1 00:00:07,670 --> 00:00:05,910 material sciences are one of the major 2 00:00:09,669 --> 00:00:07,680 areas of laboratory research that the 3 00:00:11,669 --> 00:00:09,679 international space station supports and 4 00:00:13,990 --> 00:00:11,679 a new instrument from the european space 5 00:00:16,070 --> 00:00:14,000 agency is just being put into operation 6 00:00:17,830 --> 00:00:16,080 in that area the electromagnetic 7 00:00:20,150 --> 00:00:17,840 levitator was delivered to the station 8 00:00:21,910 --> 00:00:20,160 last year on the last automated transfer 9 00:00:23,910 --> 00:00:21,920 vehicle and set up in the columbus 10 00:00:26,790 --> 00:00:23,920 laboratory module and is being prepared 11 00:00:29,429 --> 00:00:26,800 for its first operations i spoke with dr 12 00:00:31,189 --> 00:00:29,439 douglas matson an associate professor of 13 00:00:33,990 --> 00:00:31,199 mechanical engineering at tufts 14 00:00:36,069 --> 00:00:34,000 university who serves as the eml's u.s 15 00:00:37,590 --> 00:00:36,079 facility scientist and as a speaker of 16 00:00:39,190 --> 00:00:37,600 the international working group 17 00:00:41,510 --> 00:00:39,200 representing all scientists doing 18 00:00:43,430 --> 00:00:41,520 research with eml i asked them to start 19 00:00:45,670 --> 00:00:43,440 by describing this new facility and tell 20 00:00:47,990 --> 00:00:45,680 me what it's capable of doing 21 00:00:50,549 --> 00:00:48,000 the electromagnetic levitator 22 00:00:53,430 --> 00:00:50,559 involves passing a high frequency 23 00:00:55,910 --> 00:00:53,440 current through copper cooled coils 24 00:00:56,709 --> 00:00:55,920 this current generates a magnetic field 25 00:00:59,830 --> 00:00:56,719 which 26 00:01:01,990 --> 00:00:59,840 causes the sample to levitate without 27 00:01:04,070 --> 00:01:02,000 touching anything therefore we can 28 00:01:06,630 --> 00:01:04,080 process samples of 29 00:01:08,789 --> 00:01:06,640 metallic substances in a very clean 30 00:01:09,910 --> 00:01:08,799 environment 31 00:01:15,030 --> 00:01:09,920 with 32 00:01:18,390 --> 00:01:15,040 chamber so what we look at is 33 00:01:21,109 --> 00:01:18,400 we look at how metals solidify 34 00:01:23,670 --> 00:01:21,119 how what the thermophysical properties 35 00:01:27,190 --> 00:01:23,680 are of those metals so that we can do 36 00:01:30,390 --> 00:01:27,200 process modeling here on earth and we 37 00:01:32,710 --> 00:01:30,400 look at the kinetics of the process you 38 00:01:34,310 --> 00:01:32,720 know how do you change from 39 00:01:36,710 --> 00:01:34,320 one uh 40 00:01:38,630 --> 00:01:36,720 crystalline structure to another 41 00:01:40,230 --> 00:01:38,640 so tell me why is it valuable for 42 00:01:42,389 --> 00:01:40,240 scientists to study the behavior of 43 00:01:44,389 --> 00:01:42,399 metals in the weightlessness 44 00:01:47,510 --> 00:01:44,399 the weightless environment allows us to 45 00:01:48,950 --> 00:01:47,520 do things that we can't do here on earth 46 00:01:51,910 --> 00:01:48,960 specifically 47 00:01:54,310 --> 00:01:51,920 the since the sample is levitated here 48 00:01:56,950 --> 00:01:54,320 on earth that means it's the sample 49 00:01:57,990 --> 00:01:56,960 itself is pulled down into the sample 50 00:01:58,709 --> 00:01:58,000 coils 51 00:02:01,350 --> 00:01:58,719 now 52 00:02:04,230 --> 00:02:01,360 therefore that creates a lot of stirring 53 00:02:05,510 --> 00:02:04,240 within the sample which is not what we'd 54 00:02:08,389 --> 00:02:05,520 like to have we'd like to have a 55 00:02:11,430 --> 00:02:08,399 quiescent sample so that we understand 56 00:02:14,070 --> 00:02:11,440 what is happening to the liquid itself 57 00:02:16,390 --> 00:02:14,080 so therefore in microgravity since the 58 00:02:19,430 --> 00:02:16,400 sample's not its weight doesn't have to 59 00:02:21,830 --> 00:02:19,440 be