1 00:00:05,430 --> 00:00:03,750 trent martin the johnson space center's 2 00:00:07,590 --> 00:00:05,440 project manager for the alpha magnetic 3 00:00:09,589 --> 00:00:07,600 spectrometer is here with us in mission 4 00:00:12,230 --> 00:00:09,599 control today for an interview 5 00:00:13,830 --> 00:00:12,240 and so uh welcome in trent 6 00:00:15,589 --> 00:00:13,840 thanks i appreciate it 7 00:00:17,510 --> 00:00:15,599 great to have you here today and to talk 8 00:00:19,429 --> 00:00:17,520 about ams as we call it on the 9 00:00:20,790 --> 00:00:19,439 international space station 10 00:00:22,710 --> 00:00:20,800 can you start off telling us a little 11 00:00:24,630 --> 00:00:22,720 bit about what an alpha magnetic 12 00:00:26,710 --> 00:00:24,640 spectrometer does 13 00:00:29,589 --> 00:00:26,720 sure the alpha magnetic spectrometer is 14 00:00:31,589 --> 00:00:29,599 a high energy physics experiment 15 00:00:33,350 --> 00:00:31,599 that was built by a collaboration of 60 16 00:00:35,910 --> 00:00:33,360 different institutes from 16 different 17 00:00:37,990 --> 00:00:35,920 countries and led by a nobel laureate 18 00:00:39,190 --> 00:00:38,000 from mit 19 00:00:41,430 --> 00:00:39,200 that 20 00:00:44,470 --> 00:00:41,440 combines a system of state-of-the-art 21 00:00:46,549 --> 00:00:44,480 high-energy particle physics detectors 22 00:00:48,869 --> 00:00:46,559 uh to sift through the particles that 23 00:00:51,189 --> 00:00:48,879 are constantly bombarding the earth 24 00:00:52,709 --> 00:00:51,199 we do it in space simply because most of 25 00:00:54,470 --> 00:00:52,719 these charged particles would not make 26 00:00:56,549 --> 00:00:54,480 it to the ground 27 00:00:58,470 --> 00:00:56,559 so the space station provides a perfect 28 00:01:00,150 --> 00:00:58,480 test bed for us to 29 00:01:02,229 --> 00:01:00,160 to utilize and 30 00:01:04,789 --> 00:01:02,239 actually measure these particles as they 31 00:01:08,149 --> 00:01:04,799 come through the detector the detector 32 00:01:11,750 --> 00:01:10,230 what type of particles we have so you 33 00:01:14,710 --> 00:01:11,760 can you can tell the difference between 34 00:01:15,590 --> 00:01:14,720 a helium atom and or an anti-helium atom 35 00:01:17,030 --> 00:01:15,600 um 36 00:01:19,350 --> 00:01:17,040 the the main science that we're looking 37 00:01:22,390 --> 00:01:19,360 for is anti-matter science dark matter 38 00:01:24,630 --> 00:01:22,400 science uh and and other cosmic ray 39 00:01:26,550 --> 00:01:24,640 propagation in the universe 40 00:01:29,590 --> 00:01:26,560 and i got to ask you why should i care 41 00:01:31,190 --> 00:01:29,600 about dark matter and antimatter and all 42 00:01:32,390 --> 00:01:31,200 those cosmic rays 43 00:01:33,749 --> 00:01:32,400 well ams 44 00:01:35,510 --> 00:01:33,759 is a detector that's essentially 45 00:01:36,789 --> 00:01:35,520 designed to probe the foundations of the 46 00:01:37,590 --> 00:01:36,799 universe 47 00:01:40,069 --> 00:01:37,600 so 48 00:01:42,230 --> 00:01:40,079 the data that we'll gather from ams we 49 00:01:44,149 --> 00:01:42,240 will we will utilize for years to come 50 00:01:46,230 --> 00:01:44,159 to help to identify 51 00:01:48,710 --> 00:01:46,240 what was the universe like at the 52 00:01:52,149 --> 00:01:48,720 beginning what is it like now and where 53 00:01:54,710 --> 00:01:52,159 are we going um how was it