1 00:00:05,950 --> 00:00:03,260 astronomers may have discovered the 2 00:00:10,900 --> 00:00:05,960 densest galaxies in the nearby universe 3 00:00:13,490 --> 00:00:10,910 the galaxies known as m60 - UCD one is 4 00:00:18,560 --> 00:00:13,500 located about 54 million light-years 5 00:00:21,019 --> 00:00:18,570 from Earth m6e UCD one is packed with an 6 00:00:23,540 --> 00:00:21,029 extraordinary number of stars and this 7 00:00:26,929 --> 00:00:23,550 has led scientists to classify it as an 8 00:00:29,419 --> 00:00:26,939 ultra-compact dwarf galaxy this means 9 00:00:32,860 --> 00:00:29,429 that this galaxy is smaller and has more 10 00:00:35,510 --> 00:00:32,870 stars than just a regular dwarf galaxy 11 00:00:37,340 --> 00:00:35,520 while astronomers already knew this 12 00:00:39,889 --> 00:00:37,350 it wasn't until these latest results 13 00:00:42,110 --> 00:00:39,899 from Chandra Hubble and telescopes on 14 00:00:48,080 --> 00:00:42,120 the ground that they knew just how dense 15 00:00:50,810 --> 00:00:48,090 this galaxy truly is m6d UCD 1 has the 16 00:00:54,110 --> 00:00:50,820 mass of about 200 million times our Sun 17 00:00:56,930 --> 00:00:54,120 and remarkably about half of this mass 18 00:01:00,139 --> 00:00:56,940 is packed into a radius of just about 80 19 00:01:02,689 --> 00:01:00,149 light years that translates into the 20 00:01:05,990 --> 00:01:02,699 density of stars in this part of M 60 21 00:01:07,820 --> 00:01:06,000 you see D 1 being about fifteen thousand 22 00:01:11,320 --> 00:01:07,830 times greater than what's found in 23 00:01:13,219 --> 00:01:11,330 Earth's neighborhood in the Milky Way 24 00:01:14,719 --> 00:01:13,229 astronomers have been trying to 25 00:01:17,109 --> 00:01:14,729 determine where these ultra-compact 26 00:01:20,420 --> 00:01:17,119 dwarf galaxies fit into the Galactic 27 00:01:23,480 --> 00:01:20,430 evolutionary chain some have suggested 28 00:01:27,140 --> 00:01:23,490 they start off not as galaxies but as 29 00:01:31,160 --> 00:01:27,150 giant star clusters the latest results 30 00:01:33,380 --> 00:01:31,170 on M 60 UCD 1 challenge that idea the 31 00:01:35,330 --> 00:01:33,390 new Chandra data indicate that there may 32 00:01:38,490 --> 00:01:35,340 be a supermassive black hole at the 33 00:01:41,580 --> 00:01:38,500 centre of M 60 you see T 1 34 00:01:43,890 --> 00:01:41,590 if that's the case then it's unlikely 35 00:01:47,400 --> 00:01:43,900 this objects could have ever been a star 36 00:01:49,200 --> 00:01:47,410 cluster instead the x-ray data point to 37 00:01:51,330 --> 00:01:49,210 this galaxy being the remnants of a 38 00:01:53,850 --> 00:01:51,340 larger galaxy that had its outer stars 39 00:01:55,440 --> 00:01:53,860 ripped away by tidal forces leaving 40 00:02:00,270 --> 00:01:55,450 behind the dense inner core of the 41 00:02:02,730 --> 00:02:00,280 galaxy other information about m60 UC d1 42 00:02:06,330 --> 00:02:02,740 including its large mass point to the 43 00:02:08,550 --> 00:02:06,340 same conclusion regardless this galaxy