1 00:00:00,524 --> 00:00:03,738 A recent NASA / ESA Hubble Space Telescope image 2 00:00:03,739 --> 00:00:07,406 captures what appears to be one very bright and bizarre galaxy 3 00:00:07,407 --> 00:00:11,471 but is actually the result of a pair of spiral galaxies, like our own Milky Way, 4 00:00:11,472 --> 00:00:14,661 smashing together at incredible speeds. 5 00:00:14,662 --> 00:00:18,368 This object was a target of Hubble's and a handful of its "sibling" spacecraft 6 00:00:18,432 --> 00:00:23,164 as part of a massive comprehensive sky survey called GOALS. 7 00:00:40,839 --> 00:00:42,921 This is the Hubblecast. 8 00:00:42,922 --> 00:00:46,409 News and images from the NASA / ESA Hubble Space Telescope. 9 00:00:46,410 --> 00:00:50,316 Travelling through time and space with our host, Dr. J 10 00:00:50,317 --> 00:00:52,868 EPISODE 31: Sky mergers yields sparkling dividends a.k.a. Dr. Joe Liske. 11 00:00:52,869 --> 00:00:55,085 Hi and welcome to the Hubblecast. 12 00:00:55,120 --> 00:01:00,276 This new image of NGC 2623, which is located in the constellation of Cancer, 13 00:01:00,277 --> 00:01:04,035 was taken by Hubble's Advanced Camera for Surveys, or ACS, 14 00:01:04,036 --> 00:01:06,579 before the recent Hubble servicing mission. 15 00:01:06,580 --> 00:01:12,042 Once two distinct galaxies, NGC 2623 is a nearly complete merger, 16 00:01:12,043 --> 00:01:16,502 with elements of both original galaxies affecting its appearance and behaviour. 17 00:01:16,503 --> 00:01:20,174 Colliding galaxies engage in a powerful exchange of material, 18 00:01:20,175 --> 00:01:24,725 they literally throw matter and gas toward one another as they race together. 19 00:01:28,685 --> 00:01:33,879 Stretching out from the center of NGC 2623, are two tidal tails of young stars 20 00:01:33,880 --> 00:01:36,251 showing that a merger has taken place. 21 00:01:36,312 --> 00:01:38,322 The dramatic exchange of mass and gases 22 00:01:38,384 --> 00:01:41,993 initiate star formation seen there in both the tails. 23 00:01:42,470 --> 00:01:46,331 The prominent lower tail is richly populated with bright star clusters. 24 00:01:46,366 --> 00:01:50,193 These star clusters may have formed as part of a loop of stretched material 25 00:01:50,194 --> 00:01:52,087 associated with the northern tail, 26 00:01:52,122 --> 00:01:55,983 or they may have formed from debris falling back onto the nucleus. 27 00:01:55,984 --> 00:01:58,080 In addition to this active star-forming region, 28 00:01:58,081 --> 00:02:00,551 both galactic arms harbour very young stars 29 00:02:00,586 --> 00:02:03,501 in the early stages of their evolutionary journey. 30 00:02:04,844 --> 00:02:08,888 The core or nucleus of this merged galaxy is exceedingly bright. 31 00:02:08,889 --> 00:02:13,532 Often this mergers, including this case, result in an active galactic nucleus, 32 00:02:13,533 --> 00:02:15,766 where one of the super-massive black holes 33 00:02:15,767 --> 00:02:18,206 found at the center of the two original galaxies 34 00:02:18,207 --> 00:02:20,315 is stirred into action. 35 00:02:20,316 --> 00:02:24,091 Matter is pulled toward the black hole forming an accretion disc. 36 00:02:24,092 --> 00:02:27,556 The energy released by the frenzied motion heats up the disc 37 00:02:27,557 --> 00:02:31,401 causing it to emit across a wide range of the electromagnetic spectrum. 38 00:02:33,412 --> 00:02:36,122 Although rare in our solar neck of the woods, 39 00:02:36,123 --> 00:02:39,632 extremely bright galaxies like NGC 2623 40 00:02:39,667 --> 00:02:42,566 exist at higher redshifts or, in other words, 41 00:02:42,601 --> 00:02:47,133 at an early stage of the Universe's evolution when these systems were dominant. 