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Migration from Source to Reservoir




Petroleum Geology AES/TA 3820
General Considerations

      Oil and gas migration are the least understood processes in
      the formation of hydrocarbon reservoirs. Much of the current
      thinking of how it happens is hypothetical and difficult to
      prove with either experiment or theory.

      When potential source and reservoir rocks are buried, they
      contain water in their pore space. The oil or gas, therefore,
      has to replace this water in the migration process when it
      reaches the reservoir rock.

      We have first a look at the composition of formation water.




Petroleum Geology AES/TA 3820
Formation Waters
   Water in hydrocarbon reservoirs is usually connate water originating
   from the water that surrounded it during or shortly after the
   depositional process. It is, therefore, fossil water. Meteoric water, on
   the other hand, is fresh water that originates from the surface; it may
   significantly alter its aqueous chemistry during burial.

   Water is special because of all hydrides that the life-forming elements
   (N, C, H, S, O) form it is the only one that is liquid at standard
   temperature and pressure, with the other ones being gaseous. It has
   other special properties that are generally caused by its dipole
   molecular structure (surface tension, dielectric constant, latent heat
   of evaporation). Its tendency to arrange molecules in tetrahedra and
   to exclude electrolytes (e.g. in freezing) causes it to assume special
   properties in the presence of minerals such as clays.


Petroleum Geology AES/TA 3820
Formation Water Composition
      Most formation waters are saline, with sodium and chlorine
      being the dominant ions, constituting over 90% of the total ionic
      concentration. Calcium and magnesium are also typical present
      with a ratio of 5:1, while sulfates are notably absent.

      There is a generally observed increase in the salinity of
      formation waters with depth, from a typical concentration of
      35,000 ppm (seawater) at shallow depths to highly concentrated
      “brines” of up to 350,000 ppm at several kilometers depths.
      This phenomenon is related to reverse osmosis, a process
      wherein the water molecules are able to migrate upwards
      through shales, while the ions and the oil stay behind in the
      aquifer. Shales contain in general water that is less saline.



Petroleum Geology AES/TA 3820
Water Salinity vs. Depth




                   Source: North, F.K. (1985) Petroleum Geology, Allen & Unwin


       An example of the salinity increase in oilfield waters with depth
                          from the US Gulf Coast.


Petroleum Geology AES/TA 3820
Pressure and Temperature During Burial

    During burial, temperature and pressure increase, leading to
    compaction of the sedimentary rocks. The pore space, therefore,
    decreases and with it the volume available for the fluids, principally
    formation water but also hydrocarbons. They have to support an
    increasing load of the overburden stress unless they escape. In
    shales, which are poorly permeable but which can be richer in
    hydrocarbon source material, the fluids take a much longer time to
    escape (and thus to equilibrate hydrodynamic pressures) than in
    porous and permeable rocks. This can lead to overpressure in the
    shales, a so-called compaction disequilibrium.

    Compaction is the primary motor that leads to the expulsion of
    hydrocarbons from shaly source rocks.



Petroleum Geology AES/TA 3820
Evidence for Migration
     Why do we need to invoke the scenario of migration in the first
     place?

     The most compelling reason comes from the way oil and gas
     accumulate: They are typically found in porous and permeable
     rocks that are arched upwards and that are topped by an
     impermeable layer (the “seal”). The second reason is the
     relationship between source and reservoir rock: The latter is usually
     younger and/or structurally higher than the source rock. Visual
     evidence of migration is provided by oil and gas seepages found in
     many parts of the world.

     But not all reservoirs need migration. There are known cases where
     the oil is internally sourced. Example: The Athel field in Oman


Petroleum Geology AES/TA 3820
Migration Evidence: Structure
                                                              In the Hassi Messaoud
                                                              Field, Algeria, the
                                                              Silurian source rock
                                                              drilled by the well on the
                                                              left is laterally and
                                                              stratigraphically
                                                              separated from the
                                                              Cambrian reservoir rock
                                                              where oil is found in the
                                                              well in the middle.

