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Fact SheetsA closer look Back to Genesis homepage   src="../../../images/spacer.gif"   SCIENCE

Mass Spectrometry - A Closer Look

The analytical instrument called a mass spectrometer was developed in 1919 by Francis Aston in Cambridge, England. A spectrometer is a spectrograph with measurement capabilities. The importance of this technology was immediately recognized, and Aston was awarded the Nobel Prize for his work in 1922. So, what does a mass spectrometer do and how does it work?

Mass spectrometers permit the experimental determination of atomic and molecular masses with great accuracy. Aston's mass spectrometer had a precision of one part in 10,000, which was sufficient for him to discover the isotopes of many elements. Modern instruments are even more precise.

Ionization of sample
Ionization of sample
Courtesy: McREL

Mass spectrometers operate under conditions of high vacuum, typically 10-8 torr. (A torr is a unit of pressure, equal to 1.316 x 10-3 atmosphere. In comparison the pressure in outer space may be in the order of 10-12 torr.) Low-pressure samples in the spectrometer's ionization chamber are exposed to a beam of rapidly moving, energetic electrons shot out of an electron gun. The samples can be a gaseous element such as neon, the vapor of a solid or liquid element such as mercury, or even the vapor of a molecule such as water or methane. With modern technology it is possible to introduce a wide variety of materials, including mixtures, into a mass spectrometer. In the ionization chamber, the atom or molecule hits or is hit by the accelerated electrons. During the collision an electron is knocked out of the sample atom or molecule, leaving it with a positive charge. In other words, positively-charged gaseous ions are formed.

Ion accelerates in spectrometer chamber
Ion accelerates in spectrometer chamber
Courtesy: McREL

These newly-formed ions are then pushed out of the ionization chamber by an electric field applied between two metal grids. This is an application of Coulomb's law: the positively-charged grid repels the positive ions and the negatively-charged grid attracts the positive ions. This attraction and repulsion both act in the same direction to give the ions a nudge (net acceleration) toward the negatively-charged grid. The negative grid, which is full of holes, allows the accelerated ions to pass through it and leave the ionization chamber. The speeds to which the ions can be accelerated by the electric field are determined by their masses. Lighter ions reach higher speeds than do the heavier ones.

Moving ion creates magnetic field
Moving ion creates magnetic field
Courtesy: McREL

The accelerated beam of positively-charged ions generates a magnetic field of its own, as do all moving electrically-charged particles. The ion beam passes through an externally-applied magnetic field. The magnetic field created by the beam of moving charged particles interacts with the external magnetic field. The net result is that the trajectory of each charged particle is bent in a curve to an extent that depends on its speed (and therefore its mass). If the beam of a mixture of particles of different masses is allowed to hit a photographic plate, the particles converge at different points, corresponding to the different radii of their semicircular paths. Modern mass spectrometers feed their results directly to computers that do the analysis and produce a graph (spectrum). To learn more about the mathematics behind mass spectrometry, read "The Mathematics of Mass Spectrometry."

Diagram of Mass Spectrometer
Diagram of Mass Spectrometer                  Courtesy: McREL
Note. From Chemistry, Molecules, Matter and Change, 3rd Ed., (p.9), by P. Atkins and L. Jones, 1997, New York: W. H. Freeman.

There are many variations in the process of mass spectrometry, but all of them are based on the principles outlined above. Mass spectrometric techniques have played an important role in science (particularly in chemistry). This historically important technology is likely to play a major role in the research phase of the Genesis project when the solar wind samples are returned to Earth for analysis. By that time the technology may be significantly improved over what is now available

 
     
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