42 00:02:47,134 --> 00:02:50,094 Their brightness signals furious activity, 43 00:02:50,095 --> 00:02:52,986 new star formation and a rambunctious core. 44 00:02:53,646 --> 00:02:58,466 The aim of the GOALS project is to use the combined powers of multiple space telescopes 45 00:02:58,467 --> 00:03:03,045 to characterise their local counterparts and give us clues as to what is happening 46 00:03:03,080 --> 00:03:07,617 in more distant galaxies while educating us about galaxy formation. 47 00:03:07,618 --> 00:03:11,428 Each telescope in the GOALS project brings different strengths. 48 00:03:12,218 --> 00:03:14,553 Hubble's incredible resolution in the visible 49 00:03:14,554 --> 00:03:18,696 allows us to scrutinise the galaxy's morphology, or structure. 50 00:03:18,697 --> 00:03:22,208 In these images, astronomers can determine the stage of the merger. 51 00:03:22,209 --> 00:03:25,505 For example, has the union produced tidal tails? 52 00:03:25,506 --> 00:03:28,912 Have the individual galaxies' cores melted together as one? 53 00:03:29,685 --> 00:03:34,310 Chandra's X-ray capabilities allow the astronomers to detect the flurry of activity 54 00:03:34,378 --> 00:03:38,085 around the black holes and to monitor new star formation. 55 00:03:38,120 --> 00:03:40,316 Spitzer contributes in the infrared, 56 00:03:40,317 --> 00:03:45,489 penetrating dust, allowing astronomers to see what lurks behind the eerie dust lanes. 57 00:03:45,490 --> 00:03:50,366 GALEX is powerful in the ultraviolet, gathering the light of developing stars. 58 00:03:50,590 --> 00:03:54,826 Data from ESA's X-ray Multi-Mirror Telescope, or XMM-Newton, 59 00:03:54,827 --> 00:03:59,237 also helped astronomers gain more information about NGC 2623. 60 00:03:59,621 --> 00:04:02,286 The joint efforts of these powerful observing facilities 61 00:04:02,354 --> 00:04:06,376 has provided a clearer picture of these standout galaxies. 62 00:04:07,000 --> 00:04:09,601 Galaxy evolution is a hot topic in astronomy 63 00:04:09,602 --> 00:04:13,184 because it is fundamental to our understanding of the Universe. 64 00:04:13,185 --> 00:04:14,150 Studying merging galaxies such as NGC 2623, 65 00:04:14,185 --> 00:04:20,531 allows astronomers to witness the shaping of new, combined galaxies 66 00:04:20,532 --> 00:04:22,804 and the subsequent birth of stars. 67 00:04:22,805 --> 00:04:26,205 This could even provide essential information about our own Milky Way, 68 00:04:26,206 --> 00:04:29,962 that has cannibalised other small galaxies and could, one day, 69 00:04:29,984 --> 00:04:33,406 collide with our neighbour, the Andromeda Galaxy. 70 00:04:33,680 --> 00:04:36,564 This is Dr. J signing off for the Hubblecast. 71 00:04:36,565 --> 00:04:41,037 Once again, nature has surprised us beyond our wildest imagination... 72 00:04:41,298 --> 00:04:43,195 Hubblecast is produced by ESA / Hubble 73 00:04:43,230 --> 00:04:45,230 at the European Southern Observatory in Germany. 74 00:04:46,306 --> 00:04:48,306 The Hubble mission is a project of international cooperation 75 00:04:48,307 --> 00:04:50,307 between NASA and the European Space Agency. 76 00:05:00,020 --> 00:05:01,755 Now that you've caught up with Hubble 77 00:05:01,756 --> 00:05:04,238 make sure to get the latest from the ground too. 78 00:05:04,239 --> 00:05:08,120 The ESOCast highlights the best of the European Southern Observatory 79 00:05:08,121 --> 00:05:12,325 and its powerful telescopes that observe from high in the Chilean Andes 80 00:05:12,326 --> 00:05:18,156 at the southern hemisphere's best known sites for astronomical observations.