WEBVTT FILE 1 00:00:00.080 --> 00:00:04.080 >>INTERVIEWER: Last November, NASA launched a new mission to Mars to investigate the mystery of how it 2 00:00:04.100 --> 00:00:08.280 became the red planet, and how it may have looked in the past. Now that mission 3 00:00:08.300 --> 00:00:12.290 is about to arrive, and here to join us from NASA's Goddard Space Flight Center in 4 00:00:12.310 --> 00:00:16.310 Greenbelt, Maryland is NASA Goddard Chief Scientist Dr. Jim Garvin. Thank you 5 00:00:16.330 --> 00:00:20.350 for joining us. >>JIM: Thanks for having me. >>INTERVIEWER: After nearly a year-long journey 6 00:00:20.370 --> 00:00:24.360 MAVEN is finally arriving at Mars. Tell us about the MAVEN mission entering Mars' 7 00:00:24.380 --> 00:00:28.380 atmosphere. >>INTERVIEWER: So MAVEN is an orbiting remote 8 00:00:28.400 --> 00:00:32.400 sensing mission that will study how Mars' atmosphere, the 9 00:00:32.420 --> 00:00:36.420 cold atmosphere of today, interacts with space weather, loses parts of 10 00:00:36.440 --> 00:00:40.470 itself to space, and connect that Mars of today to the Mars of the 11 00:00:40.490 --> 00:00:44.560 past, when we believe the atmosphere and conditions on Mars were warmer and 12 00:00:44.580 --> 00:00:48.570 wetter, more hospitable for life. So MAVEN is a time machine, 13 00:00:48.590 --> 00:00:52.610 to put the Mars of today into the context of the Mars of the past, and ask, "How did 14 00:00:52.630 --> 00:00:56.650 it evolve?" Why is it the way it is today, why is it the red planet, not the 15 00:00:56.670 --> 00:01:00.670 blue planet? >>INTERVIEWER: What will MAVEN do as it orbits Mars? 16 00:01:00.690 --> 00:01:04.710 >>JIM: So MAVEN's carrying a rich array of instruments that will allow us to 17 00:01:04.730 --> 00:01:08.760 measure for the first time how the atmosphere of Mars interacts with 18 00:01:08.780 --> 00:01:12.780 deep space, with the space weather particles from the Sun. 19 00:01:12.800 --> 00:01:16.820 It also carries instruments that will actually sample the chemistry of the 20 00:01:16.840 --> 00:01:20.830 atmosphere as it's being lossed to space, and connect that chemistry to the 21 00:01:20.850 --> 00:01:24.860 Mars chemistry of the past that we're measuring on the surface of Mars from rovers like 22 00:01:24.880 --> 00:01:28.890 Curiosity. >>INTERVIEWER: What else is NASA doing to better understand 23 00:01:28.910 --> 00:01:32.910 Mars, and what are our plans for the future? >>JIM: So right now, NASA has a rich array 24 00:01:32.930 --> 00:01:36.970 of robotic missions exploring the red planet. We're on the surface 25 00:01:36.990 --> 00:01:41.090 with two rovers, Curiosity and Opportunity. We have orbital 26 00:01:41.110 --> 00:01:45.100 constellation measuring Mars from the Mars Reconnaissance Orbiter, 27 00:01:45.120 --> 00:01:49.140 Mars Odyssey, and soon MAVEN. And we're planning new missions. A new rover mission 28 00:01:49.160 --> 00:01:53.190 that will extend what Curiosity's doing to a new place, with new instruments 29 00:01:53.210 --> 00:01:57.200 to actually capture pieces of Mars for return to Earth some day. 30 00:01:57.220 --> 00:02:01.250 All of these missions ask the question - Are there signs of 31 00:02:01.270 --> 00:02:05.300 past life recorded in the history of Mars? Its atmosphere, its rocks, 32 00:02:05.320 --> 00:02:09.310 its ices. Can we tell, could we ever tell? And to open the 33 00:02:09.330 --> 00:02:13.340 Martian frontier to the possibility of humans going there to explore 34 00:02:13.360 --> 00:02:17.390 our neighborly, brotherly planet. 35 00:02:17.410 --> 00:02:21.410 >>INTERVIEWER: How does studying the red planet's evolution help us understand the formation of other planets, 36 00:02:21.430 --> 00:02:25.450 including Earth? >>JIM: Well Mars is a canonical small rocky planet, 37 00:02:25.470 --> 00:02:29.500 in our very interesting little solar system. But, 38 00:02:29.520 --> 00:02:33.520 in the bigger scheme of things, we're discovering dozens if not hundreds of planets 39 00:02:33.540 --> 00:02:37.610 around nearby stars. Exoplanets. These planets we think 40 00:02:37.630 --> 00:02:41.690 have climates with atmospheres and histories as well. By understanding 41 00:02:41.710 --> 00:02:45.720 the difference between Mars and its evolution to its state of today, 42 00:02:45.740 --> 00:02:49.740 the cold, dry, red planet, from its Mars of the past, perhaps a wet 43 00:02:49.760 --> 00:02:53.750 blueish planet like Earth, we'll be able to understand these other worlds 44 00:02:53.770 --> 00:02:57.760 that we're discovering, and also put our solar system into the bigger context 45 00:02:57.780 --> 00:03:01.810 of this universe. It's out there beckoning, calling to us. 46 00:03:01.830 --> 00:03:05.820 >>INTERVIEWER: Sounds good, where can we learn more? >>JIM: Well you can 47 00:03:05.840 --> 00:03:09.850 go to NASA's website, www.NASA.gov/MAVEN, 48 00:03:09.870 --> 00:03:13.860 for the MAVEN mission, which will put MAVEN in context to our bigger 49 00:03:13.880 --> 00:03:17.880 journey to Mars. >>INTERVIEWER: Great, thanks so much for joining us. >>JIM: Thanks for having me. 50 00:03:17.900 --> 00:03:21.940 [beep beep... beep beep... beep beep...] 51 00:03:21.960 --> 00:03:26.010 [beep beep... beep beep... beep beep...] 52 00:03:26.030 --> 00:03:30.040 53 00:03:30.060 --> 00:03:32.326