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Probing Ancient Biosignatures: Laser Mass Spectrometric Analysis of the 3.33 Ga Josefsdal Chert Using Laboratory and Space-prototype Instrumentation

  • Authors: Salome Gruchola, Frances Westall, Luca N. Knecht, Peter Keresztes Schmidt, Andreas Riedo, Marek Tulej, Frédéric Foucher, Peter Wurz

Salome Gruchola et al 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure 2.

An illustration of the two LIMS instruments used to analyze rock samples from the JC. Panel (A): a laboratory-scale LMS-GT instrument, featuring an ion flight path of ∼4 m. Panel (B): a space-prototype LMS instrument, with a more compact ion flight path of ∼0.3 m. Both systems are equipped with a UV femtosecond laser, illustrated as a violet beam focused onto the sample surface, which ablates and ionizes the material. The red-dotted lines trace the ion trajectories through the instruments. Ions with the same m/z ratio but slightly different kinetic energies travel different distances into the ion mirror: those with higher kinetic energy travel farther and take longer to return, which ultimately enhances mass resolution. For detailed instrument specifications, refer to Table A1.

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