1 00:00:00,840 --> 00:00:04,740 In the last video we talked about how every atom really 2 00:00:04,740 --> 00:00:08,280 wants to have eight-- let me write that down-- eight 3 00:00:08,280 --> 00:00:11,030 electrons in its outermost shell. 4 00:00:11,030 --> 00:00:14,510 This is kind of the most stable configuration that an 5 00:00:14,510 --> 00:00:17,740 electron can have. And given this fact that's been 6 00:00:17,740 --> 00:00:21,180 determined just by observing the world, really, we can 7 00:00:21,180 --> 00:00:24,420 start to figure out what's likely to happen in different 8 00:00:24,420 --> 00:00:26,350 groups of the periodic table. 9 00:00:26,350 --> 00:00:28,820 A group of a periodic table is just a column of 10 00:00:28,820 --> 00:00:30,220 the periodic table. 11 00:00:30,220 --> 00:00:32,479 Like this group, right here, and actually I'll start with 12 00:00:32,479 --> 00:00:35,960 this group, because it's got a special name. 13 00:00:35,960 --> 00:00:39,160 This group right here is called the noble gases. 14 00:00:39,160 --> 00:00:41,860 And what's common when you go down a group in 15 00:00:41,860 --> 00:00:42,900 the periodic table? 16 00:00:42,900 --> 00:00:45,970 What's common about a column in the periodic table? 17 00:00:45,970 --> 00:00:50,100 Well, in the last video we saw that every element in a column 18 00:00:50,100 --> 00:00:52,700 has the same number of valence electrons. 19 00:00:52,700 --> 00:00:55,220 Or it has the same number of electrons in 20 00:00:55,220 --> 00:00:56,580 its outermost shell. 21 00:00:56,580 --> 00:00:58,000 And we figured out what that was. 22 00:00:58,000 --> 00:01:01,160 This column, right here, which we learned were the alkali 23 00:01:01,160 --> 00:01:05,830 metals, this has one electron in its outermost shell. 24 00:01:05,830 --> 00:01:08,530 And I made that one caveat that hydrogen isn't 25 00:01:08,530 --> 00:01:10,830 necessarily considered an alkali metal. 26 00:01:10,830 --> 00:01:13,230 One, it's usually not in metal form. 27 00:01:13,230 --> 00:01:16,320 And it doesn't want to give away electrons as much as 28 00:01:16,320 --> 00:01:17,490 other metals do. 29 00:01:17,490 --> 00:01:21,080 When people talk about metal-like characteristics of 30 00:01:21,080 --> 00:01:23,160 an element, they're really talking about how likely it is 31 00:01:23,160 --> 00:01:24,640 to give away electron. 32 00:01:24,640 --> 00:01:26,460 We'll talk about other characteristics of a metal, 33 00:01:26,460 --> 00:01:30,020 especially the way that we perceive metals as being 34 00:01:30,020 --> 00:01:32,610 shiny, and maybe they conduct electricity, and see how that 35 00:01:32,610 --> 00:01:34,060 plays out in the periodic table. 36 00:01:34,060 --> 00:01:35,760 But anyway, back to what I was talking about. 37 00:01:35,760 --> 00:01:37,610 This column, right here, this is called the 38 00:01:37,610 --> 00:01:40,680 alkaline earth metals. 39 00:01:40,680 --> 00:01:42,420 So this is alkaline earth. 40 00:01:51,130 --> 00:01:54,340 These all have two atoms in its outermost shell. 41 00:01:54,340 --> 00:01:56,450 So remember, everyone wants to get to eight. 42 00:01:56,450 --> 00:02:00,070 If these guys wanted to get to eight by adding electrons, 43 00:02:00,070 --> 00:02:01,130 they would have a long way to go. 44 00:02:01,130 --> 00:02:03,570 This way, we would have to add seven electrons. 