made up is 54 00:01:57,190 --> 00:01:54,720 half the universe made out of antimatter 55 00:01:58,870 --> 00:01:57,200 what is dark matter what is that 90 of 56 00:02:01,350 --> 00:01:58,880 the universe that we now know exists but 57 00:02:03,429 --> 00:02:01,360 we don't know what it is 58 00:02:05,749 --> 00:02:03,439 okay well tell us a little bit about 59 00:02:08,150 --> 00:02:05,759 yourself uh how did you get to this 60 00:02:10,150 --> 00:02:08,160 point in your career where are you from 61 00:02:12,150 --> 00:02:10,160 um i'm from 62 00:02:13,190 --> 00:02:12,160 all over the midwest and texas 63 00:02:20,949 --> 00:02:13,200 i 64 00:02:22,470 --> 00:02:20,959 houston clear lake 65 00:02:23,750 --> 00:02:22,480 so why would i be working with a bunch 66 00:02:25,750 --> 00:02:23,760 of physicists 67 00:02:27,589 --> 00:02:25,760 well mainly because nasa has the 68 00:02:29,990 --> 00:02:27,599 responsibility to do the the project 69 00:02:32,229 --> 00:02:30,000 management and integration of this uh of 70 00:02:34,630 --> 00:02:32,239 this high energy physics experiment 71 00:02:37,030 --> 00:02:34,640 so as an engineer i have to work with 72 00:02:38,869 --> 00:02:37,040 600 physicists engineers and technicians 73 00:02:40,869 --> 00:02:38,879 across the globe 74 00:02:41,990 --> 00:02:40,879 most of them being funded by other 75 00:02:43,430 --> 00:02:42,000 agencies 76 00:02:46,070 --> 00:02:43,440 to work together to build this 77 00:02:48,390 --> 00:02:46,080 experiment to operate this experiment 78 00:02:50,070 --> 00:02:48,400 it's a very interesting 79 00:02:52,470 --> 00:02:50,080 process and it's been a learning 80 00:02:53,589 --> 00:02:52,480 experience for me 81 00:02:55,190 --> 00:02:53,599 tell us a little bit about what it was 82 00:02:57,430 --> 00:02:55,200 like growing up as a kid when you grew 83 00:02:59,270 --> 00:02:57,440 up and and did you ever think you might 84 00:03:02,070 --> 00:02:59,280 be here doing this 85 00:03:04,390 --> 00:03:02,080 no absolutely not 86 00:03:05,350 --> 00:03:04,400 i grew up in small towns 87 00:03:07,990 --> 00:03:05,360 um 88 00:03:08,949 --> 00:03:08,000 never thought i would ever say that i've 89 00:03:10,790 --> 00:03:08,959 been to 90 00:03:11,589 --> 00:03:10,800 as many foreign countries as i've been 91 00:03:13,589 --> 00:03:11,599 to 92 00:03:15,990 --> 00:03:13,599 um 93 00:03:18,309 --> 00:03:16,000 no there was no way that as a kid i ever 94 00:03:20,550 --> 00:03:18,319 said i would be doing this but nasa has 95 00:03:21,670 --> 00:03:20,560 afforded that opportunity 96 00:03:23,509 --> 00:03:21,680 because of the international 97 00:03:25,030 --> 00:03:23,519 collaborations that we have 98 00:03:26,229 --> 00:03:25,040 in particular with this international 99 00:03:28,869 --> 00:03:26,239 space station 100 00:03:30,710 --> 00:03:28,879 ams is interesting in that we have as 101 00:03:31,750 --> 00:03:30,720 many countries as the space station has 102 00:03:35,350 --> 00:03:31,760 countries 103 00:03:37,990 --> 00:03:35,360 they're typically not the space 104 00:03:39,830 --> 00:03:38,000 institutions so they're not 105 00:03:42,229 --> 00:03:39,840 they're not jackson those types of 106 00:03:43,509 --> 00:03:42,239 agencies instead they're the physics 107 00:03:44,869 --> 00:03:43,519 institutions from those different 108 00:03:46,949 --> 00:03:44,879 