Topic 2: Atomic Structure and the Periodic Table Flashcards
Fundamental particles:
-the atomic structure model has evolved over time, as knowledge and scientific understanding changes
-the current, accepted model of the atom consists of a small, dense central nucleus surrounded by orbiting electrons in electron shells
-this was discovered in the Rutherford scattering experiment in 1911
-the nucleus consists of protons and neutrons giving it an overall positive charge
-it contains almost the entire mass of the atom
-in a neutral atom, the number of electrons is equal to the number of protons due to the relative charges
Protons, Neutron and Electrons:
-relative charge: proton -> +1, neutron -> 0, electron -> -1
-relative mass: proton -> 1, neutron -> 1, electron -> 1/1840
-the maximum number of orbiting electrons that can be held by any single shell, depends on the number of the shell, this can be calculated using 2n^2 where n is the number of the shell
-example: Electrons in shell 2 = 2(2^2) = 8 electrons
-each electron shell must fill before the next one can hold any electrons
Atomic Number and Mass Number:
-mass number is represented using A and can be calculated as the sum of protons and neutrons in an atom
-atomic number is represented using Z and is equal to the number of protons in an atom, hence it can be referred to as proton number
Isotopes:
-> isotopes are atoms of the same element with the same atomic number, but with a different number of neutrons, resulting in a different mass number
-neutral atoms of isotopes will react chemically in the same way because their proton number and electron configuration is the same
-the sharing and transfer of electrons is unaffected
-however, the different mass numbers means they have different physical properties
-example: the following are all isotope of hydrogen:
Hydrogen = 1 proton and 1 neutron
Deuterium = 1 proton and 2 neutrons
Tritium = 1 proton and 3 neutrons
Relative Masses:
-Relative atomic mass (Ar) is defined as:
-> the mean mass of an atom of an element, relative to 1/12 of the mean mass of an atom of the carbon-12 isotope
-this takes the relative abundances of the different isotopes of an element into account
Ar = means mass of an atom of an element/ 1/12 x mean mass of C-12 isotope
Relative isotopic mass:
-> the isotopic mass of an isotope relative to 1/12 of the mean mass of an atom of the carbon-12 isotope
Relative molecular mass (Mr):
-> the mean mass of a molecule of a compound, relative to 1/12 of the mean mass of an atom of the carbon-12 isotope
-it can be calculated for a molecule by adding together the separate Ar values of the component elements
-example: Mr of H2O = (2x1.0) + (1x16.0) = 18.0
-calculating the relative molecular mass can be used to identify the molecules present in a sample
-relative formula mass is similar to Mr but is used for compounds with giant structures
Ions and Mass Spectrometry:
-ions are formed when an atom loses or gains electrons meaning it is no longer neutral and will have an overall charge
-they are very useful in the analytical technique of mass spectrometry
-it is used to identify different isotopes and find the overall relative atomic mass of an element
Time of Flight (TOF): Mass Spectrometry
-this form of mass spectrometry records the time it takes for ions of each isotope to reach a detector, using this spectra can be produces showing each isotope present
1. Ionisation - a sample of an element is vaporised and injected into the mass spectrometer where a high voltage is passed over the chamber
-this causes electrons to be removed from the atoms (they are ionised) leaving +1 charged ions in the chamber
2. Acceleration- these positively charged ions are then accelerated towards a negatively charged detection plate
3. Ion drift - the ions are then deflected by a magnetic field into a curved path
-the radius of the path is dependent on the charge and mass of the ion
4. Detection - when the positive ions hit the negatively charged detection plate, they gain an electron, producing a flow of charge
-the greater the current produced, the greater the abundance of that particular ion
5. Analysis - these current values are then used in combination with the flight times to produce a spectra print-out with the relative abundance of each isotope displayed
-during the ionisation process, a 2+ charged ion may be produces which means it will be more affected more by the magnetic field producing a curved path of smaller radius
-as a result, this mass to charge ratio (m/z) is halved which can be seen on spectra as a trace at half the expected m/z value
Ar and Mass Spectrometry:
-using this print-out spectra, the Ar (relative atomic mass) can be calculated my multiplying each m/z value by its abundance and adding each of these together, before dividing by the total abundance of all species present
Ar = (m/z x abundance)/total abundance
-using this calculated value of Ar, the element can be identified by referring to the Periodic Table
Predicting Mass Spectra:
-if you know the abundance of an isotope you can generate the mass spectra for its molecules, including relative speak heights
-example: The relative abundance of ^35Cl atoms is 75% and ^37Cl atoms is 25%. In other words, for every 100 atoms of chlorine, 25 would be ^35Cl and 75 would be ^37Cl. Spectra produced by the mass spectrometry of chlorine display a characteristic pattern in a 3:1 ratio for Cl^+ ions and a 3:6:9 ratio for Cl2^+ ions. This is because one isotope is more common than the other and the chlorine molecule can form in different combinations
^70CL2^+ = 35 + 35
^72Cl2^+ = 35 + 37 OR 37 + 35
^74Cl2^+ = 37 + 37
Ionisation Energy: first ionisation
-> the minimum energy required to remove one mole of electrons from one mole of atoms in a gaseous state, it is measured in kJmol^-1
Na (g) -> Na^+ (g) + e^-
-successive ionisation energies occur when further electrons are removed
-this usually requires more energy because, as electrons are removed, the electrostatic force of attraction between the positive nucleus and the negative outer electron increases
-more energy is therefore needed to overcome this attraction, causing ionisation energy to increase
-all ionisation energies are endothermic, as the removal of electrons requires an energy input
Ionisation energy: second ionisation
-> the minimum energy required to remove one mole of electrons from one mole of +1 ions in a gaseous state, it is measured in kJmol^-1
Na^+ (g) -> Na^2+(g) + e^-
-the definition can be used to define successive ionisation energies
-ionisation energy is influenced by 3 factors:
1. The number of protons
2. The electron shielding
3. The sub shell from which the electron is removed
First ionisation energy: trends
-first ionisation energy follows trends within the Periodic Table as they are influenced by proton-electron forces of attraction, and electron shielding
-along a period: first ionisation energy increases due to a decreasing atomic radius and greater electrostatic forces of attraction, electrostatic forced of attraction increase since there is an increasing number of protons
-down a group: first ionisation energy decreases due to an increasing atomic radius and electron shielding which reduces the effect of the electrostatic forces of attraction
-when successive ionisation energies are plotted on a graph, a sudden large increase indicates a change in energy level which is because the electron is being removed from an orbital closer to the nucleus so more energy is required to do so
-this large energy increase provides supporting evidence for the atomic orbital theory
-the first ionisation energy of Aluminium is lower than expected due to a single pair of electrons with opposite spin
-as a result there is a natural repulsion which reduces the amount of energy needed to be put in to remove the outer electron
Electron orbitals:
-electrons are held in clouds of negative charge called orbitals
-there are different types of orbital: s,p, d and f, each orbital can hold 0,1 or 2 electrons
-when an orbital holds 2 electrons the electrons must have opposite spins which have different shapes