1 00:00:08,629 --> 00:00:06,869 right now spacecraft communicate and 2 00:00:11,030 --> 00:00:08,639 send data back and forth using radio 3 00:00:12,950 --> 00:00:11,040 frequencies much like your car radio 4 00:00:15,190 --> 00:00:12,960 well the opals investigation is proving 5 00:00:16,550 --> 00:00:15,200 that it can now be done with lasers i 6 00:00:18,870 --> 00:00:16,560 caught up with matt abrahamson at the 7 00:00:21,510 --> 00:00:18,880 jet propulsion laboratory to learn why 8 00:00:23,269 --> 00:00:21,520 opals may be the gem scientists are 9 00:00:24,870 --> 00:00:23,279 looking for 10 00:00:26,470 --> 00:00:24,880 we launched up to the space station in 11 00:00:27,830 --> 00:00:26,480 april 2014 12 00:00:29,990 --> 00:00:27,840 and we're a technology demonstration 13 00:00:32,790 --> 00:00:30,000 mission for laser communications 14 00:00:34,790 --> 00:00:32,800 technology that's sending data over 15 00:00:37,430 --> 00:00:34,800 laser beams rather than radio waves why 16 00:00:39,110 --> 00:00:37,440 is that so important uh well basically a 17 00:00:41,350 --> 00:00:39,120 laser beam is much more focused than a 18 00:00:42,709 --> 00:00:41,360 radio wave so for the 19 00:00:44,549 --> 00:00:42,719 smaller amount of power that's 20 00:00:45,830 --> 00:00:44,559 transmitted you can transmit much more 21 00:00:48,069 --> 00:00:45,840 information 22 00:00:50,310 --> 00:00:48,079 it's also at a higher frequency than 23 00:00:51,910 --> 00:00:50,320 radio waves so you can pack more bits 24 00:00:53,830 --> 00:00:51,920 into that same data stream so you can 25 00:00:55,590 --> 00:00:53,840 get data rates that are 10 to 100 times 26 00:00:57,670 --> 00:00:55,600 faster than the potential for radio 27 00:00:59,590 --> 00:00:57,680 waves so we've we've practiced this a 28 00:01:02,069 --> 00:00:59,600 few times we've we've seen it in action 29 00:01:03,670 --> 00:01:02,079 how'd it work oh worked great um we got 30 00:01:05,189 --> 00:01:03,680 up there in april as i mentioned uh we 31 00:01:07,670 --> 00:01:05,199 started operating in may 32 00:01:09,429 --> 00:01:07,680 uh everything checked out as as expected 33 00:01:11,109 --> 00:01:09,439 uh went through a few checks to make 34 00:01:12,870 --> 00:01:11,119 sure we can point because one of the 35 00:01:14,149 --> 00:01:12,880 major technologies of this is to 36 00:01:14,950 --> 00:01:14,159 demonstrate that we can point within a 37 00:01:16,789 --> 00:01:14,960 few 38 00:01:17,749 --> 00:01:16,799 micro radians of the target ground 39 00:01:20,550 --> 00:01:17,759 station 40 00:01:22,149 --> 00:01:20,560 and we had our first success on june 5th 41 00:01:24,070 --> 00:01:22,159 we were able to actually transmit a high 42 00:01:26,710 --> 00:01:24,080 definition video from the space station 43 00:01:34,310 --> 00:01:26,720 on opals down to our ground station 44 00:01:38,069 --> 00:01:36,630 so how does that work with is there crew 45 00:01:40,310 --> 00:01:38,079 involvement with this or is it just 46 00:01:41,670 --> 00:01:40,320 strictly from the ground uh there's no 47 00:01:43,670 --> 00:01:41,680 crew involvement we're an external 48 00:01:45,749 --> 00:01:43,680 payload so we sit on the outside on 49 00:01:47,590 --> 00:01:45,759 express logistics carrier one and 50 00:01:49,030 --> 00:01:47,600 everything's ground commanded from jpl 51 00:01:50,469 --> 00:01:49,040 we send the commands from there they go 52 00:01:52,469 --> 00:01:50,479 over to marshall space flight center 53 00:01:54,550 --> 00:01:52,479 then to johnson space flight center to 54 00:01:56,149 --> 00:01:54,560 white sands up through tdrs all the way 55 00:01:58,310 --> 00:01:56,159 over to our payload in a matter of a few 56 00:02:00,069 --> 00:01:58,320 seconds which is uh kind of incredible 57 00:02:02,310 --> 00:02:00,079 uh so we command each step in the 58 00:02:04,389 --> 00:02:02,320 process uh to prepare for 59 00:02:05,670 --> 00:02:04,399 uh this transmission and uh during the 