1 00:00:00,000 --> 00:00:04,655 Hubble has snapped a spectacular view of the largest "player" in the Leo Triplet, 2 00:00:04,713 --> 00:00:07,357 a galaxy with an unusual anatomy: 3 00:00:07,424 --> 00:00:13,127 it displays asymmetric spiral arms and an apparently displaced core. 4 00:00:13,128 --> 00:00:16,863 The peculiar anatomy is most likely caused by the gravitational pull 5 00:00:16,898 --> 00:00:20,112 of the other two members of the trio. 6 00:00:35,520 --> 00:00:37,313 This is the Hubblecast. 7 00:00:37,314 --> 00:00:41,598 News and images from the NASA / ESA Hubble Space Telescope. 8 00:00:41,599 --> 00:00:50,398 EPISODE 34: Hubble snaps heavyweight of the Leo Triplet 9 00:00:50,806 --> 00:00:55,633 The unusual spiral galaxy Messier 66 is located at a distance 10 00:00:55,634 --> 00:01:00,370 of about 35 million light-years in the constellation of Leo. 11 00:01:00,371 --> 00:01:07,014 Together with Messier 65 and NGC 3628, Messier 66 is one third 12 00:01:07,024 --> 00:01:11,455 of the Leo Triplet, a trio of interacting spiral galaxies, 13 00:01:11,456 --> 00:01:14,724 part of the larger Messier 66 group. 14 00:01:14,725 --> 00:01:18,759 Messier 66 wins out in size over its fellow triplets, 15 00:01:18,826 --> 00:01:23,199 it is about 100,000 light-years across. 16 00:01:23,200 --> 00:01:28,802 Messier 66 is the proud owner of exclusive asymmetric spiral arms 17 00:01:28,803 --> 00:01:32,005 which seem to climb above the galaxy's main disc 18 00:01:32,006 --> 00:01:34,928 and an apparently displaced nucleus. 19 00:01:37,153 --> 00:01:39,576 This asymmetry is unusual, 20 00:01:39,663 --> 00:01:43,941 most often dense waves of gas, dust and newly-born stars 21 00:01:43,942 --> 00:01:47,255 wind about the galaxy's center in a symmetric way. 22 00:01:47,256 --> 00:01:51,402 Astronomers believe that Messier 66's once orderly shape 23 00:01:51,437 --> 00:01:56,570 has most likely been distorted by the gravitational pull of its two neighbours. 24 00:01:58,449 --> 00:02:02,515 Hubble has imaged Messier 66's striking dust lanes 25 00:02:02,562 --> 00:02:06,996 and bright star clusters along the spiral arms in fine detail. 26 00:02:06,997 --> 00:02:11,153 Star clusters, pictured in the blue and pinkish regions of the image, 27 00:02:11,154 --> 00:02:14,773 are key tools for astronomers since they are used as indicators 28 00:02:14,774 --> 00:02:19,078 of how the parent galaxies assembled over time. 29 00:02:20,365 --> 00:02:25,278 Messier 66 boasts a remarkable record of supernovae explosions. 30 00:02:25,279 --> 00:02:29,636 The spiral galaxy has hosted three supernovae since 1989, 31 00:02:29,637 --> 00:02:32,615 the latest one occurring in 2009. 32 00:02:33,172 --> 00:02:35,689 A supernova is a stellar explosion 33 00:02:35,791 --> 00:02:39,896 that may momentarily outshine its entire host galaxy. 34 00:02:39,953 --> 00:02:44,317 It then fades away over a period lasting several weeks or months. 35 00:02:44,318 --> 00:02:48,448 During its very short life the supernova radiates as much energy 36 00:02:48,496 --> 00:02:54,127 as the Sun would radiate over a period of about 10 billion years. 37 00:02:56,100 --> 00:02:58,100 Hubblecast is produced by ESA / Hubble 38 00:02:58,101 --> 00:03:00,101 at the European Southern Observatory in Germany. 39 00:03:01,000 --> 00:03:03,000 The Hubble mission is a project of international cooperation 40 00:03:03,001 --> 00:03:05,001 between NASA and the European Space Agency. 41 00:03:15,002 --> 00:03:16,874 Now that you've caught up with Hubble 42 00:03:16,875 --> 00:03:19,330 make sure to get the latest from the ground too. 43 00:03:19,331 --> 00:03:23,309 The ESOCast highlights the best of the European Southern Observatory 44 00:03:23,310 --> 00:03:27,637 and its powerful telescopes that observe from high in the Chilean Andes 45 00:03:27,638 --> 00:03:33,022 at the southern hemisphere's best known sites for astronomical observations.