1 00:00:01,300 --> 00:00:01,790 >> Kelly Humphries: Hi, guys. 2 00:00:01,790 --> 00:00:03,900 Welcome to Mission Control Houston. 3 00:00:03,900 --> 00:00:07,910 I'm Kelly Humphries, and this is veteran astronaut Mario Runco. 4 00:00:07,910 --> 00:00:10,470 We are ready for your questions. 5 00:00:10,470 --> 00:00:11,850 >> Ms. Sukumar: [Inaudible] one of the students. 6 00:00:11,850 --> 00:00:15,760 Hi. This is Ms. Sukumar from Deptford High School. 7 00:00:15,760 --> 00:00:18,490 Do you want me to ask the questions one at a time 8 00:00:18,490 --> 00:00:21,320 or do you want the students to be asking the questions? 9 00:00:21,320 --> 00:00:23,330 >> Kelly Humphries: We'd love to hear directly from the students, 10 00:00:23,330 --> 00:00:25,900 but they do need to speak up so we can hear their voices. 11 00:00:25,900 --> 00:00:27,410 And I want to make sure they know 12 00:00:27,410 --> 00:00:29,230 that Mario knows New Jersey. 13 00:00:29,230 --> 00:00:32,990 He went to Rutgers University and is originally from New York. 14 00:00:32,990 --> 00:00:35,070 So he knows your area. 15 00:00:35,070 --> 00:00:35,710 >> Ms. Sukumar: Very nice. 16 00:00:35,710 --> 00:00:38,200 So let's start with Grant Wilson. 17 00:00:38,200 --> 00:00:39,780 He's a grade 11 student. 18 00:00:39,780 --> 00:00:41,380 He's a junior at our school. 19 00:00:41,380 --> 00:00:43,700 So Grant's question. 20 00:00:43,700 --> 00:00:44,420 Here he goes. 21 00:00:44,420 --> 00:00:45,950 Grant. 22 00:00:45,950 --> 00:00:49,500 >> Grant Wilson: How long have you, in total, been in space? 23 00:00:49,500 --> 00:00:51,580 >> Mario Runco: How long have I been in space? 24 00:00:51,580 --> 00:00:51,880 >> Grant Wilson: Yeah. 25 00:00:51,880 --> 00:00:53,960 >> Mario Runco: I had done three missions. 26 00:00:53,960 --> 00:00:57,530 The first one was in 1991 on STS 44. 27 00:00:57,530 --> 00:00:58,980 That was with the space shuttle. 28 00:00:58,980 --> 00:01:01,920 And then I did two more space shuttle missions. 29 00:01:01,920 --> 00:01:04,870 In '93 and in '96. 30 00:01:04,870 --> 00:01:09,050 And the total time among all missions is -- 31 00:01:09,050 --> 00:01:14,310 was about 21 days total, which now days compared 32 00:01:14,310 --> 00:01:15,220 to what the guys spend 33 00:01:15,220 --> 00:01:18,130 on the space station is a very small number. 34 00:01:18,130 --> 00:01:21,010 >> Kelly Humphries: Okay, that's a great question. 35 00:01:21,010 --> 00:01:24,230 And just a reminder, please get to the microphone and speak 36 00:01:24,230 --> 00:01:25,520 up so we can hear you. 37 00:01:25,520 --> 00:01:27,780 It's a little hard. 38 00:01:27,780 --> 00:01:28,130 >> Ms. Sukumar: Sure. 39 00:01:28,130 --> 00:01:31,530 The next question is from Brian McCachlan [assumed spelling]. 40 00:01:31,530 --> 00:01:33,880 He's a grade nine student. 41 00:01:33,880 --> 00:01:36,180 He's a freshman. 42 00:01:36,180 --> 00:01:37,150 Brian, where are you? 43 00:01:37,150 --> 00:01:37,220 >> [Inaudible]. 44 00:01:37,220 --> 00:01:38,750 >> Ms. Sukumar: All right. 45 00:01:38,750 --> 00:01:42,540 Brian's not here, but I'm going to ask the question 46 00:01:42,540 --> 00:01:44,950 that Brian had asked on his behalf. 47 00:01:44,950 --> 00:01:48,830 And the question is how is space always expanding, 48 00:01:48,830 --> 00:01:52,980 and where does it expand into? 49 00:01:52,980 --> 00:01:55,570 >> Mario Runco: How and why is space expanding 50 00:01:55,570 --> 00:01:57,030 and what is it expanding into? 51 00:01:57,030 --> 00:01:58,480 That is a great question, 52 00:01:58,480 --> 00:02:02,030 and I don't think we know the answer to at this point. 53 00:02:02,030 --> 00:02:05,120 Space is, as far as we have sensed 54 00:02:05,120 --> 00:02:09,680 with our Hubble space telescope and other orbiting observatories 55 00:02:09,680 --> 00:02:13,710 like the Gamma Ray Observatory, we know that there are objects 56 00:02:13,710 --> 00:02:16,730 that we can see and sense 57 00:02:16,730 --> 00:02:20,450 out 13,000,000,000 light years from Earth. 