WEBVTT FILE 1 00:00:00.030 --> 00:00:04.050 [slate] 2 00:00:04.070 --> 00:00:08.060 [slate] 3 00:00:08.080 --> 00:00:12.130 So first part of this 4 00:00:12.150 --> 00:00:16.210 discovery comes from the LIGO observatory which for the first 5 00:00:16.230 --> 00:00:20.350 time detected gravitational waves, ripples in space-time 6 00:00:20.370 --> 00:00:24.550 from two colliding neutron stars 7 00:00:24.570 --> 00:00:28.610 And if that wasn't enough just two seconds later 8 00:00:28.630 --> 00:00:32.710 with the Fermi Gamma Ray space Telescope we detected 9 00:00:32.730 --> 00:00:36.860 a short bright flash of high energy light that we call a gamma ray 10 00:00:36.880 --> 00:00:41.020 burst. This alerted the entire astronomical community 11 00:00:41.040 --> 00:00:45.080 to the fact that something very exciting was happening and over 12 00:00:45.100 --> 00:00:49.170 70 telescopes from around the world. searched for a counterpart 13 00:00:49.190 --> 00:00:53.370 in other wavelengths. They were able to identify the host galaxy and 14 00:00:53.390 --> 00:00:57.380 study the remains of this explosion in amazing details. 15 00:00:57.400 --> 00:01:01.430 [slate] 16 00:01:01.450 --> 00:01:05.560 That's exactly what I'm saying. For the first time we could actually 17 00:01:05.580 --> 00:01:09.750 weigh the amount of heavy metals that were formed in one of these 18 00:01:09.770 --> 00:01:13.810 systems. Over two hundred times the weight of the Earth. 19 00:01:13.830 --> 00:01:17.960 was formed in gold and platinum following the merger of these 20 00:01:17.980 --> 00:01:22.110 systems. They were thrown out at very high speeds and dispersed throughout 21 00:01:22.130 --> 00:01:26.180 the universe and eventually they were formed as 22 00:01:26.200 --> 00:01:30.200 stars and planets like Earth. 23 00:01:30.220 --> 00:01:34.340 [slate] So Fermi and other 24 00:01:34.360 --> 00:01:38.510 NASA satellites quite often detect what we call gamma ray bursts, very 25 00:01:38.530 --> 00:01:42.550 short high energy flashes. Gamma ray 26 00:01:42.570 --> 00:01:46.640 radiation. Several dozen times a year at least. What 27 00:01:46.660 --> 00:01:50.750 makes this really amazing is that you're actually able to see 28 00:01:50.770 --> 00:01:54.930 the source that powered this gamma ray emission 29 00:01:54.950 --> 00:01:59.030 from gravitational waves. We could link the merger of two 30 00:01:59.050 --> 00:02:03.120 neutron stars to the gamma ray burst which is something 31 00:02:03.140 --> 00:02:07.270 we hypothesized was the case for a long time 32 00:02:07.290 --> 00:02:11.440 but now we had really direct confirmation that that was happening. That's the first time 33 00:02:11.460 --> 00:02:15.460 we've been able to do that. 34 00:02:15.480 --> 00:02:19.560 [slate] Gravitational waves are often referred to 35 00:02:19.580 --> 00:02:23.680 as ripples in space-time when a very dense 36 00:02:23.700 --> 00:02:27.860 massive object accelerates, it actually causes gravitational 37 00:02:27.880 --> 00:02:31.920 energy to propagate throughout the universe, changing the distance 38 00:02:31.940 --> 00:02:36.020 between sources that are relatively close to each other. And 39 00:02:36.040 --> 00:02:40.140 with very precise detectors on the ground we can actually measure 40 00:02:40.160 --> 00:02:44.330 those changes and use them to infer the presence of these really remarkable 41 00:02:44.350 --> 00:02:45.178 collisions.