1 00:00:08,883 --> 00:00:12,262 An Einstein Ring is a very cool feature of gravitational lensing 2 00:00:12,262 --> 00:00:15,890 where a background galaxy gets stretched out into a full ring 3 00:00:16,099 --> 00:00:18,143 around the foreground lens. 4 00:00:18,643 --> 00:00:23,398 The Molten Ring is a really interesting case where it's one of the largest galaxies 5 00:00:23,398 --> 00:00:25,442 that forms a near complete Einstein ring, 6 00:00:26,276 --> 00:00:29,070 The Molten Ring, you have a very large cluster of galaxies 7 00:00:29,070 --> 00:00:32,615 that has magnified this background galaxy. 8 00:00:33,033 --> 00:00:35,785 Einstein's theory of general relativity is really sort of what 9 00:00:35,785 --> 00:00:38,788 predicted these Einstein rings in the first place. 10 00:00:38,913 --> 00:00:43,376 He created this whole machinery for how gravity is supposed to work. 11 00:00:43,376 --> 00:00:45,378 Matter would tell spacetime how to curve 12 00:00:45,712 --> 00:00:47,881 and spacetime would tell matter how to move. 13 00:00:48,173 --> 00:00:51,009 And then as you have light moving through this curved spacetime, 14 00:00:51,384 --> 00:00:55,722 that those equations led to the prediction that this light would almost move on 15 00:00:55,722 --> 00:01:01,061 what seems like curved paths and caused the phenomenon of gravitational lensing, 16 00:01:01,061 --> 00:01:03,104 which is where this light gets essentially bent 17 00:01:03,104 --> 00:01:06,483 and distorted by a foreground lens, like a galaxy cluster, 18 00:01:06,983 --> 00:01:10,528 and creates these stretched out images that are magnified of these 19 00:01:10,528 --> 00:01:12,363 distant galaxies that we see. 20 00:01:13,073 --> 00:01:15,325 It's definitely a bit of an optical illusion. 21 00:01:15,325 --> 00:01:19,913 So if you were to take the gravitational lens completely away, 22 00:01:20,205 --> 00:01:22,248 then these background galaxies would just look like, 23 00:01:22,457 --> 00:01:25,502 you know, the normal everyday galaxies that we see at these distances. 24 00:01:25,919 --> 00:01:29,422 And it'd be a lot harder to to pick apart what's going on in 25 00:01:29,464 --> 00:01:31,466 their inner workings. 26 00:01:31,466 --> 00:01:33,802 So the gravitational lensing effect, it is kind of like 27 00:01:33,802 --> 00:01:37,764 looking at a funhouse mirror and it makes the background object appear 28 00:01:38,389 --> 00:01:40,183 a little bit bigger, a little bit distorted, 29 00:01:40,183 --> 00:01:43,019 you know, just like you go to a funhouse and you see, 30 00:01:43,269 --> 00:01:45,480 you know, your head looks gigantic, your body looks tiny. 31 00:01:46,022 --> 00:01:49,400 It's a similar effect, but we can use it for science as opposed to just, 32 00:01:49,609 --> 00:01:51,986 you know, looking at ourselves and saying, oh, wow, that's kind of funny. 33 00:01:53,238 --> 00:01:56,241 The Hubble Space Telescope has definitely taken the clearest images 34 00:01:56,241 --> 00:01:57,742 of the Einstein rings 35 00:01:57,742 --> 00:02:01,371 and they've really, you know, verified this part of Einstein's theory of 36 00:02:01,371 --> 00:02:02,247 general relativity. 37 00:02:02,247 --> 00:02:06,334 They've really shown us a lot more about how gravitational lensing works 38 00:02:06,668 --> 00:02:09,712 and really sort of push the limits of what we can learn 39 00:02:09,712 --> 00:02:12,132 about these distant galaxies with gravitational lensing.