58 00:02:20,450 --> 00:02:24,920 And that's really the extent of the known Universe. 59 00:02:24,920 --> 00:02:28,890 The objects within that space, the known Universe, 60 00:02:28,890 --> 00:02:34,230 are expanding away from each other into distances farther 61 00:02:34,230 --> 00:02:36,510 than the 13,000,000,000 light years. 62 00:02:36,510 --> 00:02:40,400 Now, remember, a light year is about 6,000,000,000,000 miles. 63 00:02:40,400 --> 00:02:43,620 So I said 13,000,000,000 times 6,000,000,000,000. 64 00:02:43,620 --> 00:02:46,900 So that's the distance to the farthest known extent 65 00:02:46,900 --> 00:02:49,610 of the Universe, at least today. 66 00:02:49,610 --> 00:02:51,750 And that's a darn good question. 67 00:02:51,750 --> 00:02:56,230 And maybe Brian will be able to become the scientist 68 00:02:56,230 --> 00:02:57,710 that figures that out. 69 00:02:57,710 --> 00:02:58,530 >> Kelly Humphries: You know, the other part 70 00:02:58,530 --> 00:03:01,940 of that is what exactly is in all of that space? 71 00:03:01,940 --> 00:03:04,780 And one of the experiments on the International Space Station, 72 00:03:04,780 --> 00:03:07,940 the alpha-magnetic spectrometer, is doing -- 73 00:03:07,940 --> 00:03:11,390 sifting through the various cosmic rays and particles 74 00:03:11,390 --> 00:03:15,370 that come to Earth to try to identify a little bit more 75 00:03:15,370 --> 00:03:17,750 about things like matter, antimatter, 76 00:03:17,750 --> 00:03:21,920 and this theoretical dark matter that we believe exists 77 00:03:21,920 --> 00:03:25,240 because we can indirectly sense that. 78 00:03:25,240 --> 00:03:27,340 But we don't have any direct measurements of that. 79 00:03:27,340 --> 00:03:30,260 And so that's a really interesting experiment. 80 00:03:30,260 --> 00:03:33,550 And having the space station orbiting the Earth provides us 81 00:03:33,550 --> 00:03:36,240 the power to operate that outside the Earth's atmosphere. 82 00:03:36,240 --> 00:03:39,130 And look more at what is in between the matter 83 00:03:39,130 --> 00:03:41,400 that we can see and sense. 84 00:03:41,400 --> 00:03:47,300 And we're ready for your next question. 85 00:03:47,300 --> 00:03:47,870 >> Ms. Sukumar: [Inaudible]. 86 00:03:47,870 --> 00:03:49,420 >> Kelly Humphries: I'm sorry. 87 00:03:49,420 --> 00:03:58,780 We're not able to hear that at all. 88 00:03:58,780 --> 00:03:58,850 >> Ms. Sukumar: [Inaudible]. 89 00:03:58,850 --> 00:04:08,360 >> Kelly Humphries: Something must have happened 90 00:04:08,360 --> 00:04:12,610 to the microphone. 91 00:04:12,610 --> 00:04:13,040 I'm sorry. 92 00:04:13,040 --> 00:04:15,390 You may want to check your microphone. 93 00:04:15,390 --> 00:04:20,490 And verify that it's in a good location and plugged in. 94 00:04:20,490 --> 00:04:23,870 >> Mario Runco: And while you're doing that -- oop. 95 00:04:23,870 --> 00:04:25,470 And while you're doing that, let me comment 96 00:04:25,470 --> 00:04:27,570 about what Kelly had just said. 97 00:04:27,570 --> 00:04:29,940 And that is with the dark matter. 98 00:04:29,940 --> 00:04:35,350 Scientists believe that there is a construct, 99 00:04:35,350 --> 00:04:36,640 a thing called dark matter. 100 00:04:36,640 --> 00:04:40,110 And that's because, for example, the Milky Way Galaxy, 101 00:04:40,110 --> 00:04:42,930 our own galaxy, has matter in it, and it is spinning 102 00:04:42,930 --> 00:04:45,380 around in a disk-like fashion. 103 00:04:45,380 --> 00:04:47,720 But the rate of spin is 104 00:04:47,720 --> 00:04:50,480 such that the centrifugal acceleration outward 105 00:04:50,480 --> 00:04:56,090 that would throw the objects within the galaxy like the ball 106 00:04:56,090 --> 00:04:57,940 at the end of a string when you let go of the string, 107 00:04:57,940 --> 00:05:01,360 they would flight outward and not stay as part of the galaxy. 