Unit 13 Nuclear Chemistry
Nuclear radioactivity Natural radioactivity Radioactivity - emission of particles or energy from an unstable nucleus Discovered by Henri Bequerel Three types of radioactive decay
The nature of the nucleus Strong nuclear force Binds protons and neutrons Very short ranged, less than 10-15 m Overcomes proton-proton Coulomb repulsion Band of stability
Generalizations - nuclear stability Atomic number > 83: Nucleon number = 2, 8, 20, 28, 50, 82 or 126: added stability Pairs of protons and pairs of neutrons: added stability Neutron: proton ratios for added stability 1+increasing:1 with increasingly heavy isotopes
Nuclear equations Atomic number = Isotopes: same atomic number; Mass number = number of nucleons (protons and neutrons) in nucleus Nuclear reactions Represented by balanced equations
Types of radioactive decay Alpha emission Beta emission Gamma decay
Radioactive decay series One radioactive nucleus decays to a 2nd, which decays to a 3rd, which… Three naturally occurring series Thorium-232 to lead-208 Uranium-235 to lead-207 Uranium-238 to lead-206
Writing Nuclear Equations Write what you start with on the left side of the arrow Using conservation of mass and atomic #, determine what the new nucleus will be
Things to remember: Alpha decay gives off a He nucleus Beta decay gives off a high energy e-
Practice Thorium-232 undergoes Alpha decay Radium 228 undergoes Beta decay
Radioactive Decay Rates It is impossible to predict the exact moment a nucleus will decay We CAN predict the time for half the nuclei in a sample to decay
Half-life Time required for 1/2 of a radioactive sample to decay Example: 1 kg of an unstable isotope with a one-day half-life After 1 day: After 2 days: After 3 days: U-238 decay series: wide half-life variation
Calculating Half Lives Radium-226 has a half life of 1599 years. How long would it take seven-eighths of a radium-226 sample to decay? Step 1- List the given and unknown values
Calculating Half Lives Step 2- Calculate the fraction of radioactive sample remaining Step 3- Calculate the number of half lives
Calculating Half-Lives Radium-226 has a half life of 1599 years. How long would it take seven-eighths of a radium-226 sample to decay? Step 4- Calculate the total time required for the radioactive decay
Nuclear energy There is an overall loss of mass in nuclear reactions Why? Interconversion of mass and energy Mass defect
Nuclear Energy Binding energy Energy out? Energy required to break a nucleus into individual protons and neutrons Energy out? E=mc2 E= energy in J M= mass defect in kg C= speed of light 3.0e8 m/s
Nuclear fission Chain reactions Critical mass Possible when one reaction can lead to others One neutron in, two or more out Critical mass
Many possible fission fragments
Nuclear fusion Less massive nuclei forming more massive nuclei Requirements for fusion High temperature Sufficient confinement time
Nuclear power plants Rely on controlled fission chain reactions Steel vessel contains fuel rods and control rods Full plant very intricate Containment and auxiliary buildings necessary Spent fuel rods Contain fissionable materials U-235, Pu-239 Disposal issues not settled
Source of nuclear energy Ultimately connected to origins of the Universe and the life cycles of stars Big Bang theory Incredibly hot, dense primordial plasma cools, creating protons and neutrons Continued cooling leads to hydrogen atoms which collapse gravitationally into 1st generation stars Stellar evolution Interior temperatures and densities suitable for fusion of heavy elements beyond hydrogen and helium Certain massive stars explode in supernovae, spreading heavy elements (some radioactive) Ultimate source: gravitational attraction!