9/18/2012 Fusion, Fission, and ½ Life Objectives • To compare and contrast nuclear fusion and nuclear fission • To calculate the amount of energy generated by small changes in mass during nuclear equations • To compare and contrast chemical and nuclear reactions Nuclear Terminology • Parent isotopes are the beginning of the decay process • Daughter products are the new atoms that are made by decay • Half Life is the amount of time in takes to convert 50% of parent isotopes into daughter products. Chemical Reactions • Involve changes in electrons – Acids & Bases, combustion, displacement • The same atoms appear on both sides of the reaction. • Follows Dalton’s Law of Conservation of Mass • Small amount of energy generated – Burning fossil fuels • Rate can be influenced by temperature, pressure, presence of a catalyst Decay & ½ Life • The amount of time a radioactive isotope takes to decay can vary from a few seconds to millions of years • To measure this, scientists calculate the half life • 1 Half life is the amount of time it takes for half of the sample to decay into another element • The Red spheres are Uranium 238 molecules, which have a ½ life of 4.9 billion years. Nuclear Reactions • Involve changes in the nucleus – Nuclear fusion, nuclear fission • New atoms appear as products of the reaction. • Breaks Dalton’s Law of Conservation of Mass • Large amount of energy generated – 1 million times more than chemical reactions – Nuclear fusion on the sun – Nuclear fission for reactors • Rate does not depend on any physical properties Show Me the Energy!!! • Because nuclear reactions break Dalton’s Law of Conservation of Mass, a very small amount of mass is converted to energy. • Einstein is credited with discovering the equation to calculate the mass-energy defect. E = mc2 E = change in energy (Joules) M = change in mass (kilograms) C = speed of light = 3x108 meters/second • How Much Energy? The energy released from the nuclear reaction of 1kg of uranium is equivalent to the energy released during the combustion of 4 billion kilograms of coal 1 9/18/2012 How to Use My Calculator!! • Never type in “x10” into • Type in “3x108” into your calculator!! your calculator • Your calculator either – 3 EE 8 uses: – 3 EXP 8 – EE – EXP – 10x – 3 x10x • Your calculator should show: • In some cases, the EE or EXP may be on the button or in a different color ABOVE the button – 3 08 – 3E08 – 3 x10 8 • How would you write it down? Nuclear Fission Decay vs. Nuclear Reactions • Alpha, beta, and gamma • Nuclear reactions involve decay occur as ONE atom more than just getting rid of a few protons or neutrons. tries to increase it’s stability by getting rid of a The new atoms produced few neutrons, or protons & are VERY different neutrons. elements than the reactant. • The product is an alpha, • Nuclear reactions must be beta, or gamma particle started, so there are 2 and ONE new atom. things on the left hand side. There is only ONE thing – Nuclear fission: makes 2 on the left hand side. or more much smaller atoms – Nuclear fusion: makes 1 much larger atom Nuclear Fission How is the above reaction different than a decay? • Fission is where the nucleus breaks apart into 2 or more much smaller nuclei. 1 large atom → 2 or more smaller atoms + ENERGY • Heavy atoms (mass number>60) go through fission to try to increase their stability. • Like all nuclear reactions, nuclear fission releases a large amount of energy. Chain Reaction of Uranium-235 • The true power of fission reactions comes from a chain reaction. • A chain reaction is where one fission reaction can lead to several more fission reactions. • Many, much smaller atoms are made, each one starting its’ own fission reaction. • A chain reaction can only occur if the starting material has enough mass to sustain a chain reaction. This amount is called the critical mass. • Nuclear Fission chain reactions are what occurs in Nuclear Reactors and Atomic Bombs. • The Nuclear reactor is a controlled fission reaction, the bomb is not. 2 9/18/2012 Nuclear Fusion Nuclear Fusion 2 small atoms → 1 large atom + ENERGY • The combining of 2 small atomic nuclei to form a larger atom. • Nuclear fusion occurs in the sun and generate enough energy to power the solar system • Fusion reactions release very large amount of energy, but require extremely high temperatures to start. • Nuclear fusion is how all elements bigger than Hydrogen, were made in stars. 1 4 1 H + 2 -10 e- 4 2 He + energy Other Fusion Reactions • Hydrogen Bomb or possible Fusion nuclear reactor reaction 3H 1 + 12H 4He 2 + 10n New Research Area is to create new elements using fusion • 20Ca + 95Am 115Uup • 115Uup 113Uut + 42He 3
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