WEBVTT FILE 1 00:00:00.000 --> 00:00:03.400 [ MUSIC ] 2 00:00:03.400 --> 00:00:09.340 Astronomers seem to have revealed a puzzling detail in the way dark matter behaves. 3 00:00:09.350 --> 00:00:15.000 They found small, dense concentrations of dark matter that bend and magnify light much 4 00:00:15.000 --> 00:00:17.700 more strongly than expected. 5 00:00:17.700 --> 00:00:24.361 Dark matter is a mysterious, invisible substance that makes up the bulk of a galaxy. The gravitational 6 00:00:24.361 --> 00:00:29.470 pull exerted by dark matter is thought to tie galaxies together throughout the universe. 7 00:00:29.470 --> 00:00:35.660 There is so much regular matter and dark matter concentrated in massive galaxy clusters that 8 00:00:35.660 --> 00:00:40.700 their gravity magnifies and warps light from distant background objects. 9 00:00:40.700 --> 00:00:46.820 We call this effect “gravitational lensing.” We can map where the dark matter is in galaxy 10 00:00:46.820 --> 00:00:50.440 clusters by observing how the light bends. 11 00:00:50.440 --> 00:00:54.860 Gravitational lensing distorts the appearance of background galaxies into deformed shapes 12 00:00:54.860 --> 00:01:01.290 and elongated arcs. Pictures of lensing galaxy clusters are filled with the smeared images 13 00:01:01.290 --> 00:01:04.009 of remote background galaxies. 14 00:01:04.009 --> 00:01:08.780 The higher the concentration of dark matter in a galaxy cluster, the more dramatic its 15 00:01:08.780 --> 00:01:14.719 light-bending power is. Smaller clumps of dark matter associated with individual galaxies 16 00:01:14.719 --> 00:01:21.249 in the galaxy cluster create more distortions. In some sense, the galaxy cluster acts as 17 00:01:21.249 --> 00:01:26.049 a large lens that has many smaller lenses embedded inside of it. 18 00:01:26.049 --> 00:01:32.389 But strangely, astronomers found that three galaxy clusters used in their study had concentrations 19 00:01:32.389 --> 00:01:37.450 of dark matter that are so massive that the lensing effects they produce are 10 times 20 00:01:37.450 --> 00:01:39.869 stronger than originally expected. 21 00:01:39.869 --> 00:01:46.159 Hubble’s crisp images, coupled with observations from the very large telescope in Chile, helped 22 00:01:46.159 --> 00:01:50.049 astronomers produce a more accurate dark-matter map. 23 00:01:50.049 --> 00:01:55.169 By measuring the lensing distortions, astronomers could trace out the amount and distribution 24 00:01:55.169 --> 00:01:57.609 of dark matter. 25 00:01:57.609 --> 00:02:01.950 This recent study could signal a gap in our current understanding of the nature of dark 26 00:02:01.950 --> 00:02:06.779 matter and its properties. It shows us that there’s clearly a missing feature of the 27 00:02:06.779 --> 00:02:12.260 real universe that we simply are not capturing in our current theoretical models. 28 00:02:12.260 --> 00:02:17.540 With studies like this, astronomers look forward to continuing to pin down the intriguing nature 29 00:02:17.540 --> 00:02:22.700 of dark matter to better understand the secrets of our mysterious universe. 30 00:02:22.700 --> 00:02:35.300 [ BEAUTIFUL MUSIC ]