WEBVTT FILE 1 00:00:00.020 --> 00:00:04.050 Similar to how meteorologists fly into hurricanes, NASA 2 00:00:04.070 --> 00:00:08.110 has now flown a mission through the heart of a magnetic reconnection explosion. 3 00:00:08.130 --> 00:00:12.250 We call this mission MMS. 4 00:00:12.270 --> 00:00:16.410 This team of 4 spacecraft studies magnetic reconnection, 5 00:00:16.430 --> 00:00:20.610 he powerful explosions that occur when magnetic fields collide and realign 6 00:00:20.630 --> 00:00:24.670 a process that occurs regularly throughout space. 7 00:00:24.690 --> 00:00:28.830 Close to Earth -- and throughout the universe -- space is far from empty. It contains electrons 8 00:00:28.850 --> 00:00:33.020 and ions, and most importantly, magnetic fields. This dynamic 9 00:00:33.040 --> 00:00:37.150 environment is unlike anything we experience on the ground. As we rely more 10 00:00:37.170 --> 00:00:41.210 on satellites or even prepare for a journey to Mars, we need to understand 11 00:00:41.230 --> 00:00:45.350 this complex system. Magnetic reconnection is one of the key forces driving particles 12 00:00:45.370 --> 00:00:49.550 o accelerate through space, and it’s a fundamental driver of space radiation -- 13 00:00:49.570 --> 00:00:53.730 a critical phenomenon to understand when protecting 14 00:00:53.750 --> 00:00:57.870 our satellites and astronauts. On October 16, 2015, MMS 15 00:00:57.890 --> 00:01:02.070 traveled straight through a magnetic reconnection event at the boundary 16 00:01:02.090 --> 00:01:06.130 where Earth’s magnetic fields bump up against the sun’s magnetic fields. 17 00:01:06.150 --> 00:01:10.260 In only a few seconds, MMS collected hundreds of observations 18 00:01:10.280 --> 00:01:14.350 of the way the magnetic fields and particles were moving -- represented with arrows 19 00:01:14.370 --> 00:01:18.500 in this visualization. Watch how they go along steadily and then suddenly being 20 00:01:18.520 --> 00:01:22.570 to go in every direction. This is the point where the magnetic fields reconfigured 21 00:01:22.590 --> 00:01:26.790 and particles were sent racing off at high speed. 22 00:01:26.810 --> 00:01:30.900 For the first time we have observations from the epicenter of an energy transfer as important 23 00:01:30.920 --> 00:01:35.040 to how things move in space as gravity is to how things move on Earth. 24 00:01:35.060 --> 00:01:39.200 This is just the start to understanding the huge forces at work in space. In its first year, MMS 25 00:01:39.220 --> 00:01:43.290 made more than 4,000 trips through the magnetic boundaries around Earth, each time gathering information 26 00:01:43.310 --> 00:01:47.340 about the way the magnetic fields and particles move and interact in our space environment-- 27 00:01:47.360 --> 00:01:51.390 crucial information as we make plans to explore far beyond our home planet. 28 00:01:51.410 --> 00:01:55.440 29 00:01:55.460 --> 00:01:59.590 tone 30 00:01:59.610 --> 00:02:03.690 tone 31 00:02:03.710 --> 00:02:07.780 beeping 32 00:02:07.800 --> 00:02:09.276