Mass Spectrometry

Radiogenic Isotope Laboratory

Chemistry Lab Mass Spectrometry Sample Preparation

The Radiogenic Isotope Lab houses two magnetic-sector based mass spectrometers, which are distinct primarily in their means for sample introduction.  The thermal ionization mass spectrometer (TIMS instrument) introduces the sample through evaporation and ionization off of a filament (commonly Re or Ta metal), whereas the multi-collector inductively-coupled plasma mass spectrometer (MC-ICP-MS) introduces the sample through a nebulizer (to produce a very fine aerosol), followed by introduction into a hot Ar plasma (~ 8,000 oC) as the means for ionization.

Magnetic-sector based mass spectrometry is essential for providing "flat-topped" peaks for the masses, which is required for high-precision isotope ratios; the flat top removes any changes in the relative ion intensities if small amounts of drift occurs in the instrument during analysis.  In addition, simultaneous collection of all isotopes of interest is also important for high-precision analyses, since ion beams (particularly those generated by ICP sources) always have small variations in intensities due to small changes in source conditions during analysis.  These features distinguish magnetic sector-based instruments that have multiple collection from, for example, the common quadrupol-based ICP-MS instruments.  In addition, because the sources used in the mass spectrometers are either solid- or solution-based, we must measure absolute ratios, and this contrasts with gas-source mass spectrometers, which can inlet sample and standard gases under identical source conditions, allowing isotope compositions to be determined on a relative basis.

After passing the ion beam through a magnetic field to separate the masses, isotope ratios are generally measured by passing the very small ion currents (10-16 to 10-10 Amps) through large specialized resistors (1010 to 1011 Ohm), which produces a relative range of voltages; essentially these instruments are just really expensive voltmeters!.  The highest precision work requires use of a detector such as a Faraday collector, where essentially one charge in is one charge out.  However, much smaller ion beams (smaller samples) may be analyzed on a number of multiplier detectors, which include a robust Daly multiplier, as well as channeltron ion-counting multipliers; there is no free lunch here, however, so the increased sensitivity one obtains with a multiplier is balanced by a decrease in precision.

Click on the thumbnail images below for a larger view; use your browsers "BACK" button to return to this page.

Peak_Scan.gif (5633 bytes) An example of a "flat-topped" peak (over 232Th) that is produced by a magnetic-sector-based instrument.
TIMS.jpg (74078 bytes) Our VG Instruments Sector-54 TIMS mass spectrometer, being run by graduate student Merideth Rhodes for her project on Sr isotope variations in the Green River Basin.  The source is out of the picture to the left, and the magnet is just visible on the far left.  The collector block lies just to the right of the magnet, and the main electronics rack is on the right.
Detail of the TIMS source, which can hold a 16 sample turret.  Tom Lapen's hand is shown for scale, where he is adjusting the oxygen gas bleed for ultra-low-level Nd isotope analysis as NdO+.
Our Micromass IsoProbe MC-ICP-MS mass spectrometer.  Tom Lapen (far left) is adjusting the sweep gas, while post-doc Rene Wiesli (left) watches graduate student Nancy Mahlen (right) set up files for an analytical session.  The main part of the instrument that is visible is the collector block.
IsoProbe_Schematic.gif (35328 bytes) A general schematic of the Micromass IsoProbe (courtesy of the manufacturer).  Samples are introduced on the left, and ion beams traverse from left to right in the instrument.
Collectors.jpg (90732 bytes) A view of the collector block of the Micromass IsoProbe, our MC-ICP-MS instrument.  The ion beam would come in from the top of the photo.  The drives that move the collectors to various positions are seen on the sides of the block.  The movable channeltron multipliers are on the left side of the block.  In the lower part of the photo is the Daly multiplier, which has better noise and stability specifications than the channeltron multipliers; the Daly is fixed in the axial position.  Between the Daly and the main block is a wide-angle energy retarding filter (WARP), which is essential for high-abundance-sensitivity work, such as is required for 230Th/232Th measurements.
Collectors_Large_View.jpg (80613 bytes) Another view of the collector block for the MC-ICP-MS instrument.  The collector block for the TIMS instrument is similar, although it has fewer Faraday collectors, no movable channeltron multipliers, and no WARP filter.
IsoProbe_Collectors.gif (30027 bytes) A schematic of the collector configuration of the MC-ICP-MS instrument.  The variety of movable and fixed detectors provide an opportunity to analyze just about any element on the periodic table that exists as a liquid or solid at STP.  Of course, we will ignore the monoisotopic elements!
372_Laminar_Flow.jpg (37836 bytes) Pre-sample handling for the MC-ICP-MS is more complicated than for the TIMS instrument, requiring careful aliquoting of solutions in a clean environment.  Shown here is one of the laminar flow fume hoods in the lab, this one located in the Mass Spectrometry Lab (Room 375).
Aridus.jpg (62343 bytes) Sample introduction into the MC-ICP-MS instrument starts with nebulization of the sample solution.  Shown here is one of the nebulizers we use, in this case, the Aridus micro-concentric desolvating nebulizer, as well as an autosampler.  Both are housed in a clean bench.
IsoProbe_Collision_Cell_In.jpg (69810 bytes) One of the special features of the new IsoProbe is the collision cell (hexapol) that is employed to tighten the energy spread (ie: make flat-topped peaks), increase sensitivity, and remove polyatomic interferences.  In this photo, the ICP source is on the left, and the ion beam would be passed from left to right.
 

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For more information, contact Clark Johnson at clarkj@geology.wisc.edu

Last revised: 07/20/08