1.1 Atomic Structure Flashcards
Time of Flight Mass Spectrometry - function
It is the most useful instrument for accurate determination of the relative atomic mass of an element, based on the abundance and mass of each of its isotopes
Time of Flight Mass Spectrometry - condition
Must be kept under a high vacuum to prevent the ions that are produced from colliding with molecules present in the air
Stages of Time of Flight Mass Spectrometry
- Ionisation (Electron bombardment / Impact or Electrospray Ionisation)
- Acceleration
- Ion drift
- Ion Detection
- data analysis
1) Electrospray Ionisation - use and properties
- This method is used for substances which have a higher molecular mass
- Unlike with electron impact ionisation, fragmentation is unlikely to happen - This is often called a soft ionisation technique
1) Electrospray Ionisation - process
- the sample is dissolved in a volatile & polar solvent
- the solvent is injected at high pressure through a fine hollow needle connected to the positive terminal of a high voltage supply producing a fine mist
- Causes the sample molecule (X) to be ionised and to gain a
proton (H+) from the solvent, forming XH+ - The solvent evaporates into the vacuum while the XH+ ions are attracted towards a negatively charged plate
X (g) + H+ –> XH+ (g)
Electron impact / bombardment Ionisation - use and properties
This method of ionisation is used for elements and substances which have a lower molecular mass.
this technique cannot be used with larger moleculesas it will cause them to fragment and negatively impact the spectra analysis
Electron impact / bombardment Ionisation - process
- The sample is vapourised and
injected at low pressure - An electron gun fires high energy
electrons at the injected sample - This causes an outer electron to be knocked
out from each particle, forming a 1+ ion
X (g) -> X+ (g) + e-
Acceleration
The positive ions formed from either ionisation method are accelerated to a constant kinetic energy (KE) by an electric field towards a negatively charged plate
All ions have constant kinetic energy so lighter ions travel fastest Since their velocity (speed) is dependent on their mass
Stage 3: Ion Drift
The 1+ ions will pass through a hole in the negatively charged plate and move into a flight tube
The time of flight of each 1+ ion in this tube depends on their velocity
Stage 4: Ion Detection
The ions travel along a tube, called the flight
tube, where they then reach a detector (another negatively charged plate)
The positive ions reach the negatively charged detection plate and gain an electron and produce a current
This size of the current is proportional to the abundance of those ions hitting the plate and gaining an electron
data analysis
Two pieces of information are
analysed in combination:
1. The current that is produced
2. The flight tube times (TOF)
This produces a spectra with the relative
abundance produced by ions with varying
mass/charge (m/z) ratios
electron configuration
The arrangement of electrons in an atom is called the electron configuration
principal energy levels or principal quantum shells
Electrons are arranged around the nucleus in principal energy levels or principal quantum shells
Principal quantum numbers (n) are used to number the energy levels or quantum shells
The lower the principal quantum number, the closer the shell is to the nucleus and the lower the energy
The higher the principal quantum number, the greater the energy of the shell and the further away from the nucleus
subshells
The principal quantum shells are split into subshells which are given the letters s, p, d and f
The energy of the electrons in the subshells increases in the order s < p < d < f
All the orbitals in the same subshell have the same energy and are said to be degenerate
Orbitals
Subshells contain one or more atomic orbitals
Orbitals exist at specific energy levels and electrons can only be found at these specific levels, not in between them
Each atomic orbital can be occupied by a maximum of two electrons
This means that the number of orbitals in each subshell is as follows:
s : one orbital (1 x 2 = total of 2 electrons)
p : three orbitals ( 3 x 2 = total of 6 electrons)
d : five orbitals (5 x 2 = total of 10 electrons)
f : seven orbitals (7 x 2 = total of 14 electrons)
s orbital shape
The s orbitals are spherical
The size of the s orbitals increases with increasing shell number
E.g. the s orbital of the third quantum shell (n = 3) is bigger than the s orbital of the first quantum shell (n = 1)
p orbital shape
The p orbitals have a dumbbell shape
Every shell has three p orbitals except for the first one (n = 1)
The p orbitals occupy the x, y and z axes and point at right angles to each other, so are oriented perpendicular to one another
The lobes of the p orbitals become larger and longer with increasing shell number
Ground state
The ground state is the most stable electronic configuration of an atom which has the lowest amount of energy
This is achieved by filling the subshells of energy with the lowest energy first (1s)
3d vs 4s
The subshells increase in energy as follows: s < p < d < f
The only exception to these rules is the 3d orbital which has slightly higher energy than the 4s orbital
Because of this, the 4s orbital is filled before the 3d orbital
electrons are put in 4s then in 3d
electrons are taken out of 4s then from 3d
The electron configuration
The electron configuration gives information about the number of electrons in each shell, subshell and orbital of an atom
Writing out the electron configuration tells us how the electrons in an atom or ion are arranged in their shells, subshells and orbitals
The electron configuration - ions
Ions are formed when atoms lose or gain electrons
Negative ions are formed by adding electrons to the outer subshell
Positive ions are formed by removing electrons from the outer subshell