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Laser Ablation Sampling With Low-Power Plasma: A LA-MIP-MS Instrument for Spaceflight
Benjamin J Farcy1,2, Jacob Graham2, Madeline Raith3
1Department of Astronomy, University of Maryland, College Park, Maryland, USA.
A new laser ablation microwave-induced plasma mass spectrometer (LA-MIP-MS) offers low-resource elemental and isotopic analysis for planetary missions. This technology significantly reduces power and gas consumption compared to traditional inductively coupled plasma mass spectrometry (ICP-MS).
Area of Science:
- Planetary Science
- Analytical Chemistry
- Mass Spectrometry
Background:
- Traditional inductively coupled plasma (ICP) mass spectrometry (MS) is resource-intensive, using high power and gas flows.
- These limitations make conventional ICP-MS unsuitable for spaceflight applications, particularly for planetary missions requiring compact and efficient instrumentation.
Purpose of the Study:
- To develop and validate a low-resource mass spectrometry system for in-situ chemical analysis during planetary science missions.
- To address the technology gap by creating a laser ablation microwave-induced plasma mass spectrometer (LA-MIP-MS) suitable for spaceflight.
Main Methods:
- Designed and developed a prototype LA-MIP-MS instrument.
- Utilized a low-pressure ( < 1 Torr) microwave-induced plasma ion source powered by 30 W and 50 mL/min of Helium.
- Interfaced the plasma source with a quadrupole mass spectrometer (QMS) for elemental and isotopic analysis of solid samples via laser ablation (266 nm).
Main Results:
- Achieved quantification accuracy for stainless steel within 1.4-4% of X-ray fluorescence (XRF) values.
- Demonstrated precision for elemental analysis ranging from ±9.1 to 22% (2σm).
- Measured Cu and Ni isotopic ratios with ±0.8-3% (2σm) precision and reproducibility from 0.12% to 11.8%.
Conclusions:
- The developed LA-MIP-MS enables elemental and isotopic analysis with significantly lower power and plasma gas requirements than commercial ICP-MS systems.
- This technology expands instrumentation options for planetary missions, offering a viable technique for terrestrial and spaceflight chemical analysis of geologic materials.
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