1 00:00:03,160 --> 00:00:04,000 >> Pat Ryan: Our mission 2 00:00:04,000 --> 00:00:06,440 to the International Space Station is not the only thing 3 00:00:06,440 --> 00:00:08,250 that NASA is doing of course. 4 00:00:08,250 --> 00:00:11,020 In fact, we're now less than one week away 5 00:00:11,020 --> 00:00:13,650 from the next Mars landing. 6 00:00:13,650 --> 00:00:18,210 NASA's Mars Science Laboratory with the rover Curiosity is due 7 00:00:18,210 --> 00:00:19,740 to land on Mars early 8 00:00:19,740 --> 00:00:22,560 in the morning next Monday August the 6th. 9 00:00:22,560 --> 00:00:25,200 You're going to be seeing more coverage of the MSL mission 10 00:00:25,200 --> 00:00:28,070 on NASA Television as we get closer to landing. 11 00:00:28,070 --> 00:00:31,000 That'll include features from the Jet Propulsion Laboratory 12 00:00:31,000 --> 00:00:34,450 in California, which manages the mission, as well as here 13 00:00:34,450 --> 00:00:36,390 at the Johnson Space Center in Houston, 14 00:00:36,390 --> 00:00:38,100 where some of the members 15 00:00:38,100 --> 00:00:41,620 of the Mars Science Laboratory team are located and one 16 00:00:41,620 --> 00:00:43,560 of them is here with us today to talk 17 00:00:43,560 --> 00:00:45,170 about the goals of that mission. 18 00:00:45,170 --> 00:00:48,900 Dr. Doug Archer is a fellow in NASA's post doctoral program 19 00:00:48,900 --> 00:00:53,240 and a member of the Sample Analysis at Mars Science Team. 20 00:00:53,240 --> 00:00:55,310 Doug let's tell me first 21 00:00:55,310 --> 00:00:58,620 of all how long have you been a part of the SAM team? 22 00:00:58,620 --> 00:01:00,280 >> Dr. Doug Archer: Well I've been a part of the SAM team 23 00:01:00,280 --> 00:01:04,350 for a little bit over two years now and I got involved 24 00:01:04,350 --> 00:01:08,230 by working with some Mars scientists here at JSC 25 00:01:08,230 --> 00:01:11,480 and I knew that they were involved in MSL and came 26 00:01:11,480 --> 00:01:14,760 out here to JSC to work with them and to work on MSL. 27 00:01:14,760 --> 00:01:17,020 >> Pat: This isn't even your first trip to Mars; 28 00:01:17,020 --> 00:01:18,500 I think that's pretty cool. 29 00:01:18,500 --> 00:01:21,930 You were part of a previous landing on Mars team right? 30 00:01:21,930 --> 00:01:24,680 >> Dr. Archer: Yeah I had the amazing experience to work 31 00:01:24,680 --> 00:01:29,550 as a science team member on the 2008 Phoenix Mars Scout Mission 32 00:01:29,550 --> 00:01:32,960 that landed on the northern plains of Mars a few years ago 33 00:01:32,960 --> 00:01:37,490 and I was able to help participate in the buildup 34 00:01:37,490 --> 00:01:40,880 to the mission and then landed ops and things like looking 35 00:01:40,880 --> 00:01:43,660 at sample acquisition and how to get a sample and where to dig 36 00:01:43,660 --> 00:01:47,060 for a sample and we're actually still involved here at JSC 37 00:01:47,060 --> 00:01:49,530 and analyzing some of the data that we're returned 38 00:01:49,530 --> 00:01:52,080 by the [inaudible] instrument on Phoenix, 39 00:01:52,080 --> 00:01:56,620 which as mass spectrometer that has some capabilities similar 40 00:01:56,620 --> 00:01:58,900 to that of the SAM instrument on MSL. 41 00:01:58,900 --> 00:02:02,280 >> Pat: Is landing on Mars all we might imagine it to be? 42 00:02:02,280 --> 00:02:04,800 >> Dr. Archer: I've got to say it's probably one 43 00:02:04,800 --> 00:02:06,470 of the most exciting thing that's ever happened 44 00:02:06,470 --> 00:02:07,210 to me in my life. 45 00:02:07,210 --> 00:02:11,740 It's a nerve raking few minutes but incredibly exciting. 46 00:02:11,740 --> 00:02:14,820 >> Pat: The MSL mission has got some big goals. 47 00:02:14,820 --> 00:02:16,150 Can you summarize it for us? 48 00:02:16,150 --> 00:02:20,190 What is MSL intending to find or to learn? 49 00:02:20,190 --> 00:02:22,910 >> Dr. Archer: Yeah so in one word its habitability. 