roger summons department of earth, atmospheric and planetary sciences mit preservation of organic...
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![Page 1: Roger Summons Department of Earth, Atmospheric and Planetary Sciences MIT Preservation of Organic Biomarkers on Earth: Generic Biosignatures, Petroleum](https://reader036.vdocuments.mx/reader036/viewer/2022062713/56649cbf5503460f94985794/html5/thumbnails/1.jpg)
Roger SummonsDepartment of Earth, Atmospheric and
Planetary SciencesMIT
Preservation of Organic Biomarkers on Earth:
Generic Biosignatures, Petroleum Source Rocks,
Early Earth Organic Record, OM & Hydrothermal Ecosystems
OM & Deep Biosphere,
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What is a biomarker? Criteria for discriminating biogenic vs non-biogenic organic compounds on Earth & Mars
Petroleum Source RocksPotentially useful analogues for understanding organic matter concentration & preservation on Earth
OM in Ancient Sediments
OM & Hydrothermal Ecosystems
OM & Deep Biosphere
Topics
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Non-biogenic Organic Materials
Ideal reference point is OM in meteorites
Predominantly macromolecular OM – kerogen– Pyrolysis to convert to small, identifiable molecules
Simple organic acids, diacids, amino acids, hydroxy acids, alcohols, amines
n- and branched hydrocarbons incl. methane
Aromatic hydrocarbons (PAH)Message: Characterized by simple ‘random’
chemical structures
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Biogenic organic materials
Macromolecular material – kerogenPyrolysis to convert to small, identifiable molecules
Complex structures with very specific patternsDNA, proteins, cellulose, membrane lipids
Made from simpler building blocks4 bases for DNA
20 amino acids
2 lipid precursors (2-C acetate and 5C isoprene)
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Biogenic organic materials
Patterns in spatial arrangements of C-atomsstereochemistry
HO
310 8
13
14
17
20
H H
9
28 stereoisomers possible for cholesterol
‘Biology’ makes only one
CCH3
H
COOH
CH3C
H
HOOC
H2N NH2
L-alanine D-alanine
CCH3
H
COOH
CH3C
H
HOOC
H2N NH2
L-alanine D-alanine
Amino acids ‘L’-helix in proteins
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• Patterns in the way C-atoms are linked together– Patterned structures
Biogenic organic materials
Patterning is preserved in the fossilized remains of chlorophyll
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Biogenic organic materials• Patterning is a generic ‘biomarker’
Patterns of C-number- example of a leaf wax
Patterning is a consequence of universal biochemical pathwaysmin10 20 30 40 50 60 70 min10 20 30 40 50 60 70 min10 20 30 40 50 60 70
C15
‘cluster’
C20
‘cluster’isoprenoids
‘odd over even’C29-C33 ‘cluster’ of
n-alkanes
low 11,12,13, 14
low16-19
low 21-24
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Microbial organic matter can be ‘ephemeral’Often eaten (ecology), oxidized, > 99% recycled on short timescales
Often at low concentration where it is being formed:most plankton communities ‘dilute’often thin biofilms on solid substrates (mineral surfaces)layered accumulations (mats) an exception
Can be massively concentrated by surface processes:exported as fecal pellets & adsorbed on mineral surfaces focussed by aqueous transport processes
Best preserved when:its isolated (from biology, O2 or other oxidants, radiation)concentrated (old productivity vs preservation argument!)it has a ‘tight’ association with minerals (clays, carbonates,
evaporites)
Organic Rich Rocks (1)
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Organic Rich Rocks (2)
OM concentration mechanisms vary in time and space
Predictable with knowledge of local sedimentary geology
OM concentrated in depocentres (eg lakes) sediments: predictable by cyclostratigraphy
OM concentrated & preserved in fine gained
(clay) sediments: predictable by
sequence stratigraphy
