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These are the user uploaded subtitles that are being translated: 1 00:00:00,000 --> 00:00:02,730 (technological music) 2 00:00:02,730 --> 00:00:05,590 - [Narrator] NASA's latest robotic lander, InSight, 3 00:00:05,590 --> 00:00:08,180 descends to the surface of Mars, 4 00:00:08,180 --> 00:00:11,215 the challenging effort greeted with elation. 5 00:00:11,215 --> 00:00:12,397 - [Operator] Touchdown confirmed. 6 00:00:12,397 --> 00:00:14,980 (crowd cheers) 7 00:00:19,855 --> 00:00:20,688 - [Narrator] Meanwhile, 8 00:00:20,688 --> 00:00:22,920 an orbiting ESA satellite, ExoMars, 9 00:00:22,920 --> 00:00:26,073 begins its own exploration of this enthralling planet. 10 00:00:30,484 --> 00:00:35,084 (flames roar) (intense music) 11 00:00:35,084 --> 00:00:37,584 (flame roars) 12 00:00:39,686 --> 00:00:42,448 (flames roar) 13 00:00:42,448 --> 00:00:44,948 (flames roar) 14 00:00:46,153 --> 00:00:49,150 (meteor strikes) 15 00:00:49,150 --> 00:00:52,108 (space whooshes) 16 00:00:52,108 --> 00:00:54,858 (light explodes) 17 00:00:59,914 --> 00:01:02,331 (logo soars) 18 00:01:04,468 --> 00:01:07,218 (soothing music) 19 00:01:18,140 --> 00:01:21,690 The majestic stereo imagery of Mars as seen from orbit 20 00:01:21,690 --> 00:01:25,170 reveals a planet of dynamic texture and form 21 00:01:25,170 --> 00:01:27,610 slowly revealing its secrets. 22 00:01:27,610 --> 00:01:30,360 (soothing music) 23 00:02:20,022 --> 00:02:21,940 - We've sent a lot of missions to Mars in the past. 24 00:02:21,940 --> 00:02:24,339 We've sent rovers, we've sent orbiters, 25 00:02:24,339 --> 00:02:28,150 and they've done a lot of really, really great science 26 00:02:28,150 --> 00:02:30,130 and a lot of really interesting measurements, 27 00:02:30,130 --> 00:02:32,990 but those measurements just scratch the surface of Mars. 28 00:02:32,990 --> 00:02:34,730 We know a lot about the surface of Mars, 29 00:02:34,730 --> 00:02:36,640 we know a lot about its atmosphere, 30 00:02:36,640 --> 00:02:38,500 and even about its ionosphere, 31 00:02:38,500 --> 00:02:40,070 but we don't know very much about 32 00:02:40,070 --> 00:02:42,340 what goes on a mile below the surface, 33 00:02:42,340 --> 00:02:45,410 much less 2000 miles below the surface down to the center. 34 00:02:45,410 --> 00:02:46,600 And this will be the first mission 35 00:02:46,600 --> 00:02:48,260 that's going to Mars specifically 36 00:02:48,260 --> 00:02:53,260 to investigate the huge extent of Mars below the surface. 37 00:02:54,900 --> 00:02:57,530 (soothing music) (machinery whirring) 38 00:02:57,530 --> 00:03:01,090 The basic idea of InSight is to map out 39 00:03:01,090 --> 00:03:04,010 the deep structure of Mars for the very first time. 40 00:03:04,010 --> 00:03:06,590 We're gonna map out the thickness of the crust, 41 00:03:06,590 --> 00:03:08,220 the size of the core, 42 00:03:08,220 --> 00:03:11,370 the composition of the mantle and core of the planet. 43 00:03:11,370 --> 00:03:15,881 Sort of get the first map of the deep inside of Mars. 44 00:03:15,881 --> 00:03:19,730 (machinery whirring) 45 00:03:19,730 --> 00:03:22,790 It's going to Mars to do the science, 46 00:03:22,790 --> 00:03:24,630 to make the measurements, 47 00:03:24,630 --> 00:03:27,610 that scientifically and personally, 48 00:03:27,610 --> 00:03:31,160 I've been waiting for over 30 years for. 49 00:03:31,160 --> 00:03:35,430 As a graduate student, I was doing research on Mars 50 00:03:35,430 --> 00:03:39,020 and I just needed to have the thickness of the crust. 51 00:03:39,020 --> 00:03:40,600 I just needed the thickness of the crust, 52 00:03:40,600 --> 00:03:42,050 and we didn't have it. 53 00:03:42,050 --> 00:03:44,390 And seismology was the way to do it, 54 00:03:44,390 --> 00:03:46,475 and so I thought, well maybe someday somebody will put 55 00:03:46,475 --> 00:03:49,160 a seismometer on Mars and get this measurement 56 00:03:49,160 --> 00:03:50,340 so I can do my research. 