                                                              Migration is an obvious
                                                              mechanism to explain
                                                              this situation.

Source: North, F.K. (1985) Petroleum Geology, Allen & Unwin

Petroleum Geology AES/TA 3820
Migration Evidence: Seepages




                                 Oil seepages can be seen from satellite images
                                 with SAR. Left: Santa Monica Bay, California.
                                 Above: Caspian Sea, Azerbaijan.	




Petroleum Geology AES/TA 3820
Migration Evidence: Oil Seepages




   The La Brea Tar Pits in Los Angeles are probably the most spectacular oil
   seepage. They are puddles of asphalt that seeped to the surface from young
   (Miocene) source rocks through faults. In the Pleistocene and Holocene many
   animals perished in them and became fossilized, giving us an extraordinary
   glimpse of the fauna at that time. Visit the George C. Page Museum.


Petroleum Geology AES/TA 3820
Primary Migration

     Mature hydrocarbons first have to migrate out of the source rock.
     This is in general a fine-grained rock that has a low permeability,
     for reasons outlined earlier in this course. During burial, this rock
     gets compacted and its interstitial fluid become overpressured
     with respect to surrounding rocks that have higher permeabilities
     and from which fluids can migrate with greater ease upwards.

     Therefore, a fluid pressure gradient develops between the source
     rock and the surrounding, more permeable rocks. This causes the
     fluids - the water and the hydrocarbons - to migrate along the
     pressure gradient, usually upwards, although a downward
     migration is possible. This process is called primary migration,
     and it generally takes place across the stratification. Why?



Petroleum Geology AES/TA 3820
Porosity Decrease with
          Compaction
  Shown are shale porosities from
  various regions. The Dickinson
  curve is from undercompacted
  shales in the Gulf Coast. The Athy
  curve from Paleozoic shales in
  compaction equilibrium.

  Smectite curves are from the Gulf
  Coast and indicate progressive,
  stepwise transformation to mixed-
  layer clays and illite. This releases
  more water into the rock, therefore
  the slower compaction of smectite-
  rich rocks.


Petroleum Geology AES/TA 3820    Source: Hunt, J.M. (1995) Petroleum Geochemistry and Geology, 2nd edition.
                                 W.H. Freeman & Co
Porosity Decrease with Compaction
            Source: North, F.K. (1985) Petroleum Geology, Allen & Unwin




                     Average clay-rock density and porosity values
                            as compiled by Dickey (1975)


Petroleum Geology AES/TA 3820
Source: Hunt, J.M. (1995) Petroleum Geochemistry and Geology, 2nd edition.
                                     W.H. Freeman & Co

Shale Pore Size with Depth

 Concurrent with the decrease of
 porosity with depth, the pore
 size decreases in an almost
 linear relationship. The diameter
 of many molecules may be too
 large to form globules and
 migrate through the shale
 pores, particularly since
 structured water on the clay
 surfaces further restricts the
 pathways. This is why a number
 of migration mechanisms are
 postulated.



Petroleum Geology AES/TA 3820
Primary Migration Controversy

     If we put the principal requirements for oil generation and
     migration together, we end up in a substantial dilemma:

     1. Oil is generated at temperatures of 60° to 120 °C, which are
     typically found at depths of 2 to 4 km.

     2. Source rocks at these depths are so compacted that their
     permeability is too low for efficient primary migration.

     This dilemma is not solved yet, but many ideas have been
     proposed to circumvent it.
     At the core of the problem is the question of how hydrocarbons
     migrate.


