1 00:00:07,030 --> 00:00:04,710 over the years the hubble space 2 00:00:09,509 --> 00:00:07,040 telescope has taken hundreds of images 3 00:00:11,589 --> 00:00:09,519 of different kinds of incredible nebulae 4 00:00:14,390 --> 00:00:11,599 in our universe 5 00:00:17,349 --> 00:00:14,400 a nebula is a giant cloud of dust and 6 00:00:19,750 --> 00:00:17,359 gas in space there are different types 7 00:00:22,470 --> 00:00:19,760 of nebulae ranging from sites where 8 00:00:25,509 --> 00:00:22,480 stars are being born under gravitational 9 00:00:28,310 --> 00:00:25,519 pressures to expanding gaseous remnants 10 00:00:30,310 --> 00:00:28,320 thrown off by dying stars 11 00:00:33,190 --> 00:00:30,320 the famous orion nebula is a 12 00:00:34,389 --> 00:00:33,200 star-forming region only 1500 light 13 00:00:37,270 --> 00:00:34,399 years away 14 00:00:39,350 --> 00:00:37,280 making it the closest large star-forming 15 00:00:41,430 --> 00:00:39,360 region to earth 16 00:00:44,389 --> 00:00:41,440 because it is so bright and prominent 17 00:00:46,310 --> 00:00:44,399 located just below orion's belt this 18 00:00:48,150 --> 00:00:46,320 nebula is one we can see with the 19 00:00:50,229 --> 00:00:48,160 unaided eye 20 00:00:53,590 --> 00:00:50,239 it also offers an excellent peak at 21 00:00:56,630 --> 00:00:53,600 stellar birth for those with telescopes 22 00:00:59,430 --> 00:00:56,640 this nebula is an enormous cloud of gas 23 00:01:01,029 --> 00:00:59,440 and dust where vast numbers of new stars 24 00:01:03,510 --> 00:01:01,039 are forged 25 00:01:06,149 --> 00:01:03,520 its bright central region is the home of 26 00:01:07,750 --> 00:01:06,159 four massive young stars that shape the 27 00:01:09,830 --> 00:01:07,760 nebula 28 00:01:12,550 --> 00:01:09,840 these four hefty stars are called the 29 00:01:15,350 --> 00:01:12,560 trapezium because they are arranged in a 30 00:01:17,590 --> 00:01:15,360 trapezoidal pattern 31 00:01:20,630 --> 00:01:17,600 ultraviolet light unleashed by these 32 00:01:22,789 --> 00:01:20,640 stars is carving a cavity in the nebula 33 00:01:25,030 --> 00:01:22,799 and disrupting the growth of hundreds of 34 00:01:27,429 --> 00:01:25,040 smaller stars 35 00:01:29,830 --> 00:01:27,439 this stunning hubble image offers the 36 00:01:31,270 --> 00:01:29,840 sharpest view of the orion nebula ever 37 00:01:34,230 --> 00:01:31,280 obtained 38 00:01:37,030 --> 00:01:34,240 created using 520 different hubble 39 00:01:38,149 --> 00:01:37,040 exposures taken in multiple wavelengths 40 00:01:40,870 --> 00:01:38,159 of light 41 00:01:42,630 --> 00:01:40,880 this mosaic contains over 1 billion 42 00:01:45,030 --> 00:01:42,640 pixels 43 00:01:46,310 --> 00:01:45,040 the image's orange color represents 44 00:01:49,510 --> 00:01:46,320 hydrogen 45 00:01:52,310 --> 00:01:49,520 green is oxygen and red represents both 46 00:01:54,230 --> 00:01:52,320 sulfur and observations made in infrared 47 00:01:56,389 --> 00:01:54,240 light 48 00:01:59,270 --> 00:01:56,399 while the orion nebula is in the midst 49 00:02:03,510 --> 00:01:59,280 of creating new stars other nebulae 50 00:02:06,230 --> 00:02:03,520 result from aging and dying stars 51 00:02:09,029 --> 00:02:06,240 this image of the cat's eye nebula shows 52 00:02:11,190 --> 00:02:09,039 a bull's-eye pattern of 11 or even more 53 00:02:13,589 --> 00:02:11,200 concentric rings 54 00:02:16,150 --> 00:02:13,599 each ring is actually the edge of a 55 00:02:18,869 --> 00:02:16,160 spherical bubble seen projected onto the 56 00:02:20,949 --> 00:02:18,879 sky that's why it appears bright along 57 