1 00:00:00,030 --> 00:00:03,130 [ Music ] 2 00:00:03,150 --> 00:00:06,380 I'm Conor Nixon, I'm a planetary scientist at NASA's Goddard Space Flight Center, 3 00:00:06,400 --> 00:00:09,780 and I study the atmospheric composition of the outer planets. 4 00:00:09,800 --> 00:00:13,980 Titan is Saturn's largest moon, it's actually the second-largest moon in the solar system, 5 00:00:14,000 --> 00:00:17,880 and it's the only moon in the solar system that has a large and substantial atmosphere, 6 00:00:17,900 --> 00:00:24,560 and that atmosphere in some respects is really similar to that of the Earth, being composed mainly of nitrogen, but in other respects it's really different. 7 00:00:24,580 --> 00:00:29,900 It has methane as the second-most abundant gas, and that takes the same role as water vapor in the Earth's atmosphere. 8 00:00:29,920 --> 00:00:34,120 It evaporates from the surface, it forms clouds, and then rains down again 9 00:00:34,140 --> 00:00:40,980 and in fact forms lakes that we see at Titan's north pole, including ethane and propane and all sorts of complex chemicals. 10 00:00:41,000 --> 00:00:48,370 We also see these vast dune fields at the equator, which are not made of silicates as they are on the Earth but actually made of organic substances, 11 00:00:48,390 --> 00:00:52,060 essentially plastics which have actually sedimented from the atmosphere 12 00:00:52,080 --> 00:00:58,880 and are being blown around into dune fields the same as we'd see on a desert on the Earth. 13 00:00:58,900 --> 00:01:03,510 Back in 1980 when Voyager 1 flew by Titan and made the first close encounter with that moon, 14 00:01:03,530 --> 00:01:08,280 it discovered many new chemical species in the atmosphere, and a lot of these are what we call hydrocarbons, 15 00:01:08,300 --> 00:01:14,890 which are composed of two types of atom, carbon and hydrogen. And these are derived from methane after the methane is broken apart by sunlight 16 00:01:14,910 --> 00:01:21,260 it forms into longer and longer chain molecules. So you can add first two carbons together to make a family of molecules, 17 00:01:21,280 --> 00:01:27,050 and you can also form three carbons together to form a heavier family of molecules. 18 00:01:27,070 --> 00:01:33,020 So it was actually very mysterious that Voyager only discovered the heaviest and the lightest members of the three carbon family, 19 00:01:33,040 --> 00:01:38,610 but it didn't find the middle member of the family, propylene, that was missing. 20 00:01:38,630 --> 00:01:43,600 So NASA has this wonderful flagship spacecraft called Cassini which is currently orbiting Saturn, 21 00:01:43,620 --> 00:01:50,730 and it's making multiple close flybys of Titan. Now in visible light, Titan appears quite bland and featureless just like an orange globe, 22 00:01:50,750 --> 00:01:55,580 but Cassini has techniques to peer through that haze, including the Composite Infrared Spectrometer or CIRS, 23 00:01:55,600 --> 00:02:00,900 which can look at the heat coming from the atmosphere and split it apart into its different frequencies, 24 00:02:00,920 --> 00:02:06,660 and this forms a characteristic pattern of peaks, which give the characteristic signatures of different molecules. 25 00:02:06,680 --> 00:02:13,060 And through this we can detect which molecules are in the atmosphere, and we see all the molecules that were previously discovered by Voyager. 26 00:02:13,080 --> 00:02:19,110 But we're also able to look for new molecules, and in fact, buried within the signatures of these more abundant molecular species 27 00:02:19,130 --> 00:02:24,260 we saw a very small spike which was due to a new species which had not been seen before, 28 00:02:24,280 --> 00:02:29,060 and in fact this was propylene, and we saw it at multiple altitudes in Titan's atmosphere. 29 00:02:29,080 --> 00:02:34,300 When we added all the signal together, we had more than 99% confidence that we were discovering a new molecule. 30 00:02:34,320 --> 00:02:38,630 [ Music, wind blowing ] 31 00:02:38,650 --> 00:02:42,690 So this object I have right here, this is polypropylene. 32 00:02:42,710 --> 00:02:48,730 This is a plastic that we use on the Earth in everyday household objects such as this plastic tub here, 33 00:02:48,750 --> 00:02:54,910 and if we turn it over on the bottom, we find a symbol with the number 5 that says PP, polypropylene. 34 00:02:54,930 --> 00:03:00,880 This is the propylene that we found on Titan, but polymerized, that means that the molecule is formed into long chains, 35 00:03:00,900 --> 00:03:06,080 and when these chains are tangled together it forms a hard, clear plastic that we use in many household objects. 36 00:03:06,100 --> 00:03:13,280 So that was really fun for me to realize that something that we'd discovered in space was in fact something that I was touching every day on the Earth. 37 00:03:13,300 --> 00:03:16,360 So the discovery of propylene on Titan is really exciting. 38 00:03:16,380 --> 00:03:23,310 First of all, it completes this chemical family where we had this missing link dating thirty-two years back to Voyager, 39 00:03:23,330 --> 00:03:27,680 but also, it shows that there's much more there still in Titan's atmosphere to be discovered. 40 00:03:27,700 --> 00:03:34,740 Some people think that Titan is similar to the prebiotic Earth long ago, when the molecules were forming the basis of life. 41 00:03:34,760 --> 00:03:40,580 And we don't know what we're going to find on Titan if we send back further spacecraft with new instruments, more sensitive instruments, 42 00:03:40,600 --> 00:03:46,240 if some of the molecules on Titan could be similar to the basis of life on Earth. 43 00:03:46,260 --> 00:03:57,251 [ Music, satellite beeping ]