45 00:02:03,570 --> 00:02:05,850 They would have to add six electrons. 46 00:02:05,850 --> 00:02:07,340 And who are they going to take it from? 47 00:02:07,340 --> 00:02:09,090 Because these guys don't want to give away their electrons. 48 00:02:09,090 --> 00:02:10,860 They're so close to getting to eight. 49 00:02:10,860 --> 00:02:12,980 So it's much easier when you're on the left-hand side 50 00:02:12,980 --> 00:02:15,350 of the periodic table to give away electrons. 51 00:02:15,350 --> 00:02:19,120 In fact, when you only have one to give away-- especially 52 00:02:19,120 --> 00:02:22,150 in the case of elements other than hydrogen-- when you only 53 00:02:22,150 --> 00:02:24,980 have one to give away, it really wants to do that. 54 00:02:24,980 --> 00:02:28,330 And because of that, these elements right here are very 55 00:02:28,330 --> 00:02:30,440 seldom found in their elemental state. 56 00:02:30,440 --> 00:02:32,900 When I say elemental state, it means there's nothing but 57 00:02:32,900 --> 00:02:36,730 lithium there, there's nothing but sodium there, there's 58 00:02:36,730 --> 00:02:37,950 nothing but potassium there. 59 00:02:37,950 --> 00:02:40,610 They're very likely, if you find this, it's probably 60 00:02:40,610 --> 00:02:42,530 already reacted with something. 61 00:02:42,530 --> 00:02:44,470 Probably with something on this side of the periodic 62 00:02:44,470 --> 00:02:46,520 table, because this wants to give away something really 63 00:02:46,520 --> 00:02:49,150 bad, this wants to take something really bad. 64 00:02:49,150 --> 00:02:51,340 So the reaction will probably happen. 65 00:02:51,340 --> 00:02:53,100 These are still reactive. 66 00:02:53,100 --> 00:02:56,200 The alkaline earth metals are still reactive, but not as 67 00:02:56,200 --> 00:02:59,160 reactive as the alkali metals. 68 00:02:59,160 --> 00:03:02,090 And that's because these guys are really close to getting to 69 00:03:02,090 --> 00:03:03,840 the stable magic eight number. 70 00:03:03,840 --> 00:03:06,210 These guys are a little bit further away. 71 00:03:06,210 --> 00:03:12,420 So it takes a little bit more, I guess you could say, of a 72 00:03:12,420 --> 00:03:14,670 push for them to give away two. 73 00:03:14,670 --> 00:03:16,820 These guys only have to give away one. 74 00:03:16,820 --> 00:03:19,485 And then we learned that this has two in 75 00:03:19,485 --> 00:03:20,440 its outermost shell. 76 00:03:20,440 --> 00:03:23,140 And then all of these elements, which are called the 77 00:03:23,140 --> 00:03:26,710 transition metals, as you add electrons, they're just 78 00:03:26,710 --> 00:03:31,410 backfilling the previous shell's d subshell. 79 00:03:31,410 --> 00:03:31,940 Right? 80 00:03:31,940 --> 00:03:34,920 So their outermost shell still has two. 81 00:03:34,920 --> 00:03:36,660 It still has those. 82 00:03:36,660 --> 00:03:41,300 If this is the fourth period, all of these elements' 83 00:03:41,300 --> 00:03:45,460 outermost shell has 4s2. 84 00:03:45,460 --> 00:03:48,560 And these elements are just backfilling their 3d 85 00:03:48,560 --> 00:03:50,720 suborbital. 86 00:03:50,720 --> 00:03:52,950 Or their 3d subshell. 87 00:03:52,950 --> 00:03:54,690 These are 2's. 88 00:03:54,690 --> 00:03:57,400 So these all have two outermost electrons. 89 00:03:57,400 --> 00:04:01,190 So all of these, like the alkaline earth metals, need to 90 00:04:01,190 --> 00:04:06,320 lose two electrons in order to, quote-unquote, be happy. 