1 00:00:00,000 --> 00:00:04,000 CO2 is warm in the planet. 2 00:00:04,000 --> 00:00:09,000 And the equation on CO2 is actually a very straightforward one. 3 00:00:09,000 --> 00:00:16,000 If you sum up the CO2 that gets emitted, that leads to a temperature increase. 4 00:00:16,000 --> 00:00:20,000 And that temperature increase leads to some very negative effects. 5 00:00:20,000 --> 00:00:26,000 The effects on the weather perhaps worse the indirect effects in that the natural ecosystems 6 00:00:26,000 --> 00:00:28,000 can't adjust to these rapid changes. 7 00:00:28,000 --> 00:00:31,000 And so you get ecosystem collapses. 8 00:00:31,000 --> 00:00:38,000 Now the exact amount of how you map from a certain increase in CO2 to what temperature will be 9 00:00:38,000 --> 00:00:40,000 and where the positive feedbacks are. 10 00:00:40,000 --> 00:00:43,000 There's some uncertainty there, but not very much. 11 00:00:43,000 --> 00:00:49,000 And there's certainly uncertainty about how bad those effects will be, but they will be extremely bad. 12 00:00:49,000 --> 00:00:51,000 I asked the top scientists in several times. 13 00:00:51,000 --> 00:00:54,000 Do we really have to get down to near zero? 14 00:00:54,000 --> 00:00:57,000 Can't we just cut it in half or a quarter? 15 00:00:57,000 --> 00:01:03,000 And the answer is that until we get near to zero, the temperature will continue to rise. 16 00:01:03,000 --> 00:01:05,000 And so that's a big challenge. 17 00:01:05,000 --> 00:01:10,000 It's very different than saying we're a 12 foot high truck trying to get under a 10 foot bridge. 18 00:01:10,000 --> 00:01:13,000 And we can just sort of squeeze under. 19 00:01:13,000 --> 00:01:17,000 This is something that has to get to zero. 20 00:01:17,000 --> 00:01:23,000 Now we put out a lot of carbon dioxide every year over 26 billion tons. 21 00:01:23,000 --> 00:01:27,000 For each American, it's about 20 tons. 22 00:01:27,000 --> 00:01:30,000 For people in poor countries, it's less than one ton. 23 00:01:30,000 --> 00:01:34,000 It's an average about five tons for everyone on the planet. 24 00:01:34,000 --> 00:01:39,000 And somehow we have to make changes that will bring that down to zero. 25 00:01:39,000 --> 00:01:42,000 It's been constantly going up. 26 00:01:42,000 --> 00:01:46,000 It's only very a economic changes that have even flattened it at all. 27 00:01:46,000 --> 00:01:51,000 So we have to go from rapidly rising to falling and falling all the way to zero. 28 00:01:51,000 --> 00:01:55,000 This equation has four factors, a little bit of multiplication. 29 00:01:55,000 --> 00:01:59,000 So you've got a thing on the left, CO2 that you want to get to zero. 30 00:01:59,000 --> 00:02:02,000 And that's going to be based on the number of people. 31 00:02:02,000 --> 00:02:06,000 The services, each person's using on average. 32 00:02:06,000 --> 00:02:09,000 The energy on average for each service. 33 00:02:09,000 --> 00:02:13,000 And the CO2 being put out per unit of energy. 34 00:02:13,000 --> 00:02:18,000 So let's look at each one of these and see how we can get this down to zero. 35 00:02:18,000 --> 00:02:22,000 Probably one of these numbers is going to have to get pretty near to zero. 36 00:02:22,000 --> 00:02:25,000 That's back from a high school algebra. 37 00:02:25,000 --> 00:02:27,000 But let's take a look. 38 00:02:27,000 --> 00:02:29,000 First we've got population. 39 00:02:29,000 --> 00:02:32,000 The world today has 6.8 billion people. 40 00:02:32,000 --> 00:02:34,000 That's headed up to about 9 billion. 41 00:02:34,000 --> 00:02:41,000 Now if we do a really great job on new vaccines, health care, reproductive health services, 42 00:02:42,000 --> 00:02:45,000 we could lower that by perhaps 10 or 15%. 43 00:02:45,000 --> 00:02:49,000 But there we see an increase of about 1.3.