Guide to Nuclear Chemistry: Structure, Transmutation, and Applications

Foundations of Nuclear Chemistry and Atomic Structure

  • Core Focus: Unlike traditional chemistry, which focuses on how the electrons of atoms and ions are shared, transferred, and involved in bonding, Nuclear Chemistry specifically focuses on the NUCLEUS.

  • The Nature of Nuclear Chemistry: Nuclear chemistry is described as "weird" because it involves changes within the nucleus rather than electron movement.

Essential Atomic Components and Measurements

  • Nucleus Construction: Atoms contain protons and neutrons within the nucleus, with electrons orbiting the outside.

  • Electrical Neutrality: In every neutral atom, the number of positive protons equals the number of negative electrons (p+=ep^+ = e^-).

  • Atomic Number: The Atomic Number is defined as the number of protons in an atom.

  • Atomic Mass in High School Chemistry:

    • Defined as the sum of the number of protons (pp) plus the number of neutrons (nn).

    • Measured in Atomic Mass Units (AMUs).

    • Weight of individual particles: Each proton = 1AMU1\,AMU; Each neutron = 1AMU1\,AMU.

    • Molar Mass Correlation: Atomic mass (in amu) correlates to molar mass (in g/mole).

    • Helium (HeHe): 4amu4\,amu (2p+2n2p + 2n ) = 4g/mole4\,g/mole.

    • Mercury (HgHg): 201amu201\,amu (80p+121n80p + 121n) = 201g/mole201\,g/mole.

    • Copper (CuCu): 64amu64\,amu (29p+35n29p + 35n) = 64g/mole64\,g/mole.

  • Calculating Neutrons and Electrons:

    • Example: Uranium (element 92) with an atomic mass of 238.

    • Calculation: 238(protons + neutrons)92(protons)=126neutrons238\,(\text{protons + neutrons}) - 92\,(\text{protons}) = 126\,\text{neutrons}.

    • Electron identification: Since there are 92 positive protons, there must be 92 negative electrons for the atom to remain neutral.

Element Identity and Isotopes

  • Proton Identity: Every atom has a unique number of protons that determines its identity.

    • 12 protons = Magnesium (MgMg).

    • 29 protons = Copper (CuCu).

    • 90 protons = Thorium (ThTh).

  • Isotopes: Atoms of the same element that possess a DIFFERENT number of neutrons but the SAME number of protons and electrons.

  • Radium Example (The most common isotope):

    • Atomic symbol: 88226Ra^{226}_{88}Ra

    • Atomic Number: 88, which means 88 protons and 88 electrons.

    • Atomic Mass: 226AMU226\,AMU.

    • Neutrons: 22688=138neutrons226 - 88 = 138\,\text{neutrons}.

Isotopes and Nuclear Stability

  • Stability and the Neutron-to-Proton Ratio:

    • Carbon-12 (C-12):

    • Mass: 12AMU12\,AMU.

    • Numbers: 6 protons, 6 neutrons.

    • Ratio: 6:66:6 or 1:11:1. This ratio is stable; therefore, C-12 is not radioactive.

    • Carbon-14 (C-14):

    • Mass: 14AMU14\,AMU.

    • Numbers: 6 protons, 8 neutrons.

    • Ratio: 8:68:6 or 1.33:11.33:1. This ratio is unstable; therefore, C-14 is radioactive.

    • Phosphorous-31 (Stable P):

    • Mass: 31AMU31\,AMU.

    • Numbers: 15 protons, 16 neutrons.

    • Ratio: 16:1516:15, which is stable.

    • Phosphorous-32 (Radioactive P):

    • Mass: 32AMU32\,AMU.

    • Numbers: 15 protons, 17 neutrons.

    • Ratio: 17:1517:15, which is unstable.

  • The Zone of Stability:

    • Of the 118 known elements, there are approximately 1500 known isotopes.

    • Most isotopes are stable. Only about 150 are unstable (radioactive).

    • Stable Ratios by Atom Size:

    • Smaller atoms (up to Calcium, CaCa): approximately 1n0/p+1\,n^0/p^+.

    • Medium atoms (up to Zirconium, ZrZr): approximately 1.25n0/p+1.25\,n^0/p^+.

    • Larger atoms (the rest): approximately 1.5n0/p+1.5\,n^0/p^+.

    • Ratios outside this "band of stability" are unstable and must fix the ratio to become stable.

Radioactive Particles and Radiation Properties

  • Emission Mechanism: Unstable isotopes emit radiation (nuclear particles and/or energy) to fix a "funky" neutron-to-proton ratio and achieve stability.

  • Reference Table O: Lists official symbols, masses, and charges for radioactive particles.

  • Types of Radiation:

    • Alpha (α\alpha):

    • Symbol: 24He^4_2He

    • Mass: 4AMU4\,AMU

    • Charge: +2+2

    • Penetrating Power: WEAKEST (stopped by paper).

    • Beta (Beta-minus, β\beta^-):

    • Symbol: 10e^0_{-1}e

    • Mass: Zero (as defined in High School)

    • Charge: 1-1

    • Penetrating Power: STRONG (stopped by aluminum/metal).