91 00:04:06,320 --> 00:04:08,410 And the way I think about this, and this is really just 92 00:04:08,410 --> 00:04:11,810 a way-- and it maybe it bears out in physical reality-- is 93 00:04:11,810 --> 00:04:14,870 that these guys have kind of a deep bench of electrons. 94 00:04:14,870 --> 00:04:19,649 That if they are able to shed some of these valence 95 00:04:19,649 --> 00:04:25,580 electrons-- so if I write iron has two valence electrons like 96 00:04:25,580 --> 00:04:29,890 that-- even if they shed these electrons, they kind of have a 97 00:04:29,890 --> 00:04:34,660 reserve of electrons in the d subshell for 98 00:04:34,660 --> 00:04:36,420 the previous shell. 99 00:04:36,420 --> 00:04:40,980 So if it sheds its 4s2 electrons, it still has all 100 00:04:40,980 --> 00:04:43,740 those 3d electrons that have a high energy state that can 101 00:04:43,740 --> 00:04:45,650 maybe kind of replace them. 102 00:04:45,650 --> 00:04:47,930 And I'll use everything in quotation marks, because these 103 00:04:47,930 --> 00:04:50,770 are just ways for me to visualize things. 104 00:04:50,770 --> 00:04:55,010 And the reason why I make that point is because metals are 105 00:04:55,010 --> 00:04:58,020 just very giving with their electrons. 106 00:04:58,020 --> 00:05:00,380 And these guys react. 107 00:05:00,380 --> 00:05:01,780 They say, hey, take my electrons. 108 00:05:01,780 --> 00:05:03,680 These guys say, take these two electrons. 109 00:05:03,680 --> 00:05:06,680 And these guys, they start to say, especially as you fill 110 00:05:06,680 --> 00:05:09,260 the d subshell, I've got these two electrons, and not only do 111 00:05:09,260 --> 00:05:11,420 I have those two electrons, but I have more electrons 112 00:05:11,420 --> 00:05:13,520 where-- well almost where-- that came from. 113 00:05:13,520 --> 00:05:16,050 I have some in reserve in my d. 114 00:05:16,050 --> 00:05:18,690 And what happens in these transition metals, and it 115 00:05:18,690 --> 00:05:21,470 especially happens in the metals-- so these are the 116 00:05:21,470 --> 00:05:24,110 metals right here, and these don't follow just a group, but 117 00:05:24,110 --> 00:05:27,960 this is the metals, this color right here-- is that they have 118 00:05:27,960 --> 00:05:31,940 so many electrons to hand off, not only do they have these 119 00:05:31,940 --> 00:05:35,370 extra there, but they filled their d subshell, that they 120 00:05:35,370 --> 00:05:37,660 can kind of, especially when they're in elemental form, and 121 00:05:37,660 --> 00:05:39,820 when I say elemental form, this means that you just have 122 00:05:39,820 --> 00:05:41,450 a big block of aluminum. 123 00:05:41,450 --> 00:05:45,700 Aluminum hasn't reacted with anything like oxygen. 124 00:05:45,700 --> 00:05:47,500 It's just a bunch of aluminum. 125 00:05:47,500 --> 00:05:47,810 Right? 126 00:05:47,810 --> 00:05:49,640 When you have a bunch of aluminum, what happens is you 127 00:05:49,640 --> 00:05:51,840 have these metallic bonds where all of the aluminum 128 00:05:51,840 --> 00:05:54,550 atoms say, you know what, I have all these extra, I have 129 00:05:54,550 --> 00:05:58,525 definitely, in the case of aluminum, three electrons in 130 00:05:58,525 --> 00:05:59,470 my outermost shell. 131 00:05:59,470 --> 00:06:02,840 But I have all of these kind of backfilled electrons in my 132 00:06:02,840 --> 00:06:04,040 d suborbital. 