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Poor preservation of the rocks is the biggest obstacle to finding and interpreting early Earth organics
Destructive processes include: Geology deep burial metamorphism C and CH4
uplift weathering oxidation recycling
Ionising radiation alteration to ‘pyrobitumen’
Little unambiguous record > 3 Ga3.45 Ga Strelley Pool Fm (Allwood,2006; Marshall, 2007)
2.7-2.3 Ga Transvaal (Fischer, 2008; Waldbauer, 2008)
600 Ma-present: Age of petroleum and other fossil organics ubiquitous and abundant
Organics on Early Earth
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Finding authentic biomarkers in Archean sediments is difficult -
similar analytical challenges to finding organics on Mars
Organics on Early Earth
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Strelley Pool Formation
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Aromatic hydrocarbons from Hydropyrolysis
04 Dec 01 05
SPC 120803-5 3.45 Ga
Time15.00 20.00 25.00 30.00 35.00 40.00 45.00 50.00 55.00 60.00 65.00 70.00 75.00 80.00
%
11
P MePy
Py
2MeNFlA
C2-Py MeChB(e)Py
B(ghi)Per Co
MePMeBiPh
**
++
++
Marshall et al., Precambrian Research 2007
Urapunga 4 1.5Ga
15.00 20.00 25.00 30.00 35.00 40.00 45.00 50.00 55.00 60.00 65.00 70.00 75.00 80.00
%
2
Py
P
MePy
2MeNC2-Py
MeChB(e)Py B(ghi)Per
Co
MePMeBiPh**
FlA++
++
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Murchison (hydro)pyrolysate
phenanthrene
pyrene methyl chrysene
benzo[ghi]perylene
coronene
TIC
retention time
response
S
Pyrolysis products• HMW, 3 to 7-ring aromatics• pyrenes, chrysenes• volatiles lost
methyl pyrene
chrysene
Previous work• Hayatsu et al. 1977 - chemical degradation, 2 to 4 ring• Kovalenko et al. 1992- lazer desorption ionisation, 2 to 7 ring
Mark Sephton, Cheng-Gong Sun, Gordon Love and Colin Snape GCA
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Martian PAH
5 10 15 20 25 30 35 40 45
retention time (min)
0
solvent extracted Nakhla
procedural blank
C2
CN
OH
-22.0 -21.6 -22.1 -18.013C:
Martian meteorites (e.g. Nakhla)• PAH• Contamination less likely for HMW
OM• pyrolysis products• Structures and isotopes superficially
similar to carbonaceous chodrites
Mars PAH may be abiotic andoriginate from meteoritic infall
Sephton et al., 2002 Planet Space Sci 50, 711-716.
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PAH proposed to be molecular fossils ?
‘ PAH are abundant as fossil molecules in ancient
sedimentary rocks ’
No patterns so cannot say if its biogenic or not
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Agouron Griqualand
Drilling Project
Transvaal Supergroupca. 2.67 – 2.46 Ga
Sumner & Beukes SAJG 2006
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Outside flat
Untreated
Rinsed
InsideOutside curve
10 cm
Figure 3.
Clean by removing outside surfaces
Compare ‘solvent extractable’ vs ‘mineral associated’ hydrocarbons
Crush, extract with solvent, add internal stds Bitumen 1
Demineralize extracted sediment and re-extract residue with solvents Bitumen-2
Protocols for Archean Hydrocarbons
Sherman et al., Organic Geochemistry 38, 1987–2000, 2007
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Organic Matter (0.4-11.4 wt%)
SilicateSulfideOxide
(9-99 wt%)
Carbonate(1-90 wt%)
Whole Rock
Bitumen I(14-605 ppb)
Bitumen II(70-506 ppb)
OrganicMatter
Kerogen(Insoluble, macromolecular; H/C <0.2)
S
S
O
HN
S
S
O S
NHO
O
S
O
Aromatics(1-488 ppb)
Saturates(2-386 ppb)
CyclicTerpenoids
(0.2-1 ppb) Steranes(0.07-0.48 ppb)
Hopanes(0.05-0.26 ppb)
Cheilanthanes(0.05-0.34 ppb)
Bitumen IHydrocarbons
Biomarkers
Aromatics(18-300 ppb)
Saturates(14-382 ppb)
CyclicTerpenoids(0.9-19.5 ppb)
Bitumen IIHydrocarbons
Steranes(0.36-6.31 ppb)
Hopanes(0.30-11.35 ppb)
Cheilanthanes(0.22-1.88 ppb)
Biomarkers
Composition of Core Samples
In these ancient rocks, best preserved biomarkers evidently within crystalline
minerals; these H/C accessible after dissolution
Waldbauer et al., Precambrian Res. 2008.
