1 00:00:00,190 --> 00:00:04,210 Reporter: Hubble's newest and final Frontier Field image 2 00:00:04,210 --> 00:00:07,220 shows us just how vast and crowded our universe is 3 00:00:07,220 --> 00:00:10,410 when it looked at just a tiny portion of the sky. 4 00:00:10,410 --> 00:00:13,610 So what is a galaxy and what kind of super power did Hubble use to 5 00:00:13,610 --> 00:00:15,620 capture this new image? 6 00:00:15,620 --> 00:00:18,810 We are joined by Jim Jeletic at NASA's 7 00:00:18,810 --> 00:00:21,830 Goddard Space Flight Center who's going to show us this new view. 8 00:00:21,830 --> 00:00:22,860 Thanks for joining us. 9 00:00:22,860 --> 00:00:23,880 Jim: Thanks for having me. 10 00:00:23,880 --> 00:00:26,080 Reporter: So start by telling us, what is a galaxy 11 00:00:26,080 --> 00:00:29,150 and can you show us what Hubble has seen? 12 00:00:29,150 --> 00:00:32,160 Jim: Sure, well galaxies are these flat plates 13 00:00:32,160 --> 00:00:35,170 that have lots of stars, like billions, sometimes trillions 14 00:00:35,170 --> 00:00:38,290 of stars, gas, and dust and they're all kind of circling 15 00:00:38,290 --> 00:00:39,290 around a central point. 16 00:00:39,290 --> 00:00:41,310 And this 27th anniversary image shows you 17 00:00:41,310 --> 00:00:43,330 two spiral galaxies, one edge on 18 00:00:43,330 --> 00:00:45,380 on the left and one on the right. 19 00:00:45,380 --> 00:00:47,400 The one on the right, which is the most face on would 20 00:00:47,400 --> 00:00:49,590 take you 450,000 years to get from 21 00:00:49,590 --> 00:00:49,610 one side to the other. 22 00:00:49,610 --> 00:00:51,730 one side to the other, if you were traveling 23 00:00:51,730 --> 00:00:52,840 at the speed of light. 24 00:00:52,840 --> 00:00:55,870 The speed of light is 186,000 miles per second. 25 00:00:55,870 --> 00:00:58,910 So that's why this image of just a small portion of 26 00:00:58,910 --> 00:01:00,920 the sky is so incredible. 27 00:01:00,920 --> 00:01:02,930 Look at all the galaxies there and 28 00:01:02,930 --> 00:01:04,940 think about how big these things are. 29 00:01:04,940 --> 00:01:06,960 You see all kinds, you see the spiral galaxies 30 00:01:06,960 --> 00:01:09,140 like we saw before, you see those elliptical galaxies 31 00:01:09,140 --> 00:01:11,260 which are those yellowish ones 32 00:01:11,260 --> 00:01:13,280 that have older 33 00:01:13,280 --> 00:01:15,290 stars in it. 34 00:01:15,290 --> 00:01:17,500 And you even see galaxies collitions. 35 00:01:17,500 --> 00:01:19,580 So it's incredible you can get so many galaxies in one 36 00:01:19,580 --> 00:01:21,600 part of the sky and infact no matter 37 00:01:21,600 --> 00:01:23,620 which direction you look in the sky 38 00:01:23,620 --> 00:01:25,810 your going to see the same thing 39 00:01:25,810 --> 00:01:27,880 which means there's probably about 2 trillion galaxies 40 00:01:27,880 --> 00:01:30,060 in the universe or about as many 41 00:01:30,060 --> 00:01:32,070 galaxies in the universe as there are fish in the sea. 42 00:01:32,070 --> 00:01:35,080 So there are a lot of galaxies that need guarding. 43 00:01:35,080 --> 00:01:38,090 Reporter: What superpower did Hubble use 44 00:01:38,090 --> 00:01:41,290 to see these faint and distance galaxies 45 00:01:41,290 --> 00:01:42,500 in the new image? 46 00:01:42,500 --> 00:01:44,720 Jim: Well mother nature provides a 47 00:01:44,720 --> 00:01:48,950 common magnifying glass capability 48 00:01:48,950 --> 00:01:51,140 and it uses something called gravitational lensing. 49 00:01:51,140 --> 00:01:53,150 Where if you put an object 50 00:01:53,150 --> 00:01:55,180 of heavy mass and sprinkle in some dark matter 51 00:01:55,180 --> 00:01:57,190 it will bend and warp space 52 00:01:57,190 --> 00:01:59,210 in such that the light will be magnified 53 00:01:59,210 --> 00:02:01,390 and brightened and warped around 54 00:02:01,390 --> 00:02:03,580 that big object so you can see it. 55 00:02:03,580 --> 00:02:05,600 So in this case here that 56 00:02:05,600 --> 00:02:07,610 dragon type thing you see in the center of the screen 57 00:02:07,610 --> 00:02:09,630 that's actually 5 images 58 00:02:09,630 --> 00:02:11,640 of the same galaxy mirrored 59 00:02:11,640 --> 00:02:13,670 right next to each other. 60 00:02:13,670 --> 00:02:15,690 And then in this other case we're going to see 61 00:02:15,690 --> 00:02:17,710 these really really small 62 00:02:17,710 --> 00:02:19,730 faint red galaxies 63 00:02:19,730 --> 00:02:21,750 that who's light it took 64 00:02:21,750 --> 00:02:27,940 600 million years that it was born. 65 00:02:27,940 --> 00:02:30,000 So we wouldn't be able to see 66 00:02:30,000 --> 00:02:33,010 this without this gravitational lens capability. 