1 00:00:01,400 --> 00:00:07,070 Let’s say this is the equivalent of the sun’s total energy output. 2 00:00:07,090 --> 00:00:12,230 You can accumulate a hundred dollars a lot of different ways… 3 00:00:12,250 --> 00:00:13,830 But a hundred bucks… 4 00:00:13,850 --> 00:00:17,560 …is a hundred bucks! 5 00:00:15,580 --> 00:00:18,770 If energy from the sun were a hundred dollars, 6 00:00:18,790 --> 00:00:22,530 it would be important to know what kinds of currency was coming in— 7 00:00:22,550 --> 00:00:23,810 big groups of pennies … 8 00:00:23,830 --> 00:00:25,290 …whole dollar bills… 9 00:00:25,310 --> 00:00:27,820 …or combinations. 10 00:00:27,840 --> 00:00:30,580 The total amount of solar energy falling on Earth 11 00:00:30,600 --> 00:00:34,880 generally doesn’t vary more than about 1 dime to $100 12 00:00:34,900 --> 00:00:39,390 but the kinds of energy from the Sun can fluctuate. 13 00:00:39,410 --> 00:00:42,190 Remember that light we see with our eyes 14 00:00:42,210 --> 00:47:59,890 is actually a combination of many different colors, or wavelengths. 15 00:47:59,910 --> 00:00:49,630 That’s true also for the light we do NOT see. 16 00:00:49,650 --> 00:00:53,290 The composition of that light matters to understanding Earth’s energy budget, 17 00:00:53,310 --> 00:00:59,770 and that’s the reason NASA has a new instrument designed to study this question. 18 00:00:59,790 --> 00:01:00,510 It’s called TSIS— 19 00:01:00,530 --> 00:01:06,820 —the Total and Spectral Solar Irradiance Sensor. 20 00:01:06,840 --> 00:01:08,550 It is important to know that the Sun supplies 21 00:01:08,570 --> 00:01:11,910 virtually all of the energy coming to Earth. 22 00:01:11,930 --> 00:01:15,880 But...inbetween the Earth and the Sun 23 00:01:15,900 --> 00:01:16,320 there is the atmosphere. 24 00:01:16,340 --> 00:01:19,920 In the atmosphere there are clouds, there are aerosols-- 25 00:01:19,940 --> 00:01:24,920 that is particles--there are gasses 26 00:01:24,880 --> 00:01:26,810 that interefere with solar radiation reaching Earth. 27 00:01:26,830 --> 00:01:27,170 So, that's why we need to fly a satellite.... 28 00:01:27,190 --> 00:01:28,510 to be above the atmosphere 29 00:01:28,530 --> 00:01:31,970 Mounted to the International Space Station, 30 00:01:31,990 --> 00:01:35,220 TSIS will collect detailed assessments of solar energy. 31 00:01:35,240 --> 00:01:38,340 Those data will be vital for scientists 32 00:01:38,360 --> 00:01:41,420 to make more accurate forecasts about climate change 33 00:01:41,440 --> 00:01:57,899 and other interactions between our planet and our parent star.