108 00:05:01,360 --> 00:05:05,000 But there's enough gravity within that galaxy 109 00:05:05,000 --> 00:05:06,260 to hold everything together. 110 00:05:06,260 --> 00:05:10,590 But the matter and the mass that we know of in the objects 111 00:05:10,590 --> 00:05:12,900 that we can see is not enough to do that. 112 00:05:12,900 --> 00:05:15,740 So they've invented dark matter to try 113 00:05:15,740 --> 00:05:18,590 and solve the equation so it makes sense. 114 00:05:18,590 --> 00:05:19,840 So there's something there. 115 00:05:19,840 --> 00:05:20,850 We just can't sense it. 116 00:05:20,850 --> 00:05:23,850 And we don't know what it is. 117 00:05:23,850 --> 00:05:26,160 Now, there is some -- there are things 118 00:05:26,160 --> 00:05:29,940 out there called robe planets that are like the Earth 119 00:05:29,940 --> 00:05:33,630 or Jupiter that do not revolve around the stars. 120 00:05:33,630 --> 00:05:36,330 So they would be dark planets that we can't see. 121 00:05:36,330 --> 00:05:37,660 So maybe there's -- that's one -- 122 00:05:37,660 --> 00:05:40,820 maybe that's one possibility that's not so exotic 123 00:05:40,820 --> 00:05:43,640 that would account for that extra mass. 124 00:05:43,640 --> 00:05:44,220 >> Kelly Humphries: Okay. 125 00:05:44,220 --> 00:05:46,180 I'm hearing that we may have gotten the audio 126 00:05:46,180 --> 00:05:46,950 connection fixed. 127 00:05:46,950 --> 00:05:48,750 You want to try another question, guys? 128 00:05:48,750 --> 00:05:49,450 >> Ms. Sukumar: Yes, we do. 129 00:05:49,450 --> 00:05:50,740 >> Mario Runco: Now that's better. 130 00:05:50,740 --> 00:05:52,110 >> Kelly Humphries: We can hear you now. 131 00:05:52,110 --> 00:05:54,020 >> Yeah. How do you feel in space? 132 00:05:54,020 --> 00:05:56,180 Do you feel more inspired and at ease? 133 00:05:56,180 --> 00:05:58,150 Or do you become cynical [phonetic]? 134 00:05:58,150 --> 00:05:59,630 >> Mario Runco: Ah, good question. 135 00:05:59,630 --> 00:06:02,100 I actually -- it's the former. 136 00:06:02,100 --> 00:06:05,410 I feel very inspired and uplifted. 137 00:06:05,410 --> 00:06:09,090 And the reason for that is when you're in orbit 138 00:06:09,090 --> 00:06:11,650 around the Earth, you can see most of the Earth. 139 00:06:11,650 --> 00:06:14,040 And, indeed, some of the earlier astronauts 140 00:06:14,040 --> 00:06:16,400 that traveled farther away from the Earth like those that went 141 00:06:16,400 --> 00:06:19,240 to the moon, could see the entire Earth at one time. 142 00:06:19,240 --> 00:06:23,350 And it is so spectacularly beautiful and majestic. 143 00:06:23,350 --> 00:06:25,680 And likewise, when you look out into the Universe, 144 00:06:25,680 --> 00:06:29,910 you see the stars and the celestial sky 145 00:06:29,910 --> 00:06:32,730 in a much more vivid fashion. 146 00:06:32,730 --> 00:06:35,910 And your being among them 147 00:06:35,910 --> 00:06:40,240 in that setting just is very exhilarating and inspirational. 148 00:06:40,240 --> 00:06:43,380 And actually, we had talked earlier, Kelly and I, 149 00:06:43,380 --> 00:06:47,280 about some of the work we were doing here at NASA 150 00:06:47,280 --> 00:06:53,630 that is related to that in terms of taking images of the Earth. 151 00:06:53,630 --> 00:06:55,300 >> Kelly Humphries: All right. 152 00:06:55,300 --> 00:06:56,630 Next question. 153 00:06:56,630 --> 00:06:58,360 >> Ms. Sukumar: Next question is 154 00:06:58,360 --> 00:06:59,960 from Michael Holmes [assumed spelling]. 155 00:06:59,960 --> 00:07:00,860 He's a freshman. 156 00:07:00,860 --> 00:07:02,740 And his question is -- 157 00:07:02,740 --> 00:07:06,130 >> Michael Holmes: What do you use to work out in space? 158 00:07:06,130 --> 00:07:07,400 >> Kelly Humphries: Oh, good question. 159 00:07:07,400 --> 00:07:10,130 And you really need to work out in space. 