57 00:03:50,340 --> 00:03:54,560 And so it's kind of an amazing journey for me to look back 58 00:03:54,560 --> 00:03:57,270 and say, I'm the guy who's actually going to put 59 00:03:57,270 --> 00:04:00,160 that seismometer on Mars, get that information, 60 00:04:00,160 --> 00:04:02,100 and now I can go back and finish the job 61 00:04:02,100 --> 00:04:03,798 I was trying to do 30 years ago. 62 00:04:03,798 --> 00:04:05,633 It's an amazing feeling. 63 00:04:06,770 --> 00:04:09,170 - The InSight mission will finally provide 64 00:04:09,170 --> 00:04:12,330 a seismic information of Mars 65 00:04:12,330 --> 00:04:14,810 that scientists have been wanting for 66 00:04:14,810 --> 00:04:17,080 since the very first Mars lander, Viking. 67 00:04:17,080 --> 00:04:20,200 It has a seismometer on it, but for a variety of reasons 68 00:04:20,200 --> 00:04:22,720 it never got back any seismic data. 69 00:04:22,720 --> 00:04:25,620 There's been many other attempts to get seismometers 70 00:04:25,620 --> 00:04:29,760 onto the surface of Mars for very good science reasons, 71 00:04:29,760 --> 00:04:31,590 but they've, for one reason or another, 72 00:04:31,590 --> 00:04:32,940 never been successful. 73 00:04:32,940 --> 00:04:35,420 So now, we're right on the very edge 74 00:04:35,420 --> 00:04:37,670 of getting a seismometer on Mars 75 00:04:37,670 --> 00:04:40,420 that will finally give us back seismic data. 76 00:04:40,420 --> 00:04:43,120 That seismic data's incredibly important to scientists 77 00:04:43,120 --> 00:04:46,610 because it gives them an idea what the size of the crust, 78 00:04:46,610 --> 00:04:48,690 the mantle, and the core are, 79 00:04:48,690 --> 00:04:50,750 as well as the properties of each of those, 80 00:04:50,750 --> 00:04:54,143 which are the basic internals of every rocky planet. 81 00:04:59,529 --> 00:05:02,196 (intense music) 82 00:05:04,960 --> 00:05:07,860 - The most fun or interesting thing about InSight 83 00:05:07,860 --> 00:05:09,170 from an engineer's point of view 84 00:05:09,170 --> 00:05:11,830 is really that we're playing the claw game 85 00:05:11,830 --> 00:05:13,800 super far away on Mars. 86 00:05:13,800 --> 00:05:15,380 We're taking this grapple, 87 00:05:15,380 --> 00:05:17,400 and we're gonna pick up an instrument, 88 00:05:17,400 --> 00:05:20,030 and lift it up off the deck and put it down on Mars. 89 00:05:20,030 --> 00:05:22,400 So, I like to say that we're playing the claw game, 90 00:05:22,400 --> 00:05:24,153 on Mars, with no joystick. 91 00:05:25,478 --> 00:05:28,298 (machinery clinking) 92 00:05:28,298 --> 00:05:29,150 (machinery whirring) 93 00:05:29,150 --> 00:05:31,180 - [Narrator] Next, a wind and thermal shield 94 00:05:31,180 --> 00:05:33,130 will be lowered over the seismic instrument 95 00:05:33,130 --> 00:05:35,490 to protect it from the environment. 96 00:05:35,490 --> 00:05:38,050 The second instrument, the heat flow probe, 97 00:05:38,050 --> 00:05:40,050 will be placed on the ground, and over time 98 00:05:40,050 --> 00:05:43,533 will hammer itself down to take subsurface readings. 99 00:05:49,500 --> 00:05:52,210 - There's a lot of international partners on InSight. 100 00:05:52,210 --> 00:05:54,458 It really takes a whole world to produce 101 00:05:54,458 --> 00:05:56,220 an exciting mission like this. 102 00:05:56,220 --> 00:05:58,380 So most of our science missions 103 00:05:58,380 --> 00:06:01,540 are actually being supported by our international partners. 104 00:06:01,540 --> 00:06:05,210 So for example, the SEIS instrument, our seismometer, 105 00:06:05,210 --> 00:06:08,092 has support from the French, the Germans, 106 00:06:08,092 --> 00:06:11,890 the Swiss, the UK folks. 