WEBVTT FILE 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 34 00:01:55.100 --> 00:01:59.880 protect astronauts in space and technology on Earth.