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ISOTOPE COMPOSITION OF NATURAL GASES                                 105
                Mixing of nitrogen in sedimentary rocks with the nitrogen coming from the
             mantle is quite possible, but cannot be proved at the current level of analytical
             techniques. Prasolov (1990) who studied the problem mentioned that the mantle
             nitrogen in most cases cannot be identified against the background of the crustal and
             atmospheric nitrogen.





             6.2.5. Inert gases

                Inert gases of a predominantly radioactive origin may form in the Earth’s crust as
             well as in the upper mantle. According to Prasolov (1990), the mantle helium is
             present in the natural gases of the Earth’s crust. Its content is minimal (o1%) in the
             gases of sediment cover. The mantle helium dominates only in gases associated with
             the present-day volcanism and rifting. The same writer estimated the current gas
             composition in the upper mantle taking into account the vapor pressure and isotopic
             composition:

             CO 2 /He      CH 4 /He     N 2 /He     40 Ar/He     36 Ar/He      3 He/He
             100           10           4           1            10-4          10-5



                On the basis of the above, the mantle CO 2 may be expected in gas accumulations
             of the sediment cover, in addition to negligible amounts of methane and other gases.
                The age of the gas can be determined from the He/Ar ratio, taking into account
             their radioactive origin. For instance, Fig. 6.1 shows the evolution in time of the He/
                                                       4
                                                                          40
                                                           40
             Ar ratio. Table 6.3 illustrates distributions of He/ Ar B and  40 Ar P / Ar B in gas
             accumulations of tectonic units of different age.


















                                40
                             4
             Fig. 6.1. Variation of He/ Ar p ratio with time. 1 — In gases being formed in rocks t years ago; 2 — in
             gases formed between 4.5 billion years ago to time t; 3 — in gases formed between the time t and present
             time. t — abscissa. (After Prasolov, 1990.)
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