1 00:00:22,420 --> 00:00:19,570 rosetta is a space mission on its way to 2 00:00:24,070 --> 00:00:22,430 observe comet churyumov-gerasimenko and 3 00:00:26,650 --> 00:00:24,080 we're gonna be studying that comet as it 4 00:00:30,790 --> 00:00:26,660 goes around the Sun in its comets 5 00:00:32,619 --> 00:00:30,800 journey our study of this comet will 6 00:00:34,689 --> 00:00:32,629 help to inform us about our biggest 7 00:00:36,759 --> 00:00:34,699 mysteries where did this comment form 8 00:00:39,700 --> 00:00:36,769 and what can this comet tell us about 9 00:00:41,560 --> 00:00:39,710 how our solar system formed the Rosetta 10 00:00:43,660 --> 00:00:41,570 mission will help us put the origins of 11 00:00:45,910 --> 00:00:43,670 the solar system into a galactic context 12 00:00:47,670 --> 00:00:45,920 we're interested in how we turn the gas 13 00:00:52,750 --> 00:00:47,680 and dust that was the early solar system 14 00:00:54,130 --> 00:00:52,760 into the solar system we see today in 15 00:00:55,959 --> 00:00:54,140 particular we're interested in how the 16 00:00:57,729 --> 00:00:55,969 planets acquire their compositions how 17 00:01:00,099 --> 00:00:57,739 do we make rocky planets how do we make 18 00:01:01,029 --> 00:01:00,109 gas giant planets icy planets and then 19 00:01:02,770 --> 00:01:01,039 we're also interested in the 20 00:01:04,270 --> 00:01:02,780 distribution of these planets which ones 21 00:01:05,950 --> 00:01:04,280 were migrating when during the 22 00:01:08,290 --> 00:01:05,960 construction of the solar system 23 00:01:15,070 --> 00:01:08,300 comets are key to understanding that 24 00:01:17,080 --> 00:01:15,080 kind of activity how did it all begin we 25 00:01:19,809 --> 00:01:17,090 start with this ginormous 26 00:01:22,330 --> 00:01:19,819 molecular cloud the molecules that form 27 00:01:25,180 --> 00:01:22,340 our solar systems and begin to condense 28 00:01:27,999 --> 00:01:25,190 together with a Sun protosun at the 29 00:01:30,130 --> 00:01:28,009 center and proto planets scattered 30 00:01:34,779 --> 00:01:30,140 throughout this dusty and completely 31 00:01:36,580 --> 00:01:34,789 filled disk and right at this time we 32 00:01:38,529 --> 00:01:36,590 start to ask ourselves where new 33 00:01:41,650 --> 00:01:38,539 chemicals introduced into our solar 34 00:01:42,729 --> 00:01:41,660 system at that early formative stage we 35 00:01:45,040 --> 00:01:42,739 think it has something to do with 36 00:01:47,830 --> 00:01:45,050 massive stars that are the sister stars 37 00:01:49,570 --> 00:01:47,840 to the Sun which throw out these giant 38 00:01:51,370 --> 00:01:49,580 winds and in these winds are these 39 00:01:53,440 --> 00:01:51,380 radioactive elements and it's these 40 00:01:55,029 --> 00:01:53,450 radioactive isotopes that tell us 41 00:01:57,790 --> 00:01:55,039 something about the birth environment of 42 00:02:00,639 --> 00:01:57,800 the Sun because of this connection with 43 00:02:02,979 --> 00:02:00,649 our sister stars we think that something 44 00:02:06,460 --> 00:02:02,989 happened to cause a whole bunch of 45 00:02:08,260 --> 00:02:06,470 debris to come rapidly forward from the 46 00:02:11,830 --> 00:02:08,270 outer solar system into the inner solar 47 00:02:12,640 --> 00:02:11,840 system and did that bring water to the 48 00:02:15,190 --> 00:02:12,650 inner solar 49 00:02:17,679 --> 00:02:15,200 but that have brought part of the 50 00:02:19,569 --> 00:02:17,689 composition of our oceans today on earth 51 00:02:20,860 --> 00:02:19,579 we need to know where that water came 52 00:02:23,259 --> 00:02:20,870 from to understand whether or not 53 00:02:25,420 --> 00:02:23,269 there's earths elsewhere in the galaxy 54 00:02:27,610 --> 00:02:25,430 we have a lot of questions about did we 55 00:02:29,830 --> 00:02:27,620 have planets moving around in the outer 56 00:02:32,130 --> 00:02:29,840 solar system it's possible to Uranus and 57 00:02:37,479 --> 00:02:32,140 Neptune actually swapped positions and 58 00:02:39,910 --> 00:02:37,489 excited dynamically the Kuiper belt was 59 00:02:42,280 --> 00:02:39,920 that the event that caused a huge amount 60 00:02:44,710 --> 00:02:42,290 of scattering that came forward and hit 61 00:02:47,589 --> 00:02:44,720 the inner solar system a second idea is 62 00:02:49,089 --> 00:02:47,599 perhaps Jupiter might have migrated all 63 00:02:51,069 --> 00:02:49,099 the way forward and then turned around 64 00:02:53,289 --> 00:02:51,079 and gone back out again to where it is 65 00:02:55,300 --> 00:02:53,299 now and it's exciting to think about the 66 00:02:56,610 --> 00:02:55,310 fact that the planets that we all learn 67 00:02:59,140 --> 00:02:56,620 in grade school you know where they are 68 00:03:00,819 --> 00:02:59,150 all lined up not because that's where 69 00:03:02,849 --> 00:03:00,829 they form but that's where they rested 70 00:03:06,250 --> 00:03:02,859 after a sort of violent beginning 71 00:03:08,740 --> 00:03:06,260 Rosetta will help us to either validate 72 00:03:10,780 --> 00:03:08,750 or refute some of these theories this is 73 00:03:13,539 --> 00:03:10,790 a window into our roofs literally how we 74 00:03:15,550 --> 00:03:13,549 get from star dust to people you get 75 00:03:17,589 --> 00:03:15,560 there through the solar system formation 76 00:03:18,939 --> 00:03:17,599 mechanisms to me the reason to 77 00:03:20,470 --> 00:03:18,949 understand the origins of solar system 78 00:03:22,960 --> 00:03:20,480 is to know whether or not we're normal 79 00:03:25,780 --> 00:03:22,970 well whether or not our solar system is 80 00:03:28,420 --> 00:03:25,790 a is a common phenomenon in the galaxy