1 00:00:00,264 --> 00:00:04,463 So how much energy does fall on the surface of the Earth from the Sun? 2 00:00:04,843 --> 00:00:07,458 You can work it out with a beautiful simple experiment 3 00:00:07,498 --> 00:00:11,877 using only thermometer, tin full of water, and an umbrella. 4 00:00:12,143 --> 00:00:15,909 Basically, you let the water heat off in a tin to an ambient temperature, 5 00:00:16,009 --> 00:00:20,943 which here in Death Valley today is about 46°C. 6 00:00:21,020 --> 00:00:25,138 And then you put thermometer in the water 7 00:00:25,138 --> 00:00:30,722 you take the shade away and let the Sun shine on the water. 8 00:00:32,664 --> 00:00:36,693 In direct sunlight the water temperature begins to rise. 9 00:00:36,705 --> 00:00:42,608 By timing how long it takes the Sun to raise the water temperature by one degree Celsius, 10 00:00:42,608 --> 00:00:48,409 you can figure out exactly how much energy the Sun has delivered into the can of water. 11 00:00:48,424 --> 00:00:53,207 And from that, how much energy is delivered to a square metre of the surface. 12 00:00:53,843 --> 00:00:57,049 It turns out on a clear day, when the Sun is vertically overhead, 13 00:00:57,049 --> 00:00:59,120 that number is about a kilowatt. 14 00:00:59,120 --> 00:01:03,971 That's ten a hundred watt bulbs can be powered by the Sun's energy 15 00:01:03,971 --> 00:01:06,470 for every meter squared of the Earth's surface. 16 00:01:11,826 --> 00:01:16,017 In an audacious leap of imagination, Herschel used this figure to calculate 17 00:01:16,063 --> 00:01:19,681 the entire energy given off by the Sun. 18 00:01:23,376 --> 00:01:28,129 So imagine adding up those kilowatts over this entire landscape 19 00:01:32,169 --> 00:01:38,338 and then imagine, following the Sun's rays, as they cover the entire surface of the Earth. 20 00:01:43,265 --> 00:01:45,089 But then, imagine this: 21 00:01:45,189 --> 00:01:48,632 The Earth is 150 milion kilometres away from the Sun. 22 00:01:48,648 --> 00:01:55,322 So actually, the Sun is radiating the energy out across a giant sphere 23 00:01:55,322 --> 00:02:00,567 with the radius of 150 milion kilometres surrounding our star. 24 00:02:01,117 --> 00:02:02,788 And how much energy does that make? 25 00:02:02,926 --> 00:02:07,796 It's four times π times the distance to the Sun squared 26 00:02:07,906 --> 00:02:11,142 which is about three times... 27 00:02:14,727 --> 00:02:20,447 It's four hundred million million million million Watts. 28 00:02:26,177 --> 00:02:31,017 That is a million times the power compsumption of the United States 29 00:02:31,090 --> 00:02:35,010 every year radiated in one second. 30 00:02:35,094 --> 00:02:43,334 And we worked that out by using some water, a thermometer, a tin, and an umbrella. 31 00:02:44,488 --> 00:02:46,588 That's why I love physics.