WEBVTT FILE 1 00:00:09.467 --> 00:00:13.555 This is an image of the Crab Nebula, which is one of the most famous 2 00:00:13.555 --> 00:00:16.975 and most well-studied astronomical objects ever. 3 00:00:17.726 --> 00:00:20.603 It's one of the touchstone images from the Hubble Space Telescope. 4 00:00:21.938 --> 00:00:23.690 It's just the most beautiful, 5 00:00:23.690 --> 00:00:26.192 awe inspiring image you can imagine. 6 00:00:26.776 --> 00:00:29.988 Technically, it's actually called a pulsar wind nebula, 7 00:00:30.238 --> 00:00:35.452 and we can connect it to events in history going back to the year 1054, 8 00:00:35.452 --> 00:00:37.203 where Chinese astronomers 9 00:00:37.203 --> 00:00:40.498 recorded the appearance of a new star, which they called a guest star. 10 00:00:40.874 --> 00:00:43.960 That got incredibly bright, that you could see it during the daytime, 11 00:00:43.960 --> 00:00:47.839 which we now know was a supernova explosion that was visible 12 00:00:47.839 --> 00:00:51.634 to the naked eye during the day for about two weeks, maybe longer. 13 00:00:54.304 --> 00:00:56.973 What we're seeing here, this filamentary structure 14 00:00:56.973 --> 00:01:00.810 is actually density variations in that material. 15 00:01:01.227 --> 00:01:05.273 So as that material was spewed from the star in the supernova explosion, 16 00:01:05.607 --> 00:01:09.027 it's still got the fingerprints of that explosion. 17 00:01:09.152 --> 00:01:13.656 It's still expanding out into the surrounding medium. 18 00:01:13.907 --> 00:01:16.659 So what we're able to see are knots of material 19 00:01:17.202 --> 00:01:19.621 made up of things like oxygen, sulfur. 20 00:01:19.829 --> 00:01:23.666 And in this full color image, the oxygen is coming out separately 21 00:01:23.666 --> 00:01:26.795 from the sulfur where the the greenish, yellowish 22 00:01:26.795 --> 00:01:29.130 tinge is really oxygen heavy. 23 00:01:31.841 --> 00:01:35.762 Embedded in this nebula is the pulsar at the center. 24 00:01:36.137 --> 00:01:38.056 And it's very energetic, 25 00:01:38.056 --> 00:01:42.644 so it's spewing out energy at all wavelengths, actually. 26 00:01:42.894 --> 00:01:48.358 And some of that energy is being captured by the material surrounding the pulsar. 27 00:01:48.691 --> 00:01:51.903 And then that material glows and it glows in a certain wavelength 28 00:01:52.278 --> 00:01:54.948 or color, depending on what it's made of. 29 00:01:54.948 --> 00:01:59.369 So all the material that we're seeing here is actually from the star itself. 30 00:01:59.369 --> 00:02:02.747 It's been blown out in that supernova explosion, 31 00:02:03.498 --> 00:02:07.377 but it's being illuminated by the pulsar in the center. 32 00:02:09.045 --> 00:02:09.629 Oxygen is 33 00:02:09.629 --> 00:02:13.550 such an important element of life on the planet Earth. 34 00:02:13.550 --> 00:02:15.844 We are breathing in oxygen as we speak. 35 00:02:16.261 --> 00:02:18.888 Where did that oxygen come from? 36 00:02:18.888 --> 00:02:21.224 It came from the hearts of stars. 37 00:02:21.683 --> 00:02:24.686 They made the oxygen in fusion and they expelled it 38 00:02:24.686 --> 00:02:26.312 back into the interstellar medium. 39 00:02:26.312 --> 00:02:28.606 We're actually watching that happen here. 40 00:02:28.606 --> 00:02:32.277 Maybe someday there will be a planet there with an atmosphere that includes oxygen 41 00:02:32.277 --> 00:02:35.530 that can be breathed by living organisms like us.