WEBVTT FILE 1 00:00:00.000 --> 00:00:04.319 [ HUBBLE SCIENCE ] 2 00:00:04.319 --> 00:00:08.883 [ EINSTEIN RINGS // OPTICAL ILLUSIONS ] 3 00:00:08.883 --> 00:00:12.262 An Einstein Ring is a very cool feature of gravitational lensing 4 00:00:12.262 --> 00:00:16.099 where a background galaxy gets stretched out into a full ring 5 00:00:16.099 --> 00:00:18.643 around the foreground lens. 6 00:00:18.643 --> 00:00:23.398 The Molten Ring is a really interesting case where it's one of the largest galaxies 7 00:00:23.398 --> 00:00:26.276 that forms a near complete Einstein ring, 8 00:00:26.276 --> 00:00:29.070 The Molten Ring, you have a very large cluster of galaxies 9 00:00:29.070 --> 00:00:33.033 that has magnified this background galaxy. 10 00:00:33.033 --> 00:00:35.785 Einstein's theory of general relativity is really sort of what 11 00:00:35.785 --> 00:00:39.504 predicted these Einstein rings in the first place. 12 00:00:39.504 --> 00:00:43.376 He created this whole machinery for how gravity is supposed to work. 13 00:00:43.376 --> 00:00:45.712 Matter would tell spacetime how to curve 14 00:00:45.712 --> 00:00:48.798 and spacetime would tell matter how to move. 15 00:00:48.798 --> 00:00:51.634 And then as you have light moving through this curved spacetime, 16 00:00:51.634 --> 00:00:55.722 that those equations led to the prediction that this light would almost move on 17 00:00:55.722 --> 00:01:01.061 what seems like curved paths and caused the phenomenon of gravitational lensing, 18 00:01:01.061 --> 00:01:03.738 which is where this light gets essentially bent 19 00:01:03.738 --> 00:01:06.983 and distorted by a foreground lens, like a galaxy cluster, 20 00:01:06.983 --> 00:01:10.528 and creates these stretched out images that are magnified of these 21 00:01:10.528 --> 00:01:13.534 distant galaxies that we see. 22 00:01:13.534 --> 00:01:15.786 It's definitely a bit of an optical illusion. 23 00:01:15.786 --> 00:01:20.205 So if you were to take the gravitational lens completely away, 24 00:01:20.205 --> 00:01:23.507 then these background galaxies would just look like, 25 00:01:23.507 --> 00:01:25.919 you know, the normal everyday galaxies that we see at these distances. 26 00:01:25.919 --> 00:01:29.422 And it'd be a lot harder to to pick apart what's going on in 27 00:01:29.464 --> 00:01:31.466 their inner workings. 28 00:01:31.466 --> 00:01:33.802 So the gravitational lensing effect, it is kind of like 29 00:01:33.802 --> 00:01:38.389 looking at a funhouse mirror and it makes the background object appear 30 00:01:38.389 --> 00:01:40.183 a little bit bigger, a little bit distorted, 31 00:01:40.183 --> 00:01:43.269 you know, just like you go to a funhouse and you see, 32 00:01:43.269 --> 00:01:46.022 you know, your head looks gigantic, your body looks tiny. 33 00:01:46.022 --> 00:01:49.609 It's a similar effect, but we can use it for science as opposed to just, 34 00:01:49.609 --> 00:01:53.238 you know, looking at ourselves and saying, oh, wow, that's kind of funny. 35 00:01:53.238 --> 00:01:56.579 The Hubble Space Telescope has definitely taken the clearest images 36 00:01:56.579 --> 00:01:58.080 of the Einstein rings 37 00:01:58.080 --> 00:02:01.371 and they've really, you know, verified this part of Einstein's theory of 38 00:02:01.371 --> 00:02:03.015 general relativity. 39 00:02:03.015 --> 00:02:07.102 They've really shown us a lot more about how gravitational lensing works 40 00:02:07.102 --> 00:02:09.712 and really sort of push the limits of what we can learn 41 00:02:09.712 --> 00:02:12.132 about these distant galaxies with gravitational lensing. 42 00:02:12.132 --> 00:02:19.097 Follow us on social media @NASAHubble