1 00:00:19,830 --> 00:00:17,349 as hubble looks out into these 2 00:00:21,990 --> 00:00:19,840 fields of galaxies we sometimes see 3 00:00:23,830 --> 00:00:22,000 clusters of galaxies these are galaxies 4 00:00:26,310 --> 00:00:23,840 that are held nearby each other by their 5 00:00:28,790 --> 00:00:26,320 mutual gravity 6 00:00:31,830 --> 00:00:28,800 these clusters are 7 00:00:34,310 --> 00:00:31,840 massive conglomerations 8 00:00:37,910 --> 00:00:34,320 there's so much mass that they have an 9 00:00:39,430 --> 00:00:37,920 actual observable impact on space time 10 00:00:42,709 --> 00:00:39,440 itself 11 00:00:44,470 --> 00:00:42,719 einstein predicted that mass distorts 12 00:00:46,470 --> 00:00:44,480 space but we didn't realize we could 13 00:00:49,110 --> 00:00:46,480 actually see the effects of that but 14 00:00:51,670 --> 00:00:49,120 with hubble we have been able to see 15 00:00:54,389 --> 00:00:51,680 distortions in space around clusters of 16 00:00:57,270 --> 00:00:54,399 galaxies the way we see that is when 17 00:00:59,510 --> 00:00:57,280 light from a background galaxy travels 18 00:01:01,830 --> 00:00:59,520 through that cluster of galaxies or 19 00:01:04,229 --> 00:01:01,840 around it due to this gravitational 20 00:01:07,270 --> 00:01:04,239 lensing effect the lensing also 21 00:01:09,429 --> 00:01:07,280 magnifies that background galaxy so if 22 00:01:11,350 --> 00:01:09,439 we look in some of these distorted arcs 23 00:01:13,990 --> 00:01:11,360 we can see more detail than we would 24 00:01:17,190 --> 00:01:14,000 ever have been able to see without 25 00:01:19,510 --> 00:01:17,200 gravitational lensing nature's boost 26 00:01:21,830 --> 00:01:19,520 so hubble has been used in an unexpected 27 00:01:23,990 --> 00:01:21,840 way for us to look at nature's 28 00:01:24,950 --> 00:01:24,000 magnifying glasses these gravitational 29 00:01:27,350 --> 00:01:24,960 lenses 30 00:01:29,590 --> 00:01:27,360 and using those to tell us about much 31 00:01:31,749 --> 00:01:29,600 more distant galaxies in detail we could 32 00:01:33,830 --> 00:01:31,759 never have seen without the lensing and 33 00:01:36,069 --> 00:01:33,840 also to tell us how dark matter is 34 00:01:38,310 --> 00:01:36,079 distributed in those clusters because it 35 00:01:40,230 --> 00:01:38,320 turns out that most of the mass that's 36 00:01:41,590 --> 00:01:40,240 distorting space and these clusters of 37 00:01:44,149 --> 00:01:41,600 galaxies 38 00:01:46,550 --> 00:01:44,159 is made of this unseen dark matter not 39 00:01:48,230 --> 00:01:46,560 the visible stars and the galaxies and 40 00:01:49,990 --> 00:01:48,240 we can't see the dark matter but by 41 00:01:52,069 --> 00:01:50,000 seeing how this background light is 42 00:01:54,789 --> 00:01:52,079 distorted we can kind of map out where 43 00:01:57,350 --> 00:01:54,799 that dark matter is through this effect 44 00:01:58,870 --> 00:01:57,360 we call gravitational lensing 45 00:02:01,429 --> 00:01:58,880 so we're learning a lot about dark 46 00:02:03,270 --> 00:02:01,439 matter this mystery of matter we don't 47 00:02:05,270 --> 00:02:03,280 really know what it is but we know where 48 00:02:07,030 --> 00:02:05,280 it is in these clusters because of this 49 00:02:10,969 --> 00:02:07,040 innovative use of the hubble space