Atomicity and Atomic Structure Comprehensive Study Notes

Course Introduction and Learning Outcomes

  • Institution: SEETA UNIVERSITY
  • Course: Chemistry
  • Programme: Higher Education Certificate (HEC)
  • Lecturer: MR. KYEYUNE FRANK
  • Topic: ATOMICITY

Learning Outcomes: By the end of this topic, students should be able to:

  • Describe the structure of the atom.
  • Differentiate between atomic number, mass number, and isotopes.
  • Explain radioactivity and its applications.
  • Interpret simple mass spectra.
  • Write electronic configurations.
  • Explain periodic trends.
  • Relate periodic trends to chemical bonding.

The Nature of Matter

  • Definition of Matter: Matter is anything that has mass and occupies space. It exists in different forms and is made up of tiny particles. These particles can be grouped in different ways to form the substances around us.
Classification of Matter
  • Pure Substances: These have a fixed composition and definite properties. They are subdivided into:
    • Elements: Made of only one type of atom. They cannot be broken down into simpler substances by chemical means. Examples include Iron (FeFe), Copper (CuCu), and Gold (AuAu).
    • Compounds: Made of two or more different elements chemically combined in a fixed ratio. They can be broken down into simpler substances by chemical means. Examples include Carbon dioxide (CO2CO_2) and Water (H2OH_2O).
  • Mixtures: Made of two or more substances mixed physically in any proportion. Components can be separated by physical means. An example is Sodium chloride (table salt) (NaClNaCl) dissolved in water.
Building Blocks
  • Atoms: The smallest particles of an element that retain the properties of that element. Atoms are the building blocks of matter (e.g., HeHe atom, OO atom).
  • Molecules: Two or more atoms chemically bonded together. Molecules may be of the same element (e.g., O2O_2) or of different elements (e.g., H2OH_2O).
Summary of Relationship
  • Matter forms Pure Substances or Mixtures.
  • Pure Substances consist of Elements or Compounds.
  • Elements are made of Atoms.
  • Atoms form Molecules.
  • Molecules of different elements form Compounds.

Atomic Structure and Fundamental Particles

  • The Atom: Consists of a central Nucleus containing Protons and Neutrons, with Electrons arranged in shells or energy levels around it.
Table of Fundamental Particles
ParticleRelative massElectric chargeComments
Proton (pp)11+1+1 (positive)In the nucleus (a nucleon)
Neutron (nn)1100 (zero) neutralIn the nucleus (a nucleon)
Electron (ee)1/18501/1850 or 0.00050.00051-1 (negative)Arranged in energy levels or shells around the nucleus
  • Note: These are the fundamental particles of interest to chemistry students, excluding radioactivity.

Atomic Number, Mass Number, and Isotopes

  • Atomic Number (ZZ): The number of protons in the nucleus of an atom.
  • Atomic Mass (Mass Number, AA): The sum of the number of protons and neutrons in the nucleus.
  • Example (Carbon-12):
    • Protons: 66
    • Neutrons: 66
    • Electrons: 66
    • Atomic Number = 66
    • Atomic Mass = 1212
  • Isotopes: Atoms of the same element that have the same number of protons but different numbers of neutrons.

Radioactivity and Isotope Stability

  • Radioactive Isotopes (Radioisotopes): Isotopes with unstable nuclei that spontaneously decay, emitting radiation to become more stable.
  • Radioactivity Definition: The spontaneous disintegration of an unstable atomic nucleus to stable nuclei accompanied by the emission of radiation in the form of alpha particles, beta particles, and/or gamma rays.
Factors Determining Isotope Stability
  • Neutron : proton ratio (n/pn/p ratio).
  • Atomic number.
  • Atomic mass / Mass number.
  • Binding energy: This is defined as the energy given out when a nucleus is formed from its constituent neutrons and protons, OR the energy required to separate the nucleus into its constituent neutrons and protons.
Properties of Radiations
PropertyAlpha (α\alpha)Beta (β\beta)Gamma (γ\gamma)
NatureHelium nucleusElectronElectromagnetic wave
Symbolα\alphaβ\betaγ\gamma
Charge+2+21-100
Relative Mass441/18361/183600
SpeedSlowFastSpeed of light
Ionising PowerHighModerateLow
Penetrating PowerLowModerateVery High
Stopped ByPaper or skinAluminium sheetThick lead or concrete
Deflection in FieldSlightly toward negative plateStrongly toward positive plateNot deflected

