WEBVTT FILE 1 00:00:00.030 --> 00:00:04.090 Like a lot of kids, I grew up reading about neutrinos 2 00:00:04.110 --> 00:00:08.280 and people speculating about doing neutrino astronomy. 3 00:00:08.300 --> 00:00:12.470 And here I am, doing neutrino astronomy, I feel like I need 4 00:00:12.490 --> 00:00:16.680 to pinch myself. My name is Roopesh Ojha, 5 00:00:16.700 --> 00:00:20.790 and I'm an astronomer working at the Goddard Space Flight Center. 6 00:00:20.810 --> 00:00:24.890 I work with the Fermi Gamma-ray Space Telescope. What we 7 00:00:24.910 --> 00:00:29.050 have been able to establish, for the first time, is an individual 8 00:00:29.070 --> 00:00:33.150 blazar as a potential birthplace of an individual neutrino. 9 00:00:33.170 --> 00:00:37.210 The Fermi Gamma-ray Space Telescope has an instrument called the Large Area Telescope, which 10 00:00:37.230 --> 00:00:41.330 we use to monitor the gamma-ray sky-the highest-energy electromagnetic band. 11 00:00:41.350 --> 00:00:45.410 And we just noticed that there was a tremendous 12 00:00:45.430 --> 00:00:49.510 increase in the amount of gamma-ray light coming from this one extra-galactic blazar. 13 00:00:49.530 --> 00:00:53.710 A blazar is an extremely powerful, variable, 14 00:00:53.730 --> 00:00:57.890 galaxy that is powered by a supermassive black hole. 15 00:00:57.910 --> 00:01:02.080 It went up not by a little bit, not by a few percent, it 16 00:01:02.100 --> 00:01:06.180 went up, like, 15 to 30 times its average flux. 17 00:01:06.200 --> 00:01:10.230 So we knew something was afoot, later on it 18 00:01:10.250 --> 00:01:14.360 turned out to be coincident, both in time and in space, with 19 00:01:14.380 --> 00:01:18.420 the neutrino that was detected by IceCube. 20 00:01:18.440 --> 00:01:22.570 IceCube is a neutrino telescope located at the South Pole, or to be 21 00:01:22.590 --> 00:01:26.590 more precise, under it. 22 00:01:26.610 --> 00:01:30.660 It consists of over 5,000 detectors that are spread out into a 23 00:01:30.680 --> 00:01:34.790 cube about a kilometer on each side. 24 00:01:34.810 --> 00:01:38.840 It's the world's biggest and it's coolest telescope. 25 00:01:38.860 --> 00:01:43.000 So a neutrino is an incredibly small 26 00:01:43.020 --> 00:01:47.100 particle, it moves almost at the speed of light, 27 00:01:47.120 --> 00:01:51.160 it is nearly massless, it's incredibly plentiful, 28 00:01:51.180 --> 00:01:55.300 but, it's very, very hard to detect because it 29 00:01:55.320 --> 00:01:59.380 will not interact with just about anything. If you could detect 30 00:01:59.400 --> 00:02:03.430 them though, because they have traveled through the universe essentially undeflected, 31 00:02:03.450 --> 00:02:07.500 they have information that you could not access in any other way. 32 00:02:07.520 --> 00:02:11.690 IceCube has detected a handful of extremely energetic 33 00:02:11.710 --> 00:02:15.740 neutrinos. One of them, which is called Big Bird, has an energy of 34 00:02:15.760 --> 00:02:19.870 about 2 peta-electron volts. To give you an idea of how much energy 35 00:02:19.890 --> 00:02:24.020 that is, it is about a million, million times the 36 00:02:24.040 --> 00:02:28.040 energy of dental X-ray. IceCube sees too large 37 00:02:28.060 --> 00:02:32.100 a patch of sky to let us determine exactly which blazar Big Bird 38 00:02:32.120 --> 00:02:36.220 came from. The enormous increase in gamma-ray flux seen by 39 00:02:36.240 --> 00:02:40.310 LAT and radio flux by other TANAMI telescopes let us finger 40 00:02:40.330 --> 00:02:44.410 the exact blazar which is responsible for Big Bird. 41 00:02:44.430 --> 00:02:48.600 We have long suspected that blazars are the birthplaces 42 00:02:48.620 --> 00:02:52.660 of such neutrinos. What we have been able to establish, for the 43 00:02:52.680 --> 00:02:56.740 first time, is an individual blazar as a potential 44 00:02:56.760 --> 00:03:00.810 birthplace of an individual neutrino. This is the first time that we can point 45 00:03:00.830 --> 00:03:04.960 and say "That blazar is where this neutrino came from." 46 00:03:04.980 --> 00:03:09.140 Blazars are the brightest steadily shining 47 00:03:09.160 --> 00:03:13.180 objects in the universe. However, many of the most basic questions 48 00:03:13.200 --> 00:03:17.290 about them, such as what is producing this tremendous amount of 49 00:03:17.310 --> 00:03:21.360 energy, remain open, and unanswered. The same process 50 00:03:21.380 --> 00:03:25.480 that produces this neutrino could also produce gamma rays, 51 00:03:25.500 --> 00:03:29.670 and that would move us closer to an understanding of emission from near black holes 52 00:03:29.690 --> 00:03:33.710 in blazars. [Music] 53 00:03:33.730 --> 00:03:37.760 [Music] 54 00:03:37.780 --> 00:03:41.800 [Music] 55 00:03:41.820 --> 00:03:45.860 [Music] 56 00:03:45.880 --> 00:03:49.960 [Beeping] 57 00:03:49.980 --> 00:03:57.617 [Beeping]