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