60 00:02:07,350 --> 00:02:05,680 actual time period of the transmission 61 00:02:09,190 --> 00:02:07,360 which is about two and a half minutes 62 00:02:10,630 --> 00:02:09,200 when we pass over the ground station 63 00:02:12,150 --> 00:02:10,640 everything's automated at that point so 64 00:02:14,070 --> 00:02:12,160 we have this closed-loop tracking over 65 00:02:15,510 --> 00:02:14,080 them that will track a ground station 66 00:02:16,790 --> 00:02:15,520 and transmit that video down to the 67 00:02:18,790 --> 00:02:16,800 ground 68 00:02:20,630 --> 00:02:18,800 it's the story of an endless search to 69 00:02:22,470 --> 00:02:20,640 serve the communications needs of 70 00:02:23,910 --> 00:02:22,480 america 71 00:02:25,430 --> 00:02:23,920 why the hurry 72 00:02:27,510 --> 00:02:25,440 so when we transmit things you 73 00:02:30,150 --> 00:02:27,520 transmitted a video are you trying to 74 00:02:32,150 --> 00:02:30,160 transmit several things at once or is it 75 00:02:33,830 --> 00:02:32,160 one at a time how does that work uh it's 76 00:02:35,350 --> 00:02:33,840 one video and we'll continuously loop it 77 00:02:37,509 --> 00:02:35,360 so there may be dropouts during the 78 00:02:38,869 --> 00:02:37,519 middle of the transmission 79 00:02:40,550 --> 00:02:38,879 typically we're transmitting 50 megabits 80 00:02:43,030 --> 00:02:40,560 per second and our standard video is 81 00:02:44,550 --> 00:02:43,040 about 175 megabits so every three and a 82 00:02:46,630 --> 00:02:44,560 half seconds you'll get a new copy of 83 00:02:48,229 --> 00:02:46,640 the video but you could have dropouts in 84 00:02:50,470 --> 00:02:48,239 the middle so we have an algorithm that 85 00:02:51,750 --> 00:02:50,480 if you do have a few packet dropouts 86 00:02:53,509 --> 00:02:51,760 when we reconstruct it on the ground you 87 00:02:54,470 --> 00:02:53,519 can take different portions of the video 88 00:02:55,750 --> 00:02:54,480 from 89 00:02:58,869 --> 00:02:55,760 different packets that were received and 90 00:03:00,470 --> 00:02:58,879 reconstruct one video now in practice 91 00:03:02,309 --> 00:03:00,480 it worked much better than expected so 92 00:03:05,110 --> 00:03:02,319 our bit error rate was so low it seemed 93 00:03:06,869 --> 00:03:05,120 like every copy we got the full copy 94 00:03:08,309 --> 00:03:06,879 there were a few instances where we hit 95 00:03:09,270 --> 00:03:08,319 clouds and if you hit a cloud with the 96 00:03:10,790 --> 00:03:09,280 laser 97 00:03:12,470 --> 00:03:10,800 you have a drop out so we did have a 98 00:03:14,630 --> 00:03:12,480 couple instances we had 10 seconds of 99 00:03:16,070 --> 00:03:14,640 drop out but we'd have enough of the 100 00:03:18,550 --> 00:03:16,080 video transmission to reconstruct a 101 00:03:20,470 --> 00:03:18,560 complete video at the end how does this 102 00:03:22,149 --> 00:03:20,480 translate to 103 00:03:22,949 --> 00:03:22,159 long-duration missions this is what 104 00:03:25,589 --> 00:03:22,959 we're 105 00:03:27,190 --> 00:03:25,599 right 106 00:03:28,630 --> 00:03:27,200 so i think this is really important for 107 00:03:30,869 --> 00:03:28,640 deep space 108 00:03:32,710 --> 00:03:30,879 from jpl's perspective we'd like to put 109 00:03:34,470 --> 00:03:32,720 one of these on a mars orbiter or even a 110 00:03:35,670 --> 00:03:34,480 mars rover 111 00:03:37,589 --> 00:03:35,680 and then that really increases the 112 00:03:38,710 --> 00:03:37,599 bandwidth of the amount of science data 113 00:03:41,190 --> 00:03:38,720 you can get back from the surface of 114 00:03:43,030 --> 00:03:41,200 mars instead of taking snapshots of 115 00:03:44,229 --> 00:03:43,040 images you could take video data and 116 00:03:45,509 --> 00:03:44,239 send that back to earth you can't do 117 00:03:47,670 --> 00:03:45,519 that right now 118 00:03:49,670 --> 00:03:47,680 it also will be a big game changer in 119 00:03:51,110 --> 00:03:49,680 terms of manned space flight 120 00:03:52,470 --> 