Grin Publishing
Chemical Analysis of a Lunar Meteorite by Laser Ablation Mass Spectrometry
Chemical Analysis of a Lunar Meteorite by Laser Ablation Mass Spectrometry
Couldn't load pickup availability
In a first step a set of relative sensitivity coefficients (RSCs) was determined by measurements on the regolith rock. Afterwards the chemical composition of the K-REE-P rock was successfully measured and mapped in an elemental composition map. The present minerals (e.g. zircon, ilmenite, pyroxene and K-feldspar) could be identified by analyzing elemental ratios. Special emphasis was put on the mineral zircon. Rare earth element patterns could be measured inside a zircon grain. With the amount of titanium found inside the zircon grain, the crystallization temperature of the grain could be estimated. This again can help determine whether or not the analyzed grain crystallized during an impact event or not. In the last part of this thesis the LMS instrument was coupled with a HV pulser. The HV pulser greatly enhances the detection sensitivity for heavier elements by preventing the lighter elements from reaching the detector and thus avoiding saturation effects on the detector. With the help of the HV pulser the mass spectra of rare earth elements could be readily recorded with sufficiently high signal-to-noise ratio and mass resolution to make a quantitative analysis possible. Uranium and thorium were detected as well at limited sample locations. Also lead was measured but only in one spectrum. With the lead and uranium abundance determined from the
Share
