Hi Bob<br /><br />As promised, here is the summary of possible methods from Doran et al. (2004), "Mars chronology: assessing techniques for quantifying surficial processes," Earth Surface Processes and Landforms 67: 313-237.<br /><br />The authors look at four methods:<br /><br />1. Direct gamma ray detection<br /><br />A high spectral resolution and high sensitivity detector could identify the presence and abundances of short lived isotopes like Na22, Al 26, and Co60 to dtermine exposure age and longer lived isotopes like K40 and the U-Th series to date host rocks.<br /><br />2. Luminescence methods. The high cosmic radiation, low natural radioactivity of Mars materials, and uncertainities about martian processes renders this method problematic at present.<br /><br />4. Noble gas methods. Mass spectrometers can measure abundances of He3, Ne21, Ar36. and Ar38 for both cosmogenic and whole rock dataing.<br /><br />5. Standard radiogenic techiques. Laser ablation ICP-Mass Spectroscopy should be able to perform Rb-Sr dating on rocks.<br /><br />Cheers<br /><br />Jon <div class="Discussion_UserSignature"> <p><em>Whether we become a multi-planet species with unlimited horizons, or are forever confined to Earth will be decided in the twenty-first century amid the vast plains, rugged canyons and lofty mountains of Mars</em> Arthur Clarke</p> </div>