WEBVTT FILE 1 00:00:00.020 --> 00:00:03.100 2 00:00:03.120 --> 00:00:06.290 3 00:00:06.310 --> 00:00:09.360 4 00:00:09.380 --> 00:00:12.390 5 00:00:12.410 --> 00:00:14.510 To me, Volcanism is important to study 6 00:00:14.530 --> 00:00:17.700 because it is one of the most common and fundamental geologic 7 00:00:17.720 --> 00:00:19.890 processes that occurs in our solar system. 8 00:00:19.910 --> 00:00:21.930 It's a window into 9 00:00:21.950 --> 00:00:24.110 the history of our own planet, 10 00:00:24.130 --> 00:00:25.120 of the moon, 11 00:00:25.140 --> 00:00:27.880 and the other planets and moons in our solar system. 12 00:00:27.900 --> 00:00:32.090 My name is Brent Garry, and I am a Geologist at NASA Goddard Space Flight Center. 13 00:00:32.110 --> 00:00:34.130 I specialize in planetary volcanology, 14 00:00:34.150 --> 00:00:38.270 so it's my job to study the evolution of volcanoes and lava flows 15 00:00:38.290 --> 00:00:42.410 in our solar system – primarily on the Earth, the Moon, and Mars. 16 00:00:42.430 --> 00:00:47.590 What we're trying to answer is: How did these volcanoes evolve over time? 17 00:00:47.610 --> 00:00:48.700 When did they erupt? 18 00:00:48.720 --> 00:00:52.810 And kind of, what went on during the eruption process itself? 19 00:00:52.830 --> 00:00:54.910 When we get images back 20 00:00:54.930 --> 00:00:59.960 from the moon of these long, meandering depressions, called Sinuous Rilles, 21 00:00:59.980 --> 00:01:04.010 that look like rivers here on Earth – you know, we want to understand: 22 00:01:04.030 --> 00:01:06.220 Are these the remnants of collapsed lava tubes? 23 00:01:06.240 --> 00:01:12.380 Did the lava carve its way into the surface of the moon to leave these giant channels? 24 00:01:12.400 --> 00:01:14.570 Or in the case of Mars, the debate is whether or not 25 00:01:14.590 --> 00:01:23.400 these were carved by water, or fluvial activity, or if they were carved by lava flows, or volcanic activity. 26 00:01:23.420 --> 00:01:25.550 One of the best ways to answer these questions is by 27 00:01:25.570 --> 00:01:29.590 comparing the information and data we get back from the Moon and Mars to 28 00:01:29.610 --> 00:01:31.750 geologic features that we have right here on Earth. 29 00:01:31.770 --> 00:01:35.900 One of the exciting parts of my job is I get to travel around the world. 30 00:01:35.920 --> 00:01:39.980 I get to go to New Mexico, Hawaii, even Iceland to do my research. 31 00:01:40.000 --> 00:01:43.160 I love this part of my job because I get to I hike up volcanoes all day, 32 00:01:43.180 --> 00:01:46.270 we're hiking around desolate, you know, fields of lava, 33 00:01:46.290 --> 00:01:49.450 we're taking helicopter rides over these flow fields, 34 00:01:49.470 --> 00:01:52.530 we're looking at active lava flows that are going on, 35 00:01:52.550 --> 00:01:56.760 and even collecting samples of these features to study. 36 00:01:56.780 --> 00:02:01.050 "Taadaa! Don't try this at home kids." 37 00:02:01.070 --> 00:02:04.260 Our field team uses a wide range of instruments to do our work. 38 00:02:04.280 --> 00:02:07.360 We use things like a Differential GPS, 39 00:02:07.380 --> 00:02:10.550 which gives us the topography of the lava flows. 40 00:02:10.570 --> 00:02:12.740 We use a Ground-penetrating radar, 41 00:02:12.760 --> 00:02:16.920 which allows us to see in the subsurface of the flow field. 42 00:02:16.940 --> 00:02:18.930 And we also use a thermal imaging camera 43 00:02:18.950 --> 00:02:23.430 which allows us to see the differences in temperature across an active lava flow. 44 00:02:23.450 --> 00:02:27.430 A lot of people might think that studying geology is just looking at boring rocks all day. 45 00:02:27.450 --> 00:02:31.780 But my job here at NASA proves that geology is an adventure. 46 00:02:31.800 --> 00:02:32.810 It takes you around the world 47 00:02:32.830 --> 00:02:36.840 and also to the surfaces of other planets and moons in our solar system. 48 00:02:36.860 --> 00:02:47.281