1 00:00:00,433 --> 00:00:05,939 (SCIENCE TREK MUSIC) 2 00:00:05,939 --> 00:00:07,807 JOAN CARTAN-HANSEN, HOST: Scientists have several 3 00:00:07,807 --> 00:00:09,943 different ways to find an exoplanet. 4 00:00:09,943 --> 00:00:11,077 One is called radial velocity. 5 00:00:11,077 --> 00:00:13,480 Orbiting planets cause a change in the color of the 6 00:00:13,480 --> 00:00:14,514 light of a star. 7 00:00:14,514 --> 00:00:15,782 Astronomers call it a wobble. 8 00:00:15,782 --> 00:00:17,917 Another method is called a transit. 9 00:00:17,917 --> 00:00:20,487 When a planet passed between the star and the observer, the 10 00:00:20,487 --> 00:00:23,223 light of the star dims a tiny amount. 11 00:00:23,223 --> 00:00:25,925 That change in light indicates a possible exoplanet. 12 00:00:25,925 --> 00:00:29,462 Astronomers can also take pictures of an exoplanet by 13 00:00:29,462 --> 00:00:32,132 blocking out the glare of the star it orbits. 14 00:00:32,132 --> 00:00:33,666 That's called direct imaging. 15 00:00:33,666 --> 00:00:36,603 Then there's gravitational microlensing. 16 00:00:36,603 --> 00:00:39,639 Light from a distant star get bent and focused by gravity as 17 00:00:39,639 --> 00:00:43,176 an exoplanet passes between that star and Earth. 18 00:00:43,176 --> 00:00:45,645 And finally, astronomers look for very tiny or minuscule 19 00:00:45,645 --> 00:00:49,249 movements of stars in relation to other nearby stars. 20 00:00:49,249 --> 00:00:52,519 The orbit of a planet can cause its star to wobble in its orbit. 21 00:00:52,519 --> 00:00:55,388 Exoplanets are very far away and difficult to spot, but 22 00:00:55,388 --> 00:00:58,124 scientists are working hard to find them. 23 00:00:58,458 --> 00:01:00,326 For more information about exoplanets, check out the 24 00:01:00,326 --> 00:01:01,127 Science Trek website. 25 00:01:01,127 --> 00:01:03,730 You'll find it at ScienceTrek.org.