1 00:00:02,000 --> 00:00:04,999 3.2 billion light years from Earth, 2 00:00:05,000 --> 00:00:07,999 a group of astronomers has captured live with Hubble 3 00:00:08,000 --> 00:00:10,999 something they never thought they would get to see. 4 00:00:25,000 --> 00:00:26,999 This is the Hubblecast. 5 00:00:27,000 --> 00:00:30,999 News and images from the NASA / ESA Hubble Space Telescope. 6 00:00:31,000 --> 00:00:34,999 Travelling through time and space with our host, Dr. J 7 00:00:35,000 --> 00:00:36,999 EPISODE 1: The Comet Galaxy 8 00:00:38,000 --> 00:00:40,999 There are many galaxies of different shapes and sizes 9 00:00:41,000 --> 00:00:42,999 in the universe around us today. 10 00:00:43,000 --> 00:00:46,999 Roughly half are gas poor, elliptical shaped galaxies 11 00:00:47,000 --> 00:00:48,999 with few new stars forming today. 12 00:00:49,000 --> 00:00:53,999 Whereas the other half are gas rich, spiral and irregular shaped galaxies 13 00:00:54,000 --> 00:00:56,999 with lots of new star formation activity. 14 00:00:57,000 --> 00:01:00,999 Now, observations have shown that the gas poor galaxies 15 00:01:01,000 --> 00:01:04,999 are often found near the centers of rich galaxy clusters, 16 00:01:05,000 --> 00:01:08,999 whereas the spirals spend most of their life in solitude. 17 00:01:09,000 --> 00:01:12,999 However, observations of the deep and very far away universe 18 00:01:13,000 --> 00:01:17,999 have also shown that when universe was roughly half of its present age 19 00:01:18,000 --> 00:01:22,999 things were very different. Back then, only about 1 in 10 galaxies 20 00:01:23,000 --> 00:01:25,999 was a gas poor one. So the question is: 21 00:01:26,000 --> 00:01:29,999 where did all today's gas poor galaxies come from? 22 00:01:30,000 --> 00:01:33,999 Apparently, there must has been some kind of transformation process. 23 00:01:34,000 --> 00:01:37,999 But because galaxy evolution takes place over billions of years 24 00:01:38,000 --> 00:01:41,999 astronomers have so far not been able to see it live. 25 00:01:43,000 --> 00:01:45,999 New observations with Hubble by an international team 26 00:01:46,000 --> 00:01:49,999 led by Luca Cortese of Cardiff University, United Kingdom, 27 00:01:50,000 --> 00:01:53,999 provide one of the best examples today to this metamorphosis. 28 00:01:57,000 --> 00:01:59,999 Well, we were looking at the Abell Cluster 2667 29 00:02:00,000 --> 00:02:04,999 and we realized that this galaxy was falling into the cluster center 30 00:02:05,000 --> 00:02:08,999 at a velocity of approximately 2.5 million kilometers per hour. 31 00:02:10,000 --> 00:02:12,999 Abell 2667's enormous gravitational field 32 00:02:13,000 --> 00:02:15,999 is generated by the combined contribution 33 00:02:16,000 --> 00:02:19,999 of the cluster's dark matter, hot gas and hundreds of galaxies. 34 00:02:22,000 --> 00:02:24,999 As the galaxy plunges through the cluster 35 00:02:25,000 --> 00:02:26,999 its gas and stars are been stripped away 36 00:02:27,000 --> 00:02:29,999 by the hot plasma in the cluster, which can reach temperatures 37 00:02:30,000 --> 00:02:32,999 as high as 10 to 100 million degrees. 38 00:02:34,500 --> 00:02:37,499 Also contributing to this destructive process 39 00:02:37,500 --> 00:02:39,999 are the tidal forces exerted by the cluster. 40 00:02:40,000 --> 00:02:42,999 This are just like the tidal forces of the Moon and Sun, 41 00:02:43,000 --> 00:02:45,999 which push and pull the Earth's oceans. 42 00:02:47,000 --> 00:02:49,000 Birth processes, the tidal forces 43 00:02:49,000 --> 00:02:51,999 and the aptly named "ram pressure stripping" 44 00:02:52,000 --> 00:02:54,999 resulting from the action of the hot cluster gas 45 00:02:55,000 --> 00:02:57,999 resemble those affecting comets in our Solar System. 