1 00:00:01,045 --> 00:00:05,000 since we've been talking how stars formed and the evolution of stars 2 00:00:05,000 --> 00:00:08,638 i thought it was about time that we looked at some cool pictures of stars 3 00:00:08,638 --> 00:00:12,214 forming or stars themselves, or evolution of stars. 4 00:00:12,214 --> 00:00:23,600 so this right here is from the Eagle Nebula, 5 00:00:23,600 --> 00:00:30,883 Just so you know, the word Nebula is kind of a general word for any interstellar cloud of gas or dust 6 00:00:30,883 --> 00:00:34,133 so when we're talking about the Eagle nebula, we're actually talking about a huge nebula 7 00:00:34,133 --> 00:00:36,733 and actually, it's a nebula that expands. 8 00:00:36,733 --> 00:00:44,400 and so that you have a sense, this is just one of the pillars of the "Pillars of creation" 9 00:00:44,400 --> 00:00:48,133 This is just a small part of the actual Eagle Nebula 10 00:00:48,133 --> 00:00:52,467 And just this pillar right over here, just this pillar here 11 00:00:52,467 --> 00:01:01,400 so that you have a sense of how large it is, just this pillar itself is 7 light years 12 00:01:01,400 --> 00:01:04,551 it is 7 light years talls 13 00:01:04,551 --> 00:01:06,467 so this is an enormous amount of distance 14 00:01:06,467 --> 00:01:11,425 remember, the distance from earth to the nearest star was about 4 light years 15 00:01:11,425 --> 00:01:13,839 it would take voyager, if it were pointed in the right direction 16 00:01:13,839 --> 00:01:17,333 moving at 60 thousand kilometers per hour 17 00:01:17,333 --> 00:01:21,333 it would take Voyager 80 thousand years to go 4 light years 18 00:01:21,333 --> 00:01:24,822 just this pillar is 7 light years 19 00:01:24,822 --> 00:01:29,333 but i wanted to show you this because these type of nebulae, the plural of nebula 20 00:01:29,333 --> 00:01:32,160 are where stars can form. 21 00:01:32,160 --> 00:01:37,400 so this right here, you actually see, is actually a breeding ground for the birth of new stars 22 00:01:37,400 --> 00:01:41,933 this gas is condensing, just like we talked about a couple of videos ago. Until it gets to that critical 23 00:01:41,933 --> 00:01:45,333 temperature, the critical density, where you can actually get 24 00:01:45,333 --> 00:01:49,267 fusion of hydrogen 25 00:01:49,267 --> 00:01:53,933 so this is just a huge interstellar cloud of hydrogen gas 26 00:01:53,933 --> 00:01:59,200 and over here you can see its just this breeding ground for stars 27 00:01:59,200 --> 00:02:03,159 and we don't even, we think that this structure doesn't even exist anymore 28 00:02:03,159 --> 00:02:06,400 because remember, this thing is very very far away from us 29 00:02:06,400 --> 00:02:11,267 in fact is, just so you have the number, this thing is 7000 light years away 30 00:02:11,267 --> 00:02:17,416 7000 light years away 31 00:02:17,416 --> 00:02:23,867 which means that what we are seeing now, the photons that are reaching our eyes or telescopes right now 32 00:02:23,867 --> 00:02:28,492 left this region of space 7000 years ago 33 00:02:28,492 --> 00:02:31,133 so we're seeing it as it was 7000 years ago 34 00:02:31,133 --> 00:02:36,533 so a lot of this gas, a lot of this hydrogen, may have already condensed into many many more stars 35 00:02:36,533 --> 00:02:39,800 so the structure might not be the way it looks right now 36 00:02:39,800 --> 00:02:41,267 and actually there was another 37 00:02:41,267 --> 00:02:45,867 super nova that happened that might have blown away a lot of this stuff 38 00:02:45,867 --> 00:02:49,000 and we won't even be able to see the effects of this super nova 39 00:02:49,000 --> 00:02:51,085 for another thousand years 40 00:02:51,085 --> 00:02:53,600 but anyway, this is just a pretty amazing photograph in my opinion 41 00:02:53,600 --> 00:02:56,600 especially, and its beautiful at any scale 42 00:02:56,600 --> 00:02:59,067 and it's even more mindblowing when you think that this is 7, this is a structure 43 00:02:59,067 --> 00:03:02,200 that is 7 light years tall 44 00:03:02,200 --> 00:03:04,667 and this is really just part of the Eagle Nebula 45 00:03:04,667 --> 00:03:06,921 one of the pillars of creation 46 00:03:06,921 --> 00:03:13,236 this right here is a star field, and this is as we're looking towards the center of our galaxy 47 00:03:13,236 --> 00:03:13,933 the milkyway 48 00:03:13,933 --> 00:03:16,162 this is the Sagittarius star field 49 00:03:16,162 --> 00:03:20,267 the neat thing here you see is such a diversity in stars 50 00:03:20,267 --> 00:03:24,916 this is also kind of mind numbing because every one of these stars, are inside of our galaxy 51 00:03:24,916 --> 00:03:27,933 this is looking towards the center of our galaxy 52 00:03:27,933 --> 00:03:32,333 this isn't one of those where we're looking beyond our galaxy or looking at clusters of galaxies 53 00:03:32,333 --> 00:03:34,000 this is just stars here 54 00:03:34,000 --> 00:03:37,153 but the thing here is that you see a huge variety, you see some stars that are 