1 00:00:00,000 --> 00:00:01,634 [Music throughout] 2 00:00:01,634 --> 00:00:04,137 When superdense neutron stars crash, 3 00:00:04,137 --> 00:00:07,841 the event can be felt across the cosmos. 4 00:00:09,242 --> 00:00:13,313 But astronomers would love to find these systems before they collide. 5 00:00:13,747 --> 00:00:16,750 And new simulations are guiding the way. 6 00:00:17,584 --> 00:00:20,553 Neutron stars pack the mass of our Sun 7 00:00:20,687 --> 00:00:22,956 into a ball the size of a city. 8 00:00:24,724 --> 00:00:26,760 When two orbit each other, 9 00:00:26,760 --> 00:00:28,928 they'll eventually merge. 10 00:00:31,698 --> 00:00:34,701 That event produces ripples in space-time, 11 00:00:35,235 --> 00:00:38,238 a blast of gamma rays and other light, 12 00:00:38,738 --> 00:00:41,741 and may leave behind a new black hole. 13 00:00:43,843 --> 00:00:47,213 Neutron stars have superstrong magnetic fields 14 00:00:47,213 --> 00:00:49,682 filled with energetic particles. 15 00:00:50,784 --> 00:00:53,653 New simulations run on NASA Ames’ 16 00:00:53,653 --> 00:00:55,622 Pleiades supercomputer show 17 00:00:55,688 --> 00:00:57,924 how these fields begin interacting 18 00:00:57,924 --> 00:00:59,893 long before the stars crash. 19 00:01:12,238 --> 00:01:14,441 As the magnetic fields intertwine, 20 00:01:14,441 --> 00:01:15,675 they produce a glow 21 00:01:15,675 --> 00:01:17,410 that steadily increases 22 00:01:17,410 --> 00:01:19,579 as the stars spiral closer together. 23 00:01:25,151 --> 00:01:26,519 These simulations 24 00:01:26,519 --> 00:01:28,822 map where the most energetic gamma rays 25 00:01:29,089 --> 00:01:31,024 produce a distinctive glow 26 00:01:31,024 --> 00:01:32,659 we could detect from Earth, 27 00:01:33,259 --> 00:01:35,929 a goal for next-generation telescopes. 28 00:01:40,700 --> 00:01:42,635 Simulations like these 29 00:01:42,635 --> 00:01:46,372 will help astronomers better understand how these fields interact 30 00:01:46,639 --> 00:01:48,041 and better predict 31 00:01:48,041 --> 00:01:49,843 the electromagnetic signals 32 00:01:49,843 --> 00:01:51,010 that will point 33 00:01:51,010 --> 00:01:53,480 to imminent neutron star collisions. 34 00:01:56,182 --> 00:02:00,386 [NASA]