0:00:06.989,0:00:10.242 You probably know that all stuff[br]is made up of atoms 0:00:10.266,0:00:11.424 and that an atom 0:00:11.448,0:00:15.166 is a really, really, really,[br]really tiny particle. 0:00:15.190,0:00:16.604 Every atom has a core, 0:00:16.628,0:00:18.152 which is made up of at least one 0:00:18.176,0:00:19.518 positively charged particle 0:00:19.542,0:00:21.143 called a proton, 0:00:21.167,0:00:22.397 and in most cases, 0:00:22.421,0:00:25.568 some number of neutral[br]particles called neutrons. 0:00:25.592,0:00:26.942 That core is surrounded 0:00:26.966,0:00:30.148 by negatively charged[br]particles called electrons. 0:00:30.794,0:00:32.613 The identity of an atom is determined 0:00:32.637,0:00:36.898 only by the number[br]of protons in its nucleus. 0:00:36.922,0:00:39.674 Hydrogen is hydrogen because it[br]has just one proton, 0:00:39.698,0:00:41.413 carbon is carbon because it has six, 0:00:41.437,0:00:43.399 gold is gold because it has 79, 0:00:43.423,0:00:44.680 and so on. 0:00:45.140,0:00:47.126 Indulge me in a momentary tangent. 0:00:47.150,0:00:49.492 How do we know about atomic structure? 0:00:49.516,0:00:52.723 We can't see protons,[br]neutrons, or electrons. 0:00:53.814,0:00:55.338 So, we do a bunch of experiments 0:00:55.362,0:00:58.258 and develop a model[br]for what we think is there. 0:00:58.282,0:00:59.806 Then we do some more experiments 0:00:59.830,0:01:01.592 and see if they agree with the model. 0:01:01.616,0:01:02.813 If they do, great. 0:01:02.837,0:01:05.678 If they don't, it might[br]be time for a new model. 0:01:05.702,0:01:08.345 We've had lots of very[br]different models for atoms 0:01:08.369,0:01:10.486 since Democritus in 400 BC, 0:01:10.510,0:01:11.987 and there will almost certainly 0:01:12.011,0:01:13.576 be many more to come. 0:01:13.600,0:01:15.447 Okay, tangent over. 0:01:15.471,0:01:18.208 The cores of atoms tend to stick together, 0:01:18.232,0:01:19.993 but electrons are free to move, 0:01:20.017,0:01:22.771 and this is why chemists love electrons. 0:01:22.795,0:01:24.209 If we could marry them, 0:01:24.233,0:01:25.637 we probably would. 0:01:25.661,0:01:26.957 But electrons are weird. 0:01:26.981,0:01:29.526 They appear to behave either as particles, 0:01:29.550,0:01:31.108 like little baseballs, 0:01:31.132,0:01:33.298 or as waves, like water waves, 0:01:33.322,0:01:36.499 depending on the experiment[br]that we perform. 0:01:36.523,0:01:38.523 One of the weirdest things about electrons 0:01:38.547,0:01:40.673 is that we can't exactly[br]say where they are. 0:01:40.697,0:01:42.715 It's not that we don't have the equipment, 0:01:42.739,0:01:44.117 it's that this uncertainty 0:01:44.141,0:01:46.474 is part of our model of the electron. 0:01:46.498,0:01:49.036 So, we can't pinpoint them, fine. 0:01:49.060,0:01:51.731 But we can say[br]there's a certain probability 0:01:51.755,0:01:53.716 of finding an electron in a given space 0:01:53.740,0:01:55.681 around the nucleus. 0:01:55.705,0:01:58.561 And that means that we can[br]ask the following question: 0:01:58.585,0:02:00.399 If we drew a shape around the nucleus 0:02:00.423,0:02:02.463 such that we would be 95% sure 0:02:02.487,0:02:05.496 of finding a given electron[br]within that shape, 0:02:05.520,0:02:07.067 what would it look like? 0:02:08.590,0:02:10.797 Here are a few of these shapes. 0:02:10.821,0:02:12.545 Chemists call them orbitals, 0:02:12.569,0:02:13.903 and what each one looks like 0:02:13.927,0:02:15.844 depends on, among other things, 0:02:15.868,0:02:17.691 how much energy it has. 0:02:17.715,0:02:19.341 The more energy an orbital has, 0:02:19.365,0:02:21.018 the farther most of its density is 0:02:21.042,0:02:22.270 from the nucleus. 0:02:22.294,0:02:25.251 By they way, why did we pick 95% 0:02:25.275,0:02:26.887 and not 100%? 0:02:26.911,0:02:28.191 Well, that's another quirk 0:02:28.215,0:02:29.979 of our model of the electron. 0:02:30.003,0:02:32.204 Past a certain distance from the nucleus, 0:02:32.228,0:02:34.049 the probability of finding an electron 0:02:34.073,0:02:35.600 starts to decrease 0:02:35.624,0:02:37.912 more or less exponentially, 0:02:37.936,0:02:40.131 which means that while it[br]will approach zero, 0:02:40.155,0:02:42.582 it'll never actually hit zero. 0:02:43.124,0:02:44.274 So, in every atom, 0:02:44.298,0:02:47.414 there is some small,[br]but non-zero, probability 0:02:47.438,0:02:50.525 that for a very, very[br]short period of time, 0:02:50.549,0:02:51.709 one of its electrons 0:02:51.733,0:02:54.973 is at the other end of the known universe. 0:02:55.973,0:02:58.693 But mostly electrons stay[br]close to their nucleus 0:02:58.717,0:03:00.540 as clouds of negative charged density 0:03:00.564,0:03:02.660 that shift and move with time. 0:03:02.684,0:03:04.391 How electrons from one atom 0:03:04.415,0:03:06.414 interact with electrons from another 0:03:06.438,0:03:08.761 determines almost everything. 0:03:08.785,0:03:10.547 Atoms can give up their electrons, 0:03:10.571,0:03:12.216 surrendering them to other atoms, 0:03:12.240,0:03:14.624 or they can share electrons. 0:03:15.202,0:03:17.060 And the dynamics of this social network 0:03:17.084,0:03:19.527 are what make chemistry interesting. 0:03:19.551,0:03:20.791 From plain old rocks 0:03:20.815,0:03:22.598 to the beautiful complexity of life, 0:03:22.622,0:03:24.360 the nature of everything we see, 0:03:24.384,0:03:25.896 hear, 0:03:25.920,0:03:28.113 smell, taste, touch, and even feel 0:03:28.137,0:03:30.971 is determined at the atomic level.