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Updated: Aug 3, 2026

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Molecular Beam Mass Spectrometry With Tunable Vacuum Ultraviolet (VUV) Synchrotron Radiation
Published on: October 30, 2012
Mars ultraviolet simulation facility
Journal of Molecular Evolution
|December 1, 1979
Summary
A new facility enables long-duration ultraviolet (UV) radiation exposure for Martian soil chemistry research. This system simulates Mars conditions, allowing for extensive material testing and hypothesis validation.
Area of Science:
- Planetary Science
- Astrobiology
- Materials Science
Background:
- Viking Mars landers provided initial observations of Martian soil chemistry.
- Understanding Martian soil requires simulating environmental conditions, including UV radiation.
- Long-term material exposure is crucial for validating hypotheses about Mars.
Purpose of the Study:
- To establish a facility for long-duration ultraviolet (UV) radiation exposure of materials.
- To test hypotheses concerning Martian soil chemistry under simulated conditions.
- To enable the study of natural and synthetic materials relevant to Mars.
Main Methods:
- Utilized a 2500-watt xenon lamp as the UV radiation source.
- Employed a heat-dissipating water filter to manage beam intensity.
- Designed an exposure chamber for continuous sample tumbling, sub-zero temperatures, and atmospheric control (including Mars nominal).
Main Results:
- Successfully irradiated up to 33 sealed sample ampules simultaneously.
- Completed irradiation for over 100 samples, with durations ranging from 100 to 700 hours.
- The facility demonstrated reliable performance for extended UV irradiation under simulated Martian conditions.
Conclusions:
- The established facility is effective for long-duration UV exposure testing.
- It supports the investigation of Martian soil chemistry hypotheses.
- The system provides a robust platform for simulating Mars surface conditions on various materials.

