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 00:00:22,956 --> 00:00:25,258 And have superstrong magnetic fields 9 00:00:25,258 --> 00:00:27,727 filled with energetic particles. 10 00:00:28,795 --> 00:00:31,664 New simulations run on NASA Ames’ 11 00:00:31,664 --> 00:00:33,633 Pleiades supercomputer show 12 00:00:33,700 --> 00:00:35,935 how these fields begin interacting 13 00:00:35,935 --> 00:00:37,904 long before the stars crash. 14 00:00:39,472 --> 00:00:41,674 As the magnetic fields intertwine, 15 00:00:41,674 --> 00:00:42,909 they produce a glow 16 00:00:42,909 --> 00:00:44,644 that steadily increases 17 00:00:44,644 --> 00:00:46,813 as the stars spiral closer together. 18 00:00:49,682 --> 00:00:51,317 These simulations 19 00:00:51,317 --> 00:00:53,620 map where the most energetic gamma rays 20 00:00:54,054 --> 00:00:55,989 produce a distinctive glow 21 00:00:55,989 --> 00:00:57,624 we could detect from Earth, 22 00:00:57,991 --> 00:01:00,660 a goal for next-generation telescopes. 23 00:01:01,694 --> 00:01:03,630 Simulations like these 24 00:01:03,630 --> 00:01:07,367 will help astronomers better understand how these fields interact 25 00:01:07,634 --> 00:01:09,035 and better predict 26 00:01:09,035 --> 00:01:10,837 the electromagnetic signals 27 00:01:10,837 --> 00:01:12,005 that will point 28 00:01:12,005 --> 00:01:14,474 to imminent neutron star collisions. 29 00:01:17,177 --> 00:01:21,381 [NASA]