133 00:06:04,040 --> 00:06:06,600 I'm just going to share them with the other aluminum atoms. 134 00:06:06,600 --> 00:06:09,170 So you create this sea of aluminum atoms. And they're 135 00:06:09,170 --> 00:06:10,430 attracted to each other. 136 00:06:10,430 --> 00:06:12,750 Or you create this sea of aluminum electrons. 137 00:06:12,750 --> 00:06:20,090 So you have a bunch of electrons sitting in between 138 00:06:20,090 --> 00:06:22,620 the atoms, and since the atoms kind of donated these 139 00:06:22,620 --> 00:06:24,270 electrons, they're attracted to them. 140 00:06:24,270 --> 00:06:24,950 Right? 141 00:06:24,950 --> 00:06:30,030 So the actual atoms-- so this would be an aluminum plus, and 142 00:06:30,030 --> 00:06:31,405 maybe we would have donated three electrons. 143 00:06:31,405 --> 00:06:33,470 But I'm not being exact here. 144 00:06:33,470 --> 00:06:35,410 I want to just give you the sense of how things work. 145 00:06:35,410 --> 00:06:38,320 And that's why metals conduct really well, because 146 00:06:38,320 --> 00:06:41,320 electricity is just a bunch of electrons moving, and in order 147 00:06:41,320 --> 00:06:45,460 to have electrons moving, you have to have surplus electrons 148 00:06:45,460 --> 00:06:46,330 lying around. 149 00:06:46,330 --> 00:06:48,480 So elements right around this area are really good 150 00:06:48,480 --> 00:06:48,980 conductors. 151 00:06:48,980 --> 00:06:53,650 In fact, silver is the best conductor. 152 00:06:53,650 --> 00:06:57,240 Silver, right here, is the best conductor on the planet. 153 00:06:57,240 --> 00:07:01,440 And the reason why that's not used for our wiring and copper 154 00:07:01,440 --> 00:07:04,300 is because copper is easier to find than silver. 155 00:07:04,300 --> 00:07:06,140 But silver is the best conductor. 156 00:07:06,140 --> 00:07:09,340 And the way I think about it is that these-- once you've 157 00:07:09,340 --> 00:07:11,010 filled an orbital, that orbital 158 00:07:11,010 --> 00:07:12,890 becomes somewhat stable. 159 00:07:12,890 --> 00:07:16,140 So all of these guys have filled their d orbital. 160 00:07:16,140 --> 00:07:18,960 While these guys, their d orbital is not filled. 161 00:07:18,960 --> 00:07:20,910 So they just have a lot of surplus electrons that are 162 00:07:20,910 --> 00:07:21,970 really good for conduction. 163 00:07:21,970 --> 00:07:24,120 Now, that's just an intuition. 164 00:07:24,120 --> 00:07:26,000 I haven't done the experiment to prove that. 165 00:07:26,000 --> 00:07:28,100 But it'll give you a sense of why things 166 00:07:28,100 --> 00:07:29,100 conduct and all of that. 167 00:07:29,100 --> 00:07:32,370 So these are the transition metals. 168 00:07:32,370 --> 00:07:33,870 These are actually considered the metals. 169 00:07:33,870 --> 00:07:35,940 But the reason why these are considered the transition 170 00:07:35,940 --> 00:07:37,960 metals is because they're filling the d-block. 171 00:07:37,960 --> 00:07:40,600 But transition metals kind of sound like not 172 00:07:40,600 --> 00:07:41,390 as good as a metal. 173 00:07:41,390 --> 00:07:44,460 But when I think of metals, iron is kind of the first 174 00:07:44,460 --> 00:07:45,610 metal I always think of. 175 00:07:45,610 --> 00:07:49,020 I definitely think of silver and copper and gold as metals. 