Petroleum Geology AES/TA 3820
Primary Migration Mechanisms
   1. Migration by diffusion. Because of differing concentrations of the
   fluids in the source rock and the surrounding rock there is a tendency
   to diffuse. A widely accepted theory.
   2. Migration by molecular solution in water. While aromatics are most
   soluble in aqueous solutions, they are rare in oil accumulations,
   therefore discrediting the general importance of this mechanism,
   although it may be locally important.
   3. Migration along microfractures in the source rock. During
   compaction the fluid pressures in the source rock may become so
   large that spontaneous “hydrofracing” occurs. A useful if
   underestimated hypothesis.
   4. Oil-phase migration. OM in the source rock provides a continuous
   oil-wet migration path along which the hydrocarbons diffuse along
   pressure and concentration gradient. This is a reasonable but
   unproved hypothesis, good for high TOCs.


Petroleum Geology AES/TA 3820
Further Comments on Primary Migration
    There is geological and geochemical evidence for primary migration,
    but no single hypothesis explains all scenarios. In California, very
    young oil is found (Bakersfield etc.), suggesting that early expulsion
    is possible, perhaps in the form of immature hydrocarbons. But the
    dominant fluid is water, and it is questionable why oil should be
    expulsed first. Many oil fields have very large time gaps between the
    age of the source and reservoir rocks, and the formation of the trap
    (before which migration cannot occur). Most traps are, in fact,
    relatively young. This suggests that migration and accumulation may
    proceed in two or more different stages:
    An early migration in which permeabilities are relatively high and gas
    may be available to dissolve hydrocarbons, but where the
    hydrocarbon generation is inefficient, and a later stage at which oil
    generation is efficient but permeabilities are low.


Petroleum Geology AES/TA 3820
Further Comments on Primary Migration /2
                                      Source: Hunt, J.M. (1995) Petroleum Geochemistry and Geology, 2nd edition.
                                      W.H. Freeman & Co

    It may well be that
    undercompaction is crucial for
    primary migration. It may help
    preserve the source rock’s
    permeability to a greater depth
    than in equilibrium condition,
    all the while reaching
    temperatures sufficient for
    significant hydrocarbon
    generation.
    Shown here are pressures and
    probable migration directions
    in a Gulf Coast setting.



Petroleum Geology AES/TA 3820
Secondary Migration
      The process in which hydrocarbons move along a porous and
      permeable layer to its final accumulation is called secondary
      migration. It is much less controversial than primary migration,
      and it is almost entirely governed by buoyancy forces.

      These forces are proportional to the density difference between
      hydrocarbon and water. For continuous (but physically separate)
      hydrocarbon and water columns, the hydraulic potential, or the
      difference between the products of density times height of the
      two phases governs the flow of fluids.

      The principal conduits for secondary migration are permeable
      sandstone beds and unconformities.



Petroleum Geology AES/TA 3820
Migration Pathways
    Source: Hunt, J.M. (1995) Petroleum Geochemistry and Geology, 2nd edition.
    W.H. Freeman & Co



                                                                                 In the following, migration
                                                                                 pathways - both primary
                                                                                 and secondary - are shown
                                                                                 for some typical geological
                                                                                 scenarios.

                                                                                 The example here illustrates
                                                                                 how excess hydrostatic
                                                                                 pressure may control
                                                                                 directions of fluid flow in the
                                                                                 Paria formation, Orinoco
                                                                                 delta, Venezuela.



Petroleum Geology AES/TA 3820
Migration Pathways /2
       Source: Hunt, J.M. (1995) Petroleum Geochemistry and Geology, 2nd edition.
       W.H. Freeman & Co




           Direction of fluid migration on the flank of an anticline
           into the highest possible place of the reservoir layer



Petroleum Geology AES/TA 3820
Migration Pathways /3
                Source: Hunt, J.M. (1995) Petroleum Geochemistry and Geology, 2nd edition.
                W.H. Freeman & Co




                Direction of fluid migration into stratigraphic
                        - or better: combined - traps


Petroleum Geology AES/TA 3820
Migration Pathways /4
                   Source: Hunt, J.M. (1995) Petroleum Geochemistry and Geology, 2nd edition.
                   W.H. Freeman & Co




