1 00:00:00,135 --> 00:00:02,490 The following content is provided under a Creative 2 00:00:02,490 --> 00:00:04,030 Commons license. 3 00:00:04,030 --> 00:00:06,330 Your support will help MIT OpenCourseWare 4 00:00:06,330 --> 00:00:10,720 continue to offer high-quality educational resources for free. 5 00:00:10,720 --> 00:00:13,320 To make a donation or view additional materials 6 00:00:13,320 --> 00:00:17,280 from hundreds of MIT courses, visit MIT OpenCourseWare 7 00:00:17,280 --> 00:00:20,445 at ocw.mit.edu. 8 00:00:20,445 --> 00:00:22,080 MARK HARTMAN: We said that we had 9 00:00:22,080 --> 00:00:24,420 made an observation of what elements 10 00:00:24,420 --> 00:00:27,240 were present in the supernova remnant. 11 00:00:27,240 --> 00:00:30,600 And we can tell what elements were present by identifying 12 00:00:30,600 --> 00:00:33,360 which peaks were there. 13 00:00:33,360 --> 00:00:37,547 We know that each element gives off certain energies of photons 14 00:00:37,547 --> 00:00:39,630 that have to do with the difference between energy 15 00:00:39,630 --> 00:00:43,950 levels of the electrons, and the electrons are bouncing around. 16 00:00:43,950 --> 00:00:49,770 And we saw that we had a certain bunch of elements. 17 00:00:49,770 --> 00:00:51,750 And we said to ourselves, well, we also 18 00:00:51,750 --> 00:00:54,139 know something about supernova remnants. 19 00:00:54,139 --> 00:00:55,680 So we had this question, why would we 20 00:00:55,680 --> 00:00:58,590 expect to find these particular elements in a supernova 21 00:00:58,590 --> 00:00:59,430 remnant? 22 00:00:59,430 --> 00:01:01,320 And we came with two different models. 23 00:01:01,320 --> 00:01:02,820 One was the elements were already 24 00:01:02,820 --> 00:01:05,120 around the outside of the star somewhere. 25 00:01:05,120 --> 00:01:08,340 And when the star blew up, it kind of swept him up. 26 00:01:08,340 --> 00:01:10,080 The other model was that the elements 27 00:01:10,080 --> 00:01:12,700 were created inside the star. 28 00:01:12,700 --> 00:01:15,180 And when you guys read about star formation before, 29 00:01:15,180 --> 00:01:16,340 you read fusion-- 30 00:01:16,340 --> 00:01:19,470 the process of atoms being squished together 31 00:01:19,470 --> 00:01:24,230 in the middle of stars does produce new elements. 32 00:01:24,230 --> 00:01:25,110 OK? 33 00:01:25,110 --> 00:01:26,880 And indeed, somebody asked this question, 34 00:01:26,880 --> 00:01:30,870 how does another star use the elements left behind 35 00:01:30,870 --> 00:01:32,550 by the supernova? 36 00:01:32,550 --> 00:01:36,030 These are the elements left behind by the supernova. 37 00:01:36,030 --> 00:01:41,250 If a star is mostly made of hydrogen and other gases. 38 00:01:41,250 --> 00:01:44,020 That's a really good question. 39 00:01:44,020 --> 00:01:45,810 And we said that each of these models 40 00:01:45,810 --> 00:01:47,520 is going to make a prediction about what 41 00:01:47,520 --> 00:01:49,950 we would foresee if we observed the location 42 00:01:49,950 --> 00:01:52,910 of the different elements. 43 00:01:52,910 --> 00:01:56,520 We're going to look, because we essentially 44 00:01:56,520 --> 00:01:59,550 said that this first model, we expect to see the elements 45 00:01:59,550 --> 00:02:02,490 kind of further out, because they'd be pushed out of the way 46 00:02:02,490 --> 00:02:04,890 if they were on the surface of the star. 47 00:02:04,890 --> 00:02:09,270 Whereas here, we'd expect to see the elements spread everywhere 48 00:02:09,270 --> 00:02:13,122 because they were created inside the star. 49 00:02:13,122 --> 00:02:15,330 I'm not actually going to tell you which one of these 50 00:02:15,330 --> 00:02:23,280 is correct, because this is a perfect CAI research project. 51 00:02:23,280 --> 00:02:25,050 We're developing these questions-- 52 00:02:25,050 --> 00:02:26,580 these different models. 53 00:02:26,580 --> 00:02:29,650 When you do a project, you want to think about things this way. 54 00:02:29,650 --> 00:02:33,030 What I see-- why might I see this? 55 00:02:33,030 --> 00:02:35,250 Neither one of these is completely wrong. 56 00:02:35,250 --> 00:02:38,670 But neither one of these is completely right either. 57 00:02:38,670 --> 00:02:41,820 So it's going to be your job, as part of the CAI, 58 00:02:41,820 --> 00:02:44,160 to come up with some alternate models for what 59 00:02:44,160 --> 00:02:45,750 you think might be going on. 60 00:02:45,750 --> 00:02:47,310 We're going to give you the tools 61 00:02:47,310 --> 00:02:49,920 to find the answers for yourself. 62 00:02:49,920 --> 00:02:52,800 Now you started thinking about well, OK, maybe 63 00:02:52,800 --> 00:02:55,230 if I looked at where the elements were we 64 00:02:55,230 --> 00:02:56,550 could figure that out. 65 00:02:56,550 --> 00:02:59,630 That's actually a really interesting project.