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]