1 00:00:04,120 --> 00:00:08,160 Narrator: This is the universe as we 2 00:00:08,180 --> 00:00:12,260 imagine it...objects floating quietly in space. 3 00:00:12,280 --> 00:00:16,440 This is the universe as scientists think it actually behaves. 4 00:00:16,460 --> 00:00:20,620 Objects in space affected ever so slightly by gravitational waves. 5 00:00:20,640 --> 00:00:24,800 Ripples in space-time caused for example by 6 00:00:24,820 --> 00:00:28,990 the merger of two black holes. The trick 7 00:00:29,010 --> 00:00:33,180 is to actually measure these gravitational ripples and to do that 8 00:00:33,200 --> 00:00:37,360 you need a remarkably precise measuring instrument. 9 00:00:37,380 --> 00:00:41,440 You need an atom interferometer. Babak Saif: Gravitational wave detection, 10 00:00:41,460 --> 00:00:45,580 this new carrier would allow us to go 11 00:00:45,600 --> 00:00:49,740 way further back in time and we're looking at the Big Bang, 12 00:00:49,760 --> 00:00:53,880 and it really increases our knowledge of cosmology. Narrator: Theory says these 13 00:00:53,900 --> 00:00:58,070 ripples form when big objects like galaxies and stars move in the 14 00:00:58,090 --> 00:01:02,260 universe. Long since predicted by Einstein's general theory of 15 00:01:02,280 --> 00:01:06,440 relativity, they've never been directly detected. Optical 16 00:01:06,460 --> 00:01:10,520 interferometry--that is visible light measurements--could do the job, but 17 00:01:10,540 --> 00:01:14,730 previous mission concepts were very expensive. A ground 18 00:01:14,750 --> 00:01:18,920 based observatory called advanced LIGO may one day detect 19 00:01:18,940 --> 00:01:23,150 gravity waves. So why atom interferometry? 20 00:01:23,170 --> 00:01:27,350 Mind-boggling precision, by blasting rubidium atoms 21 00:01:27,370 --> 00:01:31,540 with carefully calibrated lasers to super-chill them right above absolute 22 00:01:31,560 --> 00:01:35,720 zero, a change in position of so much as a trillionth of a 23 00:01:35,740 --> 00:01:39,890 meter--a picometer--will show up, thus adding 24 00:01:39,910 --> 00:01:44,070 evidence to the theory. So: cutting edge science 25 00:01:44,090 --> 00:01:48,240 or whiz-bang technology? Both, it turns out. 26 00:01:48,260 --> 00:01:52,360 Atom interferometry may be the best way to probe some of the most 27 00:01:52,380 --> 00:01:56,420 essential questions in astrophysics. But the new tools 28 00:01:56,440 --> 00:02:00,590 being built by The Goddard Space Flight Center and Stanford University will have 29 00:02:00,610 --> 00:02:04,780 other applications, too. For example, they could more precisely 30 00:02:04,800 --> 00:02:08,830 track speed, orientation, and inertial changes in one of these... 31 00:02:08,850 --> 00:02:12,940 or help NASA scientists figure out what asteroid