Emerging Views of SedimentBuried Ocean Basement Biosphere James P. Cowen Department of Oceanography University of Hawaii jcowen@soest.hawaii.edu Emerging Views of the Biosphere w/in Aging Ocean Basement • Ocean basement provinces • Biosphere of aging basement – Access—tough – General physical (e.g., fluid flow; temperature) and chemical characteristics – Evidence of extant biosphere – Speculated metabolic pathways – Challenges and future research directions Why do we care? • Ocean basement is a huge volume • Potential for extensive biomass – Basalt to gabbro rocks • Prone to alteration disequilibria – Fluids circulate even in old basement – Thermal, chemical gradients • Potential for exotic metabolisms/strategies • Analogue for extraterrestrial fluid covered, rocky bodies Detrick 2004 crust ocean basement Ocean crust Karson et al. 2002 Zone I: Ridge axis — active exchange — high/low temperature venting; — sharp thermal / redox / chemical gradients Zone II: Unsedimented ridge flank — active (advective) exchange, low (to high ?) temperature venting — poorly explored ~165 m Diffuse upwelling Impenetrable Zone III: Sedimented ridge flanks (a) and basin (b) —increasing sediment cover; —hydrologic seal at ~165 m thickness —conductive heat / diffusive chemical exchange Zone IV: Exposed rocky outcrops (Seamounts) — Local advective recharge or discharge; — Natural access to fluids Access to crustal fluids ODP/IODP Boreholes - Sediment and basement cores - Observatories: CORKs (Circulation Obviation retrofit Kits) * Engineered access to basement rock and fluids CORK-I Observatory Biological Diversity Biomass Metabolism Activity/survival Consortia Heat (temp) Geochemical Redox potential Essential elements Water/rock Rock mineralogy Basement age Spreading rate Sedimentation Fluid Flow Permeability Porosity Driving energy Global Ocean Basement JdF Ridge flank Lau Basin Reykajanes MAR west flank Costa Rica Rift South flank Basement temperatures (east flank JFR) 0.8 My 0 20 3.5 My 40 60 80 100 120 Distance from ridge axis (km) from Davis et al. 1999 JFR, CRR 0 10 20 30 40 50 60 Crustal Age (Ma) Wheat et al. 2003 Ocean Lithospheric Heat Flux Total: ~32 TW Hydrothermal circulation to 65 Ma: ~11 TW Off-axis (1-65 Ma) heat flux: ~9.25 TW Low Temp Associated Water Flux Near ridge (0-1 Ma): ~3.7 x 1016 g/yr Flanks (1-65 Ma): ~0.2-2 x 1019 g/yr Flank fluid flow = 50-500 X Axial flow Schultz and Elderfield 1997 Cycle entire ocean through flank basement in 70,000 to 700,000 yrs Mottl 2004 Bulk Permeability of Upper Basement Crustal Age Suggests a decrease In bulk flow w/in aging basement Consistent with seismic velocity (faster in denser, less porous media), but inconsistent with heat flow obs (signif. advective heat loss to 65 My) Fisher (2004) Channelized flow Fluid flows: Diffusive flux Tortuous advective Rapid channelized Borehole 395A: MAR flanks • Zones of deflection in SP log (10-100 m thick) Suggest: Channelized flow modified from Matthews et al. (1984), Becker et al. (1998) measures pressure differences Basement rock/fluid chemistry – Temperature of rocks (e.g., <2 to >100oC) – How much fluid previously passed • History of fluids – Composition of host rock (primary/secondary mineralogy) • age • water : rock ratios • flow rates (i.e., general and local permeability) • microbial activity Basement mineral alteration (bulk basement rock) JdFR flanks Fe2+ (Fe2++Fe3+) Age of basement Distance from ridge axis Marescotti et al 2000 Johnson and Semyan 1994, reploted by Bach and Edwards 2003 JdFR Increasing (upper) Basement Age