Models of the Atom Review

Models of the Atom

MoA.1: Experimental Evidence and Modern Atomic Models

  • Cathode Ray Tube Experiment:
    • Demonstrated that a beam of light comprises charged particles, which are 1000 times smaller than a hydrogen atom.
    • Change to Atomic Model: Showed that atoms are not indivisible and contain smaller, negatively charged particles (electrons).
  • Gold Foil Experiment:
    • Positively charged alpha particles were directed at a thin gold foil.
    • Most particles passed through undeflected, but some were deflected or bounced back.
    • Change to Atomic Model: Indicated that an atom has a small, dense, positively charged nucleus surrounded by mostly empty space.
  • Line Spectra of Energized Atoms:
    • Each element emits a unique color and line spectrum when energized.
    • Change to Atomic Model: Suggested that electrons exist in specific energy levels and emit energy (light) when transitioning between these levels.

MoA.2: Atomic Structure and Calculations

  • Atomic Number:

    • Identifies an atom of a specific element.
  • Isotopes:

    • Atoms of the same element with the same number of protons but different numbers of neutrons.
    • Example: Silicon-28, Silicon-29, and Silicon-30.
    • Same: number of protons.
    • Different: number of neutrons, mass number.
  • Isotope Notation and Calculations

    • The mass number is the sum of protons and neutrons in the nucleus.
    • Isotope Symbol: ZAX^{A}_{Z}X, where:
      • XX = element symbol
      • ZZ = atomic number (number of protons)
      • AA = mass number (number of protons + neutrons)
  • Ions:

    • Atoms that have gained or lost electrons, resulting in a net charge.
    • Cations: positively charged ions (loss of electrons).
    • Anions: negatively charged ions (gain of electrons).
  • Average Atomic Mass Calculation:

    • Weighted average of the masses of all isotopes of an element.
    • Formula: Average Atomic Mass=(Isotope Mass×Relative Abundance)Average \ Atomic \ Mass = \sum (Isotope \ Mass \times Relative \ Abundance)
      Example Calculations:
  • Radioactive Decay Equations:

    • Beta+ Decay (Positron Emission): A proton in the nucleaus is converted into a neutron, releasing a positron (e+e^+
      • Generic Equation: A<em>ZX A</em>Z1Y+ +10e^{A}<em>{Z}X \rightarrow \ ^{A}</em>{Z-1}Y + \ ^{0}_{+1}e
      • Example: Cobalt-54:
        • 54<em>27Co 54</em>26Fe+ +10e^{54}<em>{27}Co \rightarrow \ ^{54}</em>{26}Fe + \ ^{0}_{+1}e
    • Beta- Decay: A neutron in the nucleus is converted into a proton, releasing an electron (ee^-
      • Generic Equation: A<em>ZX A</em>Z+1Y+ 10e^{A}<em>{Z}X \rightarrow \ ^{A}</em>{Z+1}Y + \ ^{0}_{-1}e
      • Example: Zinc-71:
        • 71<em>30Zn 71</em>31Ga+ 10e^{71}<em>{30}Zn \rightarrow \ ^{71}</em>{31}Ga + \ ^{0}_{-1}e
    • Alpha Decay: Emission of an alpha particle (α\alpha, which is a helium nucleus, 24He^4_2He) from the nucleus.
      • Generic Equation: A<em>ZX A4</em>Z2Y+ 24He^{A}<em>{Z}X \rightarrow \ ^{A-4}</em>{Z-2}Y + \ ^{4}_{2}He
      • Example: Uranium-238:
        • 238<em>92U 234</em>90Th+ 24He^{238}<em>{92}U \rightarrow \ ^{234}</em>{90}Th + \ ^{4}_{2}He
  • Half-Life:

    • The time required for half of the radioactive atoms in a sample to decay.
    • After nn half-lives, the remaining amount is 12n\frac{1}{2^n} of the original amount.
    • Example: If a sample of 1,000 radioactive atoms has a half-life of 15 hours, to find how much time will pass until only 62 atoms remain:
    • 1000150022503125462.51000 \xrightarrow{1} 500 \xrightarrow{2} 250 \xrightarrow{3} 125 \xrightarrow{4} 62.5
    • It takes 4 half-lives, so 4×15=604 \times 15 = 60 hours

