1 00:00:00,133 --> 00:00:01,533 Gravitational lensing. 2 00:00:01,533 --> 00:00:04,433 Look at the Webb telescope's first deep field image and you may notice 3 00:00:04,433 --> 00:00:06,800 some galaxies that are stretched or banana shaped. 4 00:00:07,166 --> 00:00:09,900 They're not actually shaped like this. So what makes them look like it? 5 00:00:10,333 --> 00:00:11,966 Gravitational lensing. 6 00:00:11,966 --> 00:00:15,433 Gravitational lensing occurs when a celestial object has such a massive 7 00:00:15,433 --> 00:00:18,700 gravitational pull that it actually warps the time and space around it. 8 00:00:19,433 --> 00:00:21,533 Imagine placing a ball on a piece of squishy foam. 9 00:00:21,800 --> 00:00:22,766 The fabric of space -- 10 00:00:22,766 --> 00:00:26,166 the foam -- sinks down around the celestial object -- the ball. 11 00:00:26,166 --> 00:00:28,133 And light that would otherwise travel in a straight line 12 00:00:28,133 --> 00:00:31,833 follows the bend of the warped space, distorting and brightening light 13 00:00:31,833 --> 00:00:35,100 from behind the celestial object -- a galaxy cluster in this case. 14 00:00:35,666 --> 00:00:36,900 So why do we care? 15 00:00:36,900 --> 00:00:38,033 Well, because with a natural 16 00:00:38,033 --> 00:00:41,000 magnifying glass, we can see even more distant objects. 17 00:00:41,266 --> 00:00:43,400 In Webb's first deep field here, the banana shaped 18 00:00:43,400 --> 00:00:47,066 galaxies are actually much farther away than the galaxies in the central cluster. 19 00:00:47,266 --> 00:00:49,666 We see them as stretched because their light is being warped 20 00:00:49,666 --> 00:00:51,866 and magnified by the galaxy clusters in front of them. 21 00:00:52,200 --> 00:00:55,200 And this lets us see much farther than we would otherwise be able to.