160 00:07:10,130 --> 00:07:14,590 I'll answer the question, but let me just say, firstly, 161 00:07:14,590 --> 00:07:18,370 that on Earth, gravity is working on us all the time. 162 00:07:18,370 --> 00:07:22,080 And for example, like my heart is pumping blood right now 163 00:07:22,080 --> 00:07:25,060 up against gravity to my head to keep me conscious 164 00:07:25,060 --> 00:07:27,070 so I don't keel over in the chair. 165 00:07:27,070 --> 00:07:29,620 And when gravity is removed, 166 00:07:29,620 --> 00:07:31,670 the heart doesn't have to work so hard. 167 00:07:31,670 --> 00:07:34,240 Yet, when I come return to Earth, it has to go back 168 00:07:34,240 --> 00:07:35,430 into that environment. 169 00:07:35,430 --> 00:07:37,640 So we need to stay conditioned because muscles 170 00:07:37,640 --> 00:07:40,820 that you don't use, as everyone knows, tend to grow weaker. 171 00:07:40,820 --> 00:07:43,400 So we need to maintain at least the level of strength 172 00:07:43,400 --> 00:07:45,430 that we had when we left the Earth. 173 00:07:45,430 --> 00:07:51,410 And we use devices such as ergometers and treadmills 174 00:07:51,410 --> 00:07:56,160 and cycling machines and bungees in a fashion 175 00:07:56,160 --> 00:08:00,880 that are all designed using springs and the 176 00:08:00,880 --> 00:08:03,320 like to mimic gravity. 177 00:08:03,320 --> 00:08:05,590 For example, if I'm running on a treadmill, 178 00:08:05,590 --> 00:08:08,570 there are bungee cords holding me to the treadmill 179 00:08:08,570 --> 00:08:12,850 such that I can actually run on the treadmill and it works. 180 00:08:12,850 --> 00:08:18,440 And then we use bungees and spring-like things 181 00:08:18,440 --> 00:08:20,390 to mimic weightlifting and the like. 182 00:08:20,390 --> 00:08:22,630 So we try to do -- and there are many devices 183 00:08:22,630 --> 00:08:26,160 that have been developed to help and facilitate 184 00:08:26,160 --> 00:08:28,730 that exercise protocol. 185 00:08:28,730 --> 00:08:32,350 >> Kelly Humphries: And just to add onto that, there are -- 186 00:08:32,350 --> 00:08:35,050 bone density loss is another important thing 187 00:08:35,050 --> 00:08:37,610 when you do the long duration stays in space. 188 00:08:37,610 --> 00:08:40,720 And so doing this kind of exercise puts force 189 00:08:40,720 --> 00:08:44,810 onto your bones in the same way that you would put force 190 00:08:44,810 --> 00:08:46,820 on your heels when you walk. 191 00:08:46,820 --> 00:08:48,900 And that helps keep the bones strong, 192 00:08:48,900 --> 00:08:50,370 which is a really important thing. 193 00:08:50,370 --> 00:08:53,350 And research into that is also helping us solve problems 194 00:08:53,350 --> 00:08:55,690 that people have on Earth like osteoporosis. 195 00:08:55,690 --> 00:08:59,310 Some of your grandparents may have experienced that 196 00:08:59,310 --> 00:09:01,340 and have -- it's too easy to break a hip 197 00:09:01,340 --> 00:09:02,770 or whatnot because of that. 198 00:09:02,770 --> 00:09:03,950 And some of the research 199 00:09:03,950 --> 00:09:07,570 in space is helping us apply what we're learning there 200 00:09:07,570 --> 00:09:09,800 to diseases we have here on Earth. 201 00:09:09,800 --> 00:09:12,080 And so that's another part of exercise on orbit 202 00:09:12,080 --> 00:09:13,350 because these folks all come -- 203 00:09:13,350 --> 00:09:15,660 stay up there for about six months, and then they've got 204 00:09:15,660 --> 00:09:18,100 to readapt to being on gravity when they get home. 205 00:09:18,100 --> 00:09:20,780 >> Mario Runco: And in the case of osteoporosis, it happens -- 206 00:09:20,780 --> 00:09:24,080 if we don't exercise, we tend to develop those symptoms 207 00:09:24,080 --> 00:09:25,830 in the very short period of time, 208 00:09:25,830 --> 00:09:27,130 in a matter of weeks and months. 209 00:09:27,130 --> 00:09:30,760 So we can study that, whereas normally, on a person on Earth, 210 00:09:30,760 --> 00:09:33,530 it would take a lifetime before they had developed any symptoms. 