1 00:00:05,510 --> 00:00:03,590 research i do is in uh the field of 2 00:00:07,030 --> 00:00:05,520 planetary science has two components 3 00:00:08,790 --> 00:00:07,040 that are relevant for studies in 4 00:00:11,190 --> 00:00:08,800 microgravity research 5 00:00:12,470 --> 00:00:11,200 one is the early stages of the formation 6 00:00:14,310 --> 00:00:12,480 of the planets 7 00:00:15,190 --> 00:00:14,320 the very beginning of the solar system 8 00:00:17,029 --> 00:00:15,200 you had 9 00:00:18,790 --> 00:00:17,039 dust and gas and those dust particles 10 00:00:20,390 --> 00:00:18,800 stick together and gradually grow larger 11 00:00:21,830 --> 00:00:20,400 and larger objects 12 00:00:23,429 --> 00:00:21,840 once they're very large the gravity 13 00:00:24,390 --> 00:00:23,439 between those objects helps them stick 14 00:00:26,310 --> 00:00:24,400 together 15 00:00:28,150 --> 00:00:26,320 but getting them to that size has proved 16 00:00:30,710 --> 00:00:28,160 a theoretical challenge in order to 17 00:00:32,630 --> 00:00:30,720 study those collisions between small 18 00:00:34,549 --> 00:00:32,640 particles to see under what conditions 19 00:00:37,110 --> 00:00:34,559 they stick to each other and when they 20 00:00:39,190 --> 00:00:37,120 break apart to do that experimentally we 21 00:00:40,709 --> 00:00:39,200 need the long duration microgravity 22 00:00:42,630 --> 00:00:40,719 environment provided by the 23 00:00:44,310 --> 00:00:42,640 international space station 24 00:00:46,869 --> 00:00:44,320 the same types of collisions are 25 00:00:48,950 --> 00:00:46,879 actually also relevant in saturn's rings 26 00:00:50,869 --> 00:00:48,960 and other planetary ring systems where 27 00:00:52,310 --> 00:00:50,879 the collision velocities are very slow 28 00:00:54,790 --> 00:00:52,320 and the particles are very small and 29 00:00:55,830 --> 00:00:54,800 have a negligible gravity so we're also 30 00:00:57,350 --> 00:00:55,840 studying 31 00:00:59,029 --> 00:00:57,360 the evolution of saturn's rings 32 00:01:02,069 --> 00:00:59,039 experimentally by doing collision 33 00:01:04,310 --> 00:01:02,079 experiments in microgravity well our 34 00:01:06,149 --> 00:01:04,320 initial experiment is a small experiment 35 00:01:07,670 --> 00:01:06,159 that's designed to look at collisions 36 00:01:09,910 --> 00:01:07,680 between different kinds of particles at 37 00:01:11,910 --> 00:01:09,920 very low speeds to look at how much 38 00:01:13,510 --> 00:01:11,920 energy is lost in those collisions so 39 00:01:16,469 --> 00:01:13,520 we're just going to be using 40 00:01:18,390 --> 00:01:16,479 a small video camera to track the 41 00:01:20,070 --> 00:01:18,400 particles during 42 00:01:21,350 --> 00:01:20,080 their collisions and see how fast 43 00:01:23,510 --> 00:01:21,360 they're moving after the collisions 44 00:01:25,190 --> 00:01:23,520 we've got a chamber with a number of 45 00:01:28,310 --> 00:01:25,200 different sorts of particle samples in 46 00:01:30,310 --> 00:01:28,320 it once it's in orbit we'll agitate that 47 00:01:32,149 --> 00:01:30,320 chamber to get the particles bumping 48 00:01:33,270 --> 00:01:32,159 into each other gently and then we'll 49 00:01:35,429 --> 00:01:33,280 just 50 00:01:37,910 --> 00:01:35,439 collect video data and see the those 51 00:01:39,590 --> 00:01:37,920 collisions gently damp out over time 52 00:01:41,270 --> 00:01:39,600 we're using different sorts of particles 53 00:01:43,190 --> 00:01:41,280 with different densities some of them 54 00:01:44,950 --> 00:01:43,200 with powder coatings to try to 55 00:01:46,870 --> 00:01:44,960 understand how those different 56 00:01:48,789 --> 00:01:46,880 parameters affect how much energy is 57 00:01:50,950 --> 00:01:48,799 dissipated in the collisions 58 00:01:52,710 --> 00:01:50,960 is this a unique experiment 59 00:01:54,870 --> 00:01:52,720 uh 60 00:01:56,389 --> 00:01:54,880 to my knowledge this particular 61 00:01:58,870 --> 00:01:56,399 experiment hasn't been done on space 62 00:02:01,270 --> 00:01:58,880 station things experimental studies like 63 00:02:03,030 --> 00:02:01,280 this have been done before 64 00:02:04,789 --> 00:02:03,040 i think we're going to be able to get to 65 00:02:07,510 --> 00:02:04,799 a lower 66 00:02:08,949 --> 00:02:07,520 collision velocity regime and explore 67 00:02:11,350 --> 00:02:08,959 some different kinds of particles that 68 00:02:13,030 --> 00:02:11,360 have been explored before but this is a 69 00:02:15,030 --> 00:02:13,040 prototype experiment for us and we'd 70 00:02:16,390 --> 00:02:15,040 like to develop it into a larger 71 00:02:19,270 --> 00:02:16,400 experiment where we can do longer 72 00:02:23,510 --> 00:02:19,280 studies of bigger particles this 73 00:02:28,309 --> 00:02:26,309 got a ride up to space that's funded by 74 00:02:29,990 --> 00:02:28,319 nanoracks in space florida but the 75 00:02:32,229 --> 00:02:30,000 experiment itself is developed at the 76 00:02:35,430 --> 00:02:32,239 center for microgravity research which 77 00:02:37,270 --> 00:02:35,440 is at university of central florida and 78 00:02:40,229 --> 00:02:37,280 the experiment was designed and built 79 00:02:41,830 --> 00:02:40,239 primarily by undergraduate students 80 00:02:44,949 --> 00:02:41,840 at the university so they work in the 81 00:02:47,190 --> 00:02:44,959 lab uh they're getting real hands-on 82 00:02:49,430 --> 00:02:47,200 experience in building real space 83 00:02:51,350 --> 00:02:49,440 hardware learning how to work through 84 00:02:53,350 --> 00:02:51,360 the inevitable problems that you run 85 00:02:55,830 --> 00:02:53,360 into and trying to get things to fit in 86 00:02:57,750 --> 00:02:55,840 within your mass and power constraints 87 00:02:58,869 --> 00:02:57,760 and that sort of thing what do we learn 88 00:03:00,390 --> 00:02:58,879 from this 89 00:03:02,470 --> 00:03:00,400 well we're learning 90 00:03:06,390 --> 00:03:02,480 how to planets form where did the earth 91 00:03:08,229 --> 00:03:06,400 come from how odd is it that we've got a 92 00:03:10,149 --> 00:03:08,239 planetary system with planets like we 93 00:03:12,470 --> 00:03:10,159 have today under what conditions do 94 00:03:14,309 --> 00:03:12,480 planets form how frequently might they 95 00:03:16,710 --> 00:03:14,319 be forming around other stars what are 96 00:03:19,110 --> 00:03:16,720 the conditions necessary for that so 97 00:03:21,110 --> 00:03:19,120 it's about the history and the origin of