50 00:02:22,910 --> 00:02:27,500 MSL is trying to analyze and investigate the habitability 51 00:02:27,500 --> 00:02:30,570 of our landing site and when I say habitability I'm not talking 52 00:02:30,570 --> 00:02:34,730 about looking for life per say, really it's looking 53 00:02:34,730 --> 00:02:37,340 for an environment where life could survive, 54 00:02:37,340 --> 00:02:39,550 where life could be ok. 55 00:02:39,550 --> 00:02:43,290 Either at some point in the past on Mars or maybe up even 56 00:02:43,290 --> 00:02:46,870 to today but again it's looking for habitability, 57 00:02:46,870 --> 00:02:51,470 not for life itself and it does that by using its suite 58 00:02:51,470 --> 00:02:54,320 of ten instruments which look at things like the geology, 59 00:02:54,320 --> 00:02:57,730 the geochemistry, the radiation environment and a whole host 60 00:02:57,730 --> 00:02:59,770 of other factors which are really interesting in 61 00:02:59,770 --> 00:03:03,470 and of themselves but together they can paint a really complete 62 00:03:03,470 --> 00:03:07,250 picture of if this environment is somewhere where life 63 00:03:07,250 --> 00:03:08,880 as we know it could have survived 64 00:03:08,880 --> 00:03:12,580 in the past or possibly today. 65 00:03:12,580 --> 00:03:13,990 >> Pat: That would lead one to think 66 00:03:13,990 --> 00:03:16,440 that there's something special about the landing site 67 00:03:16,440 --> 00:03:19,460 that you've chosen, that you think there's something there 68 00:03:19,460 --> 00:03:20,850 that you need to go see. 69 00:03:20,850 --> 00:03:22,210 >> Dr. Archer: Yeah so we're landing 70 00:03:22,210 --> 00:03:25,710 in a place called Gale Crater but the first criteria 71 00:03:25,710 --> 00:03:27,960 for any landing site is it has to be safe, 72 00:03:27,960 --> 00:03:31,050 that's the number one priority because it's really difficult 73 00:03:31,050 --> 00:03:34,100 to do science on the surface of Mars if you don't land safely 74 00:03:34,100 --> 00:03:35,660 so that's your number one priority 75 00:03:35,660 --> 00:03:38,580 but it's also very interesting from a scientific perspective. 76 00:03:38,580 --> 00:03:41,030 Again we're landing at the bottom of this large crater, 77 00:03:41,030 --> 00:03:44,770 Gale Crater and when we land we think we might be on top 78 00:03:44,770 --> 00:03:48,130 of some material that's been moved down from the crater walls 79 00:03:48,130 --> 00:03:49,950 and so even though we don't really have the intention 80 00:03:49,950 --> 00:03:52,460 to go see the crater walls themselves cause they're 81 00:03:52,460 --> 00:03:54,940 so far away, we might get a little glimpse of what's 82 00:03:54,940 --> 00:03:57,770 in them just because they're going to be there where we land. 83 00:03:57,770 --> 00:03:59,390 >> Pat: How big a crater are we talking about it? 84 00:03:59,390 --> 00:04:03,460 >> Dr. Archer: Its about 150 km or 110 or 120 miles 85 00:04:03,460 --> 00:04:08,210 across so this is a very large impact crater and then 86 00:04:08,210 --> 00:04:10,650 after we land as we look around we're going 87 00:04:10,650 --> 00:04:15,250 to see this huge mountain that's 5 km or 3 miles high 88 00:04:15,250 --> 00:04:18,860 in the center of the crater and its made up of these layers 89 00:04:18,860 --> 00:04:20,740 that were laid down over millions of years 90 00:04:20,740 --> 00:04:24,440 of Martian history so as we move away from our landing site 91 00:04:24,440 --> 00:04:26,790 and we drive towards and ultimately 92 00:04:26,790 --> 00:04:32,470 up onto this mountain, we'll be investigating hundreds 93 00:04:32,470 --> 00:04:34,750 of millions of years of Martian history 94 00:04:34,750 --> 00:04:38,340 >> Pat: and investigating the area between the landing site 95 00:04:38,340 --> 00:04:39,610 and the mountain all along the way. 96 00:04:39,610 --> 00:04:42,680 >> Dr. Archer: Yeah we you know we're the