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Calibration of the SHERLOC Deep Ultraviolet Fluorescence-Raman Spectrometer on the Perseverance Rover.
Kyle Uckert1, Rohit Bhartia2, Luther W Beegle1
1Jet Propulsion Laboratory California Institution of Technology, Pasadena, CA, USA.
The Scanning of Habitable Environments with Raman and Luminescence for Organics and Chemicals (SHERLOC) instrument uses deep ultraviolet Raman and fluorescence spectroscopy for Martian sample analysis. Accurate wavelength calibration is crucial for understanding Martian mineralogy and chemistry.
Area of Science:
- Planetary Science
- Spectroscopy
- Astrochemistry
Background:
- The Perseverance Rover's SHERLOC instrument analyzes Martian surface samples using deep ultraviolet Raman and fluorescence (DUV R/F) spectroscopy.
- DUV R/F spectroscopy employs a 248.6 nm laser to detect and classify chemical and mineralogical compositions by analyzing scattered photons and fluorescence emission.
Purpose of the Study:
- To describe the wavelength calibration of the SHERLOC spectrometer.
- To ensure accurate analysis of mineralogy and chemistry of Martian materials.
Main Methods:
- Utilized a compact DUV R/F spectrometer with a spectral range of 249.9 nm to 353.6 nm.
- Developed a custom design to project high-resolution Raman and low-resolution fluorescence spectra onto a single charge-coupled device.
- Implemented a segmented, nonlinear wavelength calibration to account for curved spectral illumination.
Main Results:
- The SHERLOC spectrometer optimizes resolution for Raman spectra and wavelength range for fluorescence spectra.
- The calibration method addresses the curved spectral illumination on the charge-coupled device.
- Accurate calibration is essential for interpreting the mineralogy and chemistry of Martian samples.
Conclusions:
- The described wavelength calibration is critical for the SHERLOC instrument's success in analyzing Martian samples.
- Accurate spectral data enables a deeper understanding of the potential for past life on Mars.
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