1 00:00:01,000 --> 00:00:03,500 By scrutinising the Hubble Ultra Deep Field, 2 00:00:03,500 --> 00:00:06,000 the deepest image of the sky ever made, 3 00:00:06,000 --> 00:00:08,500 the NASA / ESA Hubble Space Telescope 4 00:00:08,500 --> 00:00:10,500 and the NASA Spitzer Space Telescope 5 00:00:10,500 --> 00:00:13,500 have joined forces to discover nine of the smallest, 6 00:00:13,500 --> 00:00:16,000 faintest, most compact galaxies 7 00:00:16,000 --> 00:00:18,000 ever observed in the distant Universe. 8 00:00:37,500 --> 00:00:39,500 This is the Hubblecast. 9 00:00:39,500 --> 00:00:43,500 News and images from the NASA / ESA Hubble Space Telescope. 10 00:00:43,500 --> 00:00:47,000 Travelling through time and space with our host, Dr. J 11 00:00:47,000 --> 00:00:50,000 EPISODE 8: A step closer to our origin... a.k.a. Dr. Joe Liske. 12 00:00:50,000 --> 00:00:52,000 Hello and welcome to the Hubblecast. 13 00:00:52,500 --> 00:00:55,000 One of the mos fundamental questions that we all ask, 14 00:00:55,000 --> 00:00:57,500 astronomers and laypersons alike, 15 00:00:57,500 --> 00:01:00,000 is: where do we come from? 16 00:01:00,500 --> 00:01:04,000 We, the Earth, the Sun and the rest of the Solar System 17 00:01:04,500 --> 00:01:06,500 are all part of the Milky Way galaxy, 18 00:01:06,500 --> 00:01:09,500 and so the question of our origin is closely linked 19 00:01:09,500 --> 00:01:12,000 to the birth and evolution of galaxies. 20 00:01:12,500 --> 00:01:15,000 Now, the Spitzer and Hubble Space Telescopes 21 00:01:15,000 --> 00:01:18,500 have joined forces to discover nine of the faintest, 22 00:01:18,500 --> 00:01:21,000 youngest and most compact galaxies 23 00:01:21,000 --> 00:01:23,500 ever observed in the distant Universe. 24 00:01:24,500 --> 00:01:26,500 Conventional theories of galaxy evolution 25 00:01:26,500 --> 00:01:29,500 predict that small galaxies in the early Universe 26 00:01:29,500 --> 00:01:32,000 evolved into the massive galaxies of today 27 00:01:32,000 --> 00:01:34,000 by merging together. 28 00:01:34,500 --> 00:01:37,500 The newly found young galaxies offer important new insights 29 00:01:37,500 --> 00:01:40,000 into the Universe's formative period, 30 00:01:40,000 --> 00:01:42,500 just 1 billion years after the Big Bang. 31 00:01:42,500 --> 00:01:45,000 Hubble has detected sapphire blue stars 32 00:01:45,000 --> 00:01:48,000 residing within the nine pristine galaxies. 33 00:01:49,500 --> 00:01:52,500 Although they are glowing with the light of millions of stars, 34 00:01:52,500 --> 00:01:54,500 each of the newly discovered galaxies 35 00:01:54,500 --> 00:01:57,500 is actually a hundred to a thousand times fainter 36 00:01:57,500 --> 00:01:59,500 than our own Milky Way. 37 00:02:00,500 --> 00:02:03,000 Now, usually smaller things in space 38 00:02:03,000 --> 00:02:06,500 tend to be less interesting to astronomers than the larger ones, 39 00:02:06,500 --> 00:02:09,500 but in this case it's the opposite. 40 00:02:09,000 --> 00:02:12,500 Three of the new galaxies appear to be slightly disrupted. 41 00:02:13,000 --> 00:02:15,500 Instead of being shaped like rounded blobs, 42 00:02:15,500 --> 00:02:19,000 they appear to be stretched into tadpole-like shapes. 43 00:02:19,500 --> 00:02:22,000 This is a sign that they may be interacting 44 00:02:22,000 --> 00:02:24,000 and merging with neighbouring galaxies 45 00:02:24,000 --> 00:02:26,500 to form larger, cohesive structures, 46 00:02:26,500 --> 00:02:29,000 just as predicted by theory. 