107 00:06:11,890 --> 00:06:15,390 So we have a variety of those people. 108 00:06:15,390 --> 00:06:17,360 The Heat Flow and Physical Properties Probe 109 00:06:17,360 --> 00:06:18,910 is being provided by the Germans 110 00:06:18,910 --> 00:06:20,933 with some support from Poland. 111 00:06:24,947 --> 00:06:25,780 (energetic music) 112 00:06:25,780 --> 00:06:26,900 - InSight is a mission to Mars, 113 00:06:26,900 --> 00:06:28,760 but it's much, much more than a Mars mission. 114 00:06:28,760 --> 00:06:30,740 In some sense, it's like a time machine. 115 00:06:30,740 --> 00:06:32,973 It's measuring the structure of Mars 116 00:06:32,973 --> 00:06:35,800 that was put in place 4.5 billion years ago. 117 00:06:35,800 --> 00:06:38,920 So we can go back and understand the processes 118 00:06:38,920 --> 00:06:40,900 that formed Mars just shortly after 119 00:06:40,900 --> 00:06:43,640 it was accreted from the solar nebula. 120 00:06:43,640 --> 00:06:46,100 By studying Mars, we'll be able to learn more 121 00:06:46,100 --> 00:06:49,260 about Earth, Venus, Mercury, even the moon, 122 00:06:49,260 --> 00:06:51,822 even exoplanets around other stars. 123 00:06:51,822 --> 00:06:53,696 (energetic music) 124 00:06:53,696 --> 00:06:56,446 (light explodes) 125 00:07:00,506 --> 00:07:03,089 (upbeat music) 126 00:07:04,811 --> 00:07:07,311 (flame roars) 127 00:07:12,486 --> 00:07:14,300 - [Narrator] ESA's Trace Gas Orbiter mission 128 00:07:14,300 --> 00:07:16,223 arrived at Mars some time ago. 129 00:07:19,480 --> 00:07:22,240 Since then, this 3.5 ton spacecraft 130 00:07:22,240 --> 00:07:24,270 has been gently brushing the atmosphere 131 00:07:24,270 --> 00:07:26,093 to gradually adjust its orbit. 132 00:07:32,126 --> 00:07:34,240 In ESA's Planetary Missions Control Room 133 00:07:34,240 --> 00:07:36,750 in Darmstadt, Germany, 134 00:07:36,750 --> 00:07:39,620 flight controllers have been checking systems 135 00:07:39,620 --> 00:07:40,950 and commissioning instruments 136 00:07:40,950 --> 00:07:43,393 on the ExoMars Trace Gas Orbiter. 137 00:07:45,460 --> 00:07:48,360 Now it's ready to begin its science mission. 138 00:07:51,620 --> 00:07:53,640 - It has been a long time since we arrived at Mars 139 00:07:53,640 --> 00:07:55,840 in October 2016, 140 00:07:55,840 --> 00:08:00,190 and we have had a long, very long period, 141 00:08:00,190 --> 00:08:02,370 one year of aerobraking, 142 00:08:02,370 --> 00:08:06,338 which consisted in reducing the orbital period 143 00:08:06,338 --> 00:08:08,760 from the time when we arrived 144 00:08:08,760 --> 00:08:12,720 where it was actually several days, to two hours, 145 00:08:12,720 --> 00:08:16,898 which is the nominal period for science observations. 146 00:08:16,898 --> 00:08:19,148 (mumbling) 147 00:08:21,920 --> 00:08:25,230 I'm looking forward to the next few months enormously 148 00:08:26,400 --> 00:08:27,690 because with TGO, 149 00:08:27,690 --> 00:08:32,690 we'll finally be able to show its full capability, 150 00:08:33,650 --> 00:08:36,230 the full capability of its instruments 151 00:08:36,230 --> 00:08:40,300 in terms of accuracy and the quantity and quality 152 00:08:40,300 --> 00:08:42,573 of data, pictures, spectra. 153 00:08:43,430 --> 00:08:47,170 And also because we will be able to do joint starts, 154 00:08:47,170 --> 00:08:51,640 joint observations, with our previous space traffic Mars, 155 00:08:51,640 --> 00:08:54,480 Mars Express, which is still alive and working 156 00:08:54,480 --> 00:08:56,123 after 15 years, actually. 157 00:08:57,173 --> 00:09:00,910 And having two space craft around Mars 158 00:09:00,910 --> 00:09:05,430 in complementary orbits, from a scientific point of view, 159 00:09:05,430 --> 00:09:08,950 is very exciting and will allow, certainly, 160 00:09:08,950 --> 00:09:13,313 some very interesting discoveries and observations. 