countries 109 00:03:47,910 --> 00:03:46,959 so certainly i've met a lot of people 110 00:03:50,149 --> 00:03:47,920 um 111 00:03:51,430 --> 00:03:50,159 very interesting people that 112 00:03:52,550 --> 00:03:51,440 that are learning things about this 113 00:03:53,589 --> 00:03:52,560 universe 114 00:03:55,030 --> 00:03:53,599 that 115 00:03:56,869 --> 00:03:55,040 there's no way i ever thought i would be 116 00:03:58,470 --> 00:03:56,879 part of that 117 00:04:02,229 --> 00:03:58,480 okay 118 00:04:03,670 --> 00:04:02,239 tell us a little bit about why ams 119 00:04:05,429 --> 00:04:03,680 can take advantage of the space station 120 00:04:07,110 --> 00:04:05,439 what's important about the space station 121 00:04:08,309 --> 00:04:07,120 for the being able to conduct this 122 00:04:09,670 --> 00:04:08,319 experiment 123 00:04:11,110 --> 00:04:09,680 so the biggest advantage that we have 124 00:04:13,350 --> 00:04:11,120 with the international space station is 125 00:04:15,910 --> 00:04:13,360 that the space station provides us 126 00:04:17,590 --> 00:04:15,920 power and data 127 00:04:20,469 --> 00:04:17,600 if we had to provide that on our own if 128 00:04:21,990 --> 00:04:20,479 we decided to make the ams a free-flying 129 00:04:24,469 --> 00:04:22,000 satellite we would have had to have 130 00:04:29,749 --> 00:04:24,479 provided our own communication systems 131 00:04:34,710 --> 00:04:32,790 data systems that that we currently get 132 00:04:36,950 --> 00:04:34,720 from the international space station so 133 00:04:39,189 --> 00:04:36,960 that allowed us to focus the amount of 134 00:04:40,469 --> 00:04:39,199 weight that we had available to launch 135 00:04:41,270 --> 00:04:40,479 into science 136 00:04:43,590 --> 00:04:41,280 so 137 00:04:45,430 --> 00:04:43,600 more detector weight 138 00:04:46,790 --> 00:04:45,440 basically means we get better science 139 00:04:48,469 --> 00:04:46,800 because we're on the international space 140 00:04:50,550 --> 00:04:48,479 station okay 141 00:04:52,550 --> 00:04:50,560 hey we had a couple of twitter questions 142 00:04:54,550 --> 00:04:52,560 we advertised your interview in advance 143 00:04:56,629 --> 00:04:54,560 and we got several different good 144 00:04:59,110 --> 00:04:56,639 questions from folks out there 145 00:05:01,189 --> 00:04:59,120 i'd like to ask you those right now and 146 00:05:02,310 --> 00:05:01,199 and the first one is pretty basic it's 147 00:05:03,830 --> 00:05:02,320 from 148 00:05:04,870 --> 00:05:03,840 cory mcdonald 149 00:05:08,550 --> 00:05:04,880 and 150 00:05:09,670 --> 00:05:08,560 corey asks how many particles has ams 151 00:05:11,990 --> 00:05:09,680 collected 152 00:05:13,749 --> 00:05:12,000 so that's a fairly easy question to 153 00:05:16,230 --> 00:05:13,759 answer and actually you can look for 154 00:05:17,830 --> 00:05:16,240 yourself if you go to ams.nasa.gov 155 00:05:18,950 --> 00:05:17,840 i put a particle counter on the front of 156 00:05:21,110 --> 00:05:18,960 our website 157 00:05:23,830 --> 00:05:21,120 and i just looked just prior to this 158 00:05:25,749 --> 00:05:23,840 interview we are currently at 12.8 159 00:05:28,070 --> 00:05:25,759 billion particles measured 160 00:05:31,350 --> 00:05:28,080 we are measuring at a rate of about 1 to 161 00:05:34,070 --> 00:05:31,360 1.2 billion particles per month 162 00:05:36,950 --> 00:05:34,080 on ams