1 00:00:00,500 --> 00:00:04,170 An unusual eruption on the Sun may offer clues to 2 00:00:04,180 --> 00:00:05,430 understanding our star's 3 00:00:05,460 --> 00:00:09,990 mysterious explosions. Solar eruptions are 4 00:00:10,000 --> 00:00:11,600 massive releases of material off the 5 00:00:11,610 --> 00:00:12,720 surface of the Sun. 6 00:00:15,980 --> 00:00:20,060 This material can travel across the solar system to 7 00:00:20,070 --> 00:00:21,170 Earth and Mars. 8 00:00:25,100 --> 00:00:28,610 The radiation in the material from the Sun can 9 00:00:28,620 --> 00:00:31,670 interact with the planets' magnetic fields, affecting 10 00:00:31,680 --> 00:00:33,620 astronauts and technology. 11 00:00:35,740 --> 00:00:38,630 Eruptions on the Sun usually come in one of three 12 00:00:38,640 --> 00:00:44,240 forms: coronal mass ejections, jets and partial eruptions. 13 00:00:47,830 --> 00:00:50,990 The new research studying an event named the 14 00:00:51,000 --> 00:00:54,870 Rosetta Stone of solar eruptions. Just as the 15 00:00:54,880 --> 00:00:56,790 Rosetta Stone was the key to understanding 16 00:00:56,800 --> 00:00:58,080 Egyptian hieroglyphics, 17 00:00:58,090 --> 00:01:00,630 studying this eruption could be the key to 18 00:01:00,690 --> 00:01:02,970 understanding all types of solar eruptions. 19 00:01:04,200 --> 00:01:08,110 In the Rosetta Stone eruption, all three types of 20 00:01:08,120 --> 00:01:09,700 eruptions happened in the same event. 21 00:01:10,390 --> 00:01:12,620 They usually occur separately. 22 00:01:14,500 --> 00:01:18,140 The main eruption was too big to be a jet, but too 23 00:01:18,150 --> 00:01:20,090 narrow to be a coronal mass ejection. 24 00:01:20,340 --> 00:01:23,700 A second cooler layer of material on the surface of 25 00:01:23,710 --> 00:01:26,340 the Sun also started to erupt about a half an hour 26 00:01:26,340 --> 00:01:32,690 later. But it fell back down as a partial solar eruption. 27 00:01:33,190 --> 00:01:36,830 This Rosetta Stone of solar eruptions will also give 28 00:01:36,840 --> 00:01:39,530 clues to help scientists predict large eruptions in 29 00:01:39,540 --> 00:01:39,920 the future. 30 00:01:42,040 --> 00:01:44,990 The better our predictions are, the more time we 31 00:01:45,050 --> 00:01:47,570 have to prepare for material from the Sun to 32 00:01:47,580 --> 00:01:49,190 interact with Earth's magnetic field. 33 00:01:52,360 --> 00:01:55,090 Predicting large solar eruptions can help better protect 34 00:01:55,100 --> 00:01:59,880 our astronauts and technology, near Earth and beyond.