1 00:00:11,350 --> 00:00:09,509 now that you know that stars vary in 2 00:00:13,190 --> 00:00:11,360 abundance for every element we can look 3 00:00:15,669 --> 00:00:13,200 at how one element affects the chance of 4 00:00:17,510 --> 00:00:15,679 life in a planetary system the habitable 5 00:00:19,990 --> 00:00:17,520 zone is the region around a star that 6 00:00:22,230 --> 00:00:20,000 can support liquid water we know that as 7 00:00:25,029 --> 00:00:22,240 stars age this region moves away from 8 00:00:26,630 --> 00:00:25,039 the star therefore any orbiting planets 9 00:00:27,910 --> 00:00:26,640 only have a certain time to remain 10 00:00:29,669 --> 00:00:27,920 habitable 11 00:00:31,910 --> 00:00:29,679 recent calculations have shown that 12 00:00:33,830 --> 00:00:31,920 variations in oxygen alone greatly 13 00:00:35,270 --> 00:00:33,840 affect the distance and lifetimes of 14 00:00:37,750 --> 00:00:35,280 habitable zones 15 00:00:39,670 --> 00:00:37,760 for example a star with half the oxygen 16 00:00:41,590 --> 00:00:39,680 of our sun would have a habitable zone 17 00:00:43,430 --> 00:00:41,600 at a greater distance and would last 18 00:00:45,830 --> 00:00:43,440 about three and a half billion years 19 00:00:47,430 --> 00:00:45,840 whereas if it had twice the oxygen it 20 00:00:48,869 --> 00:00:47,440 would be closer and last about nine 21 00:00:50,790 --> 00:00:48,879 billion years 22 00:00:52,470 --> 00:00:50,800 as well as determining the habitability