1 00:00:08,230 --> 00:00:06,309 the space between stars holds an array 2 00:00:11,270 --> 00:00:08,240 of vibrant clouds 3 00:00:15,669 --> 00:00:11,280 clouds that command our attention 4 00:00:17,830 --> 00:00:15,679 clouds that create spectacular displays 5 00:00:19,349 --> 00:00:17,840 clouds that seem familiar 6 00:00:21,590 --> 00:00:19,359 tenuous 7 00:00:24,630 --> 00:00:21,600 and fragile 8 00:00:26,310 --> 00:00:24,640 clouds that hold clues to star birth and 9 00:00:28,710 --> 00:00:26,320 death 10 00:00:32,310 --> 00:00:28,720 nasa's hubble space telescope has imaged 11 00:00:35,510 --> 00:00:32,320 hundreds of them in extraordinary detail 12 00:00:37,590 --> 00:00:35,520 these vast swirls of gas and dust get 13 00:00:40,229 --> 00:00:37,600 their name from the latin word nebula 14 00:00:42,869 --> 00:00:40,239 meaning cloud or mist 15 00:00:46,069 --> 00:00:42,879 nebulae is the plural of nebula and they 16 00:00:47,670 --> 00:00:46,079 come in a wide range of shapes sizes and 17 00:00:50,069 --> 00:00:47,680 forms 18 00:00:51,750 --> 00:00:50,079 emission nebulae are some of the most 19 00:00:54,950 --> 00:00:51,760 spectacular 20 00:00:58,630 --> 00:00:54,960 these opaque gleaming clouds of gas and 21 00:01:00,790 --> 00:00:58,640 dust radiate or emit their own light 22 00:01:03,270 --> 00:01:00,800 ultraviolet light from nearby stars 23 00:01:05,990 --> 00:01:03,280 energizes atoms in the cloud 24 00:01:07,590 --> 00:01:06,000 when the excited atoms lose that energy 25 00:01:10,230 --> 00:01:07,600 they release the light that gives 26 00:01:12,230 --> 00:01:10,240 emission nebulae their glow the orion 27 00:01:14,469 --> 00:01:12,240 nebula is one of the most famous 28 00:01:17,910 --> 00:01:14,479 emission nebulae 29 00:01:20,230 --> 00:01:17,920 its core called the trapezium holds four 30 00:01:23,350 --> 00:01:20,240 enormous young stars whose ultraviolet 31 00:01:25,429 --> 00:01:23,360 light powers the region's intense glow 32 00:01:27,830 --> 00:01:25,439 the carina nebula is another vast 33 00:01:29,990 --> 00:01:27,840 emission nebula and star-forming region 34 00:01:32,149 --> 00:01:30,000 in our galaxy 35 00:01:35,190 --> 00:01:32,159 within the nebula is a pillar three 36 00:01:38,069 --> 00:01:35,200 light-years tall dubbed mystic mountain 37 00:01:41,109 --> 00:01:38,079 it cloaks massive young stars some with 38 00:01:43,590 --> 00:01:41,119 jets emerging from the cloud 39 00:01:46,069 --> 00:01:43,600 hubble's infrared view cuts through the 40 00:01:49,670 --> 00:01:46,079 shroud of gas and dust revealing these 41 00:01:53,990 --> 00:01:51,670 reflection nebulae shine by the 42 00:01:56,230 --> 00:01:54,000 reflected or scattered light of nearby 43 00:01:58,310 --> 00:01:56,240 stars 44 00:02:00,389 --> 00:01:58,320 they often have a bluish color because 45 00:02:02,389 --> 00:02:00,399 the dust grains in the clouds scatter 46 00:02:05,270 --> 00:02:02,399 blue light more efficiently than red 47 00:02:11,830 --> 00:02:08,869 not all nebulae shine brightly dark or 48 00:02:14,070 --> 00:02:11,840 absorption nebulae are inky black clouds 49 00:02:16,470 --> 00:02:14,080 of gas and dust that block the light 50 00:02:19,030 --> 00:02:16,480 coming from objects behind them 51 00:02:20,470 --> 00:02:19,040 because they are dark absorption nebulae 52 00:02:22,790 --> 00:02:20,480 are hard to find 53 00:02:27,030 --> 00:02:22,800 we only see them as silhouettes against 54 00:02:32,070 --> 00:02:29,670 most large nebulae are a combination of 55 00:02:34,949 --> 00:02:32,080 emission reflection and absorption 56 00:02:36,949 --> 00:02:34,959 nebulae their dark dust lanes may give 57 00:02:40,869 --> 00:02:36,959 birth to new stars that provide the 58 00:02:43,270 --> 00:02:40,879 light needed to illuminate the cloud 59 00:02:45,270 --> 00:02:43,280 planetary nebulae are a type of emission 60 00:02:48,309 --> 00:02:45,280 nebula powered by a small to 61 00:02:50,630 --> 00:02:48,319 medium-sized dying star 62 00:02:54,070 --> 00:02:50,640 as these stars run out of fuel they 63 00:02:56,790 --> 00:02:54,080 periodically blow off their outer layers 64 00:02:59,350 --> 00:02:56,800 the expelled gas expands outward away 65 00:03:01,110 --> 00:02:59,360 from the star forming a bubble or shell 66 00:03:03,670 --> 00:03:01,120 around the star 67 00:03:06,149 --> 00:03:03,680 sometimes the envelope of debris holds 68 00:03:09,990 --> 00:03:06,159 clumps of dense gas that shine like the 69 00:03:15,110 --> 00:03:13,350 the term planetary nebula is misleading 70 00:03:17,110 --> 00:03:15,120 it comes from late 18th century 71 00:03:19,270 --> 00:03:17,120 astronomers who thought their rounded 72 00:03:21,990 --> 00:03:19,280 shape looked similar to planets and 73 00:03:24,789 --> 00:03:22,000 telescopes of that time 74 00:03:27,030 --> 00:03:24,799 they named them planetary nebulae as a 75 00:03:29,110 --> 00:03:27,040 result 76 00:03:31,830 --> 00:03:29,120 supernova remnants are the diffused 77 00:03:35,030 --> 00:03:31,840 clouds of expanding debris released by a 78 00:03:38,869 --> 00:03:35,040 massive star's death explosion 79 00:03:42,550 --> 00:03:38,879 the cygnus loop is a vast expanding 110 80 00:03:44,630 --> 00:03:42,560 light year wide supernova remnant 81 00:03:48,710 --> 00:03:44,640 it is so large that hubble can only 82 00:03:53,990 --> 00:03:50,789 some supernova remnants emit their light 83 00:03:56,710 --> 00:03:54,000 from a shell of shocked material 84 00:03:58,550 --> 00:03:56,720 others like the crab nebula emit most of 85 00:04:00,470 --> 00:03:58,560 their light from within the expanding 86 00:04:02,949 --> 00:04:00,480 shell 87 00:04:06,390 --> 00:04:02,959 and still other supernova remnants shine 88 00:04:08,949 --> 00:04:06,400 as a combination of the two 89 00:04:10,789 --> 00:04:08,959 nebulae are some of the most resplendent 90 00:04:12,949 --> 00:04:10,799 objects in the universe 91 00:04:14,789 --> 00:04:12,959 and thanks to the hubble space telescope