WEBVTT FILE 1 00:00:00.100 --> 00:00:04.200 [off camera] Well if you looked at the night's sky through a soda straw what would you 2 00:00:04.220 --> 00:00:08.310 see. Turns out quite a lot using the Hubble Space Telescope. 3 00:00:08.330 --> 00:00:12.490 Hubble's newest and final frontier field image shows us how 4 00:00:12.510 --> 00:00:16.560 vast and crowded our universe is when it looked at just a tiny 5 00:00:16.580 --> 00:00:20.680 portion of the sky. So what exactly is a galaxy 6 00:00:20.700 --> 00:00:24.790 and what superpower did Hubble use to capture this new image. We're joined 7 00:00:24.810 --> 00:00:28.970 by Dr. Padi Boyd at NASA's Goddard Space Flight Center. Thanks for joining us. 8 00:00:28.990 --> 00:00:33.030 [Boyd] My pleasure thanks for having me. [off camera] So start by telling us what is a galaxy 9 00:00:33.050 --> 00:00:37.110 and can you show us what Hubble has seen? 10 00:00:37.130 --> 00:00:41.230 [Boyd] Well a galaxy is a collection of many stars. The Milky Way galaxy, our galaxy 11 00:00:41.250 --> 00:00:45.390 has about a hundred billion or more stars in it. The star is just one of 12 00:00:45.410 --> 00:00:49.440 a hundred billion or million. We live in a beautiful spiral galaxy 13 00:00:49.460 --> 00:00:53.530 That's about a disk shape that has gas and stars 14 00:00:53.550 --> 00:00:57.650 orbiting around the center. And this is a beautiful Hubble image of 15 00:00:57.670 --> 00:01:01.820 two spiral galaxies. One is seen edge on, where we see that dust 16 00:01:01.840 --> 00:01:05.890 and ther one one is seen more face on where we can start to see the structure of the spirals. 17 00:01:05.910 --> 00:01:09.950 Galaxies near us look like that, but when we look at something a very small 18 00:01:09.970 --> 00:01:14.040 region of the sky and we stare at it for hours and hours up to a 19 00:01:14.060 --> 00:01:18.120 100 hours. We start to see galaxies coming out from 20 00:01:18.140 --> 00:01:22.310 very far distances from us. And we're looking at the evolution 21 00:01:22.330 --> 00:01:26.380 of galaxies as a function of time in these frontier fields. 22 00:01:26.400 --> 00:01:30.480 [off camera] Talk about what superpower did Hubble use to see the faint and distant galaxies 23 00:01:30.500 --> 00:01:34.620 in this new image. [Boyd] Well it's nothing more than the superpower 24 00:01:34.640 --> 00:01:38.790 of gravity. We know that mass influences space 25 00:01:38.810 --> 00:01:42.840 time and Einstein's theory of relativity predicted that 26 00:01:42.860 --> 00:01:46.860 mass bends space time and that even light would bend around it. What that 27 00:01:46.880 --> 00:01:51.060 means is that very massive structures can bend 28 00:01:51.080 --> 00:01:55.200 the light from behind it like a funhouse mirror. And in images like 29 00:01:55.220 --> 00:01:59.320 frontier fields, the mass of the foreground galaxy cluster 30 00:01:59.340 --> 00:02:03.440 magnifies the galaxies behind it so that we can start to put 31 00:02:03.460 --> 00:02:07.600 a picture together of those most distant galaxies. We can even use the 32 00:02:07.620 --> 00:02:11.620 mass to magnify galaxies that started, that were forming 33 00:02:11.640 --> 00:02:15.730 in the first 100 million years of the history of the universe 34 00:02:15.750 --> 00:02:19.830 and those little red specks there are what we think are some of the first galaxies 35 00:02:19.850 --> 00:02:23.970 to form. [off camera] Now I understand there's something 36 00:02:23.990 --> 00:02:28.080 called dark matter. That sounds like something a villain would use. How do 37 00:02:28.100 --> 00:02:32.120 missions like Hubble help us learn more about one of nature's biggest secrets? 38 00:02:32.140 --> 00:02:36.210 [Boyd] It is one of nature's biggest secrets because we can't study it by 39 00:02:36.230 --> 00:02:40.320 using traditional methods like looking at the light that it gives off. That's 40 00:02:40.340 --> 00:02:44.470 exactly why we call it dark matter. But even though it's dark to our eyes 41 00:02:44.490 --> 00:02:48.530 it does have mass and you can't get away from the fact that mass does have mass 42 00:02:48.550 --> 00:02:52.570 that impacts it surroundings. It impacts space time. So using an image like 43 00:02:52.590 --> 00:02:56.650 the frontier fields here and how it's distorting the galaxies behind us 44 00:02:56.670 --> 00:03:00.750 behind it, actually allows us to map out the dark 45 00:03:00.770 --> 00:03:04.940 matter. And that dark matter then we can use it as a lens 46 00:03:04.960 --> 00:03:09.000 to look further behind in the universe. We now know that dark matter makes up 47 00:03:09.020 --> 00:03:13.080 80 percent or more of the mass of the universe. 48 00:03:13.100 --> 00:03:17.260 And that's just an amazing fact. Dark matter is in individual galaxies 49 00:03:17.280 --> 00:03:21.340 and impacts the way that the stars move in those galaxies. So we can study 50 00:03:21.360 --> 00:03:25.400 the motions of stars in individual spiral galaxies and get another handle 51 00:03:25.420 --> 00:03:29.490 and a hint about where dark matter is and how it's distributed. 52 00:03:29.510 --> 00:03:33.620 [off camera] Now Hubble just celebrated it's 27th birthday. What 53 00:03:33.640 --> 00:03:37.800 is next for the famous space telescope? [Boyd] So 27 years on 54 00:03:37.820 --> 00:03:41.890 orbit and Hubble is still going strong. And that's because 55 00:03:41.910 --> 00:03:46.000 during it's lifetime astronauts visited the telescope and they outfit it with 56 00:03:46.020 --> 00:03:50.150 new components and new instruments. And the last time astronauts visited 57 00:03:50.170 --> 00:03:54.230 the telescope they really tuned it up. So it's still at the peak of it's scientific capabilities. 58 00:03:54.250 --> 00:03:58.270 And we expect that to continue for years, working very closely 59 00:03:58.290 --> 00:04:02.370 really hard to make sure that Hubble is still operational when we launch the next 60 00:04:02.390 --> 00:04:06.510 big thing. The Webb Space Telescope which will launch in 2018. 61 00:04:06.530 --> 00:04:10.700 Together these two very powerful space telescopes will be able to 62 00:04:10.720 --> 00:04:14.770 look at the universe in slightly different types of light and give us 63 00:04:14.790 --> 00:04:18.870 a broad picture of what's happening in galaxies nearby and even in the distant universe. 64 00:04:18.890 --> 00:04:23.030 [off camera] Where can we learn more and see some 65 00:04:23.050 --> 00:04:27.120 more of Hubble's images? [Boyd] If you go to nasa.gov/hubble or you follow us on 66 00:04:27.140 --> 00:04:31.170 Twitter @NASAHubble you can find all kinds of information 67 00:04:31.190 --> 00:04:35.240 and images we discussed today and many of the other programs that the Hubble Space Telescope 68 00:04:35.260 --> 00:04:39.330 has done from galaxies to objects in our solar system 69 00:04:39.350 --> 00:04:43.450 to stars, star forming nebulas. Check it out and learn more. 70 00:04:43.470 --> 00:04:50.504 [slate]