science team is 97 00:04:42,680 --> 00:04:46,070 whenever we see something interesting it's easy 98 00:04:46,070 --> 00:04:48,580 to get distracted so you see something fun, 99 00:04:48,580 --> 00:04:49,950 you want to go fun and different, 100 00:04:49,950 --> 00:04:52,170 you want to go see what it is and one of the great things 101 00:04:52,170 --> 00:04:55,010 about exploring Mars or exploring anywhere really is 102 00:04:55,010 --> 00:04:57,450 that it is exploration and you find something new 103 00:04:57,450 --> 00:05:01,130 and unexpected every time you go and that's really part 104 00:05:01,130 --> 00:05:04,790 of the fun and the reward of doing this. 105 00:05:04,790 --> 00:05:07,090 >> Pat: Cause right now you don't know what you don't know. 106 00:05:07,090 --> 00:05:07,870 >> Dr. Archer: Exactly. 107 00:05:07,870 --> 00:05:10,080 I mean you know everybody comes up with good ideas 108 00:05:10,080 --> 00:05:12,120 of what you think you're going to see when you get there 109 00:05:12,120 --> 00:05:14,400 but every single time we've been surprised. 110 00:05:14,400 --> 00:05:17,430 >> Pat: You mentioned that you were part of the SAM team; 111 00:05:17,430 --> 00:05:21,040 tell me about the components of that instrument and what it 112 00:05:21,040 --> 00:05:23,000 in particular is going to be looking for. 113 00:05:23,000 --> 00:05:25,920 >> Dr. Archer: Yeah so Sam is the main goal is to look 114 00:05:25,920 --> 00:05:29,380 for organic molecules but we're also going to be looking 115 00:05:29,380 --> 00:05:31,830 for inorganic molecules that could tell you something 116 00:05:31,830 --> 00:05:33,570 about which minerals are there and both 117 00:05:33,570 --> 00:05:36,810 of those things really tell you a lot about the habitability 118 00:05:36,810 --> 00:05:41,240 of the site and SAM at its heart is a gas analysis instrument 119 00:05:41,240 --> 00:05:45,520 so the first thing that you have to do is get a sample of gas 120 00:05:45,520 --> 00:05:48,170 to analyze and there's one of two ways to do that. 121 00:05:48,170 --> 00:05:51,950 The first and the easiest is just to open up the instruments 122 00:05:51,950 --> 00:05:55,160 of the atmosphere, take a sniff, measure the composition 123 00:05:55,160 --> 00:05:58,180 of the Martian atmosphere and see what's there. 124 00:05:58,180 --> 00:06:03,650 The second is MSL can deliver a sample of rock or soil to SAM. 125 00:06:03,650 --> 00:06:05,890 SAM takes the sample and can heat it up to 126 00:06:05,890 --> 00:06:09,100 about 1000 degrees Celsius and as you're heating 127 00:06:09,100 --> 00:06:11,300 up the sample it's giving off gas. 128 00:06:11,300 --> 00:06:12,800 Things like if there are organics 129 00:06:12,800 --> 00:06:15,330 in the sample those will start to come off 130 00:06:15,330 --> 00:06:17,010 and some minerals also will break 131 00:06:17,010 --> 00:06:20,550 down both below a 1000 degrees and so you can get a good idea 132 00:06:20,550 --> 00:06:23,670 of what's in the sample so then you have that gas 133 00:06:23,670 --> 00:06:26,900 and SAM analyzes it using one of three instruments 134 00:06:26,900 --> 00:06:30,270 within the instrument which are the mass spectrometer, 135 00:06:30,270 --> 00:06:33,770 the gas chromatograph and the tunable laser spectrometer 136 00:06:33,770 --> 00:06:36,220 and the mass spectrometer tells you what molecules are 137 00:06:36,220 --> 00:06:38,940 in the gas, the gas chromatograph can be used 138 00:06:38,940 --> 00:06:42,550 if you have a really complicated organic signal it can help tease 139 00:06:42,550 --> 00:06:45,060 apart what's there so you get a better understanding 140 00:06:45,060 --> 00:06:46,120 of what's in your sample. 141 00:06:46,120 --> 00:06:47,500 >> Pat: Tease apart the molecules? 