Mainly made up of protons and neutrons in the nucleus, with electrons orbiting in shells
Protons
Positive charge
Neutrons
Zero charge
Electrons
Negative charge, very small relative mass
Mass number
Number of protons and neutrons in the nucleus
Atomic number
Number of protons in the nucleus
Atoms are neutral because the number of protons equals the number of electrons
Ion
Has a different number of electrons and protons, forming a stable charge
Isotopes
Elements with the same number of protons but different numbers of neutrons
Isotopes of carbon
Carbon- 12
Carbon- 13
Carbon- 14
History of atomic models
1. Dalton's atomic model
2. Thomson's plum pudding model
3. Rutherford's nuclear model
4. Bohr's shell model
Time-of-flight mass spectrometer
Vaporizes and ionizes sample, accelerates ions, ions drift at constant speed, ions detected based on mass-to-charge ratio
Relative molecular mass
Average mass of an atom of an element over 1/12 of the mass of the atom C^12
Relative isotopic mass
Mass of an isotope of an element, measured relative to carbon-12
Mass spectrum
Shows the relative abundance of isotopes of an element based on their mass-to-charge ratio
Isotope
Atoms of the same element with the same number of protons but different numbers of neutrons
Mass spectrometer analysis of isotopes
Provides information about the mass-to-charge ratio of the isotopes
Provides information about the abundance of the isotopes
Calculating relative atomic mass from isotope data
1. Multiply abundance of isotope A by mass-to-charge ratio of A
2. Multiply abundance of isotope B by mass-to-charge ratio of B
3. Add the results
4. Divide by total abundance
Molecular ion peak
The peak on a mass spectrum that corresponds to the unfragmented molecular ion
Electron subshells
s
p
d
f
Electron configuration
Electrons are filled in order of increasing energy level
Electrons fill orbitals singly first before pairing up
Determining electron configuration of an atom
1. Write the configuration as 1s2 2s2 2p6 3s2 3p6 3d6 4s2
2. Fill the orbitals in order of increasing energy
3. Singly occupy orbitals before pairing up
Determining electron configuration of an ion
1. Remove electrons from the highest energy level first
2. Transition metals may have electrons move from 4s to 3d to create a more stable configuration
Ionization energy
The minimum energy required to remove one mole of electrons from one mole of atoms in the gaseous state
Removing electrons from an ion
1. Remove electrons from 4s first
2. Then remove from 3D
3. Check the numbers to ensure it adds up correctly
Ionization energy
The minimum amount of energy required to remove one mole of electrons from one mole of atoms in the gaseous state
Ionization energy is always endothermic and has a positive value
Shielding
The more shells or electron shells between the positive nucleus and the outer electron, the less energy is required and the weaker the attraction is
Atomic size
The bigger the atom, the further away the electrons are from the nucleus, the weaker the attractive force, and the less energy is required to remove the outer electron
Nuclear charge
The more protons in the nucleus, the bigger the attraction between the nucleus and the outer electron, and the more energy is required to remove the electron
Successive ionization energy
The removal of more than one electron from the same atom
There are distinctive jumps in successive ionization energies as electrons are removed from shells increasingly closer to the nucleus
As you go down a group (group 2)
The first ionization energy decreases
Reasons for decrease in first ionization energy down a group
Atomic radius increases
Shielding increases
As you go across a period
The first ionization energy generally increases
Reasons for increase in first ionization energy across a period
Nuclear charge increases
Shielding is similar
Exception at sulfur
Evidence for electron repulsion, the energy required to remove an electron from sulfur is less due to repulsion between the paired electrons in the 3p orbital