Balancing Nuclear Equations

  • Rule 1: Mass numbers (AA) must balance. Total AA on the left = Total AA on the right.
  • Rule 2: Atomic numbers (ZZ) must balance. Total ZZ on the left = Total ZZ on the right.
Examples of Nuclear Equations
  • Alpha decay:
    • 92238U90234Th+24He_{92}^{238}U \rightarrow _{90}^{234}Th + _{2}^{4}He
  • Beta decay:
    • 714N+10e614C_{7}^{14}N + _{-1}^{0}e \rightarrow _{6}^{14}C (Note: In standard beta emission, a neutron becomes a proton, e.g., Carbon-14 decay: 614C714N+10e_{6}^{14}C \rightarrow _{7}^{14}N + _{-1}^{0}e; the slide depicts a capture or reverse process).
  • Gamma emission:
    • 2760Co2760Co+00γ_{27}^{60}Co \rightarrow _{27}^{60}Co + _{0}^{0}\gamma
Practice Questions
  1. 88226Ra+24He_{88}^{226}Ra \rightarrow \dots \dots \dots + _{2}^{4}He
  2. 53131I+10e_{53}^{131}I \rightarrow \dots \dots \dots + _{-1}^{0}e

Radioactive Decay Law and Half-Life

Radioactive Decay Equations
  • lnNoNt=λt\ln \frac{N_o}{N_t} = \lambda t
  • 2.303logNoNt=λt2.303 \log \frac{N_o}{N_t} = \lambda t
  • Variables:
    • NoN_o = initial activity/mass/percentage.
    • NtN_t = activity/mass/percentage after time, tt.
    • λ\lambda = decay constant.
    • tt = time for decay.
Half-Life (T1/2T_{1/2})
  • Definition: The time it takes for half of the radioactive atoms in a sample to decay.
  • At half-life, Nt=No2N_t = \frac{N_o}{2}.
  • Calculation:
    • ln(NoNo/2)=λT1/2\ln \left(\frac{N_o}{N_o/2}\right) = \lambda T_{1/2}
    • T1/2=0.693λT_{1/2} = \frac{0.693}{\lambda}
Worked Examples
  1. Decay constant to Half-life: A radioactive isotope has a decay constant of 0.035day10.035\,day^{-1}. Calculate its half-life.
  2. Calculating Decay Constant: A radioactive sample initially contains 120g120\,g. After 10days10\,days, only 45g45\,g remains. Calculate the decay constant.
  3. Calculating Remaining Mass: A radioactive sample has a decay constant of 0.046day10.046\,day^{-1}. If the initial mass is 200g200\,g, calculate the mass remaining after 15days15\,days.
Further Practice Questions
  1. A radioactive isotope has a decay constant of 0.025day10.025\,day^{-1}. Calculate its half-life.
  2. A sample decreases from 80g80\,g to 20g20\,g in 12hours12\,hours. Calculate the decay constant.
  3. A radionuclide has a decay constant of 0.12year10.12\,year^{-1}. Calculate the mass remaining from an initial 50g50\,g after 5years5\,years.
  4. A sample has a half-life of 8hours8\,hours. Calculate its decay constant.
  5. A 150g150\,g radioactive sample is reduced to 75g75\,g in 6days6\,days. Verify the half-life using both methods.