211 00:09:33,530 --> 00:09:36,400 So we have a very accelerated laboratory in which 212 00:09:36,400 --> 00:09:39,840 to develop drugs and protocols to maybe address that. 213 00:09:39,840 --> 00:09:41,530 And that's what Kelly was talking about. 214 00:09:41,530 --> 00:09:42,540 >> Kelly Humphries: And nutrition too 215 00:09:42,540 --> 00:09:44,920 because they're learning that nutrition and exercise 216 00:09:44,920 --> 00:09:47,410 in combination have a really important effect 217 00:09:47,410 --> 00:09:50,390 on how well you're able to keep fit aboard the space station. 218 00:09:50,390 --> 00:09:52,760 >> Mario Runco: I'm sure you've heard that one before too. 219 00:09:52,760 --> 00:09:53,790 >> Kelly Humphries: Next question. 220 00:09:53,790 --> 00:09:53,880 >> Ms. Sukumar: [Inaudible]. 221 00:09:53,880 --> 00:09:56,510 >> John Gilbert [assumed spelling]: I'm John Gilbert. 222 00:09:56,510 --> 00:09:57,590 I'm a senior. 223 00:09:57,590 --> 00:10:03,740 I want to know how did your navy career prepare you 224 00:10:03,740 --> 00:10:05,040 to be an astronaut. 225 00:10:05,040 --> 00:10:06,970 >> Mario Runco: Ah, good question. 226 00:10:06,970 --> 00:10:10,720 My navy career, I was a meteorologist, oceanographer, 227 00:10:10,720 --> 00:10:17,760 and I was also a surface ship watch officer in the navy. 228 00:10:17,760 --> 00:10:21,190 And the scientific part of my background, the meteorology, 229 00:10:21,190 --> 00:10:25,680 oceanography, helped with my ability to understand all 230 00:10:25,680 --> 00:10:30,780 of the technical parts of what is needed to operate in space, 231 00:10:30,780 --> 00:10:32,130 orbital mechanics and the like. 232 00:10:32,130 --> 00:10:35,130 So I had a very rigorous engineering, 233 00:10:35,130 --> 00:10:37,140 scientific background. 234 00:10:37,140 --> 00:10:40,580 The navy portion of it is the crew of a ship, 235 00:10:40,580 --> 00:10:44,160 much like the crew of a spaceship, 236 00:10:44,160 --> 00:10:46,560 is based in operations. 237 00:10:46,560 --> 00:10:50,590 And it's very similar when you're operating on board a ship 238 00:10:50,590 --> 00:10:52,920 or a submarine to when you're operating 239 00:10:52,920 --> 00:10:54,870 in a spacecraft as a crew. 240 00:10:54,870 --> 00:10:56,970 You learn to operate as a team, 241 00:10:56,970 --> 00:10:58,920 you learn your systems on the ship. 242 00:10:58,920 --> 00:11:03,230 And indeed, many of them -- actually, they're all the same. 243 00:11:03,230 --> 00:11:05,960 Say that, for example, there's environmental systems 244 00:11:05,960 --> 00:11:07,870 on the ship, as there are on a spacecraft. 245 00:11:07,870 --> 00:11:10,850 So some of the hardware's different and how it is -- 246 00:11:10,850 --> 00:11:13,150 it functions is different, but the principle 247 00:11:13,150 --> 00:11:16,450 and why it's there is basically the same. 248 00:11:16,450 --> 00:11:20,690 So it's a very close one-to-one relationship between operating 249 00:11:20,690 --> 00:11:23,540 in the naval environment as a space environment. 250 00:11:23,540 --> 00:11:24,830 >> Kelly Humphries: And interestingly enough, 251 00:11:24,830 --> 00:11:25,560 one of the crew members 252 00:11:25,560 --> 00:11:28,070 on the space station right now also is a navy veteran. 253 00:11:28,070 --> 00:11:34,190 Chris Cassidy was a navy seal. 254 00:11:34,190 --> 00:11:35,060 Next question. 255 00:11:35,060 --> 00:11:37,710 >> Solomon [assumed spelling]: I'm Solomon, ninth grade. 256 00:11:37,710 --> 00:11:41,890 And my question is what made you want to be an astronaut? 257 00:11:41,890 --> 00:11:44,990 >> Mario Runco: Well, I've always had a desire 258 00:11:44,990 --> 00:11:46,770 to learn new things 259 00:11:46,770 --> 00:11:50,660 and to understand the Universe, what's out there. 