Mass Spectrometer and Relative Atomic Mass
Transcript of Mass Spectrometer and Relative Atomic Mass
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ppendix 4. MASS SPECTROMETER - MASS SPECTROSCOPY
Appendix 4a Introduction to the Mass Spectrometer
The mass spectrometer is an instrument by which you can separate ionised/charged (+) particles of different mass and determine the
amounts of each particle in a mixture.
The technique is called mass spectroscopy or mass spectrometry ('mass-spec' and 'MS' in shorthand!).
Mass spectrometry gives accurate information on the relative masses of isotopes and their
relative abundance (proportions).
Mass spectrometry is an important method of analysis in chemistry and can be used to
identify elements by their characteristic mass spectrum pattern - the technique is used in
planetary space probes e.g. mass spectrometer instrumentation is incorporated in the Mars
explorer vehicles.
The substance to be analysed is introduced/injected into a high vacuum (extremely low pressure) tube system (at K left diagram) where the
particles are ionised by colliding with beam of high speed electrons (at Q in left diagram).
Note: If the sample is not already a gas, then substance must be vapourised, i.e. the material must be in the gaseousstate to be analysed in a mass spectrometer.
The resulting (+) ions are accelerated down a tube (from + to - plates, P in left diagram) and then through a powerful magnetic field.
The charged or ionised particles are deflected by this powerful magnetic field ( R in left diagram).
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How much they are deflected depends on the particle mass and the speed of the particle and the strength of a magnetic field i.e. lighter
particles of lower mass (and momentum) are deflected more than heavier particles of bigger mass (see right diagram below) for a given set of
conditions.
By varying the strength of the magnetic field , it is possible to bring into focus onto an ion detector (N in left diagram) at the end of the tube
(effectively an electrical event is detected), every possible mass in turn and a measure the strength of the ion current , which is a measure of
how much of that ion has been formed from the sample under analysis.
A simplified diagram of a mass spectrometer tube system is shown below (left) with further explanation as to what is going on and an extra
diagram to show the relative paths of light to heavy ions for a given strength of magnetic field.
KEY TO DIAGRAM and more detail of each component's function
K = sample injection point, it must be a gas, so a liquid/solid must be vaporised at the injection point.
IONISATION
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Q = high voltage (high +/- p.d.) electron gun which fires a beam of high speed/energy electrons from a heated 'metal element' into the vaporised
sample under analysis and causes ionization of the atoms (or molecules) forming positive ions (mainly monopositive in charge).
The collision of high KE electrons with atoms or molecules causes another electron to be knocked off the particle leaving a negative deficit i.e. a
positively charged particle is formed e.g.
M(g) + e- ==> M+(g) + 2e
-, usually written as just
M(g) ==> M+
(g) + e- (M might represent e.g. a metal atom or a molecule)
The ions formed should be written as [M]+, a notation that is handy if you are dealing with ionised molecule fragments with an overall single
positive charge e.g. [CH3]+ is seen in the mass spectrum of methane gas, CH
4.
The low pressure (~vacuum) is needed to prevent the ions from colliding with air particles which would stop them reaching the ion detector
system.
ACCELERATION
P = are negative plates which accelerate the positive ions down the tube (there are positive plates at the start of the tube). A moving beam of
charged particles creates a magnetic field around itself, and this 'ion beam' magnetic field interacts with the magnetic field at R.
DEFLECTION-SEPARATION
R = the magnetic field that causes deflection of ions , this is can be varied to change the extent of deflection for a given mass and to focus a
beam of ions of particular mass down onto the detector. Hence, by programming the mass spectrometer to 'sweep' through all likely particle
masses, in terms of the right hand diagram, you can increase the strength of the magnetic field to bring into focus onto the ion detector
monopositive ions of increasing mass.
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DETECTION
N = an ion detection system which essentially generates a tiny electrical current when the ions hit it. The strengths of the 'electronic' signals from
the various ion peaks are sent to a computer for analysis, computation and display. They tell you the particle masses present and their relative
abundance (see the mass spectrum diagram for the element strontium below).
MASS SPECTRUM
The resulting record of the ion peaks is called the mass spectrum or mass spectra . The highest peak is called the base peak and is often given
the relative and arbitrary value of 100 , particularly in the mass spectra of organic compounds.