176 00:07:49,020 --> 00:07:51,270 So to call them transition metals is a little not fair. 177 00:07:51,270 --> 00:07:54,120 I don't really consider aluminum more of a metal than, 178 00:07:54,120 --> 00:07:55,230 let's say, iron is. 179 00:07:55,230 --> 00:07:58,140 But in chemistry classification world, aluminum 180 00:07:58,140 --> 00:08:00,370 is more of a metal. 181 00:08:00,370 --> 00:08:01,880 These elements right here. 182 00:08:01,880 --> 00:08:04,700 And I know I dropped off come from kind of the group notion. 183 00:08:04,700 --> 00:08:07,280 But let me just actually write the valence electrons. 184 00:08:07,280 --> 00:08:09,220 So these all have three valence electrons. 185 00:08:09,220 --> 00:08:13,720 Four, five, six, seven. 186 00:08:13,720 --> 00:08:16,680 So these all have three electrons in 187 00:08:16,680 --> 00:08:18,150 its outermost shell. 188 00:08:18,150 --> 00:08:21,420 It still seems easier for them to give them away than to take 189 00:08:21,420 --> 00:08:25,990 them, but maybe now, in certain cases, there could be, 190 00:08:25,990 --> 00:08:27,910 especially in the case of, let's say, boron, there could 191 00:08:27,910 --> 00:08:31,180 be a situation where it maybe could gain five electrons, 192 00:08:31,180 --> 00:08:32,820 although that seems hard. 193 00:08:32,820 --> 00:08:35,090 It's much easier to give away three and that's why a lot of 194 00:08:35,090 --> 00:08:37,470 the, quote-unquote, official metals 195 00:08:37,470 --> 00:08:39,340 show up in this category. 196 00:08:39,340 --> 00:08:43,230 And as you can see, as you go down the periodic table you 197 00:08:43,230 --> 00:08:45,480 can kind of have metals that have more and 198 00:08:45,480 --> 00:08:46,650 more valence electrons. 199 00:08:46,650 --> 00:08:50,730 So for, let's say, lead. 200 00:08:50,730 --> 00:08:52,120 It's still a metal, even though it has 201 00:08:52,120 --> 00:08:53,690 four valence electrons. 202 00:08:53,690 --> 00:09:00,490 And that's because the atom is so big, its radius is so large 203 00:09:00,490 --> 00:09:03,030 that the outermost shell is so far away from the nucleus, 204 00:09:03,030 --> 00:09:05,150 that those electrons are easier to take off. 205 00:09:05,150 --> 00:09:08,510 So for example, as you go down, carbon, those electrons 206 00:09:08,510 --> 00:09:10,470 are very close to the nucleus. 207 00:09:10,470 --> 00:09:11,820 So they're very hard to take off. 208 00:09:11,820 --> 00:09:15,290 So carbon would probably more likely gain electrons from 209 00:09:15,290 --> 00:09:16,840 somebody else to get to eight. 210 00:09:16,840 --> 00:09:20,270 While these guys' valence electrons are so far away from 211 00:09:20,270 --> 00:09:23,070 the nucleus that they're more likely to kind of want to get 212 00:09:23,070 --> 00:09:25,440 rid of them to get to eight and get back to an electron 213 00:09:25,440 --> 00:09:27,960 configuration of, let's say, xenon. 214 00:09:27,960 --> 00:09:32,260 And you go and then these guys are the nonmetals. 215 00:09:32,260 --> 00:09:32,600 Right? 216 00:09:32,600 --> 00:09:34,560 They're likely to probably gain 217 00:09:34,560 --> 00:09:36,330 electrons in most reactions. 218 00:09:36,330 --> 00:09:38,820 And then this yellow category that I said was highly 219 00:09:38,820 --> 00:09:43,720 reactive, especially highly reactive with the alkali 220 00:09:43,720 --> 00:09:46,030 metals over here, these are called halogens. 