MoA.3: Electron Configuration and Orbital Diagrams

  • Maximum Number of Electrons in Sublevels:
    • s sublevel: 2 electrons
    • p sublevel: 6 electrons
    • d sublevel: 10 electrons
    • f sublevel: 14 electrons
  • Maximum Number of Electrons in Energy Levels:
    • Energy level nn can hold 2n22n^2 electrons.
    • For example, the 5th energy level can hold 2(52)=502(5^2) = 50 electrons; however, only 32 electrons are typically accommodated due to sublevel restrictions.
  • Number of Orbitals in Sublevels:
    • s sublevel: 1 orbital
    • p sublevel: 3 orbitals
    • d sublevel: 5 orbitals
    • f sublevel: 7 orbitals
  • Comparing Energy of Sublevels:
    • Use the Aufbau principle and the n+ln + l rule to determine the order in which electrons fill sublevels.
    • Electrons first fill the orbitals with the lowest energy.
    • If two sublevels have the same n+ln + l value, the sublevel with the lower nn value is filled first.
  • Orbital Diagrams:
    • Use boxes to represent orbitals and arrows to represent electrons.
    • Follow Hund's rule: within a sublevel, electrons are individually placed into each orbital before any orbital is doubly occupied.
  • Electron Configurations:
    • Shorthand notation showing the number of electrons in each sublevel.
    • Example: Iodine (I): 1s22s22p63s23p64s23d104p65s24d105p51s^22s^22p^63s^23p^64s^23d^{10}4p^65s^24d^{10}5p^5
    • Valence electrons are those in the highest occupied energy level.
  • Electron Configurations of Ions:
    • Anions (negative ions): add electrons to the electron configuration.
      • Example: I-: 1s22s22p63s23p64s23d104p65s24d105p61s^22s^22p^63s^23p^64s^23d^{10}4p^65s^24d^{10}5p^6
    • Cations (positive ions): remove electrons from the electron configuration, starting with the outermost energy level.
      • Example: Ti2+: 1s^22s^22p^63s^23p^64s^23d^2
        \rightarrow 1s^22s^22p^63s^23p^63d^2

MoA.4: Periodic Trends

  • Families/Groups:
    • Alkali Metals (Group 1):
      • Ending electron configuration: ns1ns^1
      • Ion charge: +1
      • Number of valence electrons: 1
    • Alkaline Earth Metals (Group 2):
      • Ending electron configuration: ns2ns^2
      • Ion charge: +2
      • Number of valence electrons: 2
    • Transition Metals (Groups 3-12):
      • Variable oxidation states.
    • Halogens (Group 17):
      • Ending electron configuration: ns2np5ns^2np^5
      • Ion charge: -1
      • Number of valence electrons: 7
    • Noble Gases (Group 18):
      • Ending electron configuration: ns2np6ns^2np^6 (except Helium, which is 1s21s^2)
      • Inert (unreactive)
  • Atomic Radius:
    • The distance from the nucleus to the outermost electron.
    • Trends:
      • Decreases across a period (left to right) due to increasing nuclear charge (more protons).
      • Increases down a group due to the addition of energy levels.
    • Example: Sodium (Na) vs. Magnesium (Mg):
      • Na has a larger radius because it has fewer protons than Mg, resulting in less attraction between the nucleus and electrons.
  • Electronegativity:
    • The ability of an atom to attract electrons in a chemical bond.
    • Trends:
      • Increases across a period (left to right) due to increasing nuclear charge.
      • Decreases down a group due to increasing atomic radius (valence electrons are farther from the nucleus).
    • Example: Carbon (C) vs. Oxygen (O):
      • C has a lower electronegativity because it has fewer protons than O, resulting in less attraction for electrons.
  • Ionization Energy:
    • The energy required to remove an electron from an atom.
    • Trends:
      • Increases across a period (left to right) due to increasing nuclear charge and decreasing atomic radius.
      • Decreases down a group due to increasing atomic radius (valence electrons are farther from the nucleus).
    • Example: Chlorine (Cl) vs. Bromine (Br):
      • Cl has a larger first ionization energy because its valence electrons are closer to the nucleus than Br's valence electrons.
        *Ranking Example: Ionization Energy:
    • Boron (B), Carbon (C), Nitrogen (N): N > C > B (highest to lowest)
      *Ranking Example: Atomic Radius:
    • Boron (B), Aluminum (Al), Gallium (Ga): B < Al < Ga (lowest to highest)