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Inferno Experimental Geochemistry Laboratory
The experimental facility in the Nine Circles Experimental Cosmochemistry laboratory is designed to study gas-solid reactions under conditions relevant to the early solar system. The primary goal in designing this apparatus is to simulate the solar nebula environment more accurately that has ever been accomplished. The experimental apparatus contains four basic components: a gas-handling system, furnaces, temperature monitors, and a quadrupole mass spectrometer (QMS) residual gas analyzer. The gas-handling system was constructed with the same tolerances used by the semiconductor industry for maintaining an ultra-high purity (99.99%) rating. The system is capable of mixing five different gases: H2, He, H2S, CO, and CO2.
These five gases are delivered to a series of MKS mass-flow controllers (MFCs) using electropolished stainless steel tubing and Swagelok VCR face-seal fittings. The mass flow controllers have flow ranges designed to produce gas mixtures with variety of He/H, C/H, O/H, and S/H ratios, which bracket those expected in the solar nebula. Paradiso ICPMS Analytical Laboratory
The LPL ICP-MS lab is currently equipped with a ThermoFinnigan ELEMENT2 High-Resolution
ICP mass spectrometer. The setup includes a Cetac ASX-100 micro-autosampler and a Cetac ASX
500 autosampler for larger samples.
Our latest addition to our analytical facilities is CETAC LSX-213 Laser Ablation system. The CETAC LSX-213 delivers high
intensity 213 nm, 5 nanosecond laser pulses at rates of 1-20 Hz. The
homogeneous flat top energy profile of the laser produces aperture spot sizes from 10 to 200 micron while maintaining a constant energy density. The laser output
energy is fully adjustable to produce as much, or as little ablation necessary to analyze virtually any solid sample - ideal for geological, forensic industrial and biological samples.
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