1 00:00:00,020 --> 00:00:02,050 [music] Coming soon to the 2 00:00:02,050 --> 00:00:04,110 International Space Station, 3 00:00:04,110 --> 00:00:06,140 a multipurpose mission leveraging 4 00:00:06,140 --> 00:00:08,180 X-ray technology to uncover 5 00:00:08,180 --> 00:00:10,210 mysteries of the universe. 6 00:00:10,210 --> 00:00:12,230 It's 7 00:00:12,230 --> 00:00:14,280 nearly impossible to measure the 8 00:00:14,280 --> 00:00:16,330 sizes of neutron stars directly. 9 00:00:16,330 --> 00:00:18,390 They're only about the size of a city 10 00:00:18,390 --> 00:00:20,410 and very far away. 11 00:00:20,410 --> 00:00:22,450 They're very interesting in the sky to 12 00:00:22,450 --> 00:00:24,470 to study. 13 00:00:24,470 --> 00:00:26,500 It's matter at the cusp of 14 00:00:26,500 --> 00:00:28,530 becoming a black hole. 15 00:00:28,530 --> 00:00:30,540 NICER's 56 telescopes will 16 00:00:30,540 --> 00:00:32,580 make observations, enabling scientists 17 00:00:32,580 --> 00:00:34,610 to determine how rotating neutron 18 00:00:34,610 --> 00:00:36,630 stars - also called 19 00:00:36,630 --> 00:00:38,650 pulsars - are put together. 20 00:00:38,650 --> 00:00:40,690 What we're really interested in doing with NICER 21 00:00:40,690 --> 00:00:42,710 is understanding - um - 22 00:00:42,710 --> 00:00:44,750 really what the size of a neutron 23 00:00:44,750 --> 00:00:46,780 star is. Cause once we know the size of the 24 00:00:46,780 --> 00:00:48,800 radius of a neutron star very precisely, 25 00:00:48,800 --> 00:00:50,840 then we can put constraints on 26 00:00:50,840 --> 00:00:52,870 the density at the core. 27 00:00:52,870 --> 00:00:54,920 And once you have an idea of what the density is 28 00:00:54,920 --> 00:00:56,950 at the core you can constrain nuclear theories that 29 00:00:56,950 --> 00:00:58,970 describe how the particles at 30 00:00:58,970 --> 00:01:01,020 the core of neutron stars interact with each other. 31 00:01:01,020 --> 00:01:03,060 In addition to 32 00:01:03,060 --> 00:01:05,090 probing neutron stars, the 33 00:01:05,090 --> 00:01:07,130 two-in-one mission will advance GPS like 34 00:01:07,130 --> 00:01:09,160 navigation of spacecraft 35 00:01:09,160 --> 00:01:11,200 throughout the solar system and beyond. 36 00:01:11,200 --> 00:01:13,250 The embedded Station 37 00:01:13,250 --> 00:01:15,280 Explorer for X-ray Timing and 38 00:01:15,280 --> 00:01:17,330 Navigation Technology, or SEXTANT, 39 00:01:17,330 --> 00:01:19,400 uses NICER's observations 40 00:01:19,400 --> 00:01:21,410 of pulsars to demonstrate this 41 00:01:21,410 --> 00:01:23,440 potentially game-changing technology. 42 00:01:23,440 --> 00:01:25,460 It's goal as a technology demonstration 43 00:01:25,460 --> 00:01:27,490 as part of the NICER mission, 44 00:01:27,490 --> 00:01:29,520 is to try to turn the "G" in GPS 45 00:01:29,520 --> 00:01:31,570 into "Galactic." 46 00:01:31,570 --> 00:01:33,610 We want to use pulsars - this particular 47 00:01:33,610 --> 00:01:35,660 type of neutron star that spins 48 00:01:35,660 --> 00:01:37,700 hundreds of times a second that emits this 49 00:01:37,700 --> 00:01:39,720 atomic-like clock signal for us 50 00:01:39,720 --> 00:01:41,750 to receive. And so we observe 51 00:01:41,750 --> 00:01:43,780 multiple pulsars and stitch together a solution 52 00:01:43,780 --> 00:01:45,810 by looking at those precision timing 53 00:01:45,810 --> 00:01:47,850 signals from those pulsars to construct a 54 00:01:47,850 --> 00:01:49,900 spacecraft orbit determination solution. 55 00:01:49,900 --> 00:01:51,920 Both NICER and SEXTANT 56 00:01:51,920 --> 00:01:53,970 benefit existing and future NASA 57 00:01:53,970 --> 00:01:56,000 missions and will further 58 00:01:56,000 --> 00:01:58,060 expand humankind's understanding and 59 00:01:58,060 --> 00:02:02,130 exploration of the universe. 60 00:02:02,130 --> 00:02:05,933 nasa.gov/nicer