1 00:00:00,000 --> 00:00:07,196 "HUBBLE SCIENCE" 2 00:00:07,196 --> 00:00:14,220 "Globular Clusters / Stellar Pockets" 3 00:00:14,220 --> 00:00:19,800 A globular cluster is a big sphere of stars  that have collected together they're   4 00:00:19,800 --> 00:00:24,720 orbiting around a Common Center but it's  very spherical very organized looks like   5 00:00:24,720 --> 00:00:29,520 a huge basketball contains hundreds of  thousands of stars these clusters have   6 00:00:29,520 --> 00:00:35,040 formed early on in the formation of a  galaxy when the cluster starts forming   7 00:00:35,040 --> 00:00:40,800 it's a very diffuse and over time things get  concentrated more and more toward the center.   8 00:00:41,640 --> 00:00:45,840 Stars are actually moving all around and if  they're sort of orbiting around the center   9 00:00:45,840 --> 00:00:50,940 it's not a static cluster even though a single  picture makes everything look like it's in place. 10 00:00:53,160 --> 00:00:56,520 One of the more famous ones is Messier 13.   11 00:00:58,020 --> 00:01:01,980 Omega Centauri is a prototypical  one in the southern hemisphere   12 00:01:03,300 --> 00:01:09,720 globular clusters are very old there seem to be  some of the first stars formed in the Galaxy as   13 00:01:09,720 --> 00:01:16,560 the material that came together in the past one  of the pockets of condensed material that occurred   14 00:01:16,560 --> 00:01:22,320 around the center of the Galaxy drew together into  the selections of stars so they're mostly very old   15 00:01:22,320 --> 00:01:30,060 stars, 10 or 12 billion years old although we do  see a second generation of newer younger stars   16 00:01:30,060 --> 00:01:36,120 in globular clusters still you know relatively  old billions of years ago but it's not like it   17 00:01:36,120 --> 00:01:41,760 had one burst of star formation and that was it. It did have a chance to form a second wave later on.   18 00:01:43,140 --> 00:01:49,680 Westerlund 1 still in one is what's called an open cluster  it's a very loose collection of stars over a broad   19 00:01:49,680 --> 00:01:57,180 area it's more sort of a cloud of stars as more  stars gather in an open cluster like that and more   20 00:01:57,180 --> 00:02:02,460 material comes together it's going to naturally  pull things in toward its center. Something like   21 00:02:02,460 --> 00:02:09,060 Westerlund 1 over many millions of years could evolve  into something that looks more like a globular   22 00:02:09,060 --> 00:02:15,600 and we do think that most globulars have one or  more black holes at the center which is a source   23 00:02:15,600 --> 00:02:22,500 of immense gravity to help hold these clusters  together Hubble saw in the globular cluster NGC   24 00:02:22,500 --> 00:02:29,880 6397 the first clear evidence for multiple black  holes at the center we had previously assumed that   25 00:02:29,880 --> 00:02:35,100 most globulars would have a single black hole  at the center in this case we found a number   26 00:02:35,100 --> 00:02:40,440 of separate black holes they're moving around  each other at high speeds around a common center.   27 00:02:41,040 --> 00:02:45,720 If you have a number of black holes in  tight orbits around each other at the   28 00:02:45,720 --> 00:02:50,280 center that works as well as a single black  hole for holding together the overall cluster 29 00:02:50,280 --> 00:02:56,509 Follow us @NASAHubble