NUCLEAR CHEMISTRY Chapter 25 Introduction to Nuclear Chemistry Nuclear chemistry is the study of the structure of and the they undergo. Chemical vs. Nuclear Reactions Chemical Reactions Nuclear Reactions Occur when bonds are broken Occur when nuclei emit particles and/or rays Chemical vs. Nuclear Reactions Chemical Reactions Nuclear Reactions Occur when bonds are broken Occur when nuclei emit particles and/or rays Atoms remain Atoms often unchanged, although converted into atoms they may be of another element rearranged Chemical vs. Nuclear Reactions Chemical Reactions Nuclear Reactions Occur when bonds are broken Occur when nuclei emit particles and/or rays Atoms remain unchanged, although they may be rearranged Atoms often converted into atoms of another element Involve only valence May involve protons, electrons neutrons, and electrons Chemical vs. Nuclear Reactions Chemical Reactions Nuclear Reactions Occur when bonds are broken Occur when nuclei emit particles and/or rays Atoms remain unchanged, although they may be rearranged Atoms often converted into atoms of another element Involve only valence electrons May involve protons, neutrons, and electrons Associated with small Associated with energy changes large energy changes Chemical vs. Nuclear Reactions Chemical Reactions Nuclear Reactions Occur when bonds are broken Occur when nuclei emit particles and/or rays Atoms remain unchanged, although they may be rearranged Atoms often converted into atoms of another element Involve only valence electrons May involve protons, neutrons, and electrons Associated with small energy changes Associated with large energy changes Reaction rate influenced by temperature, particle size, concentration, etc. Reaction rate is not influenced by temperature, particle size, concentration, etc. The Discovery of Radioactivity (1895 – 1898): found that invisible rays were emitted when electrons bombarded the surface of certain materials. Becquerel accidently discovered that phosphorescent salts produced spontaneous emissions that darkened photographic plates The Discovery of Radioactivity (1895 – 1898): isolated the components ( emitting the rays atoms) – process by which particles give off particles – the penetrating rays and by a radioactive source The Discovery of Radioactivity (1895 – 1898): identified 2 new elements, and on the basis of their radioactivity These findings Dalton’s theory of indivisible atoms. The Discovery of Radioactivity (1895 – 1898): – atoms of the element with different numbers of – isotopes of atoms with nuclei (too / neutrons) – when unstable nuclei energy by emitting to attain more atomic configurations ( process) Alpha radiation Composition – Alpha particles, same as helium nuclei 4 Symbol – Helium nuclei, 2He, α Charge – 2+ Mass (amu) – 4 Approximate energy – 5 MeV Penetrating power – low (0.05 mm body tissue) Shielding – paper, clothing Beta radiation Composition – Beta particles, same as an electron Symbol – e-, β Charge – 1Mass (amu) – 1/1837 (practically 0) Approximate energy – 0.05 – 1 MeV Penetrating power – moderate (4 mm body tissue) Shielding – metal foil Gamma radiation Composition – High-energy electromagnetic radiation Symbol – γ Charge – 0 Mass (amu) – 0 Approximate energy – 1 MeV Penetrating power – high (penetrates body easily) Shielding – lead, concrete Review of Atomic Structure Nucleus Electrons 99.9% of the mass 0.01% of the mass 1/10,000 the size of the atom Review of Atomic Structure Nucleus Electrons 99.9% of the mass 1/10,000 the size of the atom 0.01% of the mass Composed of protons (p+) and neutrons (n0) Composed of electrons (e-) Review of Atomic Structure Nucleus Electrons 99.9% of the mass 1/10,000 the size of the atom 0.01% of the mass Composed of protons (p+) and neutrons (n0) Composed of electrons (e-) Positively charged Negatively charged Review of Atomic Structure Nucleus Electrons 99.9% of the mass 1/10,000 the size of the atom 0.01% of the mass Composed of protons (p+) and neutrons (n0) Composed of electrons (e-) Positively charged Negatively charged Strong nuclear force Weak electrostatic (holds the nucleus force (because they together) are charged negatively Chemical Symbols A chemical symbol looks like… 14 6 C To find the number of from the , subtract the Nuclear Stability Isotope is completely stable if the nucleus will spontaneously . Elements with atomic #s to are . ratio of protons:neutrons ( ) Example: Carbon – 12 has protons and neutrons Nuclear Stability Elements with atomic #s to are . ratio of protons:neutrons (p+ : n0) Example: Mercury – 200 has protons and neutrons Nuclear Stability Elements with atomic #s and . Examples: and are Alpha Decay Alpha decay – emission of an alpha particle ( ), denoted by the symbol 4 , because an α has 2 2 protons and 2 neutrons, just like the He nucleus. Charge is because of the 2 . Alpha decay causes the number to decrease by and the number to decrease by . determines the element. All nuclear equations are . Alpha Decay Example 1: Write the nuclear equation for the radioactive decay of polonium – 210 by alpha emission. Step 1: Write the element that you are starting with. Step 2: Draw the arrow. Mass # Atomic # Step 3: Write the alpha particle. Step 4: Determine the other product (ensuring everything is balanced). Alpha Decay Example 2: Write the nuclear equation for the radioactive decay of radium – 226 by alpha emission. Mass # Atomic # Beta decay Beta decay – emission of a beta particle ( ), a fast moving , denoted by the symbol or -10 . β has insignificant mass ( ) and the charge is because it’s an . Beta decay causes and causes the change in number number to increase by . Beta Decay Example 1: Write the nuclear equation for the radioactive decay of carbon – 14 by beta emission. Mass # Atomic # Beta Decay Example 2: Write the nuclear equation for the radioactive decay of zirconium – 97 by beta decay. Mass # Atomic # Gamma decay Gamma rays – high-energy radiation, denoted by the symbol . γ has no mass ( ) and no charge ( ). Thus, it causes change in or numbers. Gamma rays almost accompany alpha and beta radiation. However, since there is effect on mass number or atomic number, they are usually from nuclear equations. Transmutation – the of one atom of one element to an atom of a different element ( decay is one way that this occurs!) Review Type of Radioactive Decay Alpha Beta Gamma Particle Emitted 4 2 He 0 -1e α β γ Change in Change in Mass # Atomic # -4 0 0 -2 +1 0 Half-Life is the required for of a radioisotope’s nuclei to decay into its products. For any radioisotope, # of ½ lives % Remaining 0 1 2 3 100% 50% 25% 12.5% 4 5 6 6.25% 3.125% 1.5625% Half-Life Half-Life 100 90 80 % Remaining 70 60 50 40 30 20 10 0 0 1 2 3 # of Half-Lives 4 5 6 7 Half-Life For example, suppose you have 10.0 grams of strontium – 90, which has a half life of 29 years. How much will be remaining after x number of # of ½ lives Time (Years) Amount years? Remaining (g) You can use a table: 0 1 2 3 4 0 29 58 87 116 10 5 2.5 1.25 0.625 Half-Life Or an equation! Half-Life Example 1: If gallium – 68 has a half-life of 68.3 minutes, how much of a 160.0 mg sample is left after 1 half life? ________ 2 half lives? __________ 3 half lives? __________ Half-Life Example 2: Cobalt – 60, with a half-life of 5 years, is used in cancer radiation treatments. If a hospital purchases a supply of 30.0 g, how much would be left after 15 years? ______________ Half-Life Example 3: Iron-59 is used in medicine to diagnose blood circulation disorders. The half-life of iron-59 is 44.5 days. How much of a 2.000 mg sample will remain after 133.5 days? ______________ Half-Life Example 4: The half-life of polonium-218 is 3.0 minutes. If you start with 20.0 g, how long will it take before only 1.25 g remains? ______________ Half-Life Example 5: A sample initially contains 150.0 mg of radon-222. After 11.4 days, the sample contains 18.75 mg of radon-222. Calculate the half-life. Nuclear Reactions Characteristics: Isotopes of one element are isotopes of another element Contents of the amounts of into change are released Types of Nuclear Reactions decay – alpha and beta particles and gamma ray emission Nuclear - emission of a or Nuclear Fission of a nucleus - Very heavy nucleus is split into approximately fragments reaction releases several neutrons which more nuclei - If controlled, energy is released (like in ) Reaction control depends on reducing the of the neutrons (increases the reaction rate) and extra neutrons ( creases the reaction rate). Nuclear Fission - 1st controlled nuclear reaction in December 1942. 1st uncontrolled nuclear explosion occurred July 1945. - Examples – atomic bomb, current nuclear power plants Nuclear Fusion of a nuclei nuclei combine to form a - Two heavier nucleus - Does not occur under standard conditions ( - Advantages compared to fission - repels ) , - Disadvantages - requires amount of energy to , difficult to - Examples – energy output of stars, hydrogen bomb, future nuclear power plants