1 00:00:00,200 --> 00:00:02,664 In the video on black holes 2 00:00:02,664 --> 00:00:08,233 several people asked what is actually a pretty good question, which is: If the mass of 3 00:00:08,233 --> 00:00:11,958 say a black hole is only 2 or 3 solar masses, 4 00:00:11,958 --> 00:00:16,459 why is the gravity so strong? Obviously the sun's gravity isn't so strong 5 00:00:16,459 --> 00:00:21,877 that it keeps light from escaping. So, why would something or even a star that is 2 or 3 solar masses, 6 00:00:21,915 --> 00:00:24,800 it's gravity isn't so strong that it keeps light from escaping 7 00:00:24,800 --> 00:00:30,400 why would a black hole that has the same mass keep light from escaping? 8 00:00:30,431 --> 00:00:32,892 And to understand that, let's just think a little bit about it. 9 00:00:33,002 --> 00:00:35,660 I'll just do a Newtonian 10 00:00:35,756 --> 00:00:37,623 classical physics right here. 11 00:00:37,623 --> 00:00:40,187 I wont get into the whole general relativity and things. 12 00:00:40,187 --> 00:00:45,287 This will really just give us the intuition of why a smaller, denser thing with the same mass 13 00:00:45,515 --> 00:00:48,638 can exert a stronger gravitational pull. 14 00:00:48,638 --> 00:00:52,005 So let's imagine-- so let's take two examples 15 00:00:52,215 --> 00:00:58,190 Let's say I have some star here 16 00:00:58,238 --> 00:01:02,292 that has a mass-- let's just call that mass m1 17 00:01:02,446 --> 00:01:08,207 and let's say that its radius, 18 00:01:08,207 --> 00:01:10,551 lets just call this "r" 19 00:01:10,608 --> 00:01:12,327 and lets say that I have 20 00:01:12,327 --> 00:01:16,363 some other mass right at the surface 21 00:01:16,363 --> 00:01:19,458 of this star. Somehow able to survive those surface temperatures 22 00:01:19,489 --> 00:01:21,704 and this mass over here 23 00:01:21,704 --> 00:01:25,041 has a mass of m2. 24 00:01:25,250 --> 00:01:32,574 The Universal Law of Gravitation tells us that the force between these two 25 00:01:32,574 --> 00:01:38,595 masses is going to be equal to the gravitational constant 26 00:01:38,747 --> 00:01:41,217 times the product of the masses. 27 00:01:41,464 --> 00:01:48,100 So m1 times m2 28 00:01:48,100 --> 00:01:52,974 all of that over the square of the distance 29 00:01:53,051 --> 00:01:54,045 "r" squared. 30 00:01:54,045 --> 00:01:57,734 Now, let me be very clear.You might say: Wait, this magenta mass 31 00:01:57,911 --> 00:01:59,878 right here is touching this larger mass. 32 00:01:59,878 --> 00:02:01,270 Isn't the distance 0? 33 00:02:01,270 --> 00:02:02,608 You need to be very careful! 34 00:02:02,608 --> 00:02:06,415 This is the distance between their center of masses. 35 00:02:06,487 --> 00:02:14,118 So the center of mass of this large mass over here is "r" away from this mass on the surface 36 00:02:14,118 --> 00:02:16,723 Now, with that said, let's take another example. 37 00:02:17,264 --> 00:02:22,974 Let's say this large massive star or whatever it might be, eventually condenses 38 00:02:22,974 --> 00:02:26,630 into something a thousand times smaller. 39 00:02:26,630 --> 00:02:31,354 So let me draw it like this.Obviosly I'm not drawing it to scale. 40 00:02:31,354 --> 00:02:36,519 So let's say we have another case like this (I'm not drawing it to scale) 41 00:02:36,581 --> 00:02:40,379 So this object, maybe it's the same object or maybe it's a different object, 42 00:02:40,379 --> 00:02:47,592 but it has the exactly same mass as larger object, but now has a much smaller radius. 43 00:02:47,685 --> 00:02:57,213 So that radius now is 1/1000.Let's say it's 1/1000 of this radius over here. 44 00:02:57,213 --> 00:03:04,598 So it's r/1000.If this had a million kilometer radius, 45 00:03:04,598 --> 00:03:08,731 so that will make it roughly about twice the radius of the sun. 46 00:03:08,731 --> 00:03:11,571 And this was a million kilometer radius right over here. 47 00:03:11,571 --> 00:03:14,131 This would be a thousand kilometer radius, 48 00:03:14,131 --> 00:03:18,444 so maybe we are talking about something that is approaching a neutron star. 49 00:03:18,444 --> 00:03:22,377 But we don't have to think about what it actually is,just think about the thought experiment here. 50 00:03:22,392 --> 00:03:25,808 So,let's say I have this thing over here and let's say I have something 51 00:03:25,808 --> 00:03:31,685 on the surface of this.So let's say I have the same mass that's on the surface of this thing. 52 00:03:31,685 --> 00:03:34,777 So, this is m2 right over here. 53 00:03:34,777 --> 00:03:39,992 So, what's going to be the force between these 2 masses? 54 00:03:39,992 --> 00:03:47,915 What's the force pulling them together?So that's the Universal Law of Gravitation again. 55 00:03:47,915 --> 00:03:52,229 The force, let's just call this F1(force 1) and let's just call this F2(force 2). 