WEBVTT FILE 1 00:00:11.120 --> 00:00:15.089 My name is Lynn Carter I'm a research space scientist, and I work with the 2 00:00:15.089 --> 00:00:19.320 Planetary Geodynamics group here at Goddard. I study the geology of planetary 3 00:00:19.320 --> 00:00:23.220 surfaces: the Earth, Moon, Mars, Venus. There's a lot of things you can learn 4 00:00:23.220 --> 00:00:26.340 about the Earth by studying other planets. For example on the Earth we have 5 00:00:26.340 --> 00:00:30.090 a lot of erosive processes. You know, rains, it washes parts of the surface 6 00:00:30.090 --> 00:00:32.640 away, we have plate tectonics, which recycles 7 00:00:32.640 --> 00:00:36.930 the crust. But on other planets those processes don't necessarily occur. So, for 8 00:00:36.930 --> 00:00:40.260 example, when we look at the Moon we're seeing a surface that's much older. We 9 00:00:40.260 --> 00:00:44.129 can use impact cratering on the Moon, to sort of understand how many impacts happen, 10 00:00:44.129 --> 00:00:46.829 the size of the objects that we're hitting each other in the early solar 11 00:00:46.829 --> 00:00:51.629 system. Generally what I would do every day is a variety of things. Like I might 12 00:00:51.629 --> 00:00:55.680 come in and do some image analysis, and then do some writing about our 13 00:00:55.680 --> 00:00:59.579 scientific results. Sometimes I do fieldwork in Hawaii or Arizona. We take a 14 00:00:59.579 --> 00:01:02.719 ground-penetrating radar out and we learn more about lava flows on the Earth. 15 00:01:02.719 --> 00:01:07.140 One of my favorite things is to use radar remote sensing. For example, on Mars 16 00:01:07.140 --> 00:01:11.220 we can use radars to sound all the way to the bottom of Mars' polar caps and see 17 00:01:11.220 --> 00:01:13.680 all of this layering within the polar caps. And on the 18 00:01:13.680 --> 00:01:17.940 Moon we're using it to study impact cratering. Sometimes when an impact 19 00:01:17.940 --> 00:01:21.750 craters form a huge sheet of melt is thrown out. This melted rock flows across 20 00:01:21.750 --> 00:01:26.040 the surface, but then over time it's covered over by stuff from other impacts. 21 00:01:26.040 --> 00:01:28.979 But with the radar it just blows right through all of that and you can see this 22 00:01:28.979 --> 00:01:33.150 beautiful image of the melt flow coming out of the crater. Looking ahead to the 23 00:01:33.150 --> 00:01:35.910 future there are so many different things that we can learn about planetary 24 00:01:35.910 --> 00:01:39.030 science that would be interesting. One of my favorites is Venus, actually, because 25 00:01:39.030 --> 00:01:42.420 it's about the same size and it's very close to the Earth in the solar system. 26 00:01:42.420 --> 00:01:45.960 Why has there been this divergent evolution between these two worlds that 27 00:01:45.960 --> 00:01:48.990 are very similar? And I think understanding that problem would be very 28 00:01:48.990 --> 00:01:51.560 interesting. 29 00:01:51.560 --> 00:01:53.560 Music 30 00:01:53.560 --> 00:02:00.160 Beep, Beep, Beep