46 00:02:58,000 --> 00:03:02,999 For this reason, scientists have nicknamed this peculiar spiral 47 00:03:03,000 --> 00:03:04,999 with its tail, the "Comet Galaxy". 48 00:03:06,000 --> 00:03:09,999 We see a unique galaxy that has been transformed by the fact 49 00:03:10,000 --> 00:03:11,999 it's falling towards the cluster center. 50 00:03:12,000 --> 00:03:16,999 And what it is exactly, it's a kind of a spiral galaxy with lots of gas. 51 00:03:18,000 --> 00:03:21,999 And we see a trail of stars, of blue forming stars. 52 00:03:22,000 --> 00:03:28,999 And also around those stars some kind of wispy gas 53 00:03:29,000 --> 00:03:31,999 stripped away by the fall. 54 00:03:32,000 --> 00:03:35,999 Furthermore, millions of now homeless stars have been snatched away 55 00:03:36,000 --> 00:03:38,999 from their mother galaxy, which will lead it to age prematurely. 56 00:03:42,000 --> 00:03:45,999 Even though its mass is slightly larger than that of the Milky Way, 57 00:03:46,000 --> 00:03:49,999 the spiral will inevitably lose all its gas and dust and hence 58 00:03:50,000 --> 00:03:54,999 his chance of generating new stars later. So, it'll probably become 59 00:03:55,000 --> 00:03:57,999 a gas poor galaxy left with an old population of red stars. 60 00:03:58,000 --> 00:04:00,999 However, in the midst of all this destruction, 61 00:04:01,000 --> 00:04:02,999 the cluster strong tidal forces 62 00:04:03,000 --> 00:04:05,999 have triggered a baby-boom of star formation. 63 00:04:07,000 --> 00:04:09,999 Hubble's sharp eyes have caught other spectacular effects 64 00:04:10,000 --> 00:04:12,999 of Abell 2667's immense mass. 65 00:04:13,000 --> 00:04:15,999 The giant bluish arc seen just off-center 66 00:04:16,000 --> 00:04:19,999 is the magnified and distorted image of a distant background galaxy 67 00:04:20,000 --> 00:04:23,999 seen through the gravitational lens formed by the tremendous 68 00:04:24,000 --> 00:04:25,999 mass concentration of the cluster. 69 00:04:26,000 --> 00:04:29,999 At the cluster's center, another rare feature can be seen: 70 00:04:30,000 --> 00:04:32,999 the vivid blue light from millions of stars 71 00:04:33,000 --> 00:04:34,999 created in a so called cooling flow. 72 00:04:35,000 --> 00:04:38,999 Some of the hot cluster gas is cooling in a filamentary structure 73 00:04:39,000 --> 00:04:41,999 as it falls into the cluster's core, setting off the birth 74 00:04:42,000 --> 00:04:45,999 of lots of bright blue stars outshining their environment. 75 00:04:46,000 --> 00:04:48,999 This may be the clearest picture of this phenomenon yet. 76 00:04:51,000 --> 00:04:54,999 By combining the visible, infrared and x-rays views 77 00:04:55,000 --> 00:04:59,999 from Hubble, Spitzer, Chandra, the VLT and Keck 78 00:05:00,000 --> 00:05:03,999 we can see that this discovery adds a new brush-stroke 79 00:05:04,000 --> 00:05:06,999 to a painting were galaxies are being slowly shaped 80 00:05:07,000 --> 00:05:10,999 by their violent interactions with the cluster environment. 81 00:05:11,000 --> 00:05:13,999 Although there are many discoveries still to come 82 00:05:14,000 --> 00:05:18,999 the emerging elements shed new light on the painting's mysterious nature 83 00:05:19,000 --> 00:05:21,999 and are revealing some of its hidden wonders. 84 00:05:23,000 --> 00:05:25,999 This is Dr. J signing off for the Hubblecast 85 00:05:27,000 --> 00:05:30,999 Once again, nature has surprised us beyond our wildest imagination... 86 00:05:33,000 --> 00:05:34,999 Hubblecast is produced by ESA / Hubble 87 00:05:35,000 --> 00:05:37,000 at the European Southern Observatory in Germany. 88 00:05:37,001 --> 00:05:40,000 The Hubble mission is a project of international cooperation 89 00:05:40,001 --> 00:05:42,001 between NASA and the European Space Agency.