1 00:00:00,000 --> 00:00:07,145 [MUSIC PLAYING] 2 00:00:07,145 --> 00:00:08,770 JESSICA HARROP: Hi, I'm Jessica and I'm 3 00:00:08,770 --> 00:00:10,853 going to be talking about a chemical demonstration 4 00:00:10,853 --> 00:00:14,030 today that I like to call "Death of a Gummy Bear." 5 00:00:17,960 --> 00:00:19,760 We eat these little guys all the time 6 00:00:19,760 --> 00:00:21,410 and our bodies break down the sugar 7 00:00:21,410 --> 00:00:23,837 in a series of chemical reactions. 8 00:00:23,837 --> 00:00:26,420 But what happens when you break down the sugar in a gummy bear 9 00:00:26,420 --> 00:00:28,340 outside of our bodies? 10 00:00:28,340 --> 00:00:33,130 Well, MIT'S Dr. John Dolhun is going to show us. 11 00:00:33,130 --> 00:00:36,350 Here he is at the Cambridge Science Festival at MIT. 12 00:00:36,350 --> 00:00:39,740 JOHN DOLHUN: Now I'm going to actually 13 00:00:39,740 --> 00:00:43,470 be combusting a gummy candy. 14 00:00:43,470 --> 00:00:46,301 And my wife said, please don't tell them it's a bear. 15 00:00:46,301 --> 00:00:46,800 Guess what? 16 00:00:46,800 --> 00:00:48,240 It's a bear. 17 00:00:48,240 --> 00:00:49,740 And I'm going to eat one right now. 18 00:00:53,020 --> 00:00:55,450 And I'm eating a gummy candy. 19 00:00:55,450 --> 00:00:58,028 It's sugar. 20 00:00:58,028 --> 00:01:02,690 And I'm going to chew on it, and eat it, and what do you think's 21 00:01:02,690 --> 00:01:04,262 going to happen to it? 22 00:01:04,262 --> 00:01:05,720 AUDIENCE: It's going to break down. 23 00:01:05,720 --> 00:01:09,170 JOHN DOLHUN: It's going to break down into carbon dioxide. 24 00:01:09,170 --> 00:01:12,830 Tomorrow I'm going to be breathing out CO2. 25 00:01:12,830 --> 00:01:14,330 I'm going to be perspiring. 26 00:01:14,330 --> 00:01:17,210 Water is going to be coming out. 27 00:01:17,210 --> 00:01:20,090 And I'm going to make a lot of energy, 28 00:01:20,090 --> 00:01:24,160 and I'm going to take that energy and store it up as ATP, 29 00:01:24,160 --> 00:01:28,280 and it's going to help me clean all these dishes tomorrow. 30 00:01:28,280 --> 00:01:30,620 I don't want to think about that but I'm 31 00:01:30,620 --> 00:01:33,260 going to need the energy. 32 00:01:33,260 --> 00:01:36,020 And now I'm going to do this same reaction 33 00:01:36,020 --> 00:01:38,740 inside of a test tube. 34 00:01:38,740 --> 00:01:41,800 And I want you to compare what you just saw. 35 00:01:41,800 --> 00:01:43,570 You didn't see a lot of smoke and fire 36 00:01:43,570 --> 00:01:46,090 coming out of my mouth, did you? 37 00:01:46,090 --> 00:01:47,065 Not yet, OK. 38 00:01:49,970 --> 00:01:52,690 So Clifton, you can. 39 00:01:52,690 --> 00:01:55,690 Clifton's going to play a little rondo or music 40 00:01:55,690 --> 00:01:57,580 while I set this reaction up. 41 00:01:57,580 --> 00:02:29,470 [MUSIC PLAYING] 42 00:02:29,470 --> 00:02:31,500 JESSICA HARROP: So what is Dr. Dolhun doing? 43 00:02:31,500 --> 00:02:34,500 First, he put some solid potassium chlorate in a test 44 00:02:34,500 --> 00:02:35,780 tube and heated it up. 45 00:02:40,010 --> 00:02:42,885 The heat causes the solid to melt and become a liquid. 46 00:02:46,880 --> 00:02:48,390 So this little triangle means heat. 47 00:02:48,390 --> 00:02:52,320 It turned from a solid to a liquid. 