MASS SPECTRA
For elements you get a series of signals or ion peaks for each isotope present and the ratio of peak heights gives you the relative proportion of
each isotope in the element so that you can calculate the relative atomic mass of an element. This 'simple' spectra of mononuclear ions like
Sr + is only true for non-molecular elements like metals (see mass spectrum of strontium diagram below ) or noble gases, but for molecular
elements like nitrogen or the halogens things are not so simple (see chlorine example below).
For larger e.g. organic molecules, things can be very complex indeed, as molecules fragment and many different ions can be formed BUT you
can get the relative molecular mass of a molecule by identifying what is called the molecular ion peak , that is, when one electron is knocked
of the molecule but the molecule retains its full molecular structure.
e.g. benzoic acid (M r = 122) gives a molecular ion peak of m/e = 122 , due to [C 6H5COOH]+
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but you also get fragments such as [C 6H5]+ with an m/e of 77 as the molecule breaks up on further electron impact.
CHLORINE EXAMPLE
Chlorine is a good example of a molecular element whose mass spectra can be a bit tricky when first encountered ...
Chlorine consists of two principal isotopes , chlorine-37 (25% is 37 Cl) and chlorine-35 (75% is 35 Cl).
BUT, chlorine consists of Cl 2 diatomic molecules, which, on ionisation, can split into chlorine atoms.
The result is a series of 5 different mass peaks from the various isotopic atomic or molecular ion possibilities.
1. [37 Cl37 Cl] + or [37 Cl 2]+ m/z = 74 2. [37 Cl35 Cl] + m/z = 72 (note that you must show the two isotopes separately) 3. [35 Cl35 Cl] + or [35 Cl 2]+ m/z=70 4. [37 Cl] + m/z=37 5. [35 Cl] + m/z=35
m/z means the relative mass of the ion over its charge, which for our purposes the charge is taken +1 (little z) and the mass (little m) is the relative
atomic/formula mass of the particle. m/z sometimes quoted as m/e. You should write the structure of the io n in square brackets and put the chargeon the outside of them in the top right - this is an important and universally accepted notation in mass spectrometry.
Examples of the calculation of the relative atomic mass of an element using % of isotopes is given in Part 1 of GCSE-AS (basic) calculations , an
example of calculating relative atomic mass from a mass spectrum is given below for the metallic element strontium .
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The mass spectra of organic compounds can be very complex as the molecules fragment under electron bombardment, but the resulting mass
spectra can used to identify compounds from their 'finger-print' pattern of ion peaks of different mass and particular proportions for a given set
of experimental conditions.
The largest m/z value gives the molecular mass of a molecule , i.e. the ion of largest mass, prior to fragmentation, is formed when the original
whole and neutral molecule, loses one electron e.g. for ethane it would be due to the formation of [C 2H6]+, m/z = 30 and is called the molecular
ion peak .
STRONTIUM EXAMPLE
A 'simple' element spectrum to interpret AND a subsequent relative atomic mass calculation based on the mass spectrum of the
element strontium
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The relative atomic mass of an element, A r , is the weighted average mass of the isotopes present , compared to 1/12th of
the relative mass of the carbon-12 isotope. [ 12 C is given the relative mass value of 12.0000 ]
Quite often the highest m/e peak is arbitrarily given the relative value of 100, as in this case and referred to as the base peak , but the peak lines
might well indicate % abundance of isotopes. The diagram of abundances is sometimes called a stick diagram .
Relative peak height = relative abundance as measured from the ion current detector signal.
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The mass spectrum shows strontium consists of four isotopes, 84 Sr (peak height = 0.68), 86 Sr (peak height = 12.0), 87 Sr (peak height = 8.47)
and 88 Sr (peak height = 100.0)
The sum of the heights = 0.68 + 12.0 + 8.47 + 100.0 = 121.15
So we can now calculate the weighted average mass of ALL the isotopes.
Therefore Ar = {(0.68 x 84) + (12.0 x 86) + (8.47 x 87) + (100.0 x 88)}/121.15 = 87.7
The book value is 87.62, BUT this calculation does NOT take into account the very accurate relative atomic masses based on the carbon-12
scale, it merely uses the mass numbers, which are always integer.
ISOTOPIC MASSES - definition and uses
Very accurate isotopic masses are usually a tiny fraction different from a whole number but provide invaluable information.