142 00:06:47,500 --> 00:06:48,650 >> Dr. Archer: The organics yeah 143 00:06:48,650 --> 00:06:52,490 so if you say you have a big clump of organics that comes off 144 00:06:52,490 --> 00:06:55,880 at some temperature, the gas chromatograph will help 145 00:06:55,880 --> 00:06:58,590 to separate those based on the properties of the organics 146 00:06:58,590 --> 00:07:02,290 so you can get a better idea so it kind of it kind 147 00:07:02,290 --> 00:07:05,710 of slows things down I guess so you can get a better idea 148 00:07:05,710 --> 00:07:08,600 of what's there, a better understanding of what's there 149 00:07:08,600 --> 00:07:13,830 and then the tunable laser spectrometer is an instrument 150 00:07:13,830 --> 00:07:15,570 that's looking for three things. 151 00:07:15,570 --> 00:07:19,060 Carbon dioxide, water and methane 152 00:07:19,060 --> 00:07:21,340 and it can very sensitively measure the abundance 153 00:07:21,340 --> 00:07:24,800 of those three things and it also measures the isotopes 154 00:07:24,800 --> 00:07:28,070 of those different molecules and that's really important 155 00:07:28,070 --> 00:07:29,840 because for example with water is 156 00:07:29,840 --> 00:07:34,220 if you measured the isotopic ratio of water deuterium 157 00:07:34,220 --> 00:07:35,480 and hydrogen in the atmosphere 158 00:07:35,480 --> 00:07:37,930 that it can actually tell you something about the history 159 00:07:37,930 --> 00:07:43,040 of water throughout on Mars, throughout the history of Mars. 160 00:07:43,040 --> 00:07:44,820 >> Pat: Not just in that location on Mars. 161 00:07:44,820 --> 00:07:46,370 >> Dr. Archer: Yeah because you're looking at the atmosphere 162 00:07:46,370 --> 00:07:48,300 and the atmosphere is you know pretty well mixed, 163 00:07:48,300 --> 00:07:51,010 it can tell you something about Mars as a whole 164 00:07:51,010 --> 00:07:52,980 over very long time periods. 165 00:07:52,980 --> 00:07:54,410 >> Pat: Help clarify for those of us 166 00:07:54,410 --> 00:07:57,570 who did really poorly in science. 167 00:07:57,570 --> 00:07:59,840 When you talk about organic molecules are you talking 168 00:07:59,840 --> 00:08:04,040 about molecules from things that are alive or once were alive? 169 00:08:04,040 --> 00:08:07,800 >> Dr. Archer: Yeah so again MSL isn't a life detection mission 170 00:08:07,800 --> 00:08:09,870 so it's not going to be able to answer the question 171 00:08:09,870 --> 00:08:12,860 about whether these things were ever alive or not, 172 00:08:12,860 --> 00:08:16,110 but organic molecules are the chemical building blocks 173 00:08:16,110 --> 00:08:18,920 of life, they're things like amino acids and sugars, 174 00:08:18,920 --> 00:08:22,390 things that are absolutely necessary to life as we know it. 175 00:08:22,390 --> 00:08:26,280 However, there are also non-biological processes 176 00:08:26,280 --> 00:08:29,630 that can produce these organic molecules so just 177 00:08:29,630 --> 00:08:32,830 because you detect an organic molecule that doesn't mean 178 00:08:32,830 --> 00:08:36,720 that there was necessarily life so what MSL is going 179 00:08:36,720 --> 00:08:39,950 to do again is detecting these organics we can say ah that's an 180 00:08:39,950 --> 00:08:43,410 habitable environment and that's going to help us to know 181 00:08:43,410 --> 00:08:45,310 where to look for life in the future. 182 00:08:45,310 --> 00:08:48,530 >> Pat: Habitable whether or not it was habitated. 183 00:08:48,530 --> 00:08:49,980 >> Dr. Archer: Right inhabited, yes, yes. 184 00:08:49,980 --> 00:08:51,680 >> Pat: Thank you very much. 185 00:08:51,680 --> 00:08:53,950 We often talk about life as we know it. 186 00:08:53,950 --> 00:08:57,170 Is it possible that there is life there but it is 187 00:08:57,170 --> 00:08:59,080 so different than what we know 188 00:08:59,080 --> 00:09:01,770 that we don't recognize the evidence of it? 189 00:09:01,770 --> 00:09:04,340 >> Dr. Archer: Yeah so this is something that comes 190 00:09:04,340 --> 00:09:08,270 up in the astrobiology community all the time you know