overcome you can use a lot less 60 00:02:24,070 --> 00:02:21,840 magnetic force and therefore a lot less 61 00:02:25,670 --> 00:02:24,080 stirring occurs so you can look at a 62 00:02:27,670 --> 00:02:25,680 quiescent drop 63 00:02:30,070 --> 00:02:27,680 take a look at its properties and get 64 00:02:32,869 --> 00:02:30,080 much better thermophysical properties or 65 00:02:35,190 --> 00:02:32,879 much better understanding of how the 66 00:02:37,670 --> 00:02:35,200 droplet solidifies the other thing we 67 00:02:39,589 --> 00:02:37,680 can do is we can look at how does 68 00:02:41,830 --> 00:02:39,599 stirring influence 69 00:02:44,790 --> 00:02:41,840 how solidification occurs 70 00:02:46,550 --> 00:02:44,800 so this is uh something that's both the 71 00:02:48,550 --> 00:02:46,560 thermophysical properties and the 72 00:02:51,110 --> 00:02:48,560 influence of convection 73 00:02:54,070 --> 00:02:51,120 are extremely important for process 74 00:02:56,630 --> 00:02:54,080 modeling for processes here on earth so 75 00:03:00,070 --> 00:02:56,640 it's not that we're solidifying a sample 76 00:03:02,229 --> 00:03:00,080 in zero gravity it's more that we have 77 00:03:05,270 --> 00:03:02,239 better experimental control 78 00:03:07,750 --> 00:03:05,280 in order to provide better properties 79 00:03:10,630 --> 00:03:07,760 and the better ability for people to 80 00:03:13,270 --> 00:03:10,640 model earthbound processes 81 00:03:15,430 --> 00:03:13,280 uh and therefore uh create 82 00:03:17,750 --> 00:03:15,440 much better process control 83 00:03:19,030 --> 00:03:17,760 with higher quality products here on 84 00:03:20,949 --> 00:03:19,040 earth 85 00:03:23,270 --> 00:03:20,959 what is the role of the astronauts on 86 00:03:27,110 --> 00:03:23,280 the station during the experiments 87 00:03:29,430 --> 00:03:27,120 using the electromagnetic levitator 88 00:03:31,910 --> 00:03:29,440 the astronauts role is to act as our 89 00:03:34,630 --> 00:03:31,920 hands and our eyes 90 00:03:37,830 --> 00:03:34,640 they do a lot of the equipment 91 00:03:38,630 --> 00:03:37,840 monitoring they install the facility 92 00:03:41,110 --> 00:03:38,640 when 93 00:03:44,070 --> 00:03:41,120 we take our samples from ground and 94 00:03:47,830 --> 00:03:44,080 bring them to our facility it comes in a 95 00:03:50,070 --> 00:03:47,840 big giant box called a sample carousel 96 00:03:52,070 --> 00:03:50,080 it's a carousel because the samples spin 97 00:03:54,309 --> 00:03:52,080 on this inside this box 98 00:03:56,630 --> 00:03:54,319 and so there's 18 samples that are going 99 00:03:58,550 --> 00:03:56,640 to be processed at any one time 100 00:04:00,789 --> 00:03:58,560 we have multiple times that we're going 101 00:04:03,509 --> 00:04:00,799 to be bringing different carousels up so 102 00:04:05,589 --> 00:04:03,519 the astronauts install our samples on 103 00:04:08,149 --> 00:04:05,599 our facility and then 104 00:04:10,470 --> 00:04:08,159 safely pack up the samples so that they 105 00:04:13,509 --> 00:04:10,480 can be brought back here to earth so we 106 00:04:15,990 --> 00:04:13,519 can study how the samples solidified and 107 00:04:18,550 --> 00:04:16,000 what kind of structures we have formed 108 00:04:20,710 --> 00:04:18,560 during their solidification on orbit the 109 00:04:23,350 --> 00:04:20,720 other thing that the astronauts do is 110 00:04:25,430 --> 00:04:23,360 they go in and they will 111 00:04:27,510 --> 00:04:25,440 change out equipment that we need for a 112 00:04:29,030 --> 00:04:27,520 specific experiment 113 00:04:30,469 --> 00:04:29,040 for instance we have two different 114 00:04:32,870 --> 00:04:30,479 camera systems 115 00:04:35,830 --> 00:04:32,880 one that has very high spatial 116 00:04:38,230 --> 00:04:35,840 resolution so we can see fine details 117 00:04:40,070 --> 00:04:38,240 and one that