260 00:11:50,660 --> 00:11:54,040 But very specifically, when I was very young 261 00:11:54,040 --> 00:11:57,630 at age five years old, the first satellite went 262 00:11:57,630 --> 00:11:58,690 into orbit, Sputnik. 263 00:11:58,690 --> 00:12:01,710 And then shortly thereafter, a few years later, 264 00:12:01,710 --> 00:12:04,940 the first human beings, Yuri Gagarin and Alan Shepard, 265 00:12:04,940 --> 00:12:06,540 went into orbit around Earth. 266 00:12:06,540 --> 00:12:10,910 And I knew then that's exactly what I wanted to do. 267 00:12:10,910 --> 00:12:13,700 And I feel very, very fortunate and privileged 268 00:12:13,700 --> 00:12:16,050 to have had the opportunity to do so. 269 00:12:16,050 --> 00:12:21,360 And I'm very lucky to be here sitting talking to you about it. 270 00:12:23,090 --> 00:12:23,890 >> Go ahead? 271 00:12:23,890 --> 00:12:24,400 >> Ms. Sukumar: Yeah. 272 00:12:24,400 --> 00:12:26,930 >> What do you think is your most significant accomplishment 273 00:12:26,930 --> 00:12:30,070 in all your space missions as an astronaut? 274 00:12:30,070 --> 00:12:32,430 >> Mario Runco: Ah, my most significant accomplishment? 275 00:12:32,430 --> 00:12:36,330 The most memorable one was the one on my second mission, 276 00:12:36,330 --> 00:12:39,300 was when I did a spacewalk. 277 00:12:39,300 --> 00:12:45,400 And honestly, I guess the most significant accomplishment is 278 00:12:45,400 --> 00:12:48,470 on my last mission, we had a number 279 00:12:48,470 --> 00:12:51,480 of technology development experiments on board 280 00:12:51,480 --> 00:12:55,130 that spacecraft, both on the shuttle and others 281 00:12:55,130 --> 00:12:57,920 that we put overboard and we tested 282 00:12:57,920 --> 00:13:00,810 in orbit alongside the space shuttle. 283 00:13:00,810 --> 00:13:05,740 And in that sense, is those technology development 284 00:13:05,740 --> 00:13:07,600 experiments were pushing the boundaries 285 00:13:07,600 --> 00:13:10,150 of what are capabilities are to explore space. 286 00:13:10,150 --> 00:13:13,470 So I guess that, in my mind, would be something 287 00:13:13,470 --> 00:13:16,630 that if we can move to an area 288 00:13:16,630 --> 00:13:20,790 where we can explore it more efficiently and go farther 289 00:13:20,790 --> 00:13:26,000 out into space is something that I hope continues. 290 00:13:26,000 --> 00:13:26,740 >> Kelly Humphries: and I think some 291 00:13:26,740 --> 00:13:28,120 of those were directly applicable 292 00:13:28,120 --> 00:13:30,240 to the space station development, weren't they? 293 00:13:30,240 --> 00:13:31,800 >> Mario Runco: Actually, yes. 294 00:13:31,800 --> 00:13:35,580 We had attitude control satellite. 295 00:13:35,580 --> 00:13:37,050 It's called the satellite test unit. 296 00:13:37,050 --> 00:13:42,240 It was a device that we tried to use the forces in Earth's orbit 297 00:13:42,240 --> 00:13:46,140 to control the attitude of this spacecraft. 298 00:13:46,140 --> 00:13:49,250 And in a sense, they do a little bit with the space station. 299 00:13:49,250 --> 00:13:53,860 We've got gyros that move through angular momentum 300 00:13:53,860 --> 00:13:56,140 that can torque the space station around. 301 00:13:56,140 --> 00:13:59,230 We also have thrusters, but we don't use those that often. 302 00:13:59,230 --> 00:14:02,340 And we try to keep the space station in an equilibrium point 303 00:14:02,340 --> 00:14:05,650 where we don't have to use the gyros even. 304 00:14:05,650 --> 00:14:11,510 But all three together hold the spacecraft where it needs to be. 305 00:14:11,510 --> 00:14:12,870 >> Kelly Humphries: Great. 306 00:14:12,870 --> 00:14:13,610 Another question? 307 00:14:13,610 --> 00:14:18,850 >> How does your body shift from gravy to no gravity? 308 00:14:18,850 --> 00:14:21,130 And how do you feel? 309 00:14:21,130 --> 00:14:24,040 >> Mario Runco: Well, the body does a number of reactions 310 00:14:24,040 --> 00:14:27,630 when you get into space and you're in orbit 311 00:14:27,630 --> 00:14:29,830 and the gravity vector is removed. 