we're measuring particles 24 163 00:05:39,909 --> 00:05:36,960 hours a day 7 days a week 365 days a 164 00:05:43,029 --> 00:05:39,919 year 366 this year 165 00:05:45,350 --> 00:05:43,039 and we have a a cadre of 166 00:05:47,670 --> 00:05:45,360 operations team in geneva that are 167 00:05:49,350 --> 00:05:47,680 constantly monitoring the payload making 168 00:05:51,270 --> 00:05:49,360 sure that thermally and electrically 169 00:05:52,629 --> 00:05:51,280 everything is going smoothly and making 170 00:05:54,150 --> 00:05:52,639 sure that the data is coming down 171 00:05:55,510 --> 00:05:54,160 through the through the proper systems 172 00:05:56,710 --> 00:05:55,520 and making its way to the science 173 00:05:58,870 --> 00:05:56,720 community 174 00:06:01,990 --> 00:05:58,880 and that's billion with a b right a big 175 00:06:03,830 --> 00:06:02,000 b um is that more or less than you ex 176 00:06:06,629 --> 00:06:03,840 we're anticipating we actually are 177 00:06:09,830 --> 00:06:06,639 measuring a a little bit less than two 178 00:06:11,670 --> 00:06:09,840 times what we expected to measure um we 179 00:06:12,870 --> 00:06:11,680 we were a little bit surprised when we 180 00:06:15,510 --> 00:06:12,880 first got up there and we started 181 00:06:17,749 --> 00:06:15,520 measuring data at a rate a little bit 182 00:06:20,469 --> 00:06:17,759 less than twice what we were expecting 183 00:06:22,870 --> 00:06:20,479 we've managed to um 184 00:06:25,110 --> 00:06:22,880 deal with that in our systems we had 185 00:06:26,790 --> 00:06:25,120 some robust capabilities in our systems 186 00:06:28,230 --> 00:06:26,800 that allowed us to handle that we've 187 00:06:30,150 --> 00:06:28,240 done some things to ensure that we're 188 00:06:31,990 --> 00:06:30,160 not overwhelming the space station data 189 00:06:34,230 --> 00:06:32,000 systems 190 00:06:35,909 --> 00:06:34,240 but at times we are using as much as one 191 00:06:38,150 --> 00:06:35,919 third of the bandwidth coming down from 192 00:06:40,629 --> 00:06:38,160 space station uh particularly at night 193 00:06:43,670 --> 00:06:40,639 when we're not downloading video uh we 194 00:06:45,909 --> 00:06:43,680 we can burst down ams data and get it to 195 00:06:49,189 --> 00:06:45,919 the scientists in geneva 196 00:06:51,430 --> 00:06:49,199 wow double the data the next question 197 00:06:52,710 --> 00:06:51,440 comes from uh morgan spice and i'm using 198 00:06:54,469 --> 00:06:52,720 their twitter handles here i don't know 199 00:06:56,469 --> 00:06:54,479 if it's a real name but they're asking 200 00:06:58,390 --> 00:06:56,479 do you think it's possible that our big 201 00:06:59,909 --> 00:06:58,400 bang is just one of many ongoing big 202 00:07:02,070 --> 00:06:59,919 bangs 203 00:07:03,670 --> 00:07:02,080 so that's an interesting question and 204 00:07:05,350 --> 00:07:03,680 ams 205 00:07:08,309 --> 00:07:05,360 most likely will not be able to answer 206 00:07:09,830 --> 00:07:08,319 that question um we can look back almost 207 00:07:11,830 --> 00:07:09,840 to the beginnings of the universe with 208 00:07:12,629 --> 00:07:11,840 ams over the time frame that we expect 209 00:07:13,830 --> 00:07:12,639 to be 210 00:07:15,589 --> 00:07:13,840 on the international space station 211 00:07:18,230 --> 00:07:15,599 essentially longer there the further 212 00:07:20,870 --> 00:07:18,240 back