Martian biology speculations from biodegraded petroleum reservoirs Steve Larter, Ian Head - PowerPoint PPT Presentation

1 / 1
About This Presentation
Title:

Martian biology speculations from biodegraded petroleum reservoirs Steve Larter, Ian Head

Description:

... of Newcastle, UK; PRG, Petroleum Reservoir Group, University of Calgary, Canada ... Nature 411:1034-1037. 4. Uplifted sterilised reservoirs not biodegraded ... – PowerPoint PPT presentation

Number of Views:216
Avg rating:3.0/5.0
Slides: 2
Provided by: geologyand
Category:

less

Transcript and Presenter's Notes

Title: Martian biology speculations from biodegraded petroleum reservoirs Steve Larter, Ian Head


1
Martian biology - speculations from biodegraded
petroleum reservoirsSteve Larter, Ian Head Tom
Curtis CEGS, University of Newcastle, UK PRG,
Petroleum Reservoir Group, University of Calgary,
Canada
  • While much of Mars is very ancient, with a
    surface consisting of very old cratered volcanic
    terrains where life is unlikely to be found
    (1,2), any life that does exist on Mars is most
    likely to be found in the subsurface in areas
    where sedimentary processes have accumulated
    sediments and preserved them at depths where free
    liquid water exists today! To date no significant
    samples of the Martian subsurface are available
    for study but it is reasonable to conclude that
    any Martian biosphere will have similar genesis
    and survival issues to organisms in Earths deep
    biosphere. Petroleum reservoirs provide a unique
    access portal to the Earths subsurface biosphere
    and recent advances in understanding subsurface
    petroleum biodegradation provide some hints to
    what type of life, if any, we might expect in
    Mars. We discuss Martian biology from the
    speculative perspective of the petroleum geology/
    geochemistry of biodegraded oil reservoirs in
    Earth.

Zengler et al, 1999 Head et al, 2003
refs
DeltaG

-
1596kJ
4C16 H34
30H20
49CH4 15CO2
from mineral hydrolysis

H2
from kerogen maturation


From oil aromatisation
Biomass CH4 CO2
refs
K
NH4
PO4 ---
Co, Ni,
nutrients and trace elements from mineral
diagenesis
5. Biodegradation-oil plus water makes life plus
gas
9. The limits of prokaryotic diversity at all
scales-Curtis et al, 2002.
8. Curtis et al 2002- biodiversity theory. The
area under the individuals curve is NT the total
number of individualsNmax number of individuals
in most abundant species
rates and times
NT
ST
NT/Nmax
sample
Ratio ref.
Comparisons of observed degradation rates in
oilfields with the maintenance energy
requirements of microorganisms in the range
10-11 to 10-14 micrograms carbon per cell per
second allows us to make a broad assessment of
the maximum biomass size and suggests that the
degradation flux of hydrocarbons in reservoirs
could be consumed slowly by the maintenance
energy requirements of, on the order, of as
little as 109 microorganisms per square meter of
reservoir area or a few thousand organisms/ cm³
operating near the oil water contact (6). This is
in the range reported for cell counts in
sediments extrapolated to ca 2km depth (7) and
is not unreasonable as many degraded oils fields
we have seen have residual oil columns near the
oil water contact where we have had the best
results in isolating microbial nucleic acid
signatures and where we speculate much
degradation occurs. While we cannot confirm the
size nor the metabolic rate of the biomass with
this geological approach we conjecture from these
results that the deep biosphere in degrading
oilfields is possibly operating at very low
levels of metabolic activity perhaps near
maintenance states (a largobiosphere) though we
cannot eliminate the possibility that it is more
active but much smaller. On balance, it appears
that while the deep biosphere is undoubtedly hot
and exciting it is in oilfields, and probably
elsewhere, including any remnant biosphere in
Mars very slow and malnourished!
(per ml or g)
(per ml or g)
Giovanonni
4
sea
106
163
2. Surface ages of inner planets (NASA)
1. Age of Martian surface (NASA)
4
lake
106
163
Miskin Head
Milner Curtis
Map showing the distribution of Martian craters
15 km in diameter within 65O latitude. All
craters shown here superpose the surface on which
they appear (no buried craters are included). The
large volcanoes in the Tharsis and Elysium
regions and the Hellas and Argyre impact basins
are included for reference.
activated
1.5
109
72
sewage
10
dry soil 1
109
6380
McCaig et al
wet soil 2
109
30,000
100
Dykhuizen
background
Largobiosphere Oil reservoir