how do you 191 00:09:08,270 --> 00:09:10,900 look for something that you don't know what you're looking 192 00:09:10,900 --> 00:09:14,750 for so the approach that we take is say you know right now it's 193 00:09:14,750 --> 00:09:18,610 hard enough to detect life as we know it let's start there 194 00:09:18,610 --> 00:09:23,940 but certainly it's possible that Mars or life could surprise us 195 00:09:23,940 --> 00:09:27,010 and we're always open to that possibility 196 00:09:27,010 --> 00:09:30,060 but we'll see what Mars gives us. 197 00:09:30,060 --> 00:09:32,620 >> Pat: The notes indicate that the SAM work some 198 00:09:32,620 --> 00:09:35,040 of the work that's being done here in Houston has to do 199 00:09:35,040 --> 00:09:37,650 with volatile bearing minerals. 200 00:09:37,650 --> 00:09:40,180 Tell me what those are what would 201 00:09:40,180 --> 00:09:41,730 that tell you if you found that? 202 00:09:41,730 --> 00:09:44,090 >> Dr. Archer: So a volatile bearing mineral is something 203 00:09:44,090 --> 00:09:48,850 like a carbonate or a sulfate or a phyllosilicate, or a clay 204 00:09:48,850 --> 00:09:50,680 and those are important because they are minerals 205 00:09:50,680 --> 00:09:53,580 that are produced when other rocks or minerals are broken 206 00:09:53,580 --> 00:09:56,580 down and they generally imply the presence of water 207 00:09:56,580 --> 00:09:58,470 so carbonate, for example, 208 00:09:58,470 --> 00:10:02,340 will form when you have carbon dioxide reacting with atoms 209 00:10:02,340 --> 00:10:05,620 of calcium or magnesium, for example, from another rock 210 00:10:05,620 --> 00:10:07,880 and again it implies the presence of water 211 00:10:07,880 --> 00:10:11,720 and it requires a certain water chemistry so that's important 212 00:10:11,720 --> 00:10:14,480 because just by looking at a rock if you measure 213 00:10:14,480 --> 00:10:16,650 if you detect a carbonate you can say something 214 00:10:16,650 --> 00:10:19,010 about how much water was there when it formed. 215 00:10:19,010 --> 00:10:21,990 What the chemistry of that water might have been it tells you 216 00:10:21,990 --> 00:10:24,090 something about how much CO2 might have been 217 00:10:24,090 --> 00:10:26,060 in the atmosphere, which has important implications 218 00:10:26,060 --> 00:10:28,820 for climate, so you can learn all of those things 219 00:10:28,820 --> 00:10:34,330 about the history of that rock, or the history of the site just 220 00:10:34,330 --> 00:10:36,250 by looking at a rock it's pretty incredible. 221 00:10:36,250 --> 00:10:37,690 >> Pat: And SAM has the instruments 222 00:10:37,690 --> 00:10:40,120 that is able to do all of those. 223 00:10:40,120 --> 00:10:43,140 >> Dr. Archer: Yes in concert with other instruments on MSL, 224 00:10:43,140 --> 00:10:45,820 it really is an integrated science package 225 00:10:45,820 --> 00:10:49,390 or science payload that by themselves the instruments are 226 00:10:49,390 --> 00:10:52,390 pretty incredible but together you can tell a very complete 227 00:10:52,390 --> 00:10:54,660 story of the landing site. 228 00:10:54,660 --> 00:10:56,890 >> Pat: I mentioned earlier that this mission is managed 229 00:10:56,890 --> 00:11:00,470 at the Jet Propulsion Laboratory are you going to be able to go 230 00:11:00,470 --> 00:11:02,420 out there for part of the mission or do you do all 231 00:11:02,420 --> 00:11:03,870 of your work here in Houston? 232 00:11:03,870 --> 00:11:05,670 >> Dr. Archer: So for the first 90 days a lot 233 00:11:05,670 --> 00:11:08,780 of the science team is going to be co-located at JPL 234 00:11:08,780 --> 00:11:09,850 and I will be out there 235 00:11:09,850 --> 00:11:12,780 for about 4 weeks of the first 90 days. 236 00:11:12,780 --> 00:11:17,480 After that, the science team which goes home goes back 237 00:11:17,480 --> 00:11:19,030 to their home institutions, 238 00:11:19,030 --> 00:11:22,660 which is located throughout the country and even internationally 239 00:11:22,660 --> 00:11:24,910 and so the rest of the mission and the prime mission is 240 00:11:24,910 --> 00:11:27,190 for two years, we'll be done 241 00:11:27,190 --> 00:11:28,950 with the science team being remote 242 00:11:28,950 --> 00:11:31,780 but those first 90 days a lot of the science team will be 243 00:11:31,780 --> 00:11:34,570 out at JPL working on Mars time together. 