     Direction of fluid migration in an interbedded sand/shale sequence


Petroleum Geology AES/TA 3820
Migration Pathways /5
           Source: Hunt, J.M. (1995) Petroleum Geochemistry and Geology, 2nd edition.
           W.H. Freeman & Co




               Direction of fluid migration into a pinnacle reef

          Notice: Migration through the shales above the reef is greatly exaggerated




Petroleum Geology AES/TA 3820
Differential Entrapment

  This phenomenon has been
  theoretically postulated and
  subsequently found realistic in
  many cases. It results in the
  heaviest fluid (water) being
  trapped in the highest anticline,
  and the lightest (gas) in the
  lowest! Quite the opposite of
  what is generally encountered.

  Notice that for this effect to take
  place, free gas must be able to
  form.

          Source: North, F.K. (1985) Petroleum Geology, Allen & Unwin



Petroleum Geology AES/TA 3820
Differential Entrapment /2

 The same scenario as before, but
 with different structural
 relationships




                                    Source: North, F.K. (1985) Petroleum Geology, Allen & Unwin




Petroleum Geology AES/TA 3820
Seals
   Secondary migration proceeds until an impermeable barrier is
   encountered that prevents further flow. The most common seal is a
   shale layer. The most effective seals are evaporites, notably salt and
   anhydrite, partly because of their inherently low intrinsic permeability,
   and partly because their capacity for viscous flow enables them to
   heal fractures and faults.




                                                                     A dual salt-
                                                                     anhydrite seal in
                                                                     the Hassi R’Mel
                                                                     gas field, Algeria

       Source: North, F.K. (1985) Petroleum Geology, Allen & Unwin

Petroleum Geology AES/TA 3820
Conclusions on Migration

    We distinguish primary and secondary migration.

    While primary migration is slow and proceeds over short distances,
    secondary migration is faster and can proceed over very long
    distances (more than one-hundred kilometers).

    There are several theories for primary migration, among which
    diffusion, oil-phase migration, micro-fracturing and migration in
    solution.

    Secondary migration is better understood and leads to the
    accumulation of hydrocarbon in traps where a seal prevents them
    from further migration.


Petroleum Geology AES/TA 3820
Study Task

      Calculate how much water is expelled from a shale layer 1 km
      thick and 10 × 10 km in area, as it is buried from 1 km to 3 km
      depth, assuming its compaction is in equilibrium.

      Assume now that this is a source rock with 600 ppm weight
      percent mature hydrocarbon, of which 15% get expulsed in
      primary migration.

      How much oil is generated?

      What is the average concentration of oil, in ppm, in the water
      that escapes from the shale?




Petroleum Geology AES/TA 3820

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Oil migration (pinacle reef)

