1 00:00:09,610 --> 00:00:06,280 we've all heard the term of phrase 2 00:00:11,199 --> 00:00:09,620 flexing your muscles but probably not 3 00:00:13,480 --> 00:00:11,209 consider that the International Space 4 00:00:17,589 --> 00:00:13,490 Station is constantly flexing its 5 00:00:20,800 --> 00:00:17,599 muscles in a way it does wiggle and move 6 00:00:22,960 --> 00:00:20,810 as well as orbit in a straight line and 7 00:00:24,700 --> 00:00:22,970 knowing that this occurs has an 8 00:00:26,640 --> 00:00:24,710 important effect on the design of 9 00:00:28,659 --> 00:00:26,650 experiments that are going on inside 10 00:00:31,540 --> 00:00:28,669 important question though is how do you 11 00:00:33,369 --> 00:00:31,550 measure that movement nasa commentator 12 00:00:35,470 --> 00:00:33,379 Lori Meggs at the Marshall Space Flight 13 00:00:37,840 --> 00:00:35,480 Center caught up with the principal 14 00:00:39,340 --> 00:00:37,850 engineer for an experiment that has been 15 00:00:42,670 --> 00:00:39,350 measuring the movements of the space 16 00:00:44,080 --> 00:00:42,680 station since 2012 this particular 17 00:00:45,610 --> 00:00:44,090 experiment that we're running here than 18 00:00:49,630 --> 00:00:45,620 the flexure experiment really is 19 00:00:51,939 --> 00:00:49,640 designed to capture information about 20 00:00:53,650 --> 00:00:51,949 the motion of the wiggle and the flexing 21 00:00:55,420 --> 00:00:53,660 in the station that is known to occur at 22 00:00:56,979 --> 00:00:55,430 these locations but something that's not 23 00:00:59,590 --> 00:00:56,989 readily available because the sensors 24 00:01:01,479 --> 00:00:59,600 that can measure this are not always 25 00:01:03,099 --> 00:01:01,489 activated or there may not actually be 26 00:01:05,229 --> 00:01:03,109 sensors in the vicinity where we're 27 00:01:07,630 --> 00:01:05,239 operating and we're located very high in 28 00:01:09,820 --> 00:01:07,640 the station and the the ability to 29 00:01:11,590 --> 00:01:09,830 measure the the flexing motion something 30 00:01:14,020 --> 00:01:11,600 would be very useful to other 31 00:01:16,450 --> 00:01:14,030 experimenters that may have payloads 32 00:01:18,490 --> 00:01:16,460 that may actually be birth near us so 33 00:01:20,499 --> 00:01:18,500 that's really what we're trying to do or 34 00:01:22,510 --> 00:01:20,509 we're utilizing the antenna in ways not 35 00:01:24,760 --> 00:01:22,520 initially designed to be able to capture 36 00:01:26,950 --> 00:01:24,770 this data what does this flexure we're 37 00:01:28,569 --> 00:01:26,960 talking about simplest analogy be you 38 00:01:30,490 --> 00:01:28,579 know driving a minivan with your kids in 39 00:01:32,200 --> 00:01:30,500 the backseat and they push off the walls 40 00:01:33,370 --> 00:01:32,210 or they bounce around you actually feel 41 00:01:34,749 --> 00:01:33,380 that wiggle in the car and that's 42 00:01:35,950 --> 00:01:34,759 exactly what happens you know when the 43 00:01:38,950 --> 00:01:35,960 crew is activated and they're not 44 00:01:40,480 --> 00:01:38,960 sleeping they push off from the various 45 00:01:41,679 --> 00:01:40,490 modules to locomote themselves 46 00:01:43,510 --> 00:01:41,689 throughout the structure and so when 47 00:01:45,999 --> 00:01:43,520 they do that push off because space 48 00:01:48,100 --> 00:01:46,009 station is so very large starts exciting 49 00:01:49,840 --> 00:01:48,110 what we call these vibratory modes and 50 00:01:52,300 --> 00:01:49,850 the system basically flexes and moves 51 00:01:54,969 --> 00:01:52,310 and you'll start to see scissoring 52 00:01:56,590 --> 00:01:54,979 motions so you have this large 100 meter 53 00:01:59,109 --> 00:01:56,600 structure which is starting to scissor 54 00:02:00,789 --> 00:01:59,119 and twist and do all these bendings and 55 00:02:02,709 --> 00:02:00,799 that those sorts of things can play 56 00:02:04,899 --> 00:02:02,719 havoc with pointing experiments that may 57 00:02:07,120 --> 00:02:04,909 be located on these truss structure so 58 00:02:09,469 --> 00:02:07,130 we say flexure I'm talking about sort of 59 00:02:11,920 --> 00:02:09,479 this twisting motion that me 60 00:02:15,080 --> 00:02:11,930 out in the far reaches of the station 61 00:02:17,270 --> 00:02:15,090 how can it be used on earth and in space 62 00:02:17,690 --> 00:02:17,280 how can the information that you learn 63 00:02:18,890 --> 00:02:17,700 from this 64 00:02:21,259 --> 