1 00:00:00,060 --> 00:00:02,430 The following content is provided under a Creative 2 00:00:02,430 --> 00:00:03,820 Commons license. 3 00:00:03,820 --> 00:00:06,030 Your support will help MIT OpenCourseWare 4 00:00:06,030 --> 00:00:10,120 continue to offer high quality educational resources for free. 5 00:00:10,120 --> 00:00:12,660 To make a donation or to view additional materials 6 00:00:12,660 --> 00:00:16,620 from hundreds of MIT courses, visit MIT OpenCourseWare 7 00:00:16,620 --> 00:00:17,900 at ocw.mit.edu. 8 00:00:20,234 --> 00:00:21,900 SPEAKER 1: Hi, my name is Azeith and I'm 9 00:00:21,900 --> 00:00:23,560 part of the CIA program-- 10 00:00:23,560 --> 00:00:25,250 CAI program. 11 00:00:25,250 --> 00:00:28,150 SPEAKER 2: I'm Panteli and I'm also part of the CAI program. 12 00:00:28,150 --> 00:00:32,070 SPEAKER 1: Today, we're here to talk about luminously and flux. 13 00:00:32,070 --> 00:00:35,070 And I'll start off with explaining luminosity. 14 00:00:35,070 --> 00:00:38,332 Luminosity is light given by the source. 15 00:00:38,332 --> 00:00:39,790 And it has to go-- it has to travel 16 00:00:39,790 --> 00:00:43,110 through [INAUDIBLE] degrees in order 17 00:00:43,110 --> 00:00:49,484 to get to the detector, which my friend here will explain. 18 00:00:49,484 --> 00:00:51,150 SPEAKER 2: Flux is the amount of photons 19 00:00:51,150 --> 00:00:53,970 being received by the detector. 20 00:00:53,970 --> 00:00:55,800 As you can see in the drawing, the arrows 21 00:00:55,800 --> 00:00:58,430 represent the photons being released by the source. 22 00:00:58,430 --> 00:01:00,255 The clouds are these lines right here. 23 00:01:00,255 --> 00:01:02,130 And when the photons pass through the clouds, 24 00:01:02,130 --> 00:01:04,879 a lot of them are either blocked or absorbed by the cloud. 25 00:01:04,879 --> 00:01:07,150 So only a minimal amount of photons 26 00:01:07,150 --> 00:01:09,680 are able to reach the detector. 27 00:01:09,680 --> 00:01:11,330 So I'm Panteli. 28 00:01:11,330 --> 00:01:11,940 He's Azeith. 29 00:01:11,940 --> 00:01:15,650 And we just explained what luminosity and flux are.