48 00:02:52,320 --> 00:02:55,560 As it's being heated, the liquid potassium chlorate immediately 49 00:02:55,560 --> 00:02:59,220 starts breaking down into two products, potassium chloride 50 00:02:59,220 --> 00:03:02,370 and oxygen. Now potassium chloride is a solid 51 00:03:02,370 --> 00:03:04,230 and the oxygen is a gas. 52 00:03:04,230 --> 00:03:05,070 Looks like this. 53 00:03:10,339 --> 00:03:14,050 Now let's see what happens when Dr. Dolhun adds the gummy bear. 54 00:03:14,050 --> 00:03:42,685 [MUSIC PLAYING] 55 00:03:42,685 --> 00:03:44,650 So let's break down what just happened. 56 00:03:44,650 --> 00:03:46,930 The sugar from the gummy bear and oxygen 57 00:03:46,930 --> 00:03:49,960 reacted to produce carbon dioxide and water, 58 00:03:49,960 --> 00:03:52,709 releasing a lot of energy as heat and light. 59 00:03:52,709 --> 00:03:54,250 This is what that looks like, and I'm 60 00:03:54,250 --> 00:03:57,296 going to draw sucrose, or sugar, in red 61 00:03:57,296 --> 00:03:58,670 because it's from the gummy bear. 62 00:04:08,120 --> 00:04:10,500 This reaction is probably familiar to you. 63 00:04:10,500 --> 00:04:11,960 It's a combustion reaction, which 64 00:04:11,960 --> 00:04:14,750 is when a fuel reacts with oxygen to produce carbon 65 00:04:14,750 --> 00:04:17,630 dioxide and water and at the same time, releasing 66 00:04:17,630 --> 00:04:19,160 a bunch of energy. 67 00:04:19,160 --> 00:04:21,019 So why is so much energy released 68 00:04:21,019 --> 00:04:22,820 and where does it come from? 69 00:04:22,820 --> 00:04:25,010 To show you, I'm going to draw the structures. 70 00:04:25,010 --> 00:04:28,040 Now, if you're unfamiliar with organic chemistry notation, 71 00:04:28,040 --> 00:04:30,800 each of the lines between the elements that I'm going to draw 72 00:04:30,800 --> 00:04:33,080 represents a covalent bond, which 73 00:04:33,080 --> 00:04:36,555 is the sharing of two electrons between two atoms. 74 00:04:36,555 --> 00:04:37,430 So let me draw those. 75 00:04:48,340 --> 00:04:52,300 So here are the reactants and here are the products. 76 00:04:52,300 --> 00:04:55,480 Now by looking at the number of bonds and the type of bonds, 77 00:04:55,480 --> 00:04:58,990 so a carbon bonded to an oxygen, or a carbon bonded 78 00:04:58,990 --> 00:05:03,010 to a carbon, and a single bond versus a double bond, 79 00:05:03,010 --> 00:05:04,750 you can calculate the energy difference 80 00:05:04,750 --> 00:05:07,690 between the left side of the reaction, the reactants, 81 00:05:07,690 --> 00:05:09,940 and the right side, or the products. 82 00:05:09,940 --> 00:05:12,220 Now all combustion reactions have more energy 83 00:05:12,220 --> 00:05:14,800 stored in the reactants than the products, 84 00:05:14,800 --> 00:05:18,130 so as the reaction progresses, this energy has to go somewhere 85 00:05:18,130 --> 00:05:20,770 and it's released as heat and light. 86 00:05:20,770 --> 00:05:23,380 Now the amount of energy released from this explosion 87 00:05:23,380 --> 00:05:25,630 is exactly the same as the amount of energy 88 00:05:25,630 --> 00:05:27,310 that would be released in my body 89 00:05:27,310 --> 00:05:29,290 when I eat this gummy bear. 90 00:05:29,290 --> 00:05:31,630 The difference is that proteins in my body 91 00:05:31,630 --> 00:05:34,390 are set up in pathways that extract the energy 92 00:05:34,390 --> 00:05:36,460 in small, manageable bundles. 93 00:05:36,460 --> 00:05:38,320 So I power my everyday activities 94 00:05:38,320 --> 00:05:41,740 like dancing and running, but I don't explode. 95 00:05:41,740 --> 00:05:44,050 Evolution has trained biological systems 96 00:05:44,050 --> 00:05:47,660 to efficiently extract energy from our environment. 97 00:05:47,660 --> 00:05:48,620 That's it for me today. 98 00:05:48,620 --> 00:05:49,578 I'll see you next time. 99 00:05:49,578 --> 00:05:51,600 [MUSIC PLAYING]