00:02:23,589 --> 00:02:20,959 its outer edge 58 00:02:26,470 --> 00:02:23,599 observations suggest cat's eye was 59 00:02:29,990 --> 00:02:26,480 created when a medium-sized star ejected 60 00:02:31,750 --> 00:02:30,000 its mass in a series of pulses at 1500 61 00:02:34,630 --> 00:02:31,760 year intervals 62 00:02:37,270 --> 00:02:34,640 these convulsions created dust shells 63 00:02:40,070 --> 00:02:37,280 that form a layered concentric structure 64 00:02:42,390 --> 00:02:40,080 around the dying star 65 00:02:45,430 --> 00:02:42,400 the view from hubble is like seeing an 66 00:02:47,430 --> 00:02:45,440 onion cut in half where each skin layer 67 00:02:50,390 --> 00:02:47,440 appears as a ring 68 00:02:52,229 --> 00:02:50,400 each shell contains as much mass as all 69 00:02:54,949 --> 00:02:52,239 of the planets in our solar system 70 00:02:59,830 --> 00:02:57,430 then there are the supernova remnants 71 00:03:02,149 --> 00:02:59,840 like the crab nebula 72 00:03:04,630 --> 00:03:02,159 these nebulae are made of debris from 73 00:03:07,350 --> 00:03:04,640 exploded stars 74 00:03:10,390 --> 00:03:07,360 in the year 1054 a.d 75 00:03:12,790 --> 00:03:10,400 chinese astronomers recorded a guest 76 00:03:16,070 --> 00:03:12,800 star that was visible even in the 77 00:03:18,390 --> 00:03:16,080 daytime sky for nearly a month 78 00:03:20,710 --> 00:03:18,400 the guest star they observed was 79 00:03:23,589 --> 00:03:20,720 actually the supernova explosion that 80 00:03:26,309 --> 00:03:23,599 created the crab nebula 81 00:03:28,949 --> 00:03:26,319 today the crab nebula is still visible 82 00:03:31,990 --> 00:03:28,959 as a six light-year-wide remnant of that 83 00:03:34,710 --> 00:03:32,000 violent event 84 00:03:37,750 --> 00:03:34,720 this large mosaic of the crab nebula was 85 00:03:40,869 --> 00:03:37,760 assembled from 24 individual exposures 86 00:03:42,949 --> 00:03:40,879 captured by hubble over three months 87 00:03:45,670 --> 00:03:42,959 the orange filaments are the tattered 88 00:03:47,270 --> 00:03:45,680 remains of the star and consist mostly 89 00:03:50,470 --> 00:03:47,280 of hydrogen 90 00:03:52,710 --> 00:03:50,480 green is sulfur and red indicates doubly 91 00:03:55,030 --> 00:03:52,720 ionized oxygen 92 00:03:57,910 --> 00:03:55,040 these elements were expelled during the 93 00:04:00,470 --> 00:03:57,920 supernova explosion 94 00:04:03,429 --> 00:04:00,480 the leftover ultra dense core of the 95 00:04:06,149 --> 00:04:03,439 exploded star remains as a rapidly 96 00:04:08,309 --> 00:04:06,159 spinning neutron star in the center of 97 00:04:11,110 --> 00:04:08,319 the crab nebula 98 00:04:13,589 --> 00:04:11,120 electrons rolling at nearly the speed of 99 00:04:16,710 --> 00:04:13,599 light around the star's magnetic field 100 00:04:19,430 --> 00:04:16,720 lines produce the eerie blue light in 101 00:04:22,310 --> 00:04:19,440 the interior of the nebula 102 00:04:25,430 --> 00:04:22,320 the neutron star like a lighthouse 103 00:04:28,310 --> 00:04:25,440 ejects twin beams of radiation that make 104 00:04:31,510 --> 00:04:28,320 it appear to pulse 30 times per second 105 00:04:35,909 --> 00:04:33,670 nebulae are some of the most beautiful 106 00:04:38,870 --> 00:04:35,919 objects in our universe 107 00:04:41,510 --> 00:04:38,880 their incredible shapes and colors will 108 00:04:43,350 --> 00:04:41,520 always inspire humanity to keep looking 109 00:04:45,189 --> 00:04:43,360 up at the stars 110 00:04:47,990 --> 00:04:45,199 and with instruments like the hubble 111 00:04:50,469 --> 00:04:48,000 space telescope we will continue to be