Marescotti et al. 2000 Alt and Mata 2000 Bach and Edwards 2003 Olivines FeOOH Celadonite/ saponite Pyrite Alteration Halo within Fracture (fluid conduit) Microbial role ? O2 reduction NO3- reduction + H2 oxidation Fe3+ reduction SO42- reduction - O2,NO3 + Fe+2 oxidation S oxidation H2 Fe2+ Olivines Furnes and Staudigal1999 estimate 75% of upper basement is microbially altered !? FeOOH Celadonite/ saponite Pyrite O2 Making a Living in Subseafloor Basement Environments Photoautotroph Chemotroph (reduced) organic carbon In situ abiogenic organic carbon Chemoorganotroph (heterotroph) Chemolithoautotroph organic carbon Chemolithoautotrophy: Energy: Oxidation/reduction reactions using inorganic e- donor & e- acceptor pairs C-source: inorganic (CO2) Relevant, microbially meaningful reactions (chemolithoautotrophic) 4FeO + O2 + 6H2O = 4Fe(OH)3,s Aerobic Fe2+ oxidation [5FeO + NO3- + H+ + 7H20 = 5Fe(OH)3,s + 0.5N2] Anaerobic Fe2+ oxidation FeS + 2O2 = Fe2+ + SO42- 2 FeO + 4 H2O = 2 Fe(OH)3 + H2 2 FeO + 2 H2O = 2 FeOOH + H2 2 FeO + H2O = Fe2O3 + H2 H2 oxid by O2, NO3-, Fe3+, SO42-, Sulfide oxidation Low-To, abiogenic anaerobic hydrolysis H2 oxidation Potential metabolic processes active in subseafloor basement e- donor e- acceptor By-product Subsurface habitat zonesa H2 NO3-, NO2-, N20, NO, N2 NH3, N2, NO2-, NO, N2O I, II, IVa,b H2 SO42-, SO32-, S2O32-, S4O62-, S H2S, S2O32 I, II, IIIa,b, IVb H2 CO2 Acetic acid I, II, IIIa,b, IVb NH3 NO2-, MnIV N2, MnII I, II, IIIa, IVa S2- NO3- NH3, SO42- I, II, IIIa, IVa S2- NO3- NH3, S0 I, II, IIIa, IVa Organic-C SO42-, SO32-, S2O32-, S CO2, CH4, CO, reduced S I, II, IIIa,b, IVb Organic-C O2 CO2 I, II, IVa Organic-C NO3- NO2-, N2, NH3, CO2 I, II, IV H2, CH4, NH3, O2 S-2, FeII, MnII H2O, CO2, NO2-, NO3-, FeIII, MnIV I, II, IIIa, IVa Organic-C Organic-C (fermentation) I, II, III, IV Organic-C, FeIII, other minerals Gr = Gr0 + RT ln(Q) I, II, IIIa,b, IVb Q = activity product? Edwards 2004 Bottom seawater Basement Fluids (1.2 Ma; 40.5oC) Basement Fluids (3.5 Ma; 64oC) pH 7.9 7.2 7.4 Alkalinity (meq/l) 2.5 1.4 0.6 SO42- (mmol/kg) 26.1 26.5 17.5 Mg2+ (mmol/kg) 52.5 27.5 4 Ca2+ (mmol/kg) 10.3 34.2 56.2 2.4 1.4 0.5 <0.002 0.4 1.8 ~0.0002 0.4 0.6 Fluid Composition TCO2 (mmol/kg) CH4 H2 (mol/kg) (mol/kg) NH3 (mol/kg) 0.9 60 90 Mn (mmol/kg) 0.0 48 4 Fe (mmol/kg) 0.0 62 1.1 190 590 750 Si (mmol/kg) Enriched Cowen et al. 2003; Wheat et al. in review; M. Lilley, unpubl. data Depleted Basement fluid chemistry Depleted Mg2+/ enriched Si, Ca2+, Sr2+, H2 – Reaction with basaltic rocks Enriched H2 – Hydrolysis of ferrous Fe in basalt rocks Depleted sulfate – Sulfate reduction (H2, Org-C) – Diffusion to sediments – Sulfate mineral precipitation (e.g., Jarosite, anhydrite) Elevated ammonia – Nitrate reduction (e.g., e- donor: Org-C, Fe2+, or H2) – N2 fixation – Diffusion from sediments Depleted TCO2, alkalinity – Carbonate precipitation Enriched Si, Fe – Seawater-basalt reactions – Contamination (e.g., drilling ops, borehole casings) Sediment-Basement Exchange: Borehole 1027 (3.5 Mya) Sediments basement Mather and Parkes 2000 Borehole 1027: sediment profiles Mather and Parkes 2000 Inferred Microbial-Produced Alteration Textures BSE-SEM images MAR 7 mbs <2 Ma Lau 3 mbs 4-7 Ma Reykj R 51 mbs 2.3 Ma MAR 45 mbs 10 Ma Reykj R 124 mbs 38 Ma MAR 157 mbs 10 Ma Furnes et al. 2001 mbs: meters below sediments Costa Rica Rift ~50 mbs Phase contrast DNA (DAPI) ~120 mbs Phase contrast DNA (DAPI) Arch344 Bac388 Bac388 Arch344 Fluorescent in situ hybridization— probes specific for Bacteria or Archaea Torsvik et al. 1998 