WEBVTT FILE 1 00:00:00.000 --> 00:00:03.980 (Music throughout) 2 00:00:04.000 --> 00:00:05.980 3 00:00:06.000 --> 00:00:13.980 This pulsar’s vast gamma-ray halo may explain a key observation about antimatter near Earth. 4 00:00:14.000 --> 00:00:20.980 [Big Dipper to scale] 5 00:00:21.000 --> 00:00:28.980 Pulsars are rapidly spinning neutron stars, the superdense remnants of supernovae explosions. 6 00:00:29.000 --> 00:00:32.980 7 00:00:33.000 --> 00:00:39.980 NASA’s Fermi mission has observed one nearby pulsar, Geminga, for more than 10 years. 8 00:00:40.000 --> 00:00:42.980 9 00:00:43.000 --> 00:00:49.980 The data are now so detailed that when scientists remove background sources… 10 00:00:50.000 --> 00:00:56.980 …Geminga’s faint but huge gamma-ray halo emerges. 11 00:00:57.000 --> 00:00:57.980 12 00:00:58.000 --> 00:01:04.980 This halo precisely matches computer models that account for positron production. 13 00:01:05.000 --> 00:01:06.980 14 00:01:07.000 --> 00:01:13.980 Positrons are antimatter versions of electrons. They’re found near Earth but have no clear origin. 15 00:01:14.000 --> 00:01:16.980 16 00:01:17.000 --> 00:01:24.980 Scientists suspected pulsars to be positron sources. This study confirms it. 17 00:01:25.000 --> 00:01:32.980 As it turns out, Geminga is likely the greatest positron source for Earth. 18 00:01:33.000 --> 00:01:40.980 It alone could produce 20% of the positrons at an energy of 1 TeV seen in orbit. 19 00:01:41.000 --> 00:01:48.980 So pulsars not only shine in the highest-energy light, they also glow in antimatter. 20 00:01:49.000 --> 00:01:52.980 21 00:01:53.000 --> 00:01:58.850 [Explore, Solar System & Beyond] 22 00:01:58.870 --> 00:01:58.799 [NASA]