56 00:03:52,229 --> 00:03:56,838 Once again, it's going to be the gravitation constant, times the product of the masses 57 00:03:56,838 --> 00:04:05,798 So, the big m1, times the smaller mass m2, all of that over this distance squared. 58 00:04:05,798 --> 00:04:07,115 This radius squared. 59 00:04:07,115 --> 00:04:09,638 Remember, it's the distance to the center of masses. 60 00:04:09,638 --> 00:04:12,152 This center of mass here we are considering m2 to the kind of view 61 00:04:12,152 --> 00:04:13,759 just to point match right over there. 62 00:04:13,759 --> 00:04:15,659 So what's the radius squared? 63 00:04:15,659 --> 00:04:22,367 It's going to be "r" over 1 thousand squared ( r/(1000^2)). 64 00:04:22,367 --> 00:04:24,782 Or, if we simplify this,what would this be? 65 00:04:24,782 --> 00:04:35,090 This is the same thing as the gravitational constant times m1 times m2 66 00:04:35,090 --> 00:04:46,469 over "r" squared over 1 thousand squared or over 1 million.That's just a thousand squared. 67 00:04:46,469 --> 00:04:50,131 Or, we can multiply the numerator and denominator by 1 million 68 00:04:50,131 --> 00:05:01,371 and this is going to be equal to 1 million times the gravitational constant 69 00:05:01,371 --> 00:05:06,131 times m1 times m2, all of that over "r" squared. 70 00:05:06,131 --> 00:05:09,659 Now, what's this things right over here? 71 00:05:09,659 --> 00:05:18,736 That's the same thing as the F1.So this is going to be 1 million times F1. 72 00:05:18,736 --> 00:05:23,715 So, even though the masses involved are the same, this yellow object right here 73 00:05:23,715 --> 00:05:27,577 is the same mass as this larger object over here. 74 00:05:27,577 --> 00:05:33,592 It's able to exert a million times the gravitational force on this point of mass 75 00:05:33,592 --> 00:05:38,279 So they are both being attracted.They are both exerting this on each other. 76 00:05:38,279 --> 00:05:43,736 And the reality is that because this thing is smaller,because this m1 on the right here, 77 00:05:43,736 --> 00:05:48,248 this one I'm coloring in,because this one is smaller and denser, this particle is able to 78 00:05:48,248 --> 00:05:51,244 get closer to its center of mass. 79 00:05:51,244 --> 00:05:55,577 Now you might be saying: Ok,well..I can buy that.That you know, this just come straight 80 00:05:55,577 --> 00:05:59,592 from the universal law of gravitation.But what if something closer to this center of mass 81 00:05:59,592 --> 00:06:00,754 experience the same thing? 82 00:06:00,831 --> 00:06:09,531 If this is a star, wouldn't photons that are over here wouldn't this experience the same force 83 00:06:09,531 --> 00:06:16,998 If this distance right here is "r" over a thousand(r/1000), wouldn't some photon here or 84 00:06:16,998 --> 00:06:23,018 atom here or molecul or whatever it's over here, wouldn't that experience the same force? 85 00:06:23,018 --> 00:06:26,464 This milllion times the force of this thing and you got to remember, 86 00:06:26,464 --> 00:06:30,925 all of the sudden when this thing is inside of this larger mass, what's happening? 87 00:06:30,925 --> 00:06:39,802 The entire mass is no longer pulling on it in that direction.It's no longer pulling it in that inward direction. 88 00:06:39,802 --> 00:06:56,100 You now have all of this mass over here is pulling it in outward direction. 89 00:06:56,115 --> 00:07:02,767 All that mass is doing is that mass itself is being pulled inword. 90 00:07:02,767 --> 00:07:07,162 It is pushing down on this.It is exerting pressure on that point. 91 00:07:07,162 --> 00:07:14,705 But, the actual gravitational force that that point is experiencing is actually going to be less, it's actually going to me mitigated 92 00:07:14,705 --> 00:07:22,715 by the fact that there are so much mass over here pulling in the other direction. 93 00:07:22,715 --> 00:07:32,223 So, you can imagine that if you are in the center of a really massive object, 94 00:07:32,223 --> 00:07:38,310 there will be no gravitational force being pulled on you,because you are at the center of the mass 95 00:07:38,310 --> 00:07:45,018 The rest of the mass is outward,so at every point it will be pulling you outward. 96 00:07:45,018 --> 00:07:47,648 So, that's why you as you enter the core of the star, 97 00:07:47,648 --> 00:07:49,859 you will get a lot closer to the center of the mass. 98 00:07:49,859 --> 00:07:54,679 It's not goint to be pulling on you with this type of force and the only way you can get this 99 00:07:54,679 --> 00:08:01,044 type of forces is if the entire mass is contained in a very dense region, 100 00:08:01,044 --> 00:08:03,171 in a very small region. 101 00:08:03,171 --> 00:08:07,423 And that's why a black hole is able to exert such strong gravity that 102 00:08:07,423 --> 00:08:09,675 not even light can escape. 103 00:08:09,675 --> 99:59:59,999 Hopefully that clarifies things a little bit.