    • Origin: A neutron emits a negative charge of no mass and becomes a proton (n0p++βn^0 \rightarrow p^+ + \beta^-).

    • Gamma (γ\gamma):

    • Symbol: 00γ^0_0\gamma

    • Mass: Zero

    • Charge: Neutral

    • Penetrating Power: STRONGEST (stopped by lead; nothing stops it completely).

    • Neutron (nn):

    • Symbol: 01n^1_0n

    • Mass: 1AMU1\,AMU

    • Charge: Neutral

    • Penetrating Power: MEDIUM (stopped by water/concrete/lead).

    • Proton (pp):

    • Symbol: 11H^1_1H

    • Mass: 1AMU1\,AMU

    • Charge: +1+1

    • Positron (Beta-plus, β+\beta^+):

    • Symbol: +10e^0_{+1}e

    • Mass: Zero (as defined in High School)

    • Charge: +1+1

    • Penetrating Power: Similar to Beta particles.

    • Origin: A proton emits a positive charge of no mass and becomes a neutron (p+n0+β+p^+ \rightarrow n^0 + \beta^+).

Transmutation: Natural and Artificial

  • Transmutation Definition: The process of a nucleus changing into a different kind of atom (changing the neutron-to-proton ratio).

  • Natural Transmutation (Radioactive Decay):

    • Occurs spontaneously on its own.

    • Nothing can speed up or slow down this process.

    • Examples from Table N:

    • Alpha Decay of U-238: 92238U24He+90234Th^{238}_{92}U \rightarrow ^4_2He + ^{234}_{90}Th. U-238 transforms into Thorium-234.

    • Beta Decay of C-14: 614C10e+714N^{14}_6C \rightarrow ^0_{-1}e + ^{14}_7N. Carbon transmutes into Nitrogen-14 as a neutron becomes a proton.

    • Positron Decay of Ca-37: 2037Ca+10e+1937K^{37}_{20}Ca \rightarrow ^0_{+1}e + ^{37}_{19}K. Calcium transmutes into Potassium-37.

    • Alpha Decay of Ra-226: 88226Ra24He+86222Rn^{226}_{88}Ra \rightarrow ^4_2He + ^{222}_{86}Rn. Radium transmutes into Radon-222.

    • Beta Decay of Cs-137: 55137Cs10e+56137Ba^{137}_{55}Cs \rightarrow ^0_{-1}e + ^{137}_{56}Ba. Cesium transmutes into Barium-137.

    • Positron Decay of Fe-53: 2653Fe+10e+2553Mn^{53}_{26}Fe \rightarrow ^0_{+1}e + ^{53}_{25}Mn. Iron transmutes into Manganese-53.

    • Beta Decay of Au-198: 79198Au10e+80198Hg^{198}_{79}Au \rightarrow ^0_{-1}e + ^{198}_{80}Hg. Gold transmutes into Mercury-198.

    • Positron Decay of Ne-19: 1019Ne+10e+919F^{19}_{10}Ne \rightarrow ^0_{+1}e + ^{19}_9F. Neon transmutes into Fluorine-19.

    • Alpha Decay of Fr-220: 87220Fr24He+85216At^{220}_{87}Fr \rightarrow ^4_2He + ^{216}_{85}At. Francium transmutes into Astatine-216.

  • Artificial Transmutation:

    • Caused by humans; done by scientists through bombardment.

    • Historical Examples:

    • Ernest Rutherford (1919): Bombarded Nitrogen with alpha particles. Reaction: 714N+24He817O+11p^{14}_7N + ^4_2He \rightarrow ^{17}_8O + ^1_1p.

    • James Chadwick (1932): Bombarded Beryllium with alpha particles (led to the discovery of the neutron). Reaction: 49Be+24He612C+01n^9_4Be + ^4_2He \rightarrow ^{12}_6C + ^1_0n.

    • Marie Curie (1934): Created the first artificial radioisotope by bombarding Aluminum. Reaction: 1327Al+24He1530P+01n^{27}_{13}Al + ^4_2He \rightarrow ^{30}_{15}P + ^1_0n.

Half-Life and Radioactive Decay Problems

  • Half-Life Definition: The amount of time required for one half of a given radioisotope to transmute.

  • Values from Table N:

    • Gold-198 (Au198Au-198): 2.695days2.695\,days

    • Carbon-14 (C14C-14): 5715years5715\,years

    • Calcium-37 (Ca37Ca-37): 182ms182\,ms

    • Uranium-238 (U238U-238): 4.47×109years4.47 \times 10^9\,years

    • Plutonium-239 (Pu239Pu-239): 2.410×104years2.410 \times 10^4\,years

    • Radium-226 (Ra226Ra-226): 1599years1599\,years

    • Radon-222 (Rn222Rn-222): 3.823days3.823\,days

    • Strontium-90 (Sr90Sr-90): 29.1years29.1\,years (derived from calculation)

  • Half-Life T-Chart Rules:

    • Always make a T-chart.

    • Used to solve for: % left/transmuted, grams left/transmuted, fractions, or time elapsed.

