WEBVTT FILE 1 00:00:00.030 --> 00:00:04.050 (music) 2 00:00:04.050 --> 00:00:08.100 (music) 3 00:00:08.100 --> 00:00:12.290 (music) 4 00:00:12.290 --> 00:00:16.310 Telescopes generally come into two different flavors. You have really powerful big 5 00:00:16.310 --> 00:00:20.370 telescopes, but those telescopes see a tiny part of the sky or 6 00:00:20.370 --> 00:00:24.390 telescopes are smaller and so they lack that power but they can see big 7 00:00:24.390 --> 00:00:28.430 parts of the sky. WFIRST is the best of both worlds. WFIRST 8 00:00:28.430 --> 00:00:32.440 is the Wide Field Infrared Survey Telescope. What I think of WFIRST is doing 9 00:00:32.440 --> 00:00:36.490 is building on what where the two great successes astronomically 10 00:00:36.490 --> 00:00:40.490 of the 1990's in the last decade, that is the Sloan Digital Sky Survey 11 00:00:40.490 --> 00:00:44.660 and the Hubble Space Telescope. WFIRST is a NASA observatory 12 00:00:44.660 --> 00:00:48.670 that has the top ranking of the National Academy of Sciences 13 00:00:48.670 --> 00:00:52.690 to launch in the twenty twenties. It has the same image precision 14 00:00:52.690 --> 00:00:56.700 and power as the Hubble Space Telescope but with one-hundred 15 00:00:56.700 --> 00:01:00.890 times the area of sky that is used. Looking at a large fraction of the sky 16 00:01:00.890 --> 00:01:04.900 allows you to get a more complete accounting. For example the stars in the Large Megellanic 17 00:01:04.900 --> 00:01:08.900 Cloud, which is the nearest galaxy to us or the stars in the galactic bulge; 18 00:01:08.900 --> 00:01:12.920 so you can do a much more complete accounting in a much shorter amount of time. 19 00:01:12.920 --> 00:01:17.120 The particular thing I'm interested in using WFIRST for, 20 00:01:17.120 --> 00:01:21.280 is to actually do a statistical census of planetary systems in 21 00:01:21.280 --> 00:01:25.280 our galaxy. And what we're looking for is gravitational microlensing events, these are 22 00:01:25.280 --> 00:01:29.470 cases when another start passes in front of our line of sight to a background star 23 00:01:29.470 --> 00:01:33.480 and it makes that background star get a little bit brighter due to the gravity of that 24 00:01:33.480 --> 00:01:37.490 foreground star, and that allows us to find planets. What WFIRST 25 00:01:37.490 --> 00:01:41.540 will do is it will have what we call a coronagraph. A coronagraph lets us 26 00:01:41.540 --> 00:01:45.550 image and characterize really dim planets, 27 00:01:45.550 --> 00:01:49.570 next to very bright stars. No matter how good a telescope 28 00:01:49.570 --> 00:01:53.580 that you build, its always going to have some residual errors. This is going to be the 29 00:01:53.580 --> 00:01:57.590 first time that we're going to fly an instrument that contains these high format deformable 30 00:01:57.590 --> 00:02:01.600 mirrors, that are going to let us correct for errors in a telescope, that's never 31 00:02:01.600 --> 00:02:05.610 been done in space before. WFIRST will allow us 32 00:02:05.610 --> 00:02:09.620 to potentially make groundbreaking discoveries in finding 33 00:02:09.620 --> 00:02:13.810 out what dark energy is. So this will tell us 34 00:02:13.810 --> 00:02:17.820 if dark energy is an unknown form of energy or if its a modification 35 00:02:17.820 --> 00:02:22.000 of general relativity. Single WFIRST images will contain 36 00:02:22.000 --> 00:02:26.120 over a million galaxies and we can't categorize 37 00:02:26.120 --> 00:02:30.130 and catalog those galaxies ourselves. Citizen science allows 38 00:02:30.130 --> 00:02:34.140 interested people in the general public to solve scientific problems 39 00:02:34.140 --> 00:02:38.150 and so one of the things that I'm really excited about is enabling this bridge 40 00:02:38.150 --> 00:02:42.330 where the general public can get involved in doing actual 41 00:02:42.330 --> 00:02:46.390 science. For me, its really an exciting opportunity to play 42 00:02:46.390 --> 00:02:50.440 a significant role in a mission that I think will be 43 00:02:50.440 --> 00:02:54.450 one of the most powerful telescopes that we have in the twenty twenties; 44 00:02:54.450 --> 00:02:58.460 and will be some of the most important things our country does in space in that 45 00:02:58.460 --> 00:03:02.650 time frame. 46 00:03:02.650 --> 00:03:06.670 (beeping) 47 00:03:06.670 --> 00:03:10.680 (beeping) 48 00:03:10.680 --> 00:03:14.680 (beeping) 49 00:03:14.680 --> 00:03:16.580