244 00:11:34,570 --> 00:11:38,620 >> Pat: What will you be doing while you're there? 245 00:11:38,620 --> 00:11:41,490 >> Dr. Archer: We plan every day we plan what the rover is going 246 00:11:41,490 --> 00:11:45,020 to do the next day so you come in the morning 247 00:11:45,020 --> 00:11:47,840 and your shift starts essentially right before you get 248 00:11:47,840 --> 00:11:50,290 data from the rover, everything that it did the day before 249 00:11:50,290 --> 00:11:53,600 so you come in and you brush up on ok what were we supposed 250 00:11:53,600 --> 00:11:56,510 to have done today and then the rover said hey here's what I 251 00:11:56,510 --> 00:11:59,860 did, you look at all that data and then you talk as a team 252 00:11:59,860 --> 00:12:02,330 and say ok what are we going to do tomorrow 253 00:12:02,330 --> 00:12:04,640 and so you spend two shifts 254 00:12:04,640 --> 00:12:08,980 over about 16 hours building a product that you're going 255 00:12:08,980 --> 00:12:12,130 to send to the space craft that tells it what to do what 256 00:12:12,130 --> 00:12:14,250 to do tomorrow and then you just you know repeat 257 00:12:14,250 --> 00:12:16,050 that for two years. 258 00:12:16,050 --> 00:12:18,490 >> Pat: Because of the distance between the two planets, 259 00:12:18,490 --> 00:12:20,920 you've got quite a lag in communications does 260 00:12:20,920 --> 00:12:25,090 that remove any flexibility you have about what 261 00:12:25,090 --> 00:12:28,170 to tell your instruments or your rover to do? 262 00:12:28,170 --> 00:12:31,950 >> Dr. Archer: Well that's right because of the light time delay 263 00:12:31,950 --> 00:12:33,090 and the complexity 264 00:12:33,090 --> 00:12:35,350 of the instruments you don't really have the flexibility 265 00:12:35,350 --> 00:12:39,630 to make changes in real time, you plan things a day at a time 266 00:12:39,630 --> 00:12:42,810 but landing is a really good example of that. 267 00:12:42,810 --> 00:12:46,060 So from the time that MSL hits the top of the atmosphere 268 00:12:46,060 --> 00:12:48,530 to the time that it lands safely on the surface 269 00:12:48,530 --> 00:12:53,410 of Mars is 7 minutes, now the light time delay between earth 270 00:12:53,410 --> 00:12:56,360 and mars right now so the time that it takes a signal traveling 271 00:12:56,360 --> 00:13:00,450 at the speed of light to go from Mars to the earth is 14 minutes 272 00:13:00,450 --> 00:13:03,470 so what that means is when we get our first indication 273 00:13:03,470 --> 00:13:07,110 that we've touched the top of the atmosphere here on earth, 274 00:13:07,110 --> 00:13:09,900 in reality the space craft has already been on the surface 275 00:13:09,900 --> 00:13:13,630 of Mars for 7 minutes so really you're kind of looking 276 00:13:13,630 --> 00:13:16,190 at a tape delay of events, you don't have the opportunity 277 00:13:16,190 --> 00:13:20,190 to respond to things in real time and then again the way 278 00:13:20,190 --> 00:13:23,890 that that plays out during operations is that we do most 279 00:13:23,890 --> 00:13:27,480 of our communications via the orbiters around Mars right now, 280 00:13:27,480 --> 00:13:30,510 which only communicate with the lander a few times a day 281 00:13:30,510 --> 00:13:33,570 so we have to uplink a product once a day 282 00:13:33,570 --> 00:13:35,810 and we say here's what you're going to do for every minute 283 00:13:35,810 --> 00:13:38,900 of this day coming up and then it goes out and tries 284 00:13:38,900 --> 00:13:41,680 to do its best to follow our instructions. 