161 00:09:17,708 --> 00:09:19,094 (machinery rumbles) 162 00:09:19,094 --> 00:09:20,710 - [Narrator] ExoMars will fill a double role 163 00:09:20,710 --> 00:09:23,280 when its partner rover is dispatched to Mars 164 00:09:23,280 --> 00:09:25,460 in the coming months in the search for life 165 00:09:25,460 --> 00:09:26,990 on the dusty planet. 166 00:09:26,990 --> 00:09:29,990 (machinery rumbles) 167 00:09:37,320 --> 00:09:39,440 - It is a communications satellite, 168 00:09:39,440 --> 00:09:42,530 on top of being a science orbiter. 169 00:09:42,530 --> 00:09:47,104 And the so-called relay function 170 00:09:47,104 --> 00:09:50,790 allows us to communicate with all landers and rovers 171 00:09:50,790 --> 00:09:52,033 on the surface of Mars. 172 00:09:53,530 --> 00:09:57,930 At the moment, we are only rovers and landers from NASA, 173 00:09:57,930 --> 00:10:00,480 Curiosity and Opportunity. 174 00:10:00,480 --> 00:10:03,550 Some tests had been done already, 175 00:10:03,550 --> 00:10:05,550 soon after arrival at Mars. 176 00:10:05,550 --> 00:10:08,210 And now we are gonna start a campaign 177 00:10:08,210 --> 00:10:12,110 to calibrate and datamine the best performance 178 00:10:12,110 --> 00:10:14,380 to relay data. 179 00:10:14,380 --> 00:10:15,570 - [Narrator] The Trace Gas Orbiter's 180 00:10:15,570 --> 00:10:17,070 primary mission, however, 181 00:10:17,070 --> 00:10:19,800 is to identify gasses in the Martian atmosphere, 182 00:10:19,800 --> 00:10:21,610 particularly methane, 183 00:10:21,610 --> 00:10:24,070 first hinted at by Mars Express, 184 00:10:24,070 --> 00:10:26,710 and then by NASA's Curiosity Rover 185 00:10:26,710 --> 00:10:30,280 as it sniffed the atmosphere with special sensors. 186 00:10:30,280 --> 00:10:33,060 - Well, we know that the lifetime on methane is very short, 187 00:10:33,060 --> 00:10:34,230 just a few hundred years. 188 00:10:34,230 --> 00:10:36,380 It will be broken down by the sunlight, 189 00:10:36,380 --> 00:10:39,350 by the UV, ultraviolet component of the sunlight, 190 00:10:39,350 --> 00:10:42,790 so if it is there now, we knew that it has to be refilled 191 00:10:42,790 --> 00:10:43,830 all the time. 192 00:10:43,830 --> 00:10:44,870 And where does it come from? 193 00:10:44,870 --> 00:10:45,876 That's the big question. 194 00:10:45,876 --> 00:10:48,749 It cannot be synthesized really in that atmosphere. 195 00:10:48,749 --> 00:10:51,510 It has to come from the surface or from the subsurface. 196 00:10:51,510 --> 00:10:53,920 But what are the processes that produces it? 197 00:10:53,920 --> 00:10:55,900 This is what we want to find out. 198 00:10:55,900 --> 00:10:59,810 One possibility is that it is some geological reaction 199 00:10:59,810 --> 00:11:04,810 between minerals and water. 200 00:11:04,910 --> 00:11:07,710 Another possibility is that actually those are microbes 201 00:11:07,710 --> 00:11:11,107 down buried underneath the surface 202 00:11:11,107 --> 00:11:14,750 that is producing it today or has produced it 203 00:11:14,750 --> 00:11:16,660 a long time ago and they are all dead now, 204 00:11:16,660 --> 00:11:19,010 but that the methane had been kept underground 205 00:11:19,010 --> 00:11:20,810 and with some mechanism is released 206 00:11:20,810 --> 00:11:22,620 to get up into the atmosphere. 207 00:11:22,620 --> 00:11:25,272 So these are all these kind of things we try to find out. 208 00:11:25,272 --> 00:11:27,939 (calming music) 209 00:11:31,980 --> 00:11:34,830 - [Narrator] By using the orbiter's powerful spectrometer, 210 00:11:34,830 --> 00:11:37,220 scientists hope to discover whether the methane 211 00:11:37,220 --> 00:11:40,403 comes from a geological or biological source. 212 00:11:41,400 --> 00:11:44,050 95% of methane on our own planet 213 00:11:44,050 --> 00:11:46,410 comes from living organisms. 