WEBVTT FILE 1 00:00:00.000 --> 00:00:05.380 (music) 2 00:00:05.380 --> 00:00:11.400 (Mikulski) Over here is the picture taken after the servicing mission and this is what the 3 00:00:11.400 --> 00:00:21.260 new 1994 Wide Field Planetary picture will show us. The pictures are remarkable. 4 00:00:21.260 --> 00:00:27.980 The science that will come from the pictures are of historical significance. 5 00:00:27.980 --> 00:00:32.510 (Postman) Just from seeing that one picture, you knew that this was going to be a 6 00:00:32.510 --> 00:00:35.320 revolutionary telescope. 7 00:00:35.320 --> 00:00:38.640 (music) 8 00:00:38.680 --> 00:00:42.440 (Heckman) Using Hubble to study the evolution of galaxies, we 9 00:00:42.440 --> 00:00:47.540 exploit the fact that telescope in astronomy acts like a time machine. When 10 00:00:47.549 --> 00:00:51.000 we look at the most distant objects in the universe with Hubble, we're actually 11 00:00:51.000 --> 00:00:55.860 looking far back into time. The light has taken something like 10 to 12 billion 12 00:00:55.860 --> 00:00:59.440 years to reach us when we look at the most distant galaxies. 13 00:00:59.440 --> 00:01:07.280 (Postman) Hubble's ability to provide very crisp images, far crisper and cleaner and clearer than any 14 00:01:07.280 --> 00:01:12.920 other telescope, allows you to see what these things look like. They're not just 15 00:01:12.920 --> 00:01:15.360 fuzzy blobs of light. 16 00:01:15.360 --> 00:01:17.180 (music) 17 00:01:17.180 --> 00:01:21.200 (Ferguson) What we're trying to do is piece together the history of galaxy evolution, 18 00:01:21.200 --> 00:01:26.360 from the very very earliest galaxies that we can see, which we now we're 19 00:01:26.360 --> 00:01:31.920 getting within about a billion years of the Big Bang all the way to to the present. 20 00:01:31.920 --> 00:01:36.540 (Postman) The other thing that Hubble allowed us to do is get very precise 21 00:01:36.540 --> 00:01:42.810 measurements of the colors of these galaxies and those colors tell us about 22 00:01:42.810 --> 00:01:48.240 the kind of stars that are in the galaxies and how old those stars are. 23 00:01:48.240 --> 00:01:52.640 (music) 24 00:01:52.640 --> 00:01:57.270 (Ferguson) There there - is sort of two different ways of thinking about a redshift: 25 00:01:57.270 --> 00:01:59.680 There's the Doppler effect. 26 00:01:59.680 --> 00:02:15.000 (music) 27 00:02:15.000 --> 00:02:21.440 So objects that are moving toward you if that were happening in light the light 28 00:02:21.440 --> 00:02:24.620 would be shifted to the blue, if it's moving away from you it would be shifted to the 29 00:02:24.620 --> 00:02:30.230 red. In cosmology, there's another aspect, the whole universe is expanding and 30 00:02:30.230 --> 00:02:34.340 that's essentially stretching the light on its way from from the distant object 31 00:02:34.340 --> 00:02:39.230 to us, and that really allows you to determine where in the universe the 32 00:02:39.230 --> 00:02:43.080 objects you're seeing are because you're measuring essentially that stretching factor. 33 00:02:43.120 --> 00:02:47.840 (Heckman) It's not like we're gonna invent a better toothpaste or solve the energy 34 00:02:47.840 --> 00:02:52.240 crisis, we're doing things that are at the sort of frontiers of knowledge. 35 00:02:52.240 --> 00:02:57.880 (Postman) One of the great things about being able to study this history of galaxies is it not 36 00:02:57.890 --> 00:03:03.350 only tells us about what the cosmic history of formation of stars and 37 00:03:03.350 --> 00:03:09.740 galaxies is, but it also can tell us stuff about our own galaxy's past and 38 00:03:09.740 --> 00:03:12.400 its potential future as well. 39 00:03:12.400 --> 00:03:17.260 (Heckman) I think people just have a powerful urge to understand their origins. 40 00:03:17.260 --> 00:03:19.560 (music) 41 00:03:19.560 --> 00:03:21.380 (Ferguson) How did we get here? 42 00:03:21.380 --> 00:03:25.790 You know. What was the, what was before the Earth? What was before the Sun? 43 00:03:25.790 --> 00:03:30.830 Those kinds of simple questions that are startlingly hard to answer and the 44 00:03:30.830 --> 00:03:35.470 amazing thing is that we can start to answer many of them. 45 00:03:35.470 --> 00:03:38.860 (music)