in time you're looking 213 00:07:22,790 --> 00:07:20,880 so with that we can see back to 214 00:07:24,790 --> 00:07:22,800 the origins of this universe maybe back 215 00:07:26,230 --> 00:07:24,800 to the beginnings of this big bang if 216 00:07:28,870 --> 00:07:26,240 there are multiple big bangs we just 217 00:07:29,749 --> 00:07:28,880 won't know that answer from ams 218 00:07:31,830 --> 00:07:29,759 and 219 00:07:34,070 --> 00:07:31,840 you know you talked about the potential 220 00:07:37,189 --> 00:07:34,080 for the instrument um the hubble space 221 00:07:41,350 --> 00:07:37,199 telescope basically rewrote the books on 222 00:07:43,670 --> 00:07:41,360 uh visible and other uh light ranges uh 223 00:07:45,749 --> 00:07:43,680 in astronomy uh do you 224 00:07:47,909 --> 00:07:45,759 anticipate that ams could have that same 225 00:07:49,749 --> 00:07:47,919 kind of uh effect on our understanding 226 00:07:51,270 --> 00:07:49,759 of the universe and uh and our thoughts 227 00:07:53,110 --> 00:07:51,280 about astronomy 228 00:07:56,230 --> 00:07:53,120 so ams at times has been called the 229 00:07:57,749 --> 00:07:56,240 hubble telescope for charged particles 230 00:07:59,670 --> 00:07:57,759 the reason for that is because over the 231 00:08:03,350 --> 00:07:59,680 last 50 years we've done a tremendous 232 00:08:07,110 --> 00:08:05,830 light rays uncharged particles 233 00:08:08,790 --> 00:08:07,120 we haven't done a very good job of 234 00:08:13,189 --> 00:08:08,800 studying charged particles 235 00:08:14,550 --> 00:08:13,199 so with ams we built a system that has 236 00:08:16,869 --> 00:08:14,560 i like to say if you got every high 237 00:08:18,309 --> 00:08:16,879 energy physicist into a room 238 00:08:19,749 --> 00:08:18,319 and you had them 239 00:08:22,070 --> 00:08:19,759 pick out which detector they would put 240 00:08:23,430 --> 00:08:22,080 on a high energy physics experiment 241 00:08:25,589 --> 00:08:23,440 we put all those on a list and we put 242 00:08:28,390 --> 00:08:25,599 them all onto ams 243 00:08:30,309 --> 00:08:28,400 so with that we have the capability to 244 00:08:32,149 --> 00:08:30,319 measure a single particle in multiple 245 00:08:34,230 --> 00:08:32,159 ways usually multiple times with 246 00:08:36,389 --> 00:08:34,240 different detectors so with that we'll 247 00:08:39,430 --> 00:08:36,399 be able to 248 00:08:41,190 --> 00:08:39,440 look at each particle identify it 249 00:08:43,430 --> 00:08:41,200 and ensure that the data that we're 250 00:08:46,150 --> 00:08:43,440 getting is accurate 251 00:08:48,150 --> 00:08:46,160 with that accurate data we hope that 252 00:08:49,829 --> 00:08:48,160 that we'll be able to potentially 253 00:08:51,670 --> 00:08:49,839 redefine what we know as high energy 254 00:08:54,230 --> 00:08:51,680 physics today 255 00:08:55,750 --> 00:08:54,240 and any idea on when we might be able to 256 00:08:57,030 --> 00:08:55,760 hear some of those results i know that 257 00:08:58,310 --> 00:08:57,040 there's a lot of peer review and 258 00:09:00,389 --> 00:08:58,320 everything that goes through that can 259 00:09:02,150 --> 00:09:00,399 you explain that process to us so the 260 00:09:04,470 --> 00:09:02,160 ams collaboration as i mentioned before 261 00:09:07,030 --> 00:09:04,480 is made up of 600 physicist engineers 262 00:09:09,030 --> 00:09:07,040 and technicians from around the