WEBVTT FILE 1 00:00:00.050 --> 00:00:04.270 [No Audio] 2 00:00:04.290 --> 00:00:08.290 What we're seeing here is a deep 3 00:00:08.310 --> 00:00:12.300 look at a newborn star. So we're looking with some of Hubble's 4 00:00:12.320 --> 00:00:16.330 instruments, its cameras, at a small region in the Orion star-forming region. 5 00:00:16.350 --> 00:00:20.510 We're seeing a baby star with material that's collapsing onto the star from gravity. 6 00:00:20.530 --> 00:00:24.520 And it's causing jets of material to spew out its poles, a bipolar 7 00:00:24.540 --> 00:00:28.550 outflow at supersonic speeds. It looks like a double-bladed "lightsaber." 8 00:00:28.570 --> 00:00:32.740 [No audio] 9 00:00:32.760 --> 00:00:36.760 [Laughing] Hubble has never actually seen 10 00:00:36.780 --> 00:00:40.780 a 'Death Star' as you see in Star Wars. But we certainly 11 00:00:40.800 --> 00:00:44.810 are able to look at regions where stars are in their death throws. 12 00:00:44.830 --> 00:00:48.890 And those are some of the most beautiful image that Hubble has captured because as 13 00:00:48.910 --> 00:00:53.070 stars die they spew material out into the interstellar medium. 14 00:00:53.090 --> 00:00:57.100 They're actually enriching the area around them. And when new stars form the chemicals 15 00:00:57.120 --> 00:01:01.160 that come from the older stars are in the mix of the new stars. 16 00:01:01.180 --> 00:01:05.210 So you're seeing some stars as they're spewing out their last layers 17 00:01:05.230 --> 00:01:09.240 calmly and others supernova remnants as the star explodes. And when we 18 00:01:09.260 --> 00:01:13.270 have a supernova explosion happening that's the type of force that would 19 00:01:13.290 --> 00:01:17.430 anilate planets around it just like a death star might. 20 00:01:17.450 --> 00:01:21.450 [No audio] 21 00:01:21.470 --> 00:01:25.470 The future for Hubble is very bright. It was serviced by astronauts 22 00:01:25.490 --> 00:01:29.490 five times on orbit, most recently in 2009. 23 00:01:29.510 --> 00:01:33.530 left it at the peak of its scientific capabilities. And we're working hard 24 00:01:33.550 --> 00:01:37.540 on the ground to keep it going until the year 2020 and beyond. We want to have 25 00:01:37.560 --> 00:01:41.540 some overlap time with the next thing, the James Webb Space Telescope 26 00:01:41.560 --> 00:01:45.570 which will launch in 2018 and will take pictures in the infrared 27 00:01:45.590 --> 00:01:49.620 beyond the visible. And when we're able to peer inside regions with the visible 28 00:01:49.640 --> 00:01:53.640 and the infrared we're really going to be able to uncover the layers and see what's 29 00:01:53.660 --> 00:01:57.660 going on in there. [No audio] 30 00:01:57.680 --> 00:02:01.840 [No audo] That's a great 31 00:02:01.860 --> 00:02:05.870 question. Of course Star Wars showed us a variety of worlds. Ice worlds 32 00:02:05.890 --> 00:02:09.900 forest worlds, desert worlds. And Hubble has been able to look at some 33 00:02:09.920 --> 00:02:13.920 of the worlds in our own solar system, right around our own backyard. So we've 34 00:02:13.940 --> 00:02:17.940 looked at Mars and seen storms there. We're looked at Jupiter. We see Jupiter 35 00:02:17.960 --> 00:02:21.980 evolving. We see the cloud structures on it evolving, the great red spot 36 00:02:22.000 --> 00:02:25.980 shrinking. We see evidence for water oceans on the 37 00:02:26.000 --> 00:02:30.010 moons around Jupiter just like there were moons where there was civilizations 38 00:02:30.030 --> 00:02:34.030 in Star Wars. We're seeing moons with water in our own solar system. 39 00:02:34.050 --> 00:02:38.060 And we're also starting to take those first steps beyond and look at planets around other stars. 40 00:02:38.080 --> 00:02:42.250 with Hubble. 41 00:02:42.270 --> 00:02:46.270 [No audio] So we're actually with Hubble 42 00:02:46.290 --> 00:02:50.280 able to get a real sense of the life cycles of galaxies through the history 43 00:02:50.300 --> 00:02:54.300 of the universe. We're now learning that galaxies commonly collide 44 00:02:54.320 --> 00:02:58.340 and that there's a certain sequence. You know younger galaxies look 45 00:02:58.360 --> 00:03:02.530 very different than the galaxies around us today, the more modern galaxies 46 00:03:02.550 --> 00:03:06.550 And it's the same concept when we look inside of our own galaxy. 47 00:03:06.570 --> 00:03:10.600 at the star forming regions or where stars have died. We're looking at the 48 00:03:10.620 --> 00:03:14.620 life cycle of stars and we're getting this beautiful coherent picture together 49 00:03:14.640 --> 00:03:18.810 of how the sun formed, the solar system and what that 50 00:03:18.830 --> 00:03:22.860 means in the place and context of everything else in the universe when it formed and how it 51 00:03:22.880 --> 00:03:26.860 evolves. 52 00:03:26.880 --> 00:03:30.870 [No audio] Well there's a vast archive 53 00:03:30.890 --> 00:03:34.910 of images at nasa.gov/hubble. 54 00:03:34.930 --> 00:03:38.081 Anything from the solar system all the way out to the edges of the universe.