00:03:51,120 we're going out to deep space even to 121 00:03:53,910 --> 00:03:52,480 the moon 122 00:03:56,470 --> 00:03:53,920 you want to have as much bandwidth as 123 00:03:58,309 --> 00:03:56,480 possible to talk to those astronauts and 124 00:04:00,630 --> 00:03:58,319 you're going to need laser con for that 125 00:04:01,990 --> 00:04:00,640 so what's next for opals well we're 126 00:04:03,910 --> 00:04:02,000 going to be on the station through 127 00:04:05,509 --> 00:04:03,920 february 2016. uh that's our current 128 00:04:07,830 --> 00:04:05,519 decommissioning date 129 00:04:09,509 --> 00:04:07,840 and we have a few more uh demonstrations 130 00:04:11,110 --> 00:04:09,519 that we're looking to do we just 131 00:04:12,710 --> 00:04:11,120 completed one which is an adaptive 132 00:04:15,190 --> 00:04:12,720 optics experiment 133 00:04:16,949 --> 00:04:15,200 in that experiment we took a test bed 134 00:04:18,789 --> 00:04:16,959 that would take the opal signals it was 135 00:04:20,390 --> 00:04:18,799 received at the telescope and it 136 00:04:22,469 --> 00:04:20,400 corrects all the atmospheric distortion 137 00:04:23,990 --> 00:04:22,479 that occurred as it was transmitted down 138 00:04:25,909 --> 00:04:24,000 we're able to couple that new fiber 139 00:04:28,870 --> 00:04:25,919 optics cable and that just demonstrates 140 00:04:30,469 --> 00:04:28,880 that we're able to take this signal and 141 00:04:31,830 --> 00:04:30,479 transmit to fiber optics cable possibly 142 00:04:33,189 --> 00:04:31,840 for transmission out to other ground 143 00:04:34,310 --> 00:04:33,199 stations those important technology to 144 00:04:35,749 --> 00:04:34,320 test out 145 00:04:37,749 --> 00:04:35,759 the next thing we'll be testing is a 146 00:04:39,270 --> 00:04:37,759 platform characterization experiment 147 00:04:41,110 --> 00:04:39,280 that's an attempt to try to measure the 148 00:04:42,629 --> 00:04:41,120 vibration or the shaking on the space 149 00:04:43,909 --> 00:04:42,639 station so it's not really output 150 00:04:45,909 --> 00:04:43,919 communications but based on our 151 00:04:47,670 --> 00:04:45,919 capabilities using lasers we can get 152 00:04:48,950 --> 00:04:47,680 some useful measurements out of it and 153 00:04:50,550 --> 00:04:48,960 then the fall time frame we're looking 154 00:04:51,670 --> 00:04:50,560 to do more transmissions to our foreign 155 00:04:53,990 --> 00:04:51,680 partners 156 00:04:56,310 --> 00:04:54,000 that's issa in the tenerife canary 157 00:04:57,270 --> 00:04:56,320 islands that's dlr and oberfunhoff in 158 00:05:00,070 --> 00:04:57,280 germany 159 00:05:02,870 --> 00:05:00,080 nict in tokyo japan and possibly canes 160 00:05:04,469 --> 00:05:02,880 in nice france so those will be nice 161 00:05:06,710 --> 00:05:04,479 collaboration to have before we begin 162 00:05:08,870 --> 00:05:06,720 the program in february 163 00:05:10,870 --> 00:05:08,880 so it's important to have those other 164 00:05:12,070 --> 00:05:10,880 ground stations around the world 165 00:05:13,430 --> 00:05:12,080 that's right i think both for 166 00:05:15,749 --> 00:05:13,440 collaboration 167 00:05:18,230 --> 00:05:15,759 and also looking at the variations you 168 00:05:20,629 --> 00:05:18,240 get with geometry variations 169 00:05:22,790 --> 00:05:20,639 when we operate in california the 170 00:05:25,110 --> 00:05:22,800 weather is fairly good for transmission 171 00:05:26,629 --> 00:05:25,120 of laser beams we operate in germany 172 00:05:28,469 --> 00:05:26,639 it's a little more challenging and so we 173 00:05:30,950 --> 00:05:28,479 learn new things uh it's also a much 174 00:05:32,550 --> 00:05:30,960 higher latitude in the planet and so the 175 00:05:35,189 --> 00:05:32,560 link availability and one we can 176 00:05:37,029 --> 00:05:35,199 transmit is quite a bit different from 177 00:05:38,230 --> 00:05:37,039 transmitting california and so by 178 00:05:40,469 --> 00:05:38,240 looking at those variations we're