1.5
103
10. Estimates of diversity at small scales
Examination of compositional gradients in
biodegrading oilfields (3) has allowed us to
tentatively establish the rates of biodegradation
active at the base of oil columns and to indicate
that the rates of destruction of oil and the
charging rates of oilfields are quite similar in
many cases (Larter et al, 2003). It appears that
that reservoirs buried to 80oC or higher are
effectively sterilized with regard to hydrocarbon
degraders and are not recolonized with near
surface organisms during uplift (4) indicating
the deep biosphere results not from continued
invasion of organisms into deep
synthesis
  • If we extrapolate these finding to Mars, where
    near surface life is unlikely to have survived
    then what does this tell us about any existing
    deep Martian biosphere inherited originally from
    evolution of near surface Martian microorganisms.
    This assumes, as in Earth, any Martian deep
    biosphere is derived from the surface. In the
    deep Martian crust where free water will exist,
    anaerobic conditions similar in many respects to
    deep oil reservoirs will exist. Similar mineral
    nitrogen and phosphorus nutrient limitations can
    be expected as in Earth (Head et al, 2003).
    Surface derived electron donor supply in the form
    of any reactive fossil carbon is unlikely to have
    persisted to the present day as on Earth as much
    of the Martian crust is very ancient (109years)
    and thus with Earth oil reservoir carbon
    consumption rates much of the reactive fossil
    carbon in more permeable parts of the crust will
    have likely been consumed by heterotrophic
    organisms within in the first billion years or
    the subsurface will represent once deeply buried
    and thus sterile uplifted crust. Heterotrophs are
    unlikely to be found on Mars! It is thus likely
    that much of Mars is either dead or that any
    persisting Martin life in the deep subsurface
    will consist of organisms either deriving energy
    from reduction of carbon dioxide with hydrogen or
    from anaerobic oxidation of methane all three
    compounds being likely still being charged from
    the Martian deep crust and mantle to this day. We
    conclude that while much of Mars is probably dead
    any existing Martians surviving today will be in
    deep porous rocks and will be low diversity
    Archaea and associated symbiotic bacteria
    associated with methane cycling.

Martian sedimentary basins are believe to be very
old (109a). Oligotrophic subsurface OM
consumption rates would have eaten all the OM
long ago so any surviving subsurface Martians
would have to be Hydrogenotrophic Methanogens-CO2
from mantle H2 from mineral hydrolysis.
3. Compositional gradients provide degradation
rates
sediments from the present surface but is a
stable isolated biosphere derived from long
period evolution of surface derived organisms
during burial (Wilhelms et al, 2001). Recent
field studies suggesting that the actual fluxes
of hydrocarbons being destroyed in oilfields
around 40-70oC are around 10-4kg/m2/year of oil
water contact area and in excess of 50 of oil
may be destroyed in reservoir at advanced levels
of biodegradation with methane the common
terminal end product produced dominantly from
carbon dioxide reduction(5- Head et al, 2003).
These rates are comparable with the total
subsurface respiration seen in ocean margin
sediments (Dhont et al, 2002).
7. Bacterial counts subsurface marine sediments
Parkes et al, Nature 1994
6. A biodegradation model run on a Chinese
reservoir
bibliography
Current reservoir temperature and reservoir
vitrinite reflectance (Ro), for reservoirs in
the uplifted Barents Sea basins (no degraded
oils) and the subsiding N.Sea basins (degraded
oils). The horizontal shaded bar indicates
reflectance levels equivalent to
paleotemperatures of 80-90 degrees centigrade,
the vertical shaded bar the current 80-90 degrees
centigrade region.
Biodegradation in deep reservoirs proceeds
slowly under anaerobic and oligotrophic
conditions, typical timescales of biodegradation
being around 10 million years with large
fractions of oil being mineralized with methane
as a common terminal product (Head et al, 2003).
It is nutrients, principally mineral derived
phosphorus and nitrogen, not electron acceptors
or donors that are limiting in Earth, but on
Mars, electron donor supply must often be
limiting with the electron donors related not to
burial of surface derived organic matter as on
earth but to supply of either hydrogen or methane
from below! Recent advances in biodiversity
theory (Curtis et al, 2002 - 8) relate NT and
Nmax (8) to different types of environments. We
suggest speciation is driven by chemical
gradients which relate to the relative rates of
metabolism and mass transport processes
homogenizing the environment. While diffusively
mixed, the low rates of metabolism of petroleum
reservoir largobiospheres suggests the biosphere
will be well mixed even though diffusion is the
predominant mixing mechanism and we suggest that
the petroleum largobiosphere will thus have low
total individual numbers (ca 103 cells/cc) and
also have a low diversity (indeed will have comparable diversity to other
well mixed/connected environments such as sewage
treatment plants, non-stratified advecting marine
and lacustrine water columns (10).
  • Curtis, T.P., Sloan, T. and Scannell, J.W. 2002.
    Estimating procaryotic diversity and its limit.
    PNAS, 99, 16, 10494-10499.
  • Dhont, S., Rutherford, S. and Spivack, A.
    Subsurface life in deep sea sediments. Science,
    295, 2067-2070.
  • Head, I. M., D. M. Jones, and S. R. Larter. 2003.
    Biological activity in the deep subsurface and
    the origin of heavy oil. Nature 426
    (6964)344-352.
  • Larter, S. R., A. Wilhelms, I. Head, M. Koopmans,
    A. Aplin, R. Di Primio, C. Zwach, M. Erdmann, and
    N. Telnaes. 2003. The controls on the composition
    of biodegraded oils in the deep subsurface (Part
    1) Biodegradation rates in petroleum reservoirs.
    Org. Geochem. 34601-613.
  • Parkes, R.J. et al, The deep biopshere, 1994,
    Nature, 371, 410-413.
  • Wilhelms, A., S. R. Larter, I. Head, P.
    Farrimond, R. di-Primio, and C. Zwach. 2001.
    Biodegradation of oil in uplifted basins
    prevented by deep-burial sterilisation. Nature
    4111034-1037.

4. Uplifted sterilised reservoirs not biodegraded
Write a Comment
User Comments (0)
About PowerShow.com