Atomic Structure

๐Ÿ”น Particles in the Atom and Atomic Radius

โš›๏ธ Subatomic Particles:

  • Atoms are made of protons, neutrons, and electrons.
  • Protons: Positive charge (+1), relative mass = 1
  • Neutrons: Neutral charge (0), relative mass = 1
  • Electrons: Negative charge (โ€“1), relative mass โ‰ˆ 1/1836
ParticleRelative MassRelative Charge
Proton1+1
Neutron10
Electron~1/1836โ€“1

โš—๏ธ Experimental Discovery:

  • J.J. Thomson discovered electrons using the cathode ray tube experiment.
  • Rutherford’s Gold Foil Experiment discovered the nucleus:
    โ†’ Most alpha particles passed through, but a few deflected.
    โ†’ Conclusion: Atoms have a small, dense, positively charged nucleus.
  • Millikan’s Oil Drop Experiment: Determined the charge of the electron.

๐Ÿ“ Atomic Radius:

  • Atomic radius decreases across a period (โ†‘ nuclear charge, electrons pulled closer).
  • Increases down a group (โ†‘ electron shells, more shielding).

๐Ÿ”น Isotopes, Relative Atomic Mass (RAM), and Relative Molecular Mass (RMM)

๐Ÿงช Isotopes:

  • Definition: Atoms of the same element with the same number of protons but different numbers of neutrons.
  • Example:
    • Hydrogen: ยนH, ยฒH (deuterium), ยณH (tritium)
    • Carbon: ยนยฒC, ยนยณC, ยนโดC

๐Ÿ“Š Relative Atomic Mass (RAM):

Weighted average mass of the isotopes of an element, relative to 1/12 of the mass of a ยนยฒC atom.

Formula: RAM=โˆ‘(isotopic massร—abundance)/100

๐Ÿงฎ Relative Molecular Mass (RMM):

  • Sum of the relative atomic masses of all atoms in a molecule.
  • E.g., for Hโ‚‚O:
    RMM = (2 ร— 1.0) + 16.0 = 18.0

๐Ÿ”น Electrons, Energy Levels and Atomic Orbitals

๐ŸŒ€ Electron Configuration:

  • Electrons occupy orbitals (s, p, d, f) in order of increasing energy.
  • Aufbau Principle: Fill lower energy orbitals first.
  • Pauli Exclusion Principle: Max 2 electrons per orbital, opposite spins.
  • Hundโ€™s Rule: Electrons occupy all orbitals singly before pairing.

๐Ÿ“‹ Order of Filling:

1s โ†’ 2s โ†’ 2p โ†’ 3s โ†’ 3p โ†’ 4s โ†’ 3d โ†’ 4p

๐Ÿ”ข Electron Configurations (Z = 1 to 36):

Examples:

  • H (Z = 1): 1sยน
  • He (Z = 2): 1sยฒ
  • O (Z = 8): 1sยฒ 2sยฒ 2pโด
  • Na (Z = 11): 1sยฒ 2sยฒ 2pโถ 3sยน
  • Cl (Z = 17): 1sยฒ 2sยฒ 2pโถ 3sยฒ 3pโต
  • Ca (Z = 20): 1sยฒ 2sยฒ 2pโถ 3sยฒ 3pโถ 4sยฒ
  • Fe (Z = 26): [Ar] 4sยฒ 3dโถ
  • Kr (Z = 36): [Ar] 4sยฒ 3dยนโฐ 4pโถ

๐ŸŒ€ Atomic Orbitals:

  • s-orbital: spherical (1 per level)
  • p-orbitals: dumbbell-shaped (3 per level from n=2)
  • d-orbitals: clover-shaped (5 per level from n=3)

๐Ÿ”น Ionisation Energy

โšก Definition:

  • The first ionisation energy is the energy required to remove one mole of electrons from one mole of gaseous atoms to form one mole of gaseous ions: X(g)โ†’X+(g)+eโˆ’X(g)

๐Ÿ“ˆ Factors Affecting Ionisation Energy:

  • Nuclear charge (โ†‘ nuclear charge = โ†‘ ionisation energy)
  • Atomic radius (โ†‘ radius = โ†“ ionisation energy)
  • Shielding (โ†‘ inner electron shielding = โ†“ ionisation energy)

๐Ÿ” First Ionisation Energies Across Period 3 (Na to Ar):

  • General trend: Increases across the period due to increasing nuclear charge and constant shielding.
  • Two exceptions:
    1. Mg โ†’ Al: Drop due to Alโ€™s electron entering a higher-energy 3p orbital.
    2. P โ†’ S: Drop due to electron pairing in 3p orbital causing repulsion.
ElementElectron ConfigurationIonisation Energy Trend
Na[Ne] 3sยนLow (easy to remove 3sยน)
Mg[Ne] 3sยฒHigher
Al[Ne] 3sยฒ 3pยนSlight drop
Si[Ne] 3sยฒ 3pยฒIncreases
P[Ne] 3sยฒ 3pยณHigher
S[Ne] 3sยฒ 3pโดDrop (electron pairing)
Cl[Ne] 3sยฒ 3pโตIncreases again
Ar[Ne] 3sยฒ 3pโถHighest (full shell)

The electronic configurations of elements using successive ionisation energy data

1. What is successive ionisation energy?

  • The first ionisation energy (IEโ‚) is the energy required to remove the first electron from a gaseous atom.
  • The second ionisation energy (IEโ‚‚) is the energy required to remove the second electron, and so on.
  • Successive ionisation energies generally increase gradually, but there is a large jump when electrons from a core (inner) shell are removed after all outer (valence) electrons have been lost.

2. How to use the data to deduce electronic configuration:

Step 1: Examine the ionisation energy values.

  • Identify where there is a large jump in the successive IE values.
  • The electrons before the jump are the valence electrons, and the jump occurs when core electrons start being removed.

Step 2: Count the number of electrons removed before the large jump.

  • This number gives the number of valence electrons.

Step 3: Deduce the shell structure.

  • Use the number of electrons and the periodic table group to assign the full electron configuration.

Example:

Successive ionisation energies (in kJ/mol) for an element X:

IEโ‚ = 590
IEโ‚‚ = 1145
IEโ‚ƒ = 4912
IEโ‚„ = 6492
IEโ‚… = 8780

Step 1: Identify the large jump.

  • Jump occurs between IEโ‚‚ (1145) and IEโ‚ƒ (4912) โ†’ After removing 2 electrons, the next is much harder โ†’ 2 valence electrons.

Step 2: Determine total electrons.

  • Element is in Group 2 โ†’ 2 valence electrons โ†’ atomic number = 4 (Li would be 3, Be is 4)

Step 3: Write electronic configuration:

  • X = Be โ†’ 1sยฒ 2sยฒ

Tips:

  • The first large jump always indicates removal of core electrons.
  • The number of electrons removed before the jump = number of valence electrons.
  • Compare with the periodic table to deduce the element and write the full configuration.

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