Applications of Radioisotopes

RadioisotopeMain UseHow it Works
Carbon-14 (14C^{14}C)Archaeological datingMeasures remaining 14C^{14}C in once-living materials to estimate age (up to 50,000\approx 50,000 years).
Iodine-131 (131I^{131}I)MedicineConcentrates in the thyroid gland to destroy overactive tissue or cancer cells.
Cobalt-60 (60Co^{60}Co)RadiotherapyEmits high-energy gamma rays to destroy cancer cells in directed tumors.
Uranium-235 ($^{235}U) | Nuclear energy | Undergoes nuclear fission to release heat used for generating steam and electricity. |\n\n# Mass Spectroscopy\n\n* **Definition:** An analytical technique used to determine relative atomic mass, relative molecular mass, isotopic composition, and molecular structure by measuring the mass-to-charge ratio (m/z) of ions.\n\n### How the Mass Spectrometer Works\n1. **Vaporisation chamber:** The sample is converted into a gas by heating. This ensures particles move individually for efficient ionisation.\n2. **Ionisation chamber:** Gaseous atoms/molecules are bombarded with fast-moving electrons. This knocks out electrons, producing positive ions (usually M^+ororM^{+\cdot}).\n * **Equation:** M(g) + e^- \rightarrow M^+(g) + 2e^-\n3. **Acceleration chamber:** Positive ions are accelerated by a strong electric field of varying potentials. Ions achieve the same velocity/kinetic energy but retain different mass-charge ratios.\n4. **Deflection chamber:** A magnetic field deflects ions according to their mass-charge ratio (m/z). Field strength is varied to focus specific ions onto the detector.\n5. **Detector, Amplifier, and Recorder:** Ions generate electric currents, which are amplified and recorded as peaks. The peaks show relative intensities of ions.\n\n### Interpreting Mass Spectra\n* **Formula for Relative Atomic Mass:**\n    \text{Relative Atomic Mass} = \frac{\sum (\text{Isotopic mass} \times \text{Relative abundance})}{\sum (\text{Relative abundance})}\n* **Chlorine Example:** The spectrum typically shows peaks at m/z35andand37, representing the isotopes of chlorine.\n\n# Electronic Configuration\n\n* **Definition:** The arrangement of electrons in the atomic orbitals of an atom according to increasing energy.\n\n### Subshell Capacities\n* **s:** 1orbital,maxorbital, max2 electrons.\n* **p:** 3orbitals,maxorbitals, max6 electrons.\n* **d:** 5orbitals,maxorbitals, max10 electrons.\n* **f:** 7orbitals,maxorbitals, max14 electrons.\n\n### Governing Rules\n* **Aufbau's Rule:** Electrons occupy orbitals of the lowest available energy before filling higher-energy orbitals (1s < 2s < 2p < 3s < 3p < 4s < 3d \dots).\n* **Pauli's Exclusion Principle:** No two electrons in the same atom can have the same set of four quantum numbers. Implication: Each orbital holds a maximum of two electrons, and they must have opposite spins.\n* **Hund's Rule of Maximum Multiplicity:** When electrons occupy orbitals of equal energy (degenerate orbitals), they first occupy each orbital singly with parallel spins before pairing.\n\n### Group 1 Electronic Configurations\n| Element | Atomic Number | Electron Configuration (Aufbau) | Shell Arrangement |\n| :--- | :--- | :--- | :--- |\n| Hydrogen (H)) |1|1s^1|1 |\n| Lithium (Li)) |3|1s^2 2s^1|2, 1 |\n| Sodium (Na)) |11|1s^2 2s^2 2p^6 3s^1|2, 8, 1 |\n| Potassium (K)) |19|1s^2 2s^2 2p^6 3s^2 3p^6 4s^1|2, 8, 8, 1 |\n| Rubidium (Rb)) |37|[\dots] 4s^2 3d^{10} 4p^6 5s^1|2, 8, 18, 8, 1 |\n| Caesium (Cs)) |55|[\dots] 5s^2 4d^{10} 5p^6 6s^1|2, 8, 18, 18, 8, 1 |\n| Francium (Fr)) |87|[\dots] 6s^2 4f^{14} 5d^{10} 6p^6 7s^1|2, 8, 18, 32, 18, 8, 1 |\n\n# Periodic Trends\n\n### Atomic Radius\n* **Definition:** Half the distance between the nuclei of two identical bonded atoms.\n* **Across a Period:** Decreases. Nuclear charge increases as protons are added. Electrons are added to the same energy level, leading to little change in shielding. The increased effective nuclear charge pulls electrons closer.\n* **Down a Group:** Increases. Additional electron shells are added, placing outer electrons further from the nucleus. Increased shielding from inner shells outweighs the increased nuclear charge.\n\n### Screening (Shielding) Effect\n* **Definition:** The reduction in attraction between the nucleus and the outermost electrons due to the presence of inner-shell electrons.\n* **Across a Period:** Remains almost constant (electrons added to the same shell).\n* **Down a Group:** Increases significantly (new shells are added).\n\n### Ionisation Energy (Ionisation Potential)\n* **Definition:** Energy required to remove one electron from one mole of gaseous atoms/ions to form one mole of gaseous positive ions.\n * **Equation:** X(g) \rightarrow X^+(g) + e^-\n* **Across a Period:** Increases (due to increased effective nuclear charge and decreased atomic radius).\n* **Down a Group:** Decreases (due to increased atomic radius and shielding).\n\n### Electron Affinity\n* **Definition:** Energy change when one mole of gaseous atoms gains one mole of electrons to form gaseous negative ions.\n * **Equation:** X(g) + e^- \rightarrow X^-(g)\n* **Exothermic vs Endothermic:** Usually energy is released (negativevalues).Addingasecondelectronisendothermic(values). Adding a second electron is endothermic (positive$$) due to repulsion.
  • Across a Period: Becomes more negative (stronger attraction for incoming electrons).
  • Down a Group: Becomes less negative (weaker attraction due to large radius and shielding).
Electronegativity
  • Definition: The tendency of an atom to attract the shared pair of electrons toward itself in a chemical bond.
  • Across a Period: Increases.
  • Down a Group: Decreases.

Questions & Discussion

Conceptual Question
  • Question: Why is gamma radiation preferred for treating cancers deep inside the body, whereas alpha radiation is not?
  • Context: Based on the properties table, gamma radiation has very high penetrating power (requiring thick lead to stop), allowing it to reach internal tumors. Alpha radiation has low penetrating power and is stopped by skin, meaning it cannot reach internal targets from outside the body.
Individual Assignment
  1. Using Aufbau’s rule, Pauli’s exclusion principle, and Hund’s rule of maximum multiplicity, write the electronic configurations of Group II and Period 3 elements.
  2. Explain the following trends in the periodic table across Period 3 and down Group II:
    • i) Ionisation energy
    • ii) Electron affinity
    • iii) Electronegativity
    • iv) Atomic radius