47 00:02:29,500 --> 00:02:33,000 The galaxies were observed in the Hubble Ultra Deep Field 48 00:02:33,000 --> 00:02:36,000 with Hubble's Advanced Camera for Surveys 49 00:02:36,000 --> 00:02:39,000 and the Near Infrared and Multi-Object Spectrometer 50 00:02:39,000 --> 00:02:41,500 as well as Spitzer's Infrared Array Camera 51 00:02:41,500 --> 00:02:43,500 and the European Southern Observatory's 52 00:02:43,500 --> 00:02:46,500 Infrared Spectrometer and Array Camera. 53 00:02:48,500 --> 00:02:51,000 In today's Hubblecast we have a special guest, 54 00:02:51,000 --> 00:02:54,500 Dr. Martin Kümmel, from the European Hubble group in Munich. 55 00:02:54,500 --> 00:02:57,000 - Welcome Martin - Hello Dr, J 56 00:02:57,000 --> 00:02:59,000 You and your colleagues are responsible 57 00:02:59,000 --> 00:03:01,500 for the particular instrument mode on Hubble 58 00:03:01,000 --> 00:03:03,000 that was used by the scientists. 59 00:03:03,000 --> 00:03:05,000 Can you tell us a little bit about that? 60 00:03:05,500 --> 00:03:06,500 The so called Grism mode 61 00:03:06,500 --> 00:03:08,500 in the Advanced Camera for Surveys 62 00:03:08,500 --> 00:03:11,500 spreads the different colours emitted by the galaxies 63 00:03:11,500 --> 00:03:13,500 into short "trails". 64 00:03:13,500 --> 00:03:16,000 This is an example of such a grism. 65 00:03:16,000 --> 00:03:19,000 One can see the rainbow colors as the light is spread out. 66 00:03:19,500 --> 00:03:21,500 So how was that used by the scientists? 67 00:03:22,500 --> 00:03:25,000 Well, the analysis of these short trails 68 00:03:25,000 --> 00:03:28,500 allows the detection of emission from glowing hydrogen gas, 69 00:03:28,500 --> 00:03:31,500 giving the distance as well as an estimate 70 00:03:31,500 --> 00:03:34,000 of the rate at which stars are formed. 71 00:03:34,500 --> 00:03:37,000 But could that not be done in a different way? 72 00:03:37,500 --> 00:03:40,000 Finding and analysing these small and faint galaxies 73 00:03:40,000 --> 00:03:42,500 at such great distances is at the very limit 74 00:03:42,500 --> 00:03:46,000 of the capabilities of the most powerful telescopes. 75 00:03:46,000 --> 00:03:48,500 The grisms on board Hubble are the only instruments 76 00:03:48,500 --> 00:03:50,500 that can make this kind of discovery. 77 00:03:52,500 --> 00:03:54,500 By finding these nine tiny 78 00:03:54,500 --> 00:04:00,500 and exceedingly faint galaxy building blocks 79 00:03:57,500 --> 00:04:00,000 we followed another branch of our galactic family tree 80 00:04:00,500 --> 00:04:03,000 and moved a small but important step closer 81 00:04:03,000 --> 00:04:05,000 to understanding our cosmic roots. 82 00:04:05,500 --> 00:04:08,500 We already know about the existence of much more massive 83 00:04:08,500 --> 00:04:11,000 and therefore considerably brighter galaxies 84 00:04:11,000 --> 00:04:13,000 at similarly great distances. 85 00:04:13,000 --> 00:04:16,500 How these monsters were assembled so quickly after the Big Bang 86 00:04:16,500 --> 00:04:19,000 remains a real puzzle for astronomers. 87 00:04:19,000 --> 00:04:21,500 But that's a story for another day... 88 00:04:22,500 --> 00:04:25,000 With these small galaxy building blocks 89 00:04:25,000 --> 00:04:28,000 we are basically witnessing galaxy formation in action. 90 00:04:28,000 --> 00:04:31,000 Something that is important if we want to understand 91 00:04:31,000 --> 00:04:33,000 our origin on the cosmic scale. 92 00:04:33,500 --> 00:04:36,500 This is Dr. J signing off for the Hubblecast. 93 00:04:36,500 --> 00:04:40,500 Once again, nature has surprised us beyond our wildest imagination... 94 00:04:42,000 --> 00:04:44,000 Hubblecast is produced by ESA / Hubble 95 00:04:44,000 --> 00:04:46,000 at the European Southern Observatory in Germany. 96 00:04:47,500 --> 00:04:49,500 The Hubble mission is a project of international cooperation 97 00:04:49,500 --> 00:04:51,000 between NASA and the European Space Agency.