goes extremely fast so that 118 00:04:41,590 --> 00:04:40,080 we can look at processes that occur 119 00:04:44,150 --> 00:04:41,600 quickly 120 00:04:47,189 --> 00:04:44,160 in order to change out these cameras we 121 00:04:49,670 --> 00:04:47,199 need to have the astronauts go in and as 122 00:04:53,030 --> 00:04:49,680 a matter of fact during a past shuttle 123 00:04:54,950 --> 00:04:53,040 mission during my experiment 124 00:04:57,670 --> 00:04:54,960 the cameras stopped working and the 125 00:05:00,310 --> 00:04:57,680 astronauts had to go in 126 00:05:02,070 --> 00:05:00,320 check the system out they found that one 127 00:05:04,230 --> 00:05:02,080 of the cables was malfunctioning and 128 00:05:06,710 --> 00:05:04,240 they were able to change that cable out 129 00:05:09,029 --> 00:05:06,720 and allow me to do my experiments so the 130 00:05:11,430 --> 00:05:09,039 astronauts do a lot for us can you give 131 00:05:13,270 --> 00:05:11,440 me some examples of some of the science 132 00:05:15,350 --> 00:05:13,280 experiment runs that you have planned 133 00:05:16,870 --> 00:05:15,360 for the astronauts on station 134 00:05:18,230 --> 00:05:16,880 all right we have uh 135 00:05:22,230 --> 00:05:18,240 many different international 136 00:05:25,029 --> 00:05:22,240 collaborations on our using our facility 137 00:05:27,990 --> 00:05:25,039 where one of the projects is looking at 138 00:05:29,909 --> 00:05:28,000 thermophysical properties and 139 00:05:33,110 --> 00:05:29,919 how we could use those properties than 140 00:05:36,310 --> 00:05:33,120 in ma in process modeling here on earth 141 00:05:38,150 --> 00:05:36,320 we have a project on sedimentation 142 00:05:39,110 --> 00:05:38,160 looking at demixing and interfacial 143 00:05:40,790 --> 00:05:39,120 tension 144 00:05:44,230 --> 00:05:40,800 one on development of composite 145 00:05:45,990 --> 00:05:44,240 structures one on magnetic materials 146 00:05:47,830 --> 00:05:46,000 and development of turbine blade 147 00:05:49,830 --> 00:05:47,840 materials 148 00:05:53,510 --> 00:05:49,840 finally we have one looking at 149 00:05:56,550 --> 00:05:53,520 icosahedral order and quasi-crystal 150 00:05:59,350 --> 00:05:56,560 formation so we have a multiple array of 151 00:06:00,629 --> 00:05:59,360 many different projects there involved 152 00:06:03,029 --> 00:06:00,639 looking at 153 00:06:05,430 --> 00:06:03,039 how metals solidify 154 00:06:07,590 --> 00:06:05,440 differently depending on what their 155 00:06:09,510 --> 00:06:07,600 composition is how many researchers 156 00:06:11,670 --> 00:06:09,520 around the world are actually using this 157 00:06:16,469 --> 00:06:11,680 hardware that you have 158 00:06:19,590 --> 00:06:16,479 currently we have 14 european teams 159 00:06:22,469 --> 00:06:19,600 four u.s teams collaborating with them 160 00:06:24,870 --> 00:06:22,479 one canadian team and i believe three 161 00:06:25,749 --> 00:06:24,880 asian teams 162 00:06:28,070 --> 00:06:25,759 so 163 00:06:30,710 --> 00:06:28,080 that involves about 50 scientists 164 00:06:33,670 --> 00:06:30,720 worldwide we also have a rather large 165 00:06:35,029 --> 00:06:33,680 support structure and from esa 166 00:06:39,110 --> 00:06:35,039 and from 167 00:06:41,350 --> 00:06:39,120 nasa and the japanese space agency jaxa 168 00:06:44,629 --> 00:06:41,360 and the german space agency 169 00:06:45,990 --> 00:06:44,639 and uh airbus a uh a 170 00:06:48,390 --> 00:06:46,000 those are the people who actually build 171 00:06:50,790 --> 00:06:48,400 the facility so it's over 100 people who 172 00:06:52,629 --> 00:06:50,800 are involved with this project 173 00:06:54,390 --> 00:06:52,639 thank you for your time today and uh 174 00:06:55,670 --> 00:06:54,400 explaining all of the science that's 175 00:06:57,270 --> 00:06:55,680 going on and all the work that you're