312 00:14:29,830 --> 00:14:33,970 Primarily -- and we had already discussed some of that 313 00:14:33,970 --> 00:14:39,010 with the bone density loss, the muscle toning loss. 314 00:14:39,010 --> 00:14:43,940 But the most immediate reaction that one feels is a fluid shift. 315 00:14:43,940 --> 00:14:47,630 And again, I'm sitting here, or if I'm standing up, 316 00:14:47,630 --> 00:14:50,210 gravity is working to hold my bodily fluids, 317 00:14:50,210 --> 00:14:57,000 the bloods in my legs and arms if I have my arms at my side. 318 00:14:57,000 --> 00:14:58,650 When you remove the gravity, that -- 319 00:14:58,650 --> 00:15:00,850 there tends to be a fluid shift out of the legs, 320 00:15:00,850 --> 00:15:02,970 into the chest cavity and the head. 321 00:15:02,970 --> 00:15:04,910 And if you look very carefully at some of the pictures 322 00:15:04,910 --> 00:15:07,560 of the astronauts in space, they do look a little puffy, 323 00:15:07,560 --> 00:15:10,940 a little more full than they do on the ground. 324 00:15:10,940 --> 00:15:12,640 And that is because of that fluid shift. 325 00:15:12,640 --> 00:15:16,420 Now, a consequence of that fluid shift is what we call space 326 00:15:16,420 --> 00:15:19,110 adaptation syndrome. 327 00:15:19,110 --> 00:15:23,660 It's not the same as, but it's not very much different as, 328 00:15:23,660 --> 00:15:27,430 it's hard to describe, as when you -- if you go aboard a ship 329 00:15:27,430 --> 00:15:30,560 and you have a tendency to be seasick. 330 00:15:30,560 --> 00:15:34,780 It is a similar reaction, but not exactly. 331 00:15:34,780 --> 00:15:36,610 And you tend not to feel very comfortable. 332 00:15:36,610 --> 00:15:38,930 You got this -- maybe a headache. 333 00:15:38,930 --> 00:15:40,530 You might have some nausea. 334 00:15:40,530 --> 00:15:42,710 It depends on the individual. 335 00:15:42,710 --> 00:15:47,620 And what's the good news is, is that goes away after a few days. 336 00:15:47,620 --> 00:15:48,970 The body adapts. 337 00:15:48,970 --> 00:15:52,450 You tend to, you know, not notice it anymore. 338 00:15:52,450 --> 00:15:55,770 An analogy I would draw is if you ever had a tooth filled, 339 00:15:55,770 --> 00:15:58,220 you know, with a cavity and you had a filling done 340 00:15:58,220 --> 00:16:01,580 or you had work done on your teeth, you know, the first day 341 00:16:01,580 --> 00:16:04,240 or two that you had that filling, you tend to notice it. 342 00:16:04,240 --> 00:16:06,530 But then after a few days or three days, 343 00:16:06,530 --> 00:16:08,260 you don't notice it anymore. 344 00:16:08,260 --> 00:16:09,810 You get used to that feeling. 345 00:16:09,810 --> 00:16:14,110 And it's sort of the same with space adaptation syndrome. 346 00:16:14,110 --> 00:16:16,130 >> Kelly Humphries: Okay. 347 00:16:16,130 --> 00:16:17,570 Another question? 348 00:16:17,570 --> 00:16:20,740 >> Brian Brookes [assumed spelling]: 349 00:16:20,740 --> 00:16:23,350 My name is Brian Brookes, I'm in ninth grade. 350 00:16:23,350 --> 00:16:24,140 I'm a freshman. 351 00:16:24,140 --> 00:16:28,810 And I wanted to know what does up in space smell like? 352 00:16:28,810 --> 00:16:30,200 >> Mario Runco: Did I get that right? 353 00:16:30,200 --> 00:16:31,290 >> Kelly Humphries: What does space -- 354 00:16:31,290 --> 00:16:33,290 >> Mario Runco: Smell -- what does space smell like? 355 00:16:33,290 --> 00:16:34,880 That's a darn good question. 356 00:16:34,880 --> 00:16:39,910 Actually, the direct answer is nobody knows 357 00:16:39,910 --> 00:16:43,400 because space would not have smell if you're outside 358 00:16:43,400 --> 00:16:46,430 because it's basically a vacuum. 359 00:16:46,430 --> 00:16:50,010 And there's no way to sense odors 'cause we need atmosphere 360 00:16:50,010 --> 00:16:52,090 and air for -- to pass over our nostrils 361 00:16:52,090 --> 00:16:54,220 to have a sense of smell. 