  • 1. Migration from Source to Reservoir Petroleum Geology AES/TA 3820
  • 2. General Considerations Oil and gas migration are the least understood processes in the formation of hydrocarbon reservoirs. Much of the current thinking of how it happens is hypothetical and difficult to prove with either experiment or theory. When potential source and reservoir rocks are buried, they contain water in their pore space. The oil or gas, therefore, has to replace this water in the migration process when it reaches the reservoir rock. We have first a look at the composition of formation water. Petroleum Geology AES/TA 3820
  • 3. Formation Waters Water in hydrocarbon reservoirs is usually connate water originating from the water that surrounded it during or shortly after the depositional process. It is, therefore, fossil water. Meteoric water, on the other hand, is fresh water that originates from the surface; it may significantly alter its aqueous chemistry during burial. Water is special because of all hydrides that the life-forming elements (N, C, H, S, O) form it is the only one that is liquid at standard temperature and pressure, with the other ones being gaseous. It has other special properties that are generally caused by its dipole molecular structure (surface tension, dielectric constant, latent heat of evaporation). Its tendency to arrange molecules in tetrahedra and to exclude electrolytes (e.g. in freezing) causes it to assume special properties in the presence of minerals such as clays. Petroleum Geology AES/TA 3820
  • 4. Formation Water Composition Most formation waters are saline, with sodium and chlorine being the dominant ions, constituting over 90% of the total ionic concentration. Calcium and magnesium are also typical present with a ratio of 5:1, while sulfates are notably absent. There is a generally observed increase in the salinity of formation waters with depth, from a typical concentration of 35,000 ppm (seawater) at shallow depths to highly concentrated “brines” of up to 350,000 ppm at several kilometers depths. This phenomenon is related to reverse osmosis, a process wherein the water molecules are able to migrate upwards through shales, while the ions and the oil stay behind in the aquifer. Shales contain in general water that is less saline. Petroleum Geology AES/TA 3820
  • 5. Water Salinity vs. Depth Source: North, F.K. (1985) Petroleum Geology, Allen & Unwin An example of the salinity increase in oilfield waters with depth from the US Gulf Coast. Petroleum Geology AES/TA 3820
  • 6. Pressure and Temperature During Burial During burial, temperature and pressure increase, leading to compaction of the sedimentary rocks. The pore space, therefore, decreases and with it the volume available for the fluids, principally formation water but also hydrocarbons. They have to support an increasing load of the overburden stress unless they escape. In shales, which are poorly permeable but which can be richer in hydrocarbon source material, the fluids take a much longer time to escape (and thus to equilibrate hydrodynamic pressures) than in porous and permeable rocks. This can lead to overpressure in the shales, a so-called compaction disequilibrium. Compaction is the primary motor that leads to the expulsion of hydrocarbons from shaly source rocks. Petroleum Geology AES/TA 3820
  • 7. Evidence for Migration Why do we need to invoke the scenario of migration in the first place? The most compelling reason comes from the way oil and gas accumulate: They are typically found in porous and permeable rocks that are arched upwards and that are topped by an impermeable layer (the “seal”). The second reason is the relationship between source and reservoir rock: The latter is usually younger and/or structurally higher than the source rock. Visual evidence of migration is provided by oil and gas seepages found in many parts of the world. But not all reservoirs need migration. There are known cases where the oil is internally sourced. Example: The Athel field in Oman Petroleum Geology AES/TA 3820
  • 8. Migration Evidence: Structure In the Hassi Messaoud Field, Algeria, the Silurian source rock drilled by the well on the left is laterally and stratigraphically separated from the Cambrian reservoir rock where oil is found in the well in the middle. Migration is an obvious mechanism to explain this situation. Source: North, F.K. (1985) Petroleum Geology, Allen & Unwin Petroleum Geology AES/TA 3820
  • 9. Migration Evidence: Seepages Oil seepages can be seen from satellite images with SAR. Left: Santa Monica Bay, California. Above: Caspian Sea, Azerbaijan. Petroleum Geology AES/TA 3820