  • Practice Problem Calculations:

    • C-14 (22.0g to 2.75g): This is 3 half-lives (22.011.05.502.7522.0 \rightarrow 11.0 \rightarrow 5.50 \rightarrow 2.75). Calculation: 3×5715=17,145years3 \times 5715 = 17,145\,years.

    • I-131 (2.00g to 0.125g): This is 4 half-lives (2.001.000.5000.2500.1252.00 \rightarrow 1.00 \rightarrow 0.500 \rightarrow 0.250 \rightarrow 0.125). Calculation: 4×8.021=32.084days4 \times 8.021 = 32.084\,days.

    • Fe-53 (400.0g to 12.5g): This is 5 half-lives. Calculation: 5×8.51minutes=42.55minutes5 \times 8.51\,minutes = 42.55\,minutes.

    • Na-25 half-life: If 1.00g remains of 16.00g after 237 seconds: (16842116 \rightarrow 8 \rightarrow 4 \rightarrow 2 \rightarrow 1) = 4 cycles. Calculation: 237/4=59.3seconds237 / 4 = 59.3\,seconds.

Nuclear Energy: Fission and Fusion

  • Einstein’s Equation: E=mc2E = mc^2. Energy equals mass times the speed of light squared. Matter and energy are different forms of the same thing.

  • Mass Defect: The missing mass in a nuclear reaction that was converted into energy. The Law of Conservation of Mass does not apply in nuclear chemistry.

  • Nuclear Fission:

    • The splitting of atoms by artificial transmutation.

    • Triggered by neutron bombardment to start a chain reaction.

    • Example: 92235U+01n56140Ba+3693Kr+301n+energy^{235}_{92}U + ^1_0n \rightarrow ^{140}_{56}Ba + ^{93}_{36}Kr + 3\,^1_0n + \text{energy}.

    • Example: 92235U+01n54144Xe+3890Sr+201n+energy^{235}_{92}U + ^1_0n \rightarrow ^{144}_{54}Xe + ^{90}_{38}Sr + 2\,^1_0n + \text{energy}.

    • Each cycle releases more neutrons, facilitating exponential growth (3, 9, 27…).

    • Comparing Bomb vs. Power Plant: In a bomb, the chain reaction is an "out of control" release of energy in seconds. In a power plant, it is controlled over months.

  • Nuclear Fusion:

    • The "squishing together" of smaller atoms to make larger ones.

    • Loss of mass occurs during the process (mass defect).

    • Fusion is much more powerful than fission.

    • Solar Fusion: The Sun squashes 4 hydrogen atoms into helium: 411H24He+2+10e+energy4\,^1_1H \rightarrow ^4_2He + 2\,^0_{+1}e + \text{energy}.

    • Laboratory Fusion: Humans use isotopes of hydrogen (H2H-2 and H3H-3) because fusing normal H1H-1 requires temperature/pressure that is too high for containment: 2H+3H24He+01n+energy^2H + ^3H \rightarrow ^4_2He + ^1_0n + \text{energy}.

Nuclear Power Plant Mechanics

  • Method of Electricity Generation: Heat from fission \rightarrow Water turns to steam \rightarrow Steam spins turbine blades \rightarrow Spinning rotates magnets around copper wire in a generator \rightarrow Electricity created.

  • Core Components:

    • Reactor Vessel: Location of the fission reaction (U-235 bombardment).

    • Control Rods: Made of materials like Cadmium, Silver, or Indium. They absorb neutrons to slow down/moderate the reaction and prevent explosion.

    • Containment Structure: Reinforced dome designed to keep radiation in and external factors out.

  • Water Loops:

    • Inner Loop (Pink/Red): Highly radioactive water in close contact with the reactor; stays sealed in the containment dome.

    • Secondary Loop (Blue): Picks up heat from the inner loop via heat exchange; turns into steam to spin turbines.

    • Cooling Loop: Uses water from an outside source (lake/ocean) to condense turbine steam back into water. This releases excess heat via cooling towers.

  • Pros and Cons of Nuclear Energy:

    • Pros: Low CO2 emissions, reliable, national energy independence, low operating costs.

    • Cons: Mining impact, potential for disasters, high setup cost, limited uranium supplies, creation of long-term radioactive waste (remains dangerous for 20,000+ years).

Practical and Medical Applications

  • Radioactive Carbon Dating:

    • Mechanism: High-energy neutrons hit nitrogen in the atmosphere: n+714N614C+11pn + ^{14}_7N \rightarrow ^{14}_6C + ^1_1p.

    • Constant ratio: Living things have a constant ratio of C-14 to C-12 because they replace carbon through eating.

    • After death: The organism stops eating; C-14 begins decaying into nitrogen without replacement.

    • Limit: Accurate up to 50,000 years. Cannot date dinosaurs.

    • Case Study: La Brea Tar Pits (Mastodons preserved in tar used for dating).

  • Medical Radioisotopes:

    • Iodine-131: Used for thyroid disorder diagnosis and treatment. The gland picks up radioactive iodine chemically; beta radiation emitted can kill thyroid cancer cells.

    • Cobalt-60: Used for internal cancer treatment. Emits beta radiation beams aimed precisely at tumors to kill cancer cells with minimal healthy cell damage.