. 28 00:01:48,000 --> 00:01:52,000 And that brings us to TESS, our newest planet hunter. 29 00:01:52,000 --> 00:01:56,000 The Transiting Exoplanet Survey Satellite works like Kepler, 30 00:01:56,000 --> 00:02:00,000 and over the next two years, it will scan almost the 31 00:02:00,000 --> 00:02:04,000 entire sky. By looking at closer and brighter stars, [on screen: A comparison view of the Kepler and TESS search regions. Kepler's is a 3,000 light-year long cone, and TESS is a 30-300 light-year wide sphere. 32 00:02:04,000 --> 00:02:08,000 TESS will find—and measure the sizes of—dozens of small 33 00:02:08,000 --> 00:02:12,000 nearby planets best suited for detailed investigation 34 00:02:12,000 --> 00:02:16,000 by powerful telescopes on the ground and in space, like 35 00:02:16,000 --> 00:02:20,000 the future James Webb Space Telescope. And by doing 36 00:02:20,000 --> 00:02:24,000 that, we might finally begin to answer the question of whether 37 00:02:24,000 --> 00:02:28,000 Earth is alone, or whether there are worlds out there 38 00:02:28,000 --> 00:02:32,000 like our own—small and rocky, covered in oceans and 39 00:02:32,000 --> 00:02:36,000 dense clouds, or even—possibly—capable 40 00:02:36,000 --> 00:02:40,000 of supporting life. [music] 41 00:02:40,000 --> 00:02:44,000 [music] 42 00:02:44,000 --> 00:02:48,000 [silence, then satellite beeping] 43 00:02:48,000 --> 00:02:53,632 [satellite beeping]