214 00:11:46,410 --> 00:11:49,650 The ExoMars Rover, landing in 2021, 215 00:11:49,650 --> 00:11:52,140 will drill up to two meters beneath the surface 216 00:11:52,140 --> 00:11:55,050 to search for this evidence of life. 217 00:11:55,050 --> 00:11:58,300 And the rover, as well as NASA rovers and landers, 218 00:11:58,300 --> 00:12:01,113 will use the orbiter to keep in touch with Earth. 219 00:12:13,680 --> 00:12:16,660 Mars exploration is an international endeavor, 220 00:12:16,660 --> 00:12:18,870 and every mission adds to our understanding 221 00:12:18,870 --> 00:12:20,970 of this alien world. 222 00:12:20,970 --> 00:12:23,833 A place that some of us might someday call home. 223 00:12:27,100 --> 00:12:30,290 - Planetary exploration is always very exciting, 224 00:12:30,290 --> 00:12:32,200 but Mars, of course, has its very special thing, 225 00:12:32,200 --> 00:12:33,880 is that there's actually a place 226 00:12:33,880 --> 00:12:37,600 that you can imagine yourself walking on eventually, 227 00:12:37,600 --> 00:12:40,240 within a not-too-far time in the future. 228 00:12:40,240 --> 00:12:42,780 Surely, people will be walking on Mars. 229 00:12:42,780 --> 00:12:44,140 That makes us very exciting. 230 00:12:44,140 --> 00:12:46,810 And then to think about this idea that there might 231 00:12:46,810 --> 00:12:48,780 have been some kind of life, 232 00:12:48,780 --> 00:12:51,350 or even exist today underground on Mars. 233 00:12:51,350 --> 00:12:52,939 That makes it a very special place. 234 00:12:52,939 --> 00:12:55,248 (energetic music) 235 00:12:55,248 --> 00:12:57,998 (light explodes) 236 00:13:02,111 --> 00:13:07,111 (machinery rumbles) (eerie music) 237 00:13:16,640 --> 00:13:18,770 - [Narrator] Curiosity landed in Gale Crater 238 00:13:18,770 --> 00:13:20,810 on an ancient lake bed. 239 00:13:20,810 --> 00:13:22,550 A few months after arrival, 240 00:13:22,550 --> 00:13:24,910 it drilled into sedimentary rocks 241 00:13:24,910 --> 00:13:27,470 and detected traces of organic molecules 242 00:13:27,470 --> 00:13:29,656 using an instrument called SAM. 243 00:13:29,656 --> 00:13:32,656 (machinery rumbles) 244 00:13:36,861 --> 00:13:39,778 (machinery whirrs) 245 00:13:42,177 --> 00:13:43,696 - Well, the SAM instrument detected 246 00:13:43,696 --> 00:13:47,280 a variety of organic molecules in a sediment 247 00:13:47,280 --> 00:13:48,990 that is from an ancient lake bed 248 00:13:48,990 --> 00:13:50,680 in the middle of Gale Crater. 249 00:13:50,680 --> 00:13:51,930 And what's important about these 250 00:13:51,930 --> 00:13:54,480 is that we now have a lot more certainty 251 00:13:54,480 --> 00:13:56,520 that there's organic molecules preserved 252 00:13:56,520 --> 00:13:58,100 at the surface of Mars. 253 00:13:58,100 --> 00:13:59,900 We didn't know that before. 254 00:13:59,900 --> 00:14:02,050 But what's interesting is that we don't know 255 00:14:02,050 --> 00:14:05,670 what the source of these organic molecules is right now. 256 00:14:05,670 --> 00:14:08,400 There's just not enough information from that. 257 00:14:08,400 --> 00:14:10,250 However, if we drill deeper 258 00:14:10,250 --> 00:14:11,730 and we look around a little bit more, 259 00:14:11,730 --> 00:14:14,270 we might actually be able to get to that information 260 00:14:14,270 --> 00:14:16,170 and tell, did they come from life? 261 00:14:16,170 --> 00:14:18,630 Did they come from geological processes? 262 00:14:18,630 --> 00:14:20,270 Or maybe they were from meteorites 263 00:14:20,270 --> 00:14:21,960 that were deposited in the lake. 264 00:14:21,960 --> 00:14:23,070 We just don't know right now, 265 00:14:23,070 --> 00:14:25,127 but hopefully we'll figure that out. 266 00:14:25,127 --> 00:14:27,080 (dramatic music) 267 00:14:27,080 --> 00:14:28,330 - [Narrator] Curiosity is searching 268 00:14:28,330 --> 00:14:30,113 for carbon-based organics. 