1 00:00:00,010 --> 00:00:04,050 Marc Kuchner: I don't know--when I was growing up, there was no such thing as planets around 2 00:00:04,070 --> 00:00:08,110 other stars. If you were to talk about it at a scientific meeting, people would laugh at you. 3 00:00:08,130 --> 00:00:12,150 Not that I was talking at scientific meetings when I was in high school, but 4 00:00:12,170 --> 00:00:16,200 so I'm told. Music swells 5 00:00:24,300 --> 00:00:28,310 Jennifer Wiseman: Planets are very small compared 6 00:00:28,330 --> 00:00:32,330 to the stars that they orbit. They're also very dim. 7 00:00:32,350 --> 00:00:36,340 Marc Kuchner: For example, the Earth is ten billion times fainter 8 00:00:36,360 --> 00:00:40,420 than the Sun--ten billion times fainter. Jennifer Wiseman: It's kind of like 9 00:00:40,440 --> 00:00:44,490 trying to see a firefly next to a lighthouse. 10 00:00:44,510 --> 00:00:48,560 It gets lost in the glare. 11 00:00:48,580 --> 00:00:52,600 Marc Kuchner: The Hubble Space Telescope takes pictures of nearby 12 00:00:52,620 --> 00:00:56,630 stars and uses a special tool called a coronagraph 13 00:00:56,650 --> 00:01:00,650 and the coronagraph blocks out the light from the star. 14 00:01:00,670 --> 00:01:04,680 Aki Roberge: It's a fancy way of putting your thumb over the star, basically, so you can see 15 00:01:04,700 --> 00:01:08,690 something faint that is right next to it. 16 00:01:08,710 --> 00:01:12,710 Jennifer Wiseman: We can also use Hubble and other telescopes to study 17 00:01:12,730 --> 00:01:16,830 regions where we think planets might be forming. 18 00:01:16,850 --> 00:01:20,900 Marc Kuchner: We see in images from Hubble, we see these rings of dust 19 00:01:20,920 --> 00:01:24,970 around nearby stars. Aki Roberge: Well what I observe 20 00:01:24,990 --> 00:01:29,030 with Hubble are those disks. Those disks of gas 21 00:01:29,050 --> 00:01:33,070 and dust around the young stars, in which we think the dust grains 22 00:01:33,090 --> 00:01:37,110 are starting to clump together and build up into pebbles, 23 00:01:37,130 --> 00:01:41,140 rocks, asteroids, comets, Earths. 24 00:01:41,160 --> 00:01:45,160 Jennifer Wiseman: We're finding baby solar systems by using 25 00:01:45,180 --> 00:01:49,190 Hubble and other telescopes, including sort of ground-based radio telescopes 26 00:01:49,210 --> 00:01:53,200 that can peer into these disks around stars and 27 00:01:53,220 --> 00:01:57,260 see young planets or regions where young planetary systems 28 00:01:57,280 --> 00:02:01,340 are forming. Aki Roberge: The study of exoplanets is 29 00:02:01,360 --> 00:02:05,390 only a little over 15 years old. Marc Kuchner: We've discovered more 30 00:02:05,410 --> 00:02:09,440 than 400 extrasolar planets now. 31 00:02:09,460 --> 00:02:13,490 Aki Roberge: You know, we're still just beginning to 32 00:02:13,510 --> 00:02:17,530 understand how the processes that formed 33 00:02:17,550 --> 00:02:21,560 our own solar system, also formed these really diverse 34 00:02:21,580 --> 00:02:25,590 types of planets. I think the thing that excites me 35 00:02:25,610 --> 00:02:29,600 most is just the basic discovery of what 36 00:02:29,620 --> 00:02:33,670 exists. You know, what's out there. Waterworlds, carbon planets? 37 00:02:33,690 --> 00:02:37,750 It sounds like science fiction, but not really. 38 00:02:37,770 --> 00:02:41,830 Not anymore. Marc Kuchner: Why did life arise on 39 00:02:41,850 --> 00:02:45,890 Earth instead of somewhere else? 40 00:02:45,910 --> 00:02:49,940 I mean if there's another planet that could have life on it, 41 00:02:49,960 --> 00:02:53,970 why aren't we there? Music