1 00:00:07,173 --> 00:00:10,443 What we're looking at here is one of the first images that Hubble took, 2 00:00:10,477 --> 00:00:13,613 trying to answer the question of how common is planet formation? 3 00:00:13,880 --> 00:00:18,651 Thirty objects in the Orion star forming region that has lots of stars in formation, 4 00:00:18,651 --> 00:00:19,552 a young system. 5 00:00:19,652 --> 00:00:23,223 Each one of these is an example of material around a young star 6 00:00:23,223 --> 00:00:25,959 that looks to be forming a planetary system. 7 00:00:26,559 --> 00:00:29,763 We know the material there is consistent with what planets 8 00:00:29,763 --> 00:00:31,398 formed from in our solar system. 9 00:00:31,398 --> 00:00:34,968 And now what we're seeing is evidence that there are disks of material 10 00:00:34,968 --> 00:00:38,872 in this case, the disk is absorbing the light coming from behind. 11 00:00:38,872 --> 00:00:41,141 It's a shadow, basically. There's another one. 12 00:00:41,141 --> 00:00:44,144 In other cases, the light from the star itself is lighting up the disk. 13 00:00:44,210 --> 00:00:46,513 So this is a really tantalizing image. 14 00:00:46,513 --> 00:00:48,314 In the early days of Hubble, it was showing us 15 00:00:48,314 --> 00:00:51,718 that when we really took a peering look at what we could do with Hubble 16 00:00:51,718 --> 00:00:55,488 at protoplanetary systems, it started to see disks everywhere 17 00:00:55,588 --> 00:00:58,391 that looked like they could be forming planetary systems. 18 00:01:00,060 --> 00:01:03,263 One of the most exciting things about this composite image in my mind 19 00:01:03,263 --> 00:01:07,734 is the diversity of young systems that are forming planets. 20 00:01:09,402 --> 00:01:13,807 When Hubble launched, the only real observational database 21 00:01:13,807 --> 00:01:17,410 we had to infer planet formation models was our own solar system. 22 00:01:17,844 --> 00:01:21,281 We've got the four rocky planets, the interior, terrestrial planets, 23 00:01:21,381 --> 00:01:24,350 Mercury, Venus, Earth and Mars. 24 00:01:24,350 --> 00:01:28,521 And then you've got the gas giants Jupiter, Saturn, Uranus and Neptune. 25 00:01:28,788 --> 00:01:32,292 And then you've got a whole bunch of comets, asteroids, smaller bodies. 26 00:01:32,525 --> 00:01:35,462 So having all that stuff here in our solar system 27 00:01:35,462 --> 00:01:37,664 allowed us to come up with planet formation models. 28 00:01:38,264 --> 00:01:41,167 The only thing we could really test them on was our own solar system. 29 00:01:41,167 --> 00:01:42,769 Now, let's fast forward to today. 30 00:01:42,769 --> 00:01:46,940 We now know that there's a planet around every star in general, at least one. 31 00:01:47,540 --> 00:01:49,309 We've discovered so many planets 32 00:01:49,309 --> 00:01:52,879 we can use Hubble to look at their atmospheres, 33 00:01:52,879 --> 00:01:55,048 which is something that was never, ever designed to do. 34 00:01:55,048 --> 00:01:58,485 Look at an atmosphere of a planet outside of our solar system. 35 00:01:59,986 --> 00:02:03,490 And look in detail at these disks to start to tease 36 00:02:03,490 --> 00:02:07,093 out the fingerprints and atmospheres of planets around other stars. 37 00:02:07,293 --> 00:02:08,795 It's kind of mind blowing. 38 00:02:09,229 --> 00:02:12,665 And that's been a really exciting area of astrophysics since Hubble launched. 39 00:02:15,001 --> 00:02:17,237 So the thing that's really cool about this image, it was sort of 40 00:02:17,237 --> 00:02:21,207 like the beginning of putting the pieces together, observationally 41 00:02:21,274 --> 00:02:25,645 of exoplanet science, planet formation around stars other than the sun.