285 00:13:41,680 --> 00:13:44,370 If we did a good job everything will go as planned 286 00:13:44,370 --> 00:13:48,190 and the next morning when we come in we find 287 00:13:48,190 --> 00:13:50,030 out how we did and we go from there. 288 00:13:50,030 --> 00:13:51,870 >> Pat: And found out if there were any issues 289 00:13:51,870 --> 00:13:54,720 that it encountered while it was trying to execute the plan 290 00:13:54,720 --> 00:13:55,130 >> Dr. Archer: Yes 291 00:13:55,130 --> 00:13:58,840 >> Pat: and then do something about it the next day. 292 00:13:58,840 --> 00:14:00,590 >> Dr. Archer: That's right. 293 00:14:00,590 --> 00:14:03,720 >> Pat: Based on what you guys all know already and the things 294 00:14:03,720 --> 00:14:07,010 that your team's investigating, what are your hypotheses 295 00:14:07,010 --> 00:14:11,630 about the habitability of Mars? 296 00:14:11,630 --> 00:14:14,320 >> Dr. Archer: Well you know I think based 297 00:14:14,320 --> 00:14:18,290 on what we know right now, there's kind of some positives 298 00:14:18,290 --> 00:14:22,330 and negatives about possible habitability of Mars 299 00:14:22,330 --> 00:14:25,090 that we have some missions that for example we've seen a lot 300 00:14:25,090 --> 00:14:28,230 of evidence for water on Mars either in the past 301 00:14:28,230 --> 00:14:31,580 or even continuing up today from the water rise 302 00:14:31,580 --> 00:14:33,770 that the Phoenix lander has found 303 00:14:33,770 --> 00:14:37,440 or the evidence the abundance evidence of past water 304 00:14:37,440 --> 00:14:39,290 that the Mur rovers have found and a lot 305 00:14:39,290 --> 00:14:42,780 of orbital measurements that have indicated the past activity 306 00:14:42,780 --> 00:14:47,030 of water and possibly continuing up to present day so that makes 307 00:14:47,030 --> 00:14:49,400 that encourages you about the possibilities for life 308 00:14:49,400 --> 00:14:52,420 because water is very important, it's absolutely necessary 309 00:14:52,420 --> 00:14:54,250 to life as we know it but then 310 00:14:54,250 --> 00:14:57,680 on the other hand the Viking mission showed us the Viking 311 00:14:57,680 --> 00:15:00,610 actually did carry life detection instruments with it 312 00:15:00,610 --> 00:15:02,890 and didn't find anything so it shows us 313 00:15:02,890 --> 00:15:05,090 that the surface can also be a pretty hostile place, 314 00:15:05,090 --> 00:15:08,420 it's a harsh UV environment, you have ionizing radiation, 315 00:15:08,420 --> 00:15:10,690 chemical oxidants that can destroy life 316 00:15:10,690 --> 00:15:15,490 so it can be a harsh place but interestingly enough it's a lot 317 00:15:15,490 --> 00:15:17,000 of the things that we've learned about life 318 00:15:17,000 --> 00:15:20,920 on earth have informed out knowledge of the possibility 319 00:15:20,920 --> 00:15:23,810 for life on Mars and life on earth is really ubiquitous, 320 00:15:23,810 --> 00:15:28,500 it's anywhere you go, it's you know an extremely acidic 321 00:15:28,500 --> 00:15:32,000 or salty environments, deep undersea, deep underground 322 00:15:32,000 --> 00:15:34,910 in solid rock and so right now there's nothing 323 00:15:34,910 --> 00:15:37,770 about there's nothing about what we know about life, 324 00:15:37,770 --> 00:15:40,380 which has proven itself to be very adaptable and nothing 325 00:15:40,380 --> 00:15:42,590 that we know about Mars that tells you 326 00:15:42,590 --> 00:15:44,270 that you can't have life there. 327 00:15:44,270 --> 00:15:46,680 You just have to know where to look and that's the question 328 00:15:46,680 --> 00:15:48,470 that MSL is going to answer. 329 00:15:48,470 --> 00:15:50,650 >> Pat: It's all very exciting, looking forward to it. 330 00:15:50,650 --> 00:15:51,770 Thanks very much Doug. 331 00:15:51,770 --> 00:15:53,650 Dr. Doug Archer is a member