1 00:00:07,909 --> 00:00:05,749 astronomers seem to have revealed a 2 00:00:09,190 --> 00:00:07,919 puzzling detail in the way dark matter 3 00:00:11,910 --> 00:00:09,200 behaves 4 00:00:14,709 --> 00:00:11,920 they found small dense concentrations of 5 00:00:17,349 --> 00:00:14,719 dark matter that bend and magnify light 6 00:00:20,230 --> 00:00:17,359 much more strongly than expected 7 00:00:22,310 --> 00:00:20,240 dark matter is a mysterious invisible 8 00:00:25,429 --> 00:00:22,320 substance that makes up the bulk of a 9 00:00:27,670 --> 00:00:25,439 galaxy the gravitational pull exerted by 10 00:00:29,910 --> 00:00:27,680 dark matter is thought to tie galaxies 11 00:00:32,310 --> 00:00:29,920 together throughout the universe there 12 00:00:34,630 --> 00:00:32,320 is so much regular matter and dark 13 00:00:37,190 --> 00:00:34,640 matter concentrated in massive galaxy 14 00:00:39,510 --> 00:00:37,200 clusters that their gravity magnifies 15 00:00:41,590 --> 00:00:39,520 and warps light from distant background 16 00:00:43,590 --> 00:00:41,600 objects we call this effect 17 00:00:45,830 --> 00:00:43,600 gravitational lensing 18 00:00:48,229 --> 00:00:45,840 we can map where the dark matter is in 19 00:00:49,670 --> 00:00:48,239 galaxy clusters by observing how the 20 00:00:51,590 --> 00:00:49,680 light bends 21 00:00:53,750 --> 00:00:51,600 gravitational lensing distorts the 22 00:00:56,950 --> 00:00:53,760 appearance of background galaxies into 23 00:00:59,349 --> 00:00:56,960 deformed shapes and elongated arcs 24 00:01:01,830 --> 00:00:59,359 pictures of lensing galaxy clusters are 25 00:01:03,750 --> 00:01:01,840 filled with the smeared images of remote 26 00:01:05,750 --> 00:01:03,760 background galaxies 27 00:01:07,990 --> 00:01:05,760 the higher the concentration of dark 28 00:01:10,789 --> 00:01:08,000 matter in a galaxy cluster the more 29 00:01:13,190 --> 00:01:10,799 dramatic its light bending power is 30 00:01:15,429 --> 00:01:13,200 smaller clumps of dark matter associated 31 00:01:18,550 --> 00:01:15,439 with individual galaxies in the galaxy 32 00:01:21,190 --> 00:01:18,560 cluster create more distortions 33 00:01:23,350 --> 00:01:21,200 in some sense the galaxy cluster acts as 34 00:01:26,149 --> 00:01:23,360 a large lens that has many smaller 35 00:01:28,789 --> 00:01:26,159 lenses embedded inside of it but 36 00:01:31,429 --> 00:01:28,799 strangely astronomers found that three 37 00:01:33,429 --> 00:01:31,439 galaxy clusters used in their study had 38 00:01:35,830 --> 00:01:33,439 concentrations of dark matter that are 39 00:01:38,469 --> 00:01:35,840 so massive that the lensing effects they 40 00:01:40,550 --> 00:01:38,479 produce are 10 times stronger than 41 00:01:42,550 --> 00:01:40,560 originally expected 42 00:01:44,230 --> 00:01:42,560 hubble's crisp images coupled with 43 00:01:46,710 --> 00:01:44,240 observations from the very large 44 00:01:49,830 --> 00:01:46,720 telescope in chile helped astronomers 45 00:01:52,069 --> 00:01:49,840 produce a more accurate dark matter map 46 00:01:54,230 --> 00:01:52,079 by measuring the lensing distortions 47 00:01:57,350 --> 00:01:54,240 astronomers could trace out the amount 48 00:01:59,670 --> 00:01:57,360 and distribution of dark matter 49 00:02:01,510 --> 00:01:59,680 this recent study could signal a gap in 50 00:02:03,749 --> 00:02:01,520 our current understanding of the nature 51 00:02:05,590 --> 00:02:03,759 of dark matter and its properties 52 00:02:07,510 --> 00:02:05,600 it shows us that there's clearly a 53 00:02:09,830 --> 00:02:07,520 missing feature of the real universe 54 00:02:11,990 --> 00:02:09,840 that we simply are not capturing in our 55 00:02:14,550 --> 00:02:12,000 current theoretical models 56 00:02:16,550 --> 00:02:14,560 with studies like this astronomers look 57 00:02:18,630 --> 00:02:16,560 forward to continuing to pin down the 58 00:02:20,630 --> 00:02:18,640 intriguing nature of dark matter to