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