1 00:00:01 --> 00:00:07 The following content is provided under a Creative 2 00:00:04 --> 00:00:10 Commons license. Your support will help MIT 3 00:00:06 --> 00:00:12 OpenCourseWare continue to offer high-quality educational 4 00:00:09 --> 00:00:15 resources for free. To make a donation or view 5 00:00:13 --> 00:00:19 additional materials from hundreds of MIT courses, 6 00:00:17 --> 00:00:23 visit MIT OpenCourseWare at ocw.mit.edu. 7 00:00:21 --> 00:00:27 Well, the goal is to introduce the students for the first time 8 00:00:26 --> 00:00:32 to physics. That's to say calculus-based 9 00:00:30 --> 00:00:36 physics. Many students have already had 10 00:00:33 --> 00:00:39 some of that in high school, but many have not. 11 00:00:35 --> 00:00:41 And 8.01, the first course of physics, covers Newtonian 12 00:00:39 --> 00:00:45 Mechanics which is at the heart of the course. 13 00:00:43 --> 00:00:49 Depending upon the lecturer, we also cover Fluid Mechanics a 14 00:00:48 --> 00:00:54 little, and we cover a little of the Kinetic Gas Theory. 15 00:00:52 --> 00:00:58 Well, this course is a general Institute requirement. 16 00:00:55 --> 00:01:01 You either have to take this course or you have to take one 17 00:00:59 --> 00:01:05 that is slightly higher level which we call 8.012. 18 00:01:02 --> 00:01:08 We evaluate the students through traditional exams. 19 00:01:07 --> 00:01:13 The lectures are given in the main lecture hall of MIT, 20 00:01:11 --> 00:01:17 26-100. And then the students meet in 21 00:01:14 --> 00:01:20 small groups with professors. We call those recitations, 22 00:01:19 --> 00:01:25 which is largely problem solving. 23 00:01:21 --> 00:01:27 I would like to think that every lecture is an event. 24 00:01:25 --> 00:01:31 And, where possible, I go outside the standard 25 00:01:28 --> 00:01:34 curriculum. I talk about neutron stars. 26 00:01:32 --> 00:01:38 I talk about black holes. I talk about Big Bang 27 00:01:37 --> 00:01:43 cosmology. In a very natural way do I 28 00:01:40 --> 00:01:46 introduce musical instruments. I talk about supernova 29 00:01:44 --> 00:01:50 explosions. And then, during my last 30 00:01:47 --> 00:01:53 lecture, I introduce students to my 31 00:01:50 --> 00:01:56 research, the research I did during my 32 00:01:53 --> 00:01:59 early days at MIT when I made observations, 33 00:01:57 --> 00:02:03 astronomical observations in x-rays from very high-flying 34 00:02:01 --> 00:02:07 balloons. Those balloons are giant in 35 00:02:03 --> 00:02:09 size, sort of the size of the Empire State Building, 36 00:02:07 --> 00:02:13 and they went up to an altitude of about 145,000 feet. 37 00:02:11 --> 00:02:17 And that is my last lecture. And all of these lectures are 38 00:02:15 --> 00:02:21 really events. Well, the course material on 39 00:02:18 --> 00:02:24 OCW are my lectures in addition to being the standard material 40 00:02:22 --> 00:02:28 that you expect from Newtonian Mechanics, 41 00:02:25 --> 00:02:31 from Fluid Mechanics and from Kinetic Gas Theory. 42 00:02:29 --> 00:02:35 As I mentioned earlier, I try, where possible, 43 00:02:32 --> 00:02:38 to go a little bit beyond that and to make them see through the 44 00:02:36 --> 00:02:42 equations. And, by doing that, 45 00:02:39 --> 00:02:45 I make them aware of the environment of neutron stars, 46 00:02:43 --> 00:02:49 of black holes, of supernova explosions, 47 00:02:46 --> 00:02:52 of musical instruments. I only do that where it comes 48 00:02:49 --> 00:02:55 naturally, but there are many places where it comes naturally. 49 00:02:52 --> 00:02:58 So my goal is not so much to cover a lot and to make them 50 00:02:58 --> 00:03:04 chew on a lot of equations. But my goal is to uncover 51 00:03:02 --> 00:03:08 several very basic things that they will remember for the rest 52 00:03:07 --> 00:03:13 of their lives. Even if they never need physics 53 00:03:10 --> 00:03:16 anymore, I want them to see the beauty of physics; 54 00:03:14 --> 00:03:20 I want them to love physics.