221 00:09:46,030 --> 00:09:48,620 And you've probably heard the word before. 222 00:09:48,620 --> 00:09:49,870 Halogen lamps. 223 00:09:54,980 --> 00:09:57,930 That's no mistake there to call them halogen lamps. 224 00:09:57,930 --> 00:10:00,070 That's not a random choice of words. 225 00:10:00,070 --> 00:10:02,560 Maybe I'll do a video on halogen lamps in the future. 226 00:10:02,560 --> 00:10:05,260 And then finally, we're at the noble gases. 227 00:10:05,260 --> 00:10:07,760 What's interesting about the noble gases? 228 00:10:07,760 --> 00:10:10,000 Well they have eight electrons in their 229 00:10:10,000 --> 00:10:11,540 outermost shell, right? 230 00:10:11,540 --> 00:10:12,220 Except for helium. 231 00:10:12,220 --> 00:10:13,850 Helium has two, right? 232 00:10:13,850 --> 00:10:19,010 Helium's electron configuration is 1s2. 233 00:10:19,010 --> 00:10:21,250 But all of these other guys, this guy's electron 234 00:10:21,250 --> 00:10:22,290 configuration is 1s2. 235 00:10:22,290 --> 00:10:24,040 This is neon. 236 00:10:24,040 --> 00:10:28,050 1s2, 2s2, 2p6. 237 00:10:28,050 --> 00:10:30,510 So he has eight electrons in his outermost shell. 238 00:10:30,510 --> 00:10:31,370 So he's happy. 239 00:10:31,370 --> 00:10:32,960 Argon, same thing. 240 00:10:32,960 --> 00:10:38,010 The outermost shell will look like 3s2, 3p6. 241 00:10:38,010 --> 00:10:41,050 Krypton will have in its outermost shell 242 00:10:41,050 --> 00:10:43,000 will be 3s2, 3p6. 243 00:10:43,000 --> 00:10:45,750 It will also have some 3d electrons around as it 244 00:10:45,750 --> 00:10:47,840 backfilled back here. 245 00:10:47,840 --> 00:10:50,070 But all of these have eight in its outermost shell, so 246 00:10:50,070 --> 00:10:51,000 they're happy. 247 00:10:51,000 --> 00:10:52,680 They have no incentive to react. 248 00:10:52,680 --> 00:10:54,700 They're kind of like, hey, all of you other elements, just, 249 00:10:54,700 --> 00:10:57,720 you know, you guys can do all that crazy reactions that 250 00:10:57,720 --> 00:10:58,960 you've got to do, but we're happy. 251 00:10:58,960 --> 00:11:00,850 And we don't want to give or take electrons. 252 00:11:00,850 --> 00:11:06,130 And because of that these guys are highly, highly unreactive. 253 00:11:06,130 --> 00:11:08,460 Very, very unreactive. 254 00:11:08,460 --> 00:11:11,550 And you know, back in the day, when they used to make these 255 00:11:11,550 --> 00:11:17,150 kind of zeppelins, these big blimps-- the Hindenburg is a 256 00:11:17,150 --> 00:11:19,290 famous example-- they used hydrogen. 257 00:11:19,290 --> 00:11:22,380 And obviously hydrogen is a pretty reactive substance. 258 00:11:22,380 --> 00:11:24,560 It's actually very combustible and that's why it blows up 259 00:11:24,560 --> 00:11:29,630 very fast. And that's why now, clowns or children's balloon 260 00:11:29,630 --> 00:11:33,930 manufacturers, they instead would prefer to use helium. 261 00:11:33,930 --> 00:11:36,840 Because helium is a noble gas and it's very unreactive. 262 00:11:36,840 --> 00:11:41,150 And it's very unlikely to explode at a 263 00:11:41,150 --> 00:11:42,790 child's birthday party. 264 00:11:42,790 --> 00:11:45,300 But anyway, I think I'm done now with this video. 265 00:11:45,300 --> 00:11:47,780 And in the next video we'll talk a little bit more about 266 00:11:47,780 --> 00:11:50,820 trends across the periodic table.