1 00:00:00,000 --> 00:00:02,386 [ MUSIC ] 2 00:00:02,386 --> 00:00:05,828 [ INSIDE THE IMAGE // HUBBLE SPACE TELESCOPE ] 3 00:00:05,828 --> 00:00:09,000 [ CRAB NEBULA ] 4 00:00:09,000 --> 00:00:13,088 This is an image of the Crab Nebula, which is one of the most famous 5 00:00:13,088 --> 00:00:16,508 and most well-studied astronomical objects ever. 6 00:00:16,508 --> 00:00:21,354 It's one of the touchstone images from the Hubble Space Telescope. 7 00:00:21,354 --> 00:00:23,106 It's just the most beautiful, 8 00:00:23,106 --> 00:00:25,608 awe inspiring image you can imagine. 9 00:00:26,341 --> 00:00:29,553 Technically, it's actually called a pulsar wind nebula, 10 00:00:29,553 --> 00:00:34,767 and we can connect it to events in history going back to the year 1054, 11 00:00:34,767 --> 00:00:36,518 where Chinese astronomers 12 00:00:36,518 --> 00:00:40,495 recorded the appearance of a new star, which they called a guest star. 13 00:00:40,495 --> 00:00:43,581 That got incredibly bright, that you could see it during the daytime, 14 00:00:43,581 --> 00:00:47,460 which we now know was a supernova explosion that was visible 15 00:00:47,460 --> 00:00:53,758 to the naked eye during the day for about two weeks, maybe longer. 16 00:00:53,758 --> 00:00:56,427 What we're seeing here, this filamentary structure 17 00:00:56,427 --> 00:01:00,264 is actually density variations in that material. 18 00:01:00,264 --> 00:01:04,310 So as that material was spewed from the star in the supernova explosion, 19 00:01:04,310 --> 00:01:08,701 it's still got the fingerprints of that explosion. 20 00:01:08,701 --> 00:01:13,205 It's still expanding out into the surrounding medium. 21 00:01:13,205 --> 00:01:15,957 So what we're able to see are knots of material 22 00:01:15,957 --> 00:01:19,199 made up of things like oxygen, sulfur. 23 00:01:19,199 --> 00:01:23,036 And in this full color image, the oxygen is coming out separately 24 00:01:23,036 --> 00:01:26,165 from the sulfur where the the greenish, yellowish 25 00:01:26,165 --> 00:01:28,500 tinge is really oxygen heavy. 26 00:01:31,185 --> 00:01:35,106 Embedded in this nebula is the pulsar at the center. 27 00:01:35,106 --> 00:01:37,423 And it's very energetic, 28 00:01:37,423 --> 00:01:42,011 so it's spewing out energy at all wavelengths, actually. 29 00:01:42,011 --> 00:01:47,475 And some of that energy is being captured by the material surrounding the pulsar. 30 00:01:47,475 --> 00:01:51,824 And then that material glows and it glows in a certain wavelength 31 00:01:51,824 --> 00:01:54,494 or color, depending on what it's made of. 32 00:01:54,494 --> 00:01:58,915 So all the material that we're seeing here is actually from the star itself. 33 00:01:58,915 --> 00:02:03,000 It's been blown out in that supernova explosion, 34 00:02:03,000 --> 00:02:08,579 but it's being illuminated by the pulsar in the center. 35 00:02:08,579 --> 00:02:09,163 Oxygen is 36 00:02:09,163 --> 00:02:13,084 such an important element of life on the planet Earth. 37 00:02:13,084 --> 00:02:15,378 We are breathing in oxygen as we speak. 38 00:02:15,378 --> 00:02:18,518 Where did that oxygen come from? 39 00:02:18,518 --> 00:02:20,814 It came from the hearts of stars. 40 00:02:20,814 --> 00:02:23,817 They made the oxygen in fusion and they expelled it 41 00:02:23,817 --> 00:02:25,831 back into the interstellar medium. 42 00:02:25,831 --> 00:02:28,125 We're actually watching that happen here. 43 00:02:28,125 --> 00:02:31,796 Maybe someday there will be a planet there with an atmosphere that includes oxygen 44 00:02:31,796 --> 00:02:35,003 that can be breathed by living organisms like us. 45 00:02:35,003 --> 00:02:41,536 [ FOLLOW US ON SOCIAL MEDIA @NASAHubble ]