Modern mass spectrometers are exceedingly accurate and very sophisticated instruments and can measure mass to at least 4 decimal places.
They can readily distinguish between N 2, CO and C 2H4 molecules, all with an integer M r of 28.
The very accurate molecular ion masses are [N 2]+ = 28.0061, [CO] + = 27.9949 and [C 2H4]
+ = 28.0313
A very accurate mass spectrometer (for high resolution mass spectroscopy) can even differentiate between organic molecules of the same
integer molecular mass.
e.g. for the molecular mass 103, some possible, however unlikely, molecular formulae could theoretically be
C5HN3 = 103.0170 , C3H5NO 3 = 103.0269 , C2H5N3O 2 = 103.0382 , C7H5N = 103.0427 , CH 5N5O = 103.0494
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Calculations of % composition of isotopes
It is possible to do the reverse of a relative atomic mass calculation if you know the A r and which isotopes are present.
It involves a little bit of arithmetical algebra.
The A r of boron is 10.81 and consists of only two isotopes, boron-10 and boron-11
The relative atomic mass of boron was obtained accurately in the past and mass spectrometers can sort out the isotopes present.
If you let X = % of boron 10, then 100-X is equal to % of boron-11
Therefore A r (B) = ( X x 10) + [(100- X) x 11) / 100 = 10.81
so, 10 X -11 X +1100 =100 x 10.81
-X + 1100 = 1081, 1100 - 1081 = X (change sides change sign!)
therefore X = 19
so naturally occurring boron consists of 19% 10 B and 81% 11 B (the data books quote 18.7 and 81.3)
It should be pointed out that the relative ratio of isotopes can be very accurately determined using a modern mass spectrometer AND individual
isotopic masses can be measured to four decimal places - which were NOT used in the above calculation.
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Appendix 4b The Time of Flight Mass Spectrometer (for advanced level students only!)
Ion mass separation using a time-of-flight mass spectrometer - a more modern instrument
In a time-of-flight mass spectrometer the ions are formed in a similar manner by electron bombardment, and the resulting ions accelerated
between electrically charged plates.
Again, the sample must be a gas or vapourised and is bombarded with an electron beam or laser beam to knock off electrons to produce
positive ions.
However, the method of separation due to different m/e (mass/charge) values is then dependent on how long it takes the ion to
travel in the drift region' i.e. the region NOT under the influence of an accelerating electric field.
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The ions are accelerated in the same way between positive to negative plates in an electric field of fixed strength i.e. constant
potential difference.
The smaller the mass of the ionised particle (ionized atom, fragment or whole molecule) the shorter the time of flight in the drift
region where no electric field operates.
This is because for a given accelerating potential difference, a lighter particle is accelerated more to a higher speed than a
heavier ion, so the 'time of flight' down the tube is shorter .
Therefore the ions are distinguished by different flight times NOT by different masses being brought into focus with a magnetic field
as described in section 4a BUT the separation by time of flight is still determined by the m/e (m/z) value of the ion.
The general principles of the separation are required knowledge but the mathematics is NOT needed by A level students , but if you are
interested, a simplified summary is given below
o t = K inst (m/q) o t = time of flight, m = mass of ion, q = charge on ion,
o Kinst = a proportionality constant based on the instrument settings and characteristics e.g. the electric field strength, length of
analysing tube etc.
o Therefore t is proportional to the square root of the mass of the ion for particles carrying the same charge - the bigger the
mass the longer the 'flight time'.
o The first equation is derived partly from the extra mathematics outlined below.
o KE = qV , the kinetic energy imparted to the ion is given by its charge x the potential difference of the accelerating electric field.
o The acceleration, for a fixed electric field, results in an ion having the same kinetic energy (KE) as any other ion of the same
charge q but the velocity v of the ion depends on the m/e (m/z) value.
o v = d/t (or t = d/v ), where v = velocity of accelerated particle in the drift region, d = length of tube in the drift region. (or t = d/v )
o KE = 1 /2mv2, so the bigger m, the smaller is v in the drift region and hence the basis of detecting ions of different mass by
different 'flight times'.
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o The diagram makes the method look simple, but far from it, the instrument works in a pulsed manner i.e. pulsed electric field, and
some pretty sophisticated electronics are used to analyse the signals from the detector and the so ftware calculates the mass of
the ion based on the drift flight time.