55 00:03:37,153 --> 00:03:40,467 shining red, right over here 56 00:03:40,467 --> 00:03:42,819 and obviously, the apparent size, you cannot completely tell 57 00:03:42,819 --> 00:03:46,933 because the different stars are at different distances and at difference intensities 58 00:03:46,933 --> 00:03:52,933 but the redder stars, these are stars in their red giant phase 59 00:03:52,933 --> 00:03:55,400 or they're probably at their red giant phase 60 00:03:55,400 --> 00:03:57,333 i haven't done specific research on these stars 61 00:03:57,333 --> 00:03:58,957 but that's what we suspect 62 00:03:58,957 --> 00:04:00,467 those are in their red giant phase 63 00:04:00,467 --> 00:04:04,933 the ones that are kind of in the yellowish white part of the spectrum 64 00:04:04,933 --> 00:04:07,133 these are stars that are probably in their main sequence 65 00:04:07,133 --> 00:04:10,892 probably not too different than own sun 66 00:04:10,892 --> 00:04:16,348 the ones that are in the yellowish white, closer to orange-yellowish-white part of the spectrum 67 00:04:16,348 --> 00:04:22,641 and the ones that look a little more bluish, or a little bit more greenish 68 00:04:22,641 --> 00:04:24,986 these are burning super fast 69 00:04:24,986 --> 00:04:27,867 let me see if i can find, this one looks a little big bluish to me, 70 00:04:27,867 --> 00:04:34,800 these are burning super super fast, and so 71 00:04:34,800 --> 00:04:40,218 the super massive stars, they burn kind of fast and furious and then just die out 72 00:04:41,609 --> 00:04:43,000 but the smaller stars, the ones with less mass 73 00:04:43,000 --> 00:04:48,020 they burn slower over a much much longer period of time 74 00:04:48,020 --> 00:04:50,017 so the ones that are burning fast 75 00:04:50,017 --> 00:04:56,101 are emitting a lot of energy at the smaller wavelength part of the light spectrum 76 00:04:56,101 --> 00:05:00,267 that's why they look bluer or greener and these are going to be more massive stars 77 00:05:00,267 --> 00:05:03,438 the ones that look white or bluer or greener 78 00:05:03,438 --> 00:05:04,933 while the redder ones 79 00:05:04,933 --> 00:05:09,800 the redder ones are less massive stars that are kind of in their super giant phase 80 00:05:09,800 --> 00:05:14,000 and so they are at this point cooler than the main sequence stars 81 00:05:14,000 --> 00:05:18,333 this right here, this right here is the cat's eye nebula 82 00:05:18,333 --> 00:05:20,933 and the word nebula, this is actually a planetary nebula 83 00:05:20,933 --> 00:05:27,680 this one here is a planetary nebula 84 00:05:27,680 --> 00:05:34,019 and it's called a nebula because it is kind of this gas that's kinda floating out in space 85 00:05:34,019 --> 00:05:38,067 but it's at a completely different kind of scale than this Eagle nebula 86 00:05:38,067 --> 00:05:41,200 that we drew over here 87 00:05:41,200 --> 00:05:43,200 so when people talk about nebulas, they normally talking about something like the eagle nebula 88 00:05:43,200 --> 00:05:46,467 these huge masses of interstella gas 89 00:05:46,467 --> 00:05:51,318 when people talk about planetary nebulas; this is actually still a huge radius 90 00:05:51,318 --> 00:05:53,267 but no where near 7 light years 91 00:05:53,267 --> 00:05:59,538 but this is the bi-product of a star shedding all of its outer material 92 00:05:59,538 --> 00:06:03,400 so at the center of this, we see kind of a mature star here 93 00:06:03,400 --> 00:06:07,133 and it's shed of kind of its outer layers 94 00:06:07,133 --> 00:06:09,174 and it did that in its red giant phase 95 00:06:09,174 --> 00:06:12,733 so the core would keep flaring up, having these hot explosions 96 00:06:12,733 --> 00:06:18,485 and every time you have one of these hot explosions, you had more and more of its outer layers getting 97 00:06:18,485 --> 00:06:21,156 pushed off, pushed off into space 98 00:06:21,156 --> 00:06:23,467 forming this planetary nebula 99 00:06:23,467 --> 00:06:25,267 so this as we see it right now 100 00:06:25,267 --> 00:06:29,467 its still not yet a white dwarf, it is still an active star 101 00:06:29,467 --> 00:06:35,867 fusion is still occurring in this star, but it is well on its way onto becoming a a white dwarf 102 00:06:35,867 --> 00:06:37,502 once all its fuel runs out 103 00:06:37,502 --> 00:06:42,200 it's past its red giant phase, it's thrown all of this material into space and it's on its way onto becoming 104 00:06:42,200 --> 00:06:43,333 a white dwarf 105 00:06:43,333 --> 00:06:44,600 anyway hopefully you enjoyed that 106 00:06:44,600 --> 00:06:49,267 i actually find all of these images to be pretty captivating 107 00:06:49,267 --> 00:06:50,800 especially the star field one 108 00:06:50,800 --> 00:06:52,502 because this just inside of our galaxy 109 00:06:52,502 --> 00:06:55,933 hopefully it gives more appreciation for how many stars there are 110 00:06:55,933 --> 99:59:59,999 i mean this is just a small fraction of the 200 to 400 billion stars inside the milky way