1 00:00:00,300 --> 00:00:03,304 The Hubble Space Telescope has solved a long-standing puzzle 2 00:00:03,364 --> 00:00:08,239 by resolving giant but delicate filaments shaped by a strong magnetic field 3 00:00:08,273 --> 00:00:11,548 around the active galaxy NGC 1275. 4 00:00:11,583 --> 00:00:14,199 It is the most striking example so far 5 00:00:14,200 --> 00:00:19,230 of the influence of the immense tentacles of extra-galactic magnetic fields. 6 00:00:38,251 --> 00:00:40,092 This is the Hubblecast. 7 00:00:40,093 --> 00:00:43,456 News and images from the NASA / ESA Hubble Space Telescope. 8 00:00:43,457 --> 00:00:46,868 Travelling through time and space with our host, Dr. J 9 00:00:46,922 --> 00:00:50,096 EPISODE 18: Hubble sees magnetic monster in erupting galaxy. a.k.a. Dr. Joe Liske. 10 00:00:50,097 --> 00:00:52,529 Hi and welcome to another episode of the Hubblecast. 11 00:00:52,530 --> 00:00:56,154 Today we are going to interrupt our series of seven Hubblecast specials 12 00:00:56,212 --> 00:00:58,150 to bring you a breaking new story. 13 00:00:59,399 --> 00:01:02,423 Now this doesn't happen very often, but the subject of today's show 14 00:01:02,480 --> 00:01:04,471 is in fact completely invisible. 15 00:01:04,658 --> 00:01:08,673 And no, I'm not talking about dark matter, I'm talking about magnetic fields. 16 00:01:09,334 --> 00:01:11,492 Although most people are completely unaware of them, 17 00:01:11,493 --> 00:01:14,611 magnetic fields in fact surround us all the time. 18 00:01:14,612 --> 00:01:18,973 For starters, the Earth has a magnetic field of course, which any compass will show you. 19 00:01:18,974 --> 00:01:23,506 But power lines, and pretty much any electrical device also produces magnetic fields. 20 00:01:23,507 --> 00:01:26,128 And moreover, they're not just down here on Earth, 21 00:01:26,183 --> 00:01:28,226 they're also sprinkled throughout the Universe. 22 00:01:28,583 --> 00:01:30,318 Take our Sun for example. 23 00:01:30,319 --> 00:01:32,818 Particularly strong magnetic flares from our Sun 24 00:01:32,819 --> 00:01:35,677 can even disrupt radio communication down here on Earth, 25 00:01:35,678 --> 00:01:39,578 including your mobile phone calls and your favourite radio station. 26 00:01:43,773 --> 00:01:49,307 In the direction of the constellation Perseus we find the Perseus cluster of galaxies. 27 00:01:49,465 --> 00:01:55,322 NGC 1275, in its centre, is one of the closest giant elliptical galaxies. 28 00:01:55,370 --> 00:01:59,966 Its most spectacular feature is the lazy filigree of gaseous filaments 29 00:01:59,967 --> 00:02:03,548 reaching out beyond the galaxy into the multi-million degree 30 00:02:03,574 --> 00:02:06,801 x- ray emitting gas that pervades the cluster. 31 00:02:06,802 --> 00:02:11,692 This is an active galaxy, hosting a super-massive black hole at its core, 32 00:02:11,693 --> 00:02:16,029 which blows bubbles of material into the surrounding cluster gas. 33 00:02:16,227 --> 00:02:18,916 Exploiting Hubble's view, a team of astronomers 34 00:02:18,976 --> 00:02:22,694 led by Andy Fabian from the University of Cambridge in the United Kingdom, 35 00:02:22,695 --> 00:02:28,440 have for the first time resolved individual threads of gas, which make up the filaments. 36 00:02:31,703 --> 00:02:36,025 So, the amount of gas in one of these threads is about a million times the mass of the Sun. 37 00:02:36,091 --> 00:02:39,309 They are only about 200 light years across, but they are very straight 38 00:02:39,310 --> 00:02:42,131 and they can extend for up to 20,000 light years. 39 00:02:42,601 --> 00:02:46,388 These filaments are formed when cold gas from the core of the galaxy 40 00:02:46,389 --> 00:02:50,563 is dragged out in the wake of the raising bubbles blown by the black hole. 41 00:02:50,894 --> 00:02:53,248 But the really interesting thing is that these filaments 42 00:02:53,295 --> 00:02:56,880 appear to be able to survive for up to 100 million years. 43 00:02:56,881 --> 00:02:59,627 And that's what had astronomers really puzzled. 44 00:02:59,628 --> 00:03:03,362 How is it possible that these delicate filamentary structures can survive 45 00:03:03,419 --> 00:03:07,912 in the hostile high-energy environment of the galaxy cluster for so long? 46 00:03:08,554 --> 00:03:13,991 Either they should have heated up, disperse and evaporated in a very short period of time, 47 00:03:13,992 --> 00:03:16,620 or, if they are somehow shielded, they should have collapsed 48 00:03:16,667 --> 00:03:19,787 under their own weight and form stars long ago. 49 00:03:21,544 --> 00:03:26,930 The new study published in Nature on the 21st of August 2008 gives the explanation. 50 00:03:26,997 --> 00:03:29,626 Magnetic fields provide a skeletal structure 51 00:03:29,627 --> 00:03:32,255 strong enough to resist gravitational collapse 52 00:03:32,256 --> 00:03:35,038 Preventing the filaments from forming into stars. 53 00:03:35,230 --> 00:03:38,385 These magnetic fields have been able to contain and suspend 54 00:03:38,424 --> 00:03:42,273 the peculiarly long threads for over 100 million years. 55 00:03:43,901 --> 00:03:45,420 Well, there you have it! 56 00:03:45,808 --> 00:03:50,181 But why is it so important that scientists have resolved these fine filamentary structures? 57 00:03:50,815 --> 00:03:54,512 Well, first of all it's allowed them to finally measure the strength 58 00:03:54,513 --> 00:03:56,612 of an extragalactic magnetic field. 59 00:03:56,704 --> 00:04:01,154 But in addition to that, these filaments are clear evidence of the intricate relationship 60 00:04:01,212 --> 00:04:05,386 between the central super-massive black hole and the surrounding cluster gas. 61 00:04:05,387 --> 00:04:08,858 Understanding this relationship provides us with important clues 62 00:04:08,893 --> 00:04:13,643 on how the giant black hole interacts with and affects their surrounding environment. 63 00:04:14,632 --> 00:04:17,436 This is Dr. J signing off for the Hubblecast. 64 00:04:17,437 --> 00:04:21,422 Once again, nature has surprised us beyond our wildest imagination... 65 00:04:23,245 --> 00:04:25,245 Hubblecast is produced by ESA / Hubble 66 00:04:25,246 --> 00:04:27,246 at the European Southern Observatory in Germany. 67 00:04:28,494 --> 00:04:30,494 The Hubble mission is a project of international cooperation 68 00:04:30,495 --> 00:04:32,495 between NASA and the European Space Agency.