362 00:16:54,220 --> 00:16:58,400 Having said that, there is a sense of odor in space. 363 00:16:58,400 --> 00:17:03,400 And that tends to be like a new car smell. 364 00:17:03,400 --> 00:17:04,500 If you get into a new car. 365 00:17:04,500 --> 00:17:06,590 Everybody -- most people like the smell. 366 00:17:06,590 --> 00:17:07,610 You take it in. 367 00:17:07,610 --> 00:17:10,970 And that is from the outgassing of the materials 368 00:17:10,970 --> 00:17:13,000 of which the car is made. 369 00:17:13,000 --> 00:17:14,970 And depending upon the spacecraft, 370 00:17:14,970 --> 00:17:17,150 in the case of the space shuttle, 371 00:17:17,150 --> 00:17:18,300 I was not aware of that. 372 00:17:18,300 --> 00:17:20,700 And you kind of get used to it because you operate 373 00:17:20,700 --> 00:17:22,980 in a similar environment in simulators. 374 00:17:22,980 --> 00:17:26,820 You actually train in the space shuttle at times before launch. 375 00:17:26,820 --> 00:17:28,520 So you're in the real vehicle. 376 00:17:28,520 --> 00:17:32,680 And you're also inside your suits at times. 377 00:17:32,680 --> 00:17:36,120 And what I noticed one time after being removed 378 00:17:36,120 --> 00:17:40,350 from the space shuttle after several years, I got back inside 379 00:17:40,350 --> 00:17:44,900 of one, and what struck me was the odor. 380 00:17:44,900 --> 00:17:50,000 The smell of the space shuttle itself is 381 00:17:50,000 --> 00:17:54,200 that combined collective of outgassing from the materials 382 00:17:54,200 --> 00:17:56,190 in the space shuttle, at least 383 00:17:56,190 --> 00:17:57,720 in the case of the space shuttle. 384 00:17:57,720 --> 00:18:02,700 And it hit me that that's the smell of space. 385 00:18:02,700 --> 00:18:06,580 So it's not really the space outside that smells. 386 00:18:06,580 --> 00:18:08,580 It's the things that we bring with us 387 00:18:08,580 --> 00:18:12,780 that actually give us a sense of orientation 388 00:18:12,780 --> 00:18:15,470 from a sense of smell perspective. 389 00:18:15,470 --> 00:18:17,190 >> Kelly Humphries: Now, you're a veteran spacewalker. 390 00:18:17,190 --> 00:18:19,540 I understand there is a special smell that comes 391 00:18:19,540 --> 00:18:20,960 with coming back in the airlock 392 00:18:20,960 --> 00:18:22,950 after a spacewalk, for some folks. 393 00:18:22,950 --> 00:18:23,460 >> Mario Runco: Yes. 394 00:18:23,460 --> 00:18:27,010 When you come back in and pop your helmet off, again, 395 00:18:27,010 --> 00:18:32,470 it's that odor of the spacecraft that hits you, 396 00:18:32,470 --> 00:18:35,810 that it's like a sense of home. 397 00:18:35,810 --> 00:18:40,030 I mean, if you walk into various retail stores 398 00:18:40,030 --> 00:18:42,870 or somebody's home, there's a slightly different 399 00:18:42,870 --> 00:18:44,240 characteristic odor. 400 00:18:44,240 --> 00:18:47,420 And that's -- you know, if it's your home and that's -- 401 00:18:47,420 --> 00:18:48,970 and if it's something wrong or different, 402 00:18:48,970 --> 00:18:50,490 then you'll notice it. 403 00:18:50,490 --> 00:18:50,820 >> Kelly Humphries: Okay. 404 00:18:50,820 --> 00:18:51,330 >> Mario Runco: Yeah. 405 00:18:51,330 --> 00:18:51,560 >> Kelly Humphries: Well, 406 00:18:51,560 --> 00:18:53,950 I understand that's all the time we have for today. 407 00:18:53,950 --> 00:18:56,770 We want to thank you folks for being with us today. 408 00:18:56,770 --> 00:18:58,210 And thank you, Mario -- 409 00:18:58,210 --> 00:18:58,490 >> Mario Runco: My pleasure. 410 00:18:58,490 --> 00:18:59,040 >> Kelly Humphries: For joining us 411 00:18:59,040 --> 00:19:00,440 and answering the students' questions. 412 00:19:00,440 --> 00:19:08,160 We hope you have a great rest of your day and a great weekend. 413 00:19:08,160 --> 00:19:09,580 >> Mario Runco: Take care, guys. 414 00:19:09,580 --> 00:19:09,810 >> Thank you.