1 00:00:08,070 --> 00:00:04,040 Music 2 00:00:08,090 --> 00:00:12,120 NASA's STEREO spacecraft 3 00:00:12,140 --> 00:00:16,130 resolved a 40-year mystery about how coronal mass ejections, or 4 00:00:16,150 --> 00:00:20,160 CME's, change shape during their long journey. With new data 5 00:00:20,180 --> 00:00:24,190 processing techniques, STEREO scientists have succeeded in continuously 6 00:00:24,210 --> 00:00:28,220 tracking space weather events from the Sun's ultra hot corona to 7 00:00:28,240 --> 00:00:32,290 the Earth, 93 million miles away. A CME 8 00:00:32,310 --> 00:00:36,340 is a huge, magnetized cloud of electrified gas, or plasma, 9 00:00:36,360 --> 00:00:41,960 that bursts out of the sun's atmosphere. It can be as big as one-and-a-half trillion tons of 10 00:00:41,980 --> 00:00:46,000 gas and travel at 3 million miles per hour. 11 00:00:46,020 --> 00:00:50,050 If a powerful CME hits the Earth's protective magnetosphere, it 12 00:00:50,070 --> 00:00:54,080 makes brilliant aurora, and can disrupt satellites, radio communications, 13 00:00:54,100 --> 00:00:58,130 and even our electrical power grids. Despite decades of observations 14 00:00:58,150 --> 00:01:02,170 with NASA's Heliophysics fleet of spacecraft, the details 15 00:01:02,190 --> 00:01:06,200 of the connection between activity on the sun and its effect on Earth has 16 00:01:06,220 --> 00:01:10,240 been poorly understood. This is because CMEs change while traveling 17 00:01:10,260 --> 00:01:14,290 from the sun to Earth and it's difficult to track their movement with only a 18 00:01:14,310 --> 00:01:18,430 head-on perspective. Now, with STEREO's two spacecraft 19 00:01:18,450 --> 00:01:22,460 sitting on either side of the sun, we can monitor the sky at large 20 00:01:22,480 --> 00:01:26,480 angles from Earth, and can see the full ocean of empty space between the sun 21 00:01:26,500 --> 00:01:30,480 and Earth. But CME's are some 10 billion times 22 00:01:30,500 --> 00:01:34,510 fainter than the full moon and were still too dark to see until 23 00:01:34,530 --> 00:01:38,530 scientists applied cutting-edge image processing techniques to separate 24 00:01:38,550 --> 00:01:42,550 the CME's from the starfield. 25 00:01:42,570 --> 00:01:46,560 By applying this new technology scientists 26 00:01:46,580 --> 00:01:50,590 were able to measure the absolute brightness of detailed features in the first 27 00:01:50,610 --> 00:01:54,610 large Earth-directed CME seen by STEREO, which occurred 28 00:01:54,630 --> 00:01:58,620 in late 2008. By the time the data were collected, 29 00:01:58,640 --> 00:02:02,650 STEREO-A was nearly 45 degrees ahead of Earth in its orbit, 30 00:02:02,670 --> 00:02:06,690 affording a very clear view of the CME's path from 31 00:02:06,710 --> 00:02:10,710 sun to Earth. For the first time ever, 32 00:02:10,730 --> 00:02:14,740 scientists can watch a CME from its formation on the sun to its 33 00:02:14,760 --> 00:02:18,750 impact with Earth's magnetosphere ending decades of speculation 34 00:02:18,770 --> 00:02:22,810 about how features in the sun's corona cause the massive, complex shape of a 35 00:02:22,830 --> 00:02:26,850 CME as it expands to ten million times 36 00:02:26,870 --> 00:02:30,880 its size. This new ability to see developing space weather during 37 00:02:30,900 --> 00:02:34,900 its entire transit from the Sun will enable scientists to better predict when 38 00:02:34,920 --> 00:02:38,980 and how a CME will impact Earth and understand how 39 00:02:39,000 --> 00:02:43,010 CME's change between the sun and our home. 40 00:02:43,030 --> 00:02:47,020 Music