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C27
0.0 0.5 1.0 1.5
GKF Bitumen IGKP Bitumen IDwyka (GKF)Dwyka (GKP)GKF Bitumen II
C28
0.0 0.5 1.0 1.5 2.0
C29
0.0 0.5 1.0 1.5GKF
DepthGKPDepth
L
KN
R
N
K
D
M
V
B
167.3178.5192.3230.0268.4
314.7
450.1
705.3
895.5
966.2
1309.81326.3
1424.71435.0
173.4228.5239.5316.4
332.5
418.7
636.9
678.2
960.0980.1
1051.2
1248.9
HH
H
H
H
H
HH
H
H
H
H
Diasteranes/Regular Steranes
27
27
28
28
29
29
GKF Bitumen I
GKP Bitumen I
GKF Bitumen II
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Low TOC sediments Low TOC sediments colonized by chemosyntheticcolonized by chemosynthetic
communities in ventcommunities in ventand > 70and > 70˚̊C outflowC outflow
High TOC sediments based on High TOC sediments based on photosynthetic communitiesphotosynthetic communities
< 70< 70˚̊C outflowC outflow
To what degree are they ultimately dependent on O2-photosynthesis ???
(Spear et al., PNAS 2005)
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“Bison Pool”
Water chemistry similar to Octopus Spring, pH c. 8, silica pptn
Silicious streamers & biofilms in outflow
Aquificales dominate silica sediments and streamers
Meyer-Dombard et al., 2005, Geobiology & DRMD, Raymond and Shock work in progress
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“Bison Pool” 16S rRNA survey
Aquificales
Thermotoga
Geothermobacterium
Thermus
OP11
Desulfurococcales 1
UnculturedCrenarchaea 1
BACTERIA
Desulfuro. 2
Uncult. Cren. 2ARCHAEA
Chemosythetic: Zone 1Pink Streamers
Aquifex = water maker
H2 + O2 for energy
CO2 or formate for C
Crenarchaeal taxatypically heterotrophic
Meyer-Dombard et al., Geochim.Cosmochim. Acta 71 Supp, A661 & work in progress
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Bison Pool ‘chemosynthetic’ silicious biofilm community
dependent on O2 from photosynthesis
Abundant O2 suggests OM preservation in continental hydrothermal systems
problematic
‘Fossil’ Yellowstones rare in Earth’s geological record; difficult to evaluate them
as potential Mars analogues
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Marine hydrothermal microbial community independent of sunlight; preservable in ophiolite ?
Atlantis Massif
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olivine + water serpentine + brucite + magnetite + H2
Serpentinization: source of H2 and alkalinity
Kelly et al., 2005
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Lost City Hydrothermal FieldTowers
CaCO3 and Mg(OH)2
0.05% and 0.6% TOC δ13C from -27.7‰ to -2.8‰
Vent Fluids
Hydrogen – up to 15 mmol/kg
Methane – up to 2 mmol/kg
Calcium – up to 30 mmol/kg
pH – 9 to 11Kelly et al., 2005; Bradley et al., GCA 2008 In Press
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Lost City Hydrothermal FieldArchaeal biomass dominated by
Methanosarcinales (Schrenk, 2004)
O
OH
O
O
OH
O
OH
archaeol
sn-2 hydroxyarchaeol
Firmicutes prominent in bacterial biomass (Brazelton et al., 2006)
Likely acting as sulfate reducers
Bradley et al., GCA 2008 In Press
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-140
-120
-100
-80
-60
-40
-20
0
20
13
, ‰
methane archaeal diethers
Lost CityMethanotrophs
AOM communitiesMethanogens
Cultures
H2/CO2 Acetate TMAHMMV HR ERB NW BS
Location Substrate
Lost City Methanosarcinales are methanogensBradley et al., GCA 2008 In Press
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Who are they & what are they doing??
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JS Lipp et al. Nature 000, 1-4 (2008) doi:10.1038/nature07174
Depth profiles of IPLs in marine sediments.
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Crenarchaeal biomass correlates with TOC
Labeling shows consumption of complex organics only:a predominantly heterotrophic community
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Concluding ThoughtsOrganic compounds made by terrestrial organisms have generic
structural & isotopic traits. Searching for biosynthetic patterning in extraterrestrial OM is a sound approach to life detection
On Earth, organic matter is largely concentrated in sediments deposited in aquatic environments
If OM preserved on Mars, expect a tight association with low temperature, sedimentary minerals – clays, evaporites, silica