world 263 00:09:09,829 --> 00:09:09,040 the way that the the group works is they 264 00:09:10,550 --> 00:09:09,839 take 265 00:09:15,750 --> 00:09:10,560 the 266 00:09:17,910 --> 00:09:15,760 separate physics research uh groups and 267 00:09:19,670 --> 00:09:17,920 they take the data as it comes down the 268 00:09:22,790 --> 00:09:19,680 raw data and each one of them takes the 269 00:09:24,230 --> 00:09:22,800 data and analyzes for particular things 270 00:09:25,750 --> 00:09:24,240 they get back together every once in a 271 00:09:27,269 --> 00:09:25,760 while and say well let's let's look at 272 00:09:28,949 --> 00:09:27,279 this area let's look at that area but 273 00:09:30,790 --> 00:09:28,959 they want an independent verification of 274 00:09:31,990 --> 00:09:30,800 that that's what we do within our own 275 00:09:33,750 --> 00:09:32,000 team 276 00:09:35,750 --> 00:09:33,760 once that is 277 00:09:39,350 --> 00:09:35,760 finalized we 278 00:09:40,630 --> 00:09:39,360 go out for publication and so that will 279 00:09:43,430 --> 00:09:40,640 happen 280 00:09:44,949 --> 00:09:43,440 i don't know when uh at with 12.8 281 00:09:46,310 --> 00:09:44,959 billion particles so far it's a lot of 282 00:09:47,590 --> 00:09:46,320 data to go through 283 00:09:50,070 --> 00:09:47,600 and so 284 00:09:51,190 --> 00:09:50,080 i i certainly would expect that that 285 00:09:53,030 --> 00:09:51,200 sometime 286 00:09:55,190 --> 00:09:53,040 you know within the next year or so we 287 00:09:57,430 --> 00:09:55,200 would have some data coming out 288 00:09:58,710 --> 00:09:57,440 um we certainly have a lot of of 289 00:10:01,350 --> 00:09:58,720 potential 290 00:10:03,509 --> 00:10:01,360 with the 12.8 billion particles 291 00:10:06,069 --> 00:10:03,519 and you're still collecting more 292 00:10:07,670 --> 00:10:06,079 1.2 billion particles a month 293 00:10:09,269 --> 00:10:07,680 okay the last question i'm going to ask 294 00:10:10,790 --> 00:10:09,279 you today and thanks again for being 295 00:10:13,110 --> 00:10:10,800 here is uh 296 00:10:15,430 --> 00:10:13,120 as someone from from humble beginnings 297 00:10:18,470 --> 00:10:15,440 do you have any advice for 298 00:10:20,069 --> 00:10:18,480 kids or students or folks out there that 299 00:10:22,389 --> 00:10:20,079 think they might want to get involved in 300 00:10:24,470 --> 00:10:22,399 this in the future 301 00:10:26,949 --> 00:10:24,480 when you grow up in a small town or even 302 00:10:28,310 --> 00:10:26,959 a big city and and you may have 303 00:10:29,990 --> 00:10:28,320 disadvantages 304 00:10:31,750 --> 00:10:30,000 what do you need to do to 305 00:10:33,030 --> 00:10:31,760 get through school so that you can take 306 00:10:35,350 --> 00:10:33,040 advantage of these kinds of 307 00:10:36,790 --> 00:10:35,360 opportunities that might be out there 308 00:10:38,230 --> 00:10:36,800 yeah the biggest thing that this 309 00:10:40,150 --> 00:10:38,240 question comes up sometimes and the 310 00:10:42,069 --> 00:10:40,160 biggest thing that that i always point 311 00:10:44,949 --> 00:10:42,079 out is you just have to continue 312 00:10:47,590 --> 00:10:44,959 studying your math and science 313 00:10:50,150 --> 00:10:47,600 go get an education in in an engineering 314 00:10:52,389 --> 00:10:50,160 discipline or a science discipline 315 00:10:53,829 --> 00:10:52,399 and go out there and try