Luminescence dating on Mars: OSL characteristics of Martian analogue materials and GCR dosimetry

M. Jain, C.E. Andersen, L. Bøtter-Jensen, A.S. Murray, H. Haack, J.C. Bridges

    Research output: Contribution to journalJournal articleResearchpeer-review

    Abstract

    Luminescence chronology may be the key to understanding climatically and tectonically driven changes on Mars. However, the success of Martian luminescence dating will depend upon our understanding of the luminescence properties of silicates such as olivine, pyroxenes and plagioclases, and sedimentary precipitates such as sulphates and chlorides. We present here a preliminary investigation of the luminescence characteristics (sensitivity, dose response, fading) of some Martian analogue mineral and rock samples. These materials are likely to be zeroed by the solar UV light (200-300nm) under sub-aerial transport; this may allow possibility of using deep traps for extending the age range on Mars. Dose rates on Mars are largely due to charged particles present in the galactic cosmic rays. Some new results on proton dosimetry with Al2O3:C (Bragg curve and luminescence efficiency as a function of LET), and the effect of radiation damage due to cosmic ray exposure are presented and implications discussed for Martian luminescence dating. (c) 2006 Elsevier Ltd. All rights reserved.
    Original languageEnglish
    JournalRadiation Measurements
    Volume41
    Issue numberSp. Iss.
    Pages (from-to)755-761
    ISSN1350-4487
    DOIs
    Publication statusPublished - 2006
    Event11th International Conference on Luminescence and Electron Spin Resonance Dating - Köln, Germany
    Duration: 24 Jul 200529 Jul 2005

    Conference

    Conference11th International Conference on Luminescence and Electron Spin Resonance Dating
    CountryGermany
    CityKöln
    Period24/07/200529/07/2005

    Cite this