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