Elemental X-ray maps C N (K) resin in fracture Costa Rica Rift ~100 mbs 5.9 Ma Costa Rica Rift ~100 mbs Other maps: 5.9 Ma Si, Mg, Ca, Na depleted Ti, Al, Fe, Mn, enriched P (S) Torsvik et al. 1998 ‘BioColumn’ basement fluid sampler Cowen et al. 2003 Cell products from basement fluids (1026b, JFR) Propidium iodine-stained Giovannoni 0.5 um Low G+C Borehole 1026b basement fluids: Phylogenetic tree (ssu rRNA): bacterial groups -Proteobacteria 1026B clones’ closest known relations: Cowen et al. 2003 Sulfate reducers Fermentative heterotrophs Nitrate reducers (NH3 production) N2 fixers? (NH3 production) Thermophilic members Borehole 1026b fluids: Phylogenetic tree (ssu rRNA): Archaea 1026B clones’ closest known relations to: Sulfate reducers Genes from Yellowstone hot springs Thermophiles Cowen et al. 2003 Basement fluid ages (east flank JFR) recharge Fluid 14C ages: 4.5ky 1ky 9.9ky 0.8 My 0 20 3.5 My 40 60 80 100 120 Distance from ridge axis (km) from Davis et al. 1999 (partially) Reset time clock and redox conditions Older, reduced Cowen 2004, as modified from Wheat et al. 2002 Fisher et al. 2003 Wheat et al. 2002 Speculated characteristics of buried ocean basement biosphere • Low cell abundance • Slow growing • Highly heterogeneous distributions (& activities) – Localized populations consistent w/ channelized flow – Punctuated by recharge zones • Diverse chemoautolithotrophic and heterotrophic (& unusual) metabolisms • Microbial consortia likely important and associated with biofilm formation Summary • Ocean Basement environments are dynamic and complex • Biosphere within aging basement is predicted: – – – – Favorable temperature ranges, Active fluid flow (is it enough?) Reactive basaltic rocks Existing (preliminary) phylogentic data consistent w/ chemical data • Challenges – Accessibility – Contamination – Life perhaps ubiquitous, but low biomass/activity? Future borehole observatory opportunities • Cores from drilling operations • Short and long-term observations – In situ (downhole) instrumentation – Fluid collections – In situ incubations (seafloor and downhole) – Other experiments (e.g., push-pull) Contamination issues Drilling operations • Drilling muds, bottom seawater, sediments Observatory materials • Packing cement • Borehole casing • Sample delivery tubing CORK-II Observatory Downhole sampling Cowen and Taylor, in development In situ Chemical Redox Analyzer 2e-6 free H2S FeS dissolved O2, H2S, MnII, FeII, S2O32-, S4O62-, Sx2-, S0, aqueous species of FeIII and FeS i (A) 1e-6 0 * A SAVS -1e-6 -1.5 500 concentration (M) -1.0 -0.5 Volts (vs AgCl) 400 Free H2S 300 SAVS FeS In situ Voltammetric 200 Electrochemical measurements 100 B Starring Brian Glazer! 0 0 30 60 90 120 time (sec) 150 180 Cabled IODP CORK Observatory (Ocean Observatory Initiative) – Power: • In situ filtrations • Temperature controlled in situ incubations – Two-way communication: directed sampling • Fine-scale coordination w/geophysical exp. • Response to perturbation (e.g., seismic/magmatic events) • Chemical/particle tracer transport studies Colleagues Co-Investigators Stephen Giovannoni (OSU) Michael Rappe (OSU,UH) Fabien Kenig (UI, Chicago) Craig Taylor (WHOI) Brian Glazer (IfA, UH) David Butterfield (PMEL-NOAA) Paul Johnson (UW) Students Rachel Shackelford (UH) Phyllis Lam (UH) Michael Hutnak (UW/UCSC) Other indispensable colleagues Andy Fisher (UCSC) Michael Mottl (UH) Geoff Wheat (UA, MBARI) Funding: NSF--Ocean Instrumentation, LExEn, MO, NASA-UHNAI Propidium iodine-stained sediment-buried basement fluids (1026b, JFR) Giovannoni