1 00:00:09,450 --> 00:00:12,789 [Music] 2 00:00:20,230 --> 00:00:15,110 these beautiful colorful images that 3 00:00:24,390 --> 00:00:21,750 i love them they're colorful they're 4 00:00:30,550 --> 00:00:24,400 beautiful but they're signposts of star 5 00:00:34,150 --> 00:00:32,709 the reason these gas clouds are so 6 00:00:36,150 --> 00:00:34,160 colorful 7 00:00:38,630 --> 00:00:36,160 is that there are massive stars bigger 8 00:00:41,830 --> 00:00:38,640 than our sun that have recently formed 9 00:00:44,470 --> 00:00:41,840 recently in a in a cosmic sense 10 00:00:47,029 --> 00:00:44,480 but perhaps within the last million 11 00:00:49,350 --> 00:00:47,039 years or so these stars have coalesced 12 00:00:51,510 --> 00:00:49,360 and their radiation is so powerful that 13 00:00:59,110 --> 00:00:51,520 it goes out and ionizes the surrounding 14 00:01:03,430 --> 00:01:00,950 so astronomers see these colorful 15 00:01:05,350 --> 00:01:03,440 nebulae such that hubble reveals in 16 00:01:07,590 --> 00:01:05,360 great detail and we say oh that's 17 00:01:09,670 --> 00:01:07,600 beautiful but we also say aha that's a 18 00:01:11,750 --> 00:01:09,680 sign that star formation is still active 19 00:01:14,469 --> 00:01:11,760 in this region we can hone in with 20 00:01:16,149 --> 00:01:14,479 hubble and other telescopes and see 21 00:01:18,550 --> 00:01:16,159 exactly what's going on in the 22 00:01:19,749 --> 00:01:18,560 continuation of star formation in these 23 00:01:21,590 --> 00:01:19,759 regions 24 00:01:23,749 --> 00:01:21,600 we didn't really realize when hubble was 25 00:01:25,830 --> 00:01:23,759 launched that we could see such details 26 00:01:28,149 --> 00:01:25,840 about the dynamics of continuing star 27 00:01:29,670 --> 00:01:28,159 formation and that's something that now 28 00:01:31,590 --> 00:01:29,680 people love hubble for are these 29 00:01:41,310 --> 00:01:31,600 beautiful images of activity in our