1 00:00:13,270 --> 00:00:11,430 mineral dust can travel thousands of 2 00:00:15,190 --> 00:00:13,280 miles where it interacts throughout the 3 00:00:17,590 --> 00:00:15,200 earth system in our case we're going to 4 00:00:19,750 --> 00:00:17,600 study how that mineral dust heats or 5 00:00:21,510 --> 00:00:19,760 cools planet earth currently we aren't 6 00:00:24,390 --> 00:00:21,520 sure whether mineral dust 7 00:00:27,189 --> 00:00:24,400 heats the planet or cools the planet 8 00:00:29,349 --> 00:00:27,199 we're looking at dust sources 9 00:00:32,790 --> 00:00:29,359 on the earth's surface so deserts arid 10 00:00:35,190 --> 00:00:32,800 regions wind can basically emit 11 00:00:37,190 --> 00:00:35,200 that dust into the atmosphere 12 00:00:39,270 --> 00:00:37,200 and so we are very interested in knowing 13 00:00:40,549 --> 00:00:39,280 what it is and depending on what it is 14 00:00:43,110 --> 00:00:40,559 it will tell us whether or not it is 15 00:00:45,190 --> 00:00:43,120 warming or cooling our environment 16 00:00:47,110 --> 00:00:45,200 some minerals are dark maybe more red 17 00:00:48,950 --> 00:00:47,120 they would absorb solar energy and they 18 00:00:50,630 --> 00:00:48,960 could be heating elements other cases 19 00:00:52,790 --> 00:00:50,640 minerals are bright white and they could 20 00:00:54,630 --> 00:00:52,800 reflect sunlight back into space and 21 00:00:56,709 --> 00:00:54,640 cool the atmosphere 22 00:00:58,790 --> 00:00:56,719 and these desert dust plumes once they 23 00:01:00,630 --> 00:00:58,800 get into the atmosphere they are not 24 00:01:03,910 --> 00:01:00,640 small if you look at some of the 25 00:01:07,270 --> 00:01:03,920 satellite imagery you can see these huge 26 00:01:08,550 --> 00:01:07,280 desert dust plumes larger than spain for 27 00:01:10,950 --> 00:01:08,560 example 28 00:01:13,109 --> 00:01:10,960 coming across the north atlantic so this 29 00:01:14,950 --> 00:01:13,119 is an important impact potentially on 30 00:01:16,950 --> 00:01:14,960 climate change looking into the future 31 00:01:18,870 --> 00:01:16,960 as more lands become dust-forming 32 00:01:20,390 --> 00:01:18,880 regions as they become desertified we'll 33 00:01:22,390 --> 00:01:20,400 want to understand how those changes 34 00:01:24,789 --> 00:01:22,400 will affect our climate in the future 35 00:01:26,550 --> 00:01:24,799 this experiment is so important for us 36 00:01:28,310 --> 00:01:26,560 to understand what's going on at the 37 00:01:35,900 --> 00:01:28,320 surface of the earth in terms of the 38 00:01:35,910 --> 00:01:40,069 [Music] 39 00:01:44,710 --> 00:01:42,789 first we'll launch on a resupply service 40 00:01:47,350 --> 00:01:44,720 vehicle to the international space 41 00:01:49,350 --> 00:01:47,360 station and once we're on the iss we 42 00:01:51,670 --> 00:01:49,360 would attach to the exterior of the 43 00:01:54,230 --> 00:01:51,680 space station and i can't imagine a 44 00:01:56,310 --> 00:01:54,240 better platform than the international 45 00:01:58,310 --> 00:01:56,320 space station to measure 46 00:02:01,190 --> 00:01:58,320 earth science 47 00:02:03,429 --> 00:02:01,200 emit is an imaging spectrometer so it 48 00:02:05,429 --> 00:02:03,439 has a telescope which basically collects 49 00:02:06,950 --> 00:02:05,439 a lot of light and we image all of that 50 00:02:08,949 --> 00:02:06,960 light onto 51 00:02:10,309 --> 00:02:08,959 the slit of what we call a spectrometer 52 00:02:11,910 --> 00:02:10,319 that measures light in many different 53 00:02:14,070 --> 00:02:11,920 wavelengths of the electromagnetic 54 00:02:15,830 --> 00:02:14,080 spectrum our eyes see three wavelengths 55 00:02:17,670 --> 00:02:15,840 red green and blue but emits c's in 56 00:02:20,229 --> 00:02:17,680 hundreds of wavelengths out into the the 57 00:02:21,589 --> 00:02:20,239 infrared they give us signatures like 58 00:02:23,830 --> 00:02:21,599 fingerprints 59 00:02:26,390 --> 00:02:23,840 as we're traveling on the iss looking 60 00:02:28,710 --> 00:02:26,400 down at earth focusing on the spectral 61 00:02:29,830 --> 00:02:28,720 characteristics of minerals that are on 62 00:02:32,470 --> 00:02:29,840 the earth and so the imaging 63 00:02:34,790 --> 00:02:32,480 spectrometer allows us to detect those 64 00:02:36,470 --> 00:02:34,800 spectral signatures that tell us what 65 00:02:38,470 --> 00:02:36,480 type of mineral they're actually looking 66 00:02:40,390 --> 00:02:38,480 at 67 00:02:42,710 --> 00:02:40,400 this is setting a new benchmark for the 68 00:02:45,270 --> 00:02:42,720 quality of this class of instrumentation 69 00:02:47,270 --> 00:02:45,280 this is just extraordinary it's really a 70 00:02:49,190 --> 00:02:47,280 convergence of state-of-the-art 71 00:02:51,589 --> 00:02:49,200 technology and state-of-the-art science 72 00:02:56,330 --> 00:02:51,599 so that we better understand the climate