WEBVTT FILE 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.