67 00:02:33,010 --> 00:02:36,010 So it really provides us new capability where by Hubble 68 00:02:36,010 --> 00:02:39,030 can look into the magnifying glass of nature 69 00:02:39,030 --> 00:02:42,040 and see even further into space then we would have been see otherwise. 70 00:02:42,040 --> 00:02:45,220 Reporter: Now you mention dark matter 71 00:02:45,220 --> 00:02:48,400 that sounds like something a villain might use. 72 00:02:48,400 --> 00:02:50,410 How do missions like Hubble help us learn about 73 00:02:50,410 --> 00:02:52,420 one of natures biggest secrets? 74 00:02:52,420 --> 00:02:54,430 Jim: Well dark matter is this really exoctic stuff 75 00:02:54,430 --> 00:02:56,440 and we don't know what it is 76 00:02:56,440 --> 00:02:58,450 we can't see it because it doesn't give out 77 00:02:58,450 --> 00:03:00,480 any light but it takes over 80% 78 00:03:00,480 --> 00:03:02,490 of all the matter in the universe 79 00:03:02,490 --> 00:03:04,510 What we can do is we can see effects that it has 80 00:03:04,510 --> 00:03:06,570 do to its gravity and we can map those 81 00:03:06,570 --> 00:03:08,590 effects and that's what you're seeing here with the blue 82 00:03:08,590 --> 00:03:10,780 we're mapping where we believe the dark matter is 83 00:03:10,780 --> 00:03:12,800 by how it distorts 84 00:03:12,800 --> 00:03:14,810 the light from background galaxies 85 00:03:14,810 --> 00:03:16,820 but we also then can take a look at 86 00:03:16,820 --> 00:03:18,840 galaxies themselves because 87 00:03:18,840 --> 00:03:20,860 dark matter is the glue that holds 88 00:03:20,860 --> 00:03:22,870 galaxies together 89 00:03:22,870 --> 00:03:24,880 and makes them spin the way they do 90 00:03:24,880 --> 00:03:26,990 so if we study galaxies as well 91 00:03:26,990 --> 00:03:29,010 hopefully we can learn a little bit more about 92 00:03:29,010 --> 00:03:31,020 this dark matter and maybe someday even figure out 93 00:03:31,020 --> 00:03:33,110 how we can detect it directly as opposed 94 00:03:33,110 --> 00:03:36,120 to just by seeing it by its gravitational pull on other things. 95 00:03:36,120 --> 00:03:39,150 Reporter: Now Hubble just celebrated 96 00:03:39,150 --> 00:03:42,160 its 27th birthday, what's next for the 97 00:03:42,160 --> 00:03:45,180 famous space telescope? 98 00:03:45,180 --> 00:03:48,240 Jim: Well Hubble is at the peak of its scientific capability 99 00:03:48,240 --> 00:03:50,430 and still has redundancy in all its critical systems 100 00:03:50,430 --> 00:03:52,440 so we're really hopeful we can get it 101 00:03:52,440 --> 00:03:54,620 to continue to make ground breaking observations 102 00:03:54,620 --> 00:03:56,640 well into the next decade and that's 103 00:03:56,640 --> 00:03:58,820 due to all of the servicing missions 104 00:03:58,820 --> 00:04:01,040 and where the astronauts went up and they 105 00:04:01,040 --> 00:04:03,060 worked on Hubble upgrading it and repair it. 106 00:04:03,060 --> 00:04:05,230 But what we are really excited about is 107 00:04:05,230 --> 00:04:07,250 the James Webb Space Telescope 108 00:04:07,250 --> 00:04:09,260 and James Webb is going to see 109 00:04:09,260 --> 00:04:11,440 the infered light, much further into the infered 110 00:04:11,440 --> 00:04:13,460 part of the spectrum so 111 00:04:13,460 --> 00:04:15,490 if you think looking at a visible light like the Sombrero galaxy 112 00:04:15,490 --> 00:04:17,490 here the picture that Hubble took 113 00:04:17,490 --> 00:04:19,500 it will be able to take a look at 114 00:04:19,500 --> 00:04:21,520 infered light so we can see 115 00:04:21,520 --> 00:04:23,710 these different objects in different 116 00:04:23,710 --> 00:04:25,720 wavelengths and it tells us a lot more information 117 00:04:25,720 --> 00:04:27,750 about it. So we're really excited 118 00:04:27,750 --> 00:04:30,750 James Webb and it's due to launch at the end of 2018. 119 00:04:30,750 --> 00:04:33,770 Reporter: Where can we see more of Hubble's 120 00:04:33,770 --> 00:04:36,780 beautiful images like the new one you just released? 121 00:04:36,780 --> 00:04:39,810 Jim: Well if you want images, if you want videos 122 00:04:39,810 --> 00:04:41,830 if you want to see what are the biggest discoveries 123 00:04:41,830 --> 00:04:43,840 Hubble's ever made, if you want to learn about 124 00:04:43,840 --> 00:04:45,850 the telescope, you go to nasa.gov/hubble 125 00:04:45,850 --> 00:04:47,860 or you can follow us on Twitter 126 00:04:47,860 --> 00:04:49,860 @nasahubble 127 00:04:49,860 --> 00:04:50,203