269 00:14:35,900 --> 00:14:37,450 - SAM made the new detections 270 00:14:37,450 --> 00:14:40,740 by heating samples of crushed rock to very high temperatures 271 00:14:40,740 --> 00:14:42,720 above 1000 degrees fahrenheit. 272 00:14:42,720 --> 00:14:44,100 This vaporized the samples, 273 00:14:44,100 --> 00:14:46,510 and released several species of small hydrocarbons 274 00:14:46,510 --> 00:14:48,580 like benzene and propane. 275 00:14:48,580 --> 00:14:49,890 Because the hydrocarbons 276 00:14:49,890 --> 00:14:52,190 were released at such high temperatures, 277 00:14:52,190 --> 00:14:54,040 they may be the fragments of bigger, 278 00:14:54,040 --> 00:14:57,930 heavier molecules within the rock, similar to kerogens. 279 00:14:57,930 --> 00:15:00,160 On Earth, kerogens are found in rocks 280 00:15:00,160 --> 00:15:02,270 like black shale and coal, 281 00:15:02,270 --> 00:15:05,822 and are the products of ancient plant and bacteria. 282 00:15:05,822 --> 00:15:08,350 (technological music) 283 00:15:08,350 --> 00:15:10,390 - [Narrator] Some other organics have been detected 284 00:15:10,390 --> 00:15:13,470 like thiophene, which contains sulfur. 285 00:15:13,470 --> 00:15:15,910 Introduced by geological processes, 286 00:15:15,910 --> 00:15:18,340 this sulfur acts as a preservative, 287 00:15:18,340 --> 00:15:20,820 binding organic molecules together 288 00:15:20,820 --> 00:15:23,320 and making them resistant to oxidation, 289 00:15:23,320 --> 00:15:26,150 so preserving them for millennia. 290 00:15:26,150 --> 00:15:29,730 - Organic molecules could be the food for life, 291 00:15:29,730 --> 00:15:31,770 or they could be the product of life, 292 00:15:31,770 --> 00:15:34,060 or maybe they're from something altogether different, 293 00:15:34,060 --> 00:15:36,410 such as geology or meteorites 294 00:15:36,410 --> 00:15:38,370 that were deposited into the lake. 295 00:15:38,370 --> 00:15:42,300 We don't know what the source is, but there's a story there 296 00:15:42,300 --> 00:15:45,058 and we're going to uncover what that is. 297 00:15:45,058 --> 00:15:47,808 (machinery hums) 298 00:15:49,200 --> 00:15:51,450 - [Narrator] Scientists still don't know if the discovered 299 00:15:51,450 --> 00:15:54,580 organics on Mars are biological in origin, 300 00:15:54,580 --> 00:15:57,040 but it's exciting to find such old material 301 00:15:57,040 --> 00:15:59,370 preserved right at the surface. 302 00:15:59,370 --> 00:16:02,723 This finding is also encouraging for future exploration. 303 00:16:04,050 --> 00:16:07,210 So for a time, Curiosity continued to travel, 304 00:16:07,210 --> 00:16:11,350 find interesting outcrops, drill holes, take samples. 305 00:16:11,350 --> 00:16:14,363 Then, inexplicably, something went wrong. 306 00:16:20,047 --> 00:16:21,180 - [Man] The drill's feed mechanism, 307 00:16:21,180 --> 00:16:23,930 which is responsible for moving Curiosity's drill bit 308 00:16:23,930 --> 00:16:26,700 into and out of rocks, didn't move when commanded. 309 00:16:26,700 --> 00:16:28,700 When Curiosity drills into a rock 310 00:16:28,700 --> 00:16:29,920 the way it was designed to, 311 00:16:29,920 --> 00:16:32,515 the drill's two stabilizer posts touch the rock first 312 00:16:32,515 --> 00:16:35,020 to steady the arm while the drill's feed mechanism 313 00:16:35,020 --> 00:16:36,649 moves the bit forward into the rock. 314 00:16:36,649 --> 00:16:37,510 (beeping) (machinery hums) 315 00:16:37,510 --> 00:16:41,320 Without the feed mechanism working, we can't drill that way. 316 00:16:41,320 --> 00:16:43,650 To solve this problem, we do what we always do. 317 00:16:43,650 --> 00:16:44,980 We worked it out in the testbed 318 00:16:44,980 --> 00:16:47,540 using Curiosity's twin, Honor. 