  • 10. Migration Evidence: Oil Seepages The La Brea Tar Pits in Los Angeles are probably the most spectacular oil seepage. They are puddles of asphalt that seeped to the surface from young (Miocene) source rocks through faults. In the Pleistocene and Holocene many animals perished in them and became fossilized, giving us an extraordinary glimpse of the fauna at that time. Visit the George C. Page Museum. Petroleum Geology AES/TA 3820
  • 11. Primary Migration Mature hydrocarbons first have to migrate out of the source rock. This is in general a fine-grained rock that has a low permeability, for reasons outlined earlier in this course. During burial, this rock gets compacted and its interstitial fluid become overpressured with respect to surrounding rocks that have higher permeabilities and from which fluids can migrate with greater ease upwards. Therefore, a fluid pressure gradient develops between the source rock and the surrounding, more permeable rocks. This causes the fluids - the water and the hydrocarbons - to migrate along the pressure gradient, usually upwards, although a downward migration is possible. This process is called primary migration, and it generally takes place across the stratification. Why? Petroleum Geology AES/TA 3820
  • 12. Porosity Decrease with Compaction Shown are shale porosities from various regions. The Dickinson curve is from undercompacted shales in the Gulf Coast. The Athy curve from Paleozoic shales in compaction equilibrium. Smectite curves are from the Gulf Coast and indicate progressive, stepwise transformation to mixed- layer clays and illite. This releases more water into the rock, therefore the slower compaction of smectite- rich rocks. Petroleum Geology AES/TA 3820 Source: Hunt, J.M. (1995) Petroleum Geochemistry and Geology, 2nd edition. W.H. Freeman & Co
  • 13. Porosity Decrease with Compaction Source: North, F.K. (1985) Petroleum Geology, Allen & Unwin Average clay-rock density and porosity values as compiled by Dickey (1975) Petroleum Geology AES/TA 3820
  • 14. Source: Hunt, J.M. (1995) Petroleum Geochemistry and Geology, 2nd edition. W.H. Freeman & Co Shale Pore Size with Depth Concurrent with the decrease of porosity with depth, the pore size decreases in an almost linear relationship. The diameter of many molecules may be too large to form globules and migrate through the shale pores, particularly since structured water on the clay surfaces further restricts the pathways. This is why a number of migration mechanisms are postulated. Petroleum Geology AES/TA 3820
  • 15. Primary Migration Controversy If we put the principal requirements for oil generation and migration together, we end up in a substantial dilemma: 1. Oil is generated at temperatures of 60° to 120 °C, which are typically found at depths of 2 to 4 km. 2. Source rocks at these depths are so compacted that their permeability is too low for efficient primary migration. This dilemma is not solved yet, but many ideas have been proposed to circumvent it. At the core of the problem is the question of how hydrocarbons migrate. Petroleum Geology AES/TA 3820
  • 16. Primary Migration Mechanisms 1. Migration by diffusion. Because of differing concentrations of the fluids in the source rock and the surrounding rock there is a tendency to diffuse. A widely accepted theory. 2. Migration by molecular solution in water. While aromatics are most soluble in aqueous solutions, they are rare in oil accumulations, therefore discrediting the general importance of this mechanism, although it may be locally important. 3. Migration along microfractures in the source rock. During compaction the fluid pressures in the source rock may become so large that spontaneous “hydrofracing” occurs. A useful if underestimated hypothesis. 4. Oil-phase migration. OM in the source rock provides a continuous oil-wet migration path along which the hydrocarbons diffuse along pressure and concentration gradient. This is a reasonable but unproved hypothesis, good for high TOCs. Petroleum Geology AES/TA 3820
  • 17. Further Comments on Primary Migration There is geological and geochemical evidence for primary migration, but no single hypothesis explains all scenarios. In California, very young oil is found (Bakersfield etc.), suggesting that early expulsion is possible, perhaps in the form of immature hydrocarbons. But the dominant fluid is water, and it is questionable why oil should be expulsed first. Many oil fields have very large time gaps between the age of the source and reservoir rocks, and the formation of the trap (before which migration cannot occur). Most traps are, in fact, relatively young. This suggests that migration and accumulation may proceed in two or more different stages: An early migration in which permeabilities are relatively high and gas may be available to dissolve hydrocarbons, but where the hydrocarbon generation is inefficient, and a later stage at which oil generation is efficient but permeabilities are low. Petroleum Geology AES/TA 3820
