WEBVTT FILE 1 00:00:04.000 --> 00:00:08.150 Tone 2 00:00:08.170 --> 00:00:12.180 music 3 00:00:12.200 --> 00:00:16.360 How did Earth warm enough to support life. New research suggests that the answer lies 4 00:00:16.380 --> 00:00:20.540 in a perfect coupling between a star and a planet. Today, 5 00:00:20.560 --> 00:00:24.610 Earth stays warms because carbon dioxide in the atmosphere holds in reflected heat from the 6 00:00:24.630 --> 00:00:28.800 sun. But four billion years ago, the Earth received less warmth from the sun, 7 00:00:28.820 --> 00:00:32.970 because the sun was a young star and produced less heat. 8 00:00:32.990 --> 00:00:37.160 Recent models of our young star show it was much more violent than it is now, constantly 9 00:00:37.180 --> 00:00:41.210 erupting and sending out huge particle clouds 10 00:00:41.230 --> 00:00:45.390 Young Earth was different too. It was still growing it's magnetosphere, 11 00:00:45.410 --> 00:00:49.070 the magnetic shield that protects planets from the sun's forces. 12 00:00:49.090 --> 00:00:53.140 The magnetosphere's polar caps were far wider than they are now. This 13 00:00:53.160 --> 00:00:57.320 let particles from the active sun seep into Earth's nitrogen-rich atmosphere. 14 00:00:57.340 --> 00:01:01.500 The solar particles split up the nitrogen molecules into atoms 15 00:01:01.520 --> 00:01:05.620 and carbon dioxide in the atmosphere to oxygen and carbon atoms. 16 00:01:05.640 --> 00:01:09.800 The free-roaming oxygen paired with the nitrogen. The result 17 00:01:09.820 --> 00:01:13.850 was nitrous oxide, a powerful greenhouse gas. 18 00:01:13.870 --> 00:01:18.040 Despite the weak contribution from the sun, the planet was able to warm 19 00:01:18.060 --> 00:01:22.090 enough to brew and incubate life. 20 00:01:22.110 --> 00:01:26.240 beeping 21 00:01:26.260 --> 00:01:29.503 beeping