WEBVTT FILE 1 00:00:01.070 --> 00:00:01.620 music 2 00:00:01.640 --> 00:00:03.740 I built my first AM radio with my dad 3 00:00:03.760 --> 00:00:05.900 full-on, really sodering and building. 4 00:00:05.920 --> 00:00:09.700 I built, you know, missile rockets, and we launched those. 5 00:00:09.720 --> 00:00:11.310 And we had telescopes. 6 00:00:11.330 --> 00:00:13.520 And he was the first to show me Mars. 7 00:00:13.540 --> 00:00:16.040 And I slowly got into the space program that way. 8 00:00:16.059 --> 00:00:21.509 I knew in high school that I wanted to be an astronomer. 9 00:00:21.530 --> 00:00:23.820 You can discover and find out what's going on. 10 00:00:23.840 --> 00:00:27.830 Depending on what you are studying. For me, it's Titan's atmosphere. Name's Carrie Ander and I'm a space scientist 11 00:00:27.850 --> 00:00:31.860 at NASA's Goddard Space Flight Center, and I'm a team member on 12 00:00:31.880 --> 00:00:36.010 Cassini CIRS. CIRS is called the composit infrared spectrometer, and it's one of the 13 00:00:36.030 --> 00:00:40.040 tweleve instruments on board the Cassini spacecraft, which is orbiting Satern. 14 00:00:40.060 --> 00:00:44.050 What CIRS does is it goes beyond the human visible 15 00:00:44.070 --> 00:00:48.070 spectrum part, that we see with our eyes, into the thermal infrared, what I'll call it. 16 00:00:48.090 --> 00:00:52.320 So imagine sitting in front of fire, and you 17 00:00:52.340 --> 00:00:56.520 are not looking at it, but you're feeling the fire, the heat from the fire. 18 00:00:56.540 --> 00:01:00.560 CIRS sees that heat and records it. And then we can tell what 19 00:01:00.580 --> 00:01:04.610 is going on: there's this molecule, this molecule, this type of maybe particulate, a cloud. 20 00:01:04.629 --> 00:01:08.630 to try to figure out "Ok, what could that be?" And that's what we're 21 00:01:08.650 --> 00:01:12.640 doing to to find out the types of clouds that we see 22 00:01:12.660 --> 00:01:16.660 with CIRS. But if you just kind of look at Titan from a big picture point of view, first of all 23 00:01:16.680 --> 00:01:20.720 it's a moon, and it orbits Satern. It's Satern's largest moon. 24 00:01:20.740 --> 00:01:24.770 And it's the second largest moon in our solar system, next to Jupiter's Ganymede. 25 00:01:24.790 --> 00:01:28.780 But what's really intriguing about Titan is that it is the only moon in our solar system 26 00:01:28.800 --> 00:01:32.789 with a thick, substantial planet-like atmosphere 27 00:01:32.810 --> 00:01:36.990 On Earth, in our troposphere, you know, when you look up and you see clouds 28 00:01:37.010 --> 00:01:41.030 those are all made of liquid water, ice 29 00:01:41.050 --> 00:01:45.090 crystals or a combination of the two. Well, Titan doesn't have that. 30 00:01:45.110 --> 00:01:49.130 It has methane instead. So you'd see all this 31 00:01:49.150 --> 00:01:53.150 methane rain, methane drizzle, methane clouds, all that. 32 00:01:53.170 --> 00:01:57.160 There's a lot of early Earth scientists out there who want to learn about, you know, life 33 00:01:57.180 --> 00:02:01.190 "Is there life?" You can go to Titan as one possibility, 34 00:02:01.210 --> 00:02:05.289 because it can be representative what the early Earth was like before 35 00:02:05.310 --> 00:02:09.300 we were here. It's a completely different environment than 36 00:02:09.320 --> 00:02:13.340 Earth, but it has a lot of similarities at the same time. It's a very dynamic 37 00:02:13.360 --> 00:02:17.380 world. In studying it, you can do any kind of photochemistry, 38 00:02:17.400 --> 00:02:21.580 different chemistry, different physics. 39 00:02:21.600 --> 00:02:25.620 I was always interested in math and science, but my dad, I think, was a key role. 40 00:02:25.640 --> 00:02:30.880 I wanted to keep doing it and learning, and I'm here. Dream come true! 41 00:02:30.900 --> 00:02:34.890 beeping 42 00:02:34.910 --> 00:02:45.079