  • 18. Further Comments on Primary Migration /2 Source: Hunt, J.M. (1995) Petroleum Geochemistry and Geology, 2nd edition. W.H. Freeman & Co It may well be that undercompaction is crucial for primary migration. It may help preserve the source rock’s permeability to a greater depth than in equilibrium condition, all the while reaching temperatures sufficient for significant hydrocarbon generation. Shown here are pressures and probable migration directions in a Gulf Coast setting. Petroleum Geology AES/TA 3820
  • 19. Secondary Migration The process in which hydrocarbons move along a porous and permeable layer to its final accumulation is called secondary migration. It is much less controversial than primary migration, and it is almost entirely governed by buoyancy forces. These forces are proportional to the density difference between hydrocarbon and water. For continuous (but physically separate) hydrocarbon and water columns, the hydraulic potential, or the difference between the products of density times height of the two phases governs the flow of fluids. The principal conduits for secondary migration are permeable sandstone beds and unconformities. Petroleum Geology AES/TA 3820
  • 20. Migration Pathways Source: Hunt, J.M. (1995) Petroleum Geochemistry and Geology, 2nd edition. W.H. Freeman & Co In the following, migration pathways - both primary and secondary - are shown for some typical geological scenarios. The example here illustrates how excess hydrostatic pressure may control directions of fluid flow in the Paria formation, Orinoco delta, Venezuela. Petroleum Geology AES/TA 3820
  • 21. Migration Pathways /2 Source: Hunt, J.M. (1995) Petroleum Geochemistry and Geology, 2nd edition. W.H. Freeman & Co Direction of fluid migration on the flank of an anticline into the highest possible place of the reservoir layer Petroleum Geology AES/TA 3820
  • 22. Migration Pathways /3 Source: Hunt, J.M. (1995) Petroleum Geochemistry and Geology, 2nd edition. W.H. Freeman & Co Direction of fluid migration into stratigraphic - or better: combined - traps Petroleum Geology AES/TA 3820
  • 23. Migration Pathways /4 Source: Hunt, J.M. (1995) Petroleum Geochemistry and Geology, 2nd edition. W.H. Freeman & Co Direction of fluid migration in an interbedded sand/shale sequence Petroleum Geology AES/TA 3820
  • 24. Migration Pathways /5 Source: Hunt, J.M. (1995) Petroleum Geochemistry and Geology, 2nd edition. W.H. Freeman & Co Direction of fluid migration into a pinnacle reef Notice: Migration through the shales above the reef is greatly exaggerated Petroleum Geology AES/TA 3820
  • 25. Differential Entrapment This phenomenon has been theoretically postulated and subsequently found realistic in many cases. It results in the heaviest fluid (water) being trapped in the highest anticline, and the lightest (gas) in the lowest! Quite the opposite of what is generally encountered. Notice that for this effect to take place, free gas must be able to form. Source: North, F.K. (1985) Petroleum Geology, Allen & Unwin Petroleum Geology AES/TA 3820
  • 26. Differential Entrapment /2 The same scenario as before, but with different structural relationships Source: North, F.K. (1985) Petroleum Geology, Allen & Unwin Petroleum Geology AES/TA 3820
  • 27. Seals Secondary migration proceeds until an impermeable barrier is encountered that prevents further flow. The most common seal is a shale layer. The most effective seals are evaporites, notably salt and anhydrite, partly because of their inherently low intrinsic permeability, and partly because their capacity for viscous flow enables them to heal fractures and faults. A dual salt- anhydrite seal in the Hassi R’Mel gas field, Algeria Source: North, F.K. (1985) Petroleum Geology, Allen & Unwin Petroleum Geology AES/TA 3820
  • 28. Conclusions on Migration We distinguish primary and secondary migration. While primary migration is slow and proceeds over short distances, secondary migration is faster and can proceed over very long distances (more than one-hundred kilometers). There are several theories for primary migration, among which diffusion, oil-phase migration, micro-fracturing and migration in solution. Secondary migration is better understood and leads to the accumulation of hydrocarbon in traps where a seal prevents them from further migration. Petroleum Geology AES/TA 3820
  • 29. Study Task Calculate how much water is expelled from a shale layer 1 km thick and 10 × 10 km in area, as it is buried from 1 km to 3 km depth, assuming its compaction is in equilibrium. Assume now that this is a source rock with 600 ppm weight percent mature hydrocarbon, of which 15% get expulsed in primary migration. How much oil is generated? What is the average concentration of oil, in ppm, in the water that escapes from the shale? Petroleum Geology AES/TA 3820