319 00:16:47,540 --> 00:16:49,360 Our team of engineers and scientists have been 320 00:16:49,360 --> 00:16:51,010 working for months to figure out a way 321 00:16:51,010 --> 00:16:52,640 to collect and deliver rock samples 322 00:16:52,640 --> 00:16:54,420 without using the feed mechanism. 323 00:16:54,420 --> 00:16:56,370 Here's what we came up with. 324 00:16:56,370 --> 00:16:59,100 Using our new technique, called Feed Extended Drilling, 325 00:16:59,100 --> 00:17:01,070 the stabilizers are not used. 326 00:17:01,070 --> 00:17:02,760 The bit is now in a forward position 327 00:17:02,760 --> 00:17:04,683 extended past the stabilizers. 328 00:17:06,110 --> 00:17:09,150 Moving the drill straight into a rock and retracting safely 329 00:17:09,150 --> 00:17:11,243 without the stabilizers is challenging. 330 00:17:12,370 --> 00:17:14,690 We move the arm instead of the feed mechanism 331 00:17:14,690 --> 00:17:16,160 to place the bit onto the rock 332 00:17:16,160 --> 00:17:17,860 and press it forward as it drills. 333 00:17:18,936 --> 00:17:20,430 - [Operator] Now let's start holes beginning, over. 334 00:17:20,430 --> 00:17:22,910 - [Man] After making contact, we apply a light preload 335 00:17:22,910 --> 00:17:24,680 and drill a shallow pilot hole. 336 00:17:24,680 --> 00:17:26,610 We use a force sensor in the robotic arm 337 00:17:26,610 --> 00:17:28,826 to give Curiosity a sense of touch. 338 00:17:28,826 --> 00:17:29,950 (machine whirring) 339 00:17:29,950 --> 00:17:32,380 This lets Curiosity adjust its arm motion 340 00:17:32,380 --> 00:17:34,200 and avoid getting stuck while drilling. 341 00:17:34,200 --> 00:17:35,810 Kind of like you might adjust your arm 342 00:17:35,810 --> 00:17:37,560 while drilling into a wall at home. 343 00:17:38,890 --> 00:17:40,790 After drilling, we use a similar technique 344 00:17:40,790 --> 00:17:43,230 to retract from the hole without getting stuck. 345 00:17:43,230 --> 00:17:46,397 (technological music) 346 00:18:02,736 --> 00:18:04,910 - [Narrator] With Rover 2020 design and construction 347 00:18:04,910 --> 00:18:06,220 well underway, 348 00:18:06,220 --> 00:18:08,660 engineers will be sure to avoid such a problem 349 00:18:08,660 --> 00:18:10,340 with Curiosity's cousin, 350 00:18:10,340 --> 00:18:13,190 which will land in the Jezero Crater in 2020. 351 00:18:17,906 --> 00:18:20,489 (upbeat music) 352 00:18:30,017 --> 00:18:32,289 (energetic music) 353 00:18:32,289 --> 00:18:35,039 (light explodes) 354 00:18:39,598 --> 00:18:42,431 (inspiring music) 355 00:19:09,270 --> 00:19:13,350 2020 will be a banner year for the exploration of Mars. 356 00:19:13,350 --> 00:19:16,870 In addition to the launch of NASA's Mars 2020 Rover, 357 00:19:16,870 --> 00:19:19,640 the European Space Agency and Roscosmos 358 00:19:19,640 --> 00:19:22,746 are sending the ExoMars Rover to the red planet. 359 00:19:22,746 --> 00:19:25,829 (machinery whirring) 360 00:19:30,260 --> 00:19:33,030 Rover 2020 and its companion helicopter 361 00:19:33,030 --> 00:19:36,443 will no doubt expand our search for life, past or present. 362 00:19:53,310 --> 00:19:56,450 However, the big advance forward in organic analysis 363 00:19:56,450 --> 00:19:58,440 will be the game changer. 364 00:19:58,440 --> 00:20:01,403 Both rovers will carry onboard a MOMA. 365 00:20:04,743 --> 00:20:07,940 (cool music) 366 00:20:07,940 --> 00:20:11,360 - The Mars Organic Molecule Analyzer, or MOMA, 367 00:20:11,360 --> 00:20:15,100 is the largest and most complex instrument on the rover. 368 00:20:15,100 --> 00:20:18,350 Its mass spectrometer subsystem and its main electronics 369 00:20:18,350 --> 00:20:21,570 were built and tested at NASA's Goddard Space Flight Center, 370 00:20:21,570 --> 00:20:23,640 which also contributed mass spectrometers 371 00:20:23,640 --> 00:20:27,240 to NASA's Curiosity Rover and MAVEN Orbiter. 