00:02:18,900 well I think you know we're really 65 00:02:25,039 --> 00:02:21,269 trying to supply a piece of information 66 00:02:26,390 --> 00:02:25,049 for future experimenters and most of the 67 00:02:28,580 --> 00:02:26,400 flexing that we're trying to measure 68 00:02:31,369 --> 00:02:28,590 obviously no one exists quantities the 69 00:02:33,410 --> 00:02:31,379 frequencies are useful for optical 70 00:02:34,820 --> 00:02:33,420 communications experiments these 71 00:02:36,800 --> 00:02:34,830 experiments require really high 72 00:02:39,229 --> 00:02:36,810 precision pointing and in order to 73 00:02:40,490 --> 00:02:39,239 stress their systems to be able to 74 00:02:41,600 --> 00:02:40,500 understand if they'll actually work they 75 00:02:43,970 --> 00:02:41,610 need to be able to understand what these 76 00:02:45,380 --> 00:02:43,980 flexures are and so it's important to 77 00:02:46,880 --> 00:02:45,390 have an understanding of what the 78 00:02:48,619 --> 00:02:46,890 magnitude of this is you can kind of 79 00:02:51,680 --> 00:02:48,629 prepare the experiment prior to it being 80 00:02:53,479 --> 00:02:51,690 launched prior to it being flown so I 81 00:02:55,550 --> 00:02:53,489 think what we're trying to do is provide 82 00:02:57,199 --> 00:02:55,560 useful data for future experiment or 83 00:03:00,680 --> 00:02:57,209 switching a little intern benefit and 84 00:03:03,140 --> 00:03:00,690 longer in a longer duration longer 85 00:03:05,059 --> 00:03:03,150 timeline activities for instance optical 86 00:03:06,890 --> 00:03:05,069 communications for deep-space pointing 87 00:03:08,240 --> 00:03:06,900 and things of that nature how long have 88 00:03:08,839 --> 00:03:08,250 you been on this station and how long 89 00:03:11,750 --> 00:03:08,849 will this go on 90 00:03:14,479 --> 00:03:11,760 well we've been running since 2012 you 91 00:03:17,690 --> 00:03:14,489 know we launched in August transited and 92 00:03:19,190 --> 00:03:17,700 then were birthed and began and started 93 00:03:21,080 --> 00:03:19,200 our commissioning activities in August 94 00:03:23,930 --> 00:03:21,090 of 2012 and we've been operating ever 95 00:03:26,180 --> 00:03:23,940 since we've been basically a continuous 96 00:03:27,740 --> 00:03:26,190 shift of operations of an Operations 97 00:03:29,960 --> 00:03:27,750 team and we've been supporting and will 98 00:03:31,670 --> 00:03:29,970 probably continue for several years to 99 00:03:33,979 --> 00:03:31,680 come you know with new directives from 100 00:03:38,089 --> 00:03:33,989 the scan program office what have you 101 00:03:39,409 --> 00:03:38,099 learned so far well that's that's that 102 00:03:41,720 --> 00:03:39,419 would take probably more than this 103 00:03:43,300 --> 00:03:41,730 interview to conduct that specifically 104 00:03:45,229 --> 00:03:43,310 for our tests here you know we really 105 00:03:47,270 --> 00:03:45,239 you know when we first ran this 106 00:03:48,949 --> 00:03:47,280 experiment is very difficult to extract 107 00:03:51,259 --> 00:03:48,959 this data and make sense of it but we've 108 00:03:53,509 --> 00:03:51,269 really we've really refined that and and 109 00:03:55,789 --> 00:03:53,519 we now have a very good sense of we can 110 00:03:57,170 --> 00:03:55,799 actually use this this ka-band antennae 111 00:03:59,150 --> 00:03:57,180 not originally designed to do what it is 112 00:04:00,770 --> 00:03:59,160 being used for to actually conduct these 113 00:04:02,690 --> 00:04:00,780 types of experiments to actually get 114 00:04:04,250 --> 00:04:02,700 this flexure and we're supporting other 115 00:04:05,920 --> 00:04:04,260 activities one of them as a discrete 116 00:04:08,479 --> 00:04:05,930 thruster firing tests and we hope to 117 00:04:09,890 --> 00:04:08,489 activate our payload to be able to 118 00:04:11,750 --> 00:04:09,900 capture that information as well 119 00:04:15,319 --> 00:04:11,760 something that again we have originally 120 00:04:18,449 --> 00:04:15,329 intended to do but something that we can 121 00:04:21,509 --> 00:04:18,459 the engineers normally will track a data 122 00:04:24,240 --> 00:04:21,519 satellite with a ka-band antenna but 123 00:04:26,820 --> 00:04:24,250 this team has explored using the Sun as 124 00:04:28,320 --> 00:04:26,830 a radio source for ka-band tracking 125 00:04:30,750 --> 00:04:28,330 which makes it a unique 126 00:04:33,629 --> 00:04:30,760 first-of-its-kind experiment and it's