Page 152 - Geochemistry of Oil Field Waters
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140                 INORGANIC CONSTITUENTS AND PHYSICAL PROPERTIES


            ary,  Cretaceous,  and  Jurassic  ages  to  an  evaporite-associated  sea  water
            (Collins,  1970).  Fig.5.6  illustrates  the  same  relation  for  some  subsurface
            brines  taken  from  Pennsylvanian  and  Mississippian age  sediments  (Collins,
            1969a).
              The  depletion  of  potassium  in  subsurface  brines  might  be caused  by its
            uptake  by  clays.  For  example,  montmorillonite-type clay minerals system-
            atically  change  to  illite  with  increasing  depth  of  burial,  due  to  thermal
            diagenesis;  and,  as  a  result  of  this  transformation,  they  lose  interlayer
            (bound) water  (Burst, 1969). This change appears to begin at a temperature
            above  90°C.  (This  freed  interlayer  water  can  be  readily  expelled,  and  its
            movement  probably  is important  in  the first  migration  stage  of  hydrocar-
            bons.)  Laboratory  experiments at elevated  temperatures  and  pressures  in-
            dicate  that  montmorillonite  loses its interlayer  water  and  transforms into
            illite  in  the  presence  of  potassium-enriched  water  (Khitarov  and  Pugin,
            1966). The structural  variations of  the expandable minerals in clays appar-
            ently are also influenced by  the potassium  content of the associated waters.

            Rubidium

              Rubidium,  like the other alkali metals is lithophilic, and its abundance in
            the  earth’s  crust  is about  3.0  x   wt.%,  which  is  greater  than  that of
            lithium (Fleischer, 1962). It tends to be removed from solution more readily
            than lithium,  primarily  because of  its ability to replace potassium in mineral
            structures.  Table  5.11  indicates that  it precipitates  from an evaporite along
            with  sylvite  to  a  greater  extent than  lithium,  and it has  a  high  chemical
            reactivity.  The radius  of  its ion, 1.48 a, is only about 10% larger than the
            potassium  ion,  so it  can  be  accommodated  into the same  crystal  lattices.
            Because of  this, it forms no minerals of  its own.
              Rubidium  and  cesium  occur  sympathetically  in nature; that is, both are
            commonly found in amazonite, vorobyevite, and beryl (Goldschmidt, 1958).
            Rubidium  is a member of series NH4-K-Rb-Cs,   and members of this series
            are more similar in their  chemical and physical properties than are the mem-
            bers  of  any  other  group,  with  the  exception  of  the halogens.  Rubidium
            concentrates in the late crystallates, particularly those of granitic derivation,
            and it has a greater tendency to be adsorbed by clays than has potassium. It
            is  removed  from  igneous  rocks  by  water  leaching  and  then  adsorbed  by
            hydrolysate sediments and soils.
              Shales contain about 250 ppm of rubidium; deep-sea red clays, about 400
            ppm; and some glauconites, about 500 ppm (Goldschmidt, 1958). Sea water
            contains  about  0.12  mg/l  of  rubidium;  subsurface brines  contain  up  to 4
            mg/l.  Higher  concentrations  of  rubidium  probably  can  be  found  in brines
            associated  with  rocks  containing  potassium  minerals,  such  as  microcline
            feldspars, or lepidolite mica.
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