372 00:20:27,240 --> 00:20:29,810 MOMA is designed with a mix of proven hardware 373 00:20:29,810 --> 00:20:31,853 and innovative new technologies. 374 00:20:32,700 --> 00:20:34,510 Here's how it works. 375 00:20:34,510 --> 00:20:37,320 In gas chromatrograph mode, crushed Martian rock 376 00:20:37,320 --> 00:20:40,610 is put into an oven and heated to 900 degrees celsius 377 00:20:40,610 --> 00:20:43,403 in just two minutes, vaporizing the sample. 378 00:20:45,030 --> 00:20:47,140 Molecules of hot gas rise up 379 00:20:47,140 --> 00:20:50,870 and flow into a narrow, 20 meter long tube. 380 00:20:50,870 --> 00:20:53,630 Special coatings inside the tube cause molecules 381 00:20:53,630 --> 00:20:56,540 with certain chemistries to slow down more than others, 382 00:20:56,540 --> 00:20:59,490 separating the mixture of molecules over time. 383 00:20:59,490 --> 00:21:02,720 Next, a beam of electrons ionizes the molecules, 384 00:21:02,720 --> 00:21:04,910 giving them a positive electric charge 385 00:21:04,910 --> 00:21:08,130 and deflecting them towards the linear ion trap. 386 00:21:08,130 --> 00:21:11,100 The ions are caught by a fluctuating electric field 387 00:21:11,100 --> 00:21:14,453 and sent to a detector to determine their chemical makeup. 388 00:21:15,420 --> 00:21:18,310 While gas chromatography has been used to study Mars 389 00:21:18,310 --> 00:21:19,750 since the Viking Program, 390 00:21:19,750 --> 00:21:22,400 MOMA has a second method for preparing samples 391 00:21:22,400 --> 00:21:24,733 that has never been used on another planet. 392 00:21:24,733 --> 00:21:25,566 (shards clinking) 393 00:21:25,566 --> 00:21:26,960 In laser desorption mode, 394 00:21:26,960 --> 00:21:30,303 a sample is placed beneath a powerful ultraviolet laser. 395 00:21:31,185 --> 00:21:32,018 (laser bloops) 396 00:21:32,018 --> 00:21:34,570 A beam of energetic light builds within the laser 397 00:21:34,570 --> 00:21:36,610 and fires in a billionth of a second, 398 00:21:36,610 --> 00:21:38,610 concentrating its energy onto a spot 399 00:21:38,610 --> 00:21:40,407 smaller than a grain of sand. 400 00:21:40,407 --> 00:21:41,240 (laser boops) 401 00:21:41,240 --> 00:21:43,720 This rapidly vaporizes a portion of the sample, 402 00:21:43,720 --> 00:21:45,640 releasing large organic molecules 403 00:21:45,640 --> 00:21:48,360 that could be broken down by oven heating. 404 00:21:48,360 --> 00:21:51,540 The laser shot also ionizes some of the molecules, 405 00:21:51,540 --> 00:21:53,300 allowing the vapor to head directly 406 00:21:53,300 --> 00:21:55,460 to the linear ion trap. 407 00:21:55,460 --> 00:21:58,120 Neutral molecules are ejected by a vacuum 408 00:21:58,120 --> 00:22:00,470 while the remaining ions are sent to the detector 409 00:22:00,470 --> 00:22:02,930 to determine their chemical makeup. 410 00:22:02,930 --> 00:22:04,810 Laser desorption will enable MOMA 411 00:22:04,810 --> 00:22:07,470 to detect long molecules like lipids, 412 00:22:07,470 --> 00:22:09,620 the building blocks of cell membranes, 413 00:22:09,620 --> 00:22:12,412 a leap forward in the search for life on Mars. 414 00:22:12,412 --> 00:22:15,579 (inspirational music) 415 00:22:49,260 --> 00:22:50,880 - [Narrator] The question of life on Mars 416 00:22:50,880 --> 00:22:53,453 is among the most important in planetary science. 417 00:22:55,200 --> 00:22:58,253 And the evidence may be buried just below the surface. 418 00:23:00,010 --> 00:23:03,190 With the help of MOMA, we will take one step closer 419 00:23:03,190 --> 00:23:04,813 to uncovering the answer. 420 00:23:05,760 --> 00:23:08,620 These images will pave the way to a new understanding 421 00:23:08,620 --> 00:23:10,912 of life in our solar system. 422 00:23:10,912 --> 00:23:13,745 (energetic music) 32820

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