Ocean Sediments: Why do we care? Marine
Transcription
Ocean Sediments: Why do we care? Marine
Ocean Sediments: Why do we care? Marine sediments record much of Earth’s history Marine Sediments: Why we care • Modern marine sediments – One of two ‘complete’ records of ‘recent’ past – Small changes in record imply significant events in earth history 1 Marine Sediments: Why we care • Ancient & ‘modern’ marine sediments – Host much of Earth’s fossil fuels – Marine sediments are the source of OIL – Potential ore deposits too! Two environments of deposition: • Neritic vs. Pelagic • Size of sediment (grainsize) – Neritic - range of sizes – Pelagic - clay sizes 2 Neritic = near coast • Derived from continents (15 million metric tons/year) – 25% from Tibetan Plateau (most out Ganges into Bay of Bengal) – Delivered by river drainages Drainage of Tibetan Plateau • 25% of all terrigenous sediment in oceans is from Tibetan Plateau (most out Ganges into Bay of Bengal) 3 Sediment Maturity In general, size decreases and maturity increases with distance from source/time of transport. Sediment size: sorting & energy • Sorting = degree of uniform grain size • Determined by sustained Energy – E.g. wave action vs storm event 4 Second ‘Environment’: Pelagic • Pelagic = settled from water – Wind blown or skeletal - near-shore deposits ‘swamped’ by neritic deposits – Fine grained – Slow accumulation (~0.5 cm/1000 yrs) – Thick 500 -600 m avg. Size and transport • Look at clay size - this is common size of wind blown dust and pelagic organisms • See how long it takes to sink! 130 years • Could travel 5 times around Earth in that time 5 Types of Sediment & Sources: Lithogenous, Biogenous, Hydrogenous, Cosmogenous Lithogenous = from rock Pelagic • Neritic & pelagic • Near and off-shore (everywhere) • Sources... Neritic 6 Lithogenous sources: Continental erosion • Neritic – Delivered to shelf by rivers – Distributed along shelf by currents – Trubidites transport to the Rise Lithogenous source: volcanic ash Pelagic & neritic 7 Lithogenous source: airborne dust Pelagic & neritic Distribution of Lithogenous Pelagic sediment 8 Biogenous Sediment: from organisms • Neritic, pelagic, and benthic (everywhere) • Neritic Example: Coral = limestones More neritic biogenous…atolls of Maldives 9 Limestones (CaCO3) Produced in warm, shallow seas Pelagic Biogenous Sediment • Microscopic Photosynthetic organisms – E.g. diatoms and forams – Require sunlight and nutrients (N & P) • Secrete outer shell – Die and shells accumulate on seafloor 10 pelagic ooze: > 30% biogenous sediment • Siliceous ooze – SiO2 shells – diatomes, radiolaria • Calcareous ooze – Calcite (CaCO3) shells – cocccolithophores, formaminfera Preservation of Siliceous Ooze • Ocean is not saturated with SiO2, so… • Siliceous sediment dissolves - just not very fast • Where productivity is high, sileceous ooze can accumulate 11 Preservation of Calcareous Ooze • Solubility of CaCO3 varies with water Temperature – Shallow warm ocean is saturated with CaCO3 - thus, no dissolution – Deep cold water is rich in CO2 (acidic) and dissolves CaCO3 • Carbonate Compensation Depth = depth of dissolution, avg. 4500 m – CCD in Atlantic can be as shallow as 4000 m, – CCD in Pacific can be as shallow as 3500 m – Depends on Productivity: where it is high, CCD is deep b/c cannot dissolve all the CaCO3 (buffered solution). Preservation of Calcareous Ooze • Can accumulate Calcareous ooze in shallow region (above CCD) • Cover it with clay or Silica ooze and preserve it in deeper regions 12 Hydrogenous Sediment Precipitates from seawater • Evaporites (restricted basins) • Mined for Salt Hydrogenous sediment: hydrothermal • Hot mineral laden water precipitates minerals as it mixes with cold ocean water. • Ancient deposits mined for copper - Cyprus 13 Hydrogenous: Mn Nodules • • • • Slow growth (pcpt from seawater) 1-200 mm/yr. Requires that no other sediment or current present to disrupt growth. Possible economic source of Manganese and CHROMIUM! Where abundant?... Mn nodules: • Abundant in Pacific - remember, trenches trap turbidite deposits 14 Cosmogenous Sediment Cosmic dust • Derived from space • 10% of meteors hit the surface Meteorites Now, are layers significant? • Layers in ocean sediment caused by… • Changes in sediment source & size • Thus produced by changes in Climate & Tectonics 15 Seafloor Mining: Ores • Most mining on Continental Shelf – Primarily for Sand, gravel. – Shells for lime and cement – P for fertilizers – Minor coal - Japan, Scottland – Sulfur - diminishing – Mn Nodules - Cr • Impact of seafloor mining? This is just a little science dredge, not a mining technique Seafloor mining: Oil and Gas • Oil & gas = 95% of seafloor mining • Proportion of US oil >30% • Deepest wells >2600 mbsl 16 Oil and Gas: Where do we find it in oceans? • On continental margins: e.g. Gulf, Persian G., N. Australia, S. coast CA, W. Africa • New areas: Nova Scotia, Indonesia, N Alaska, Caspian A new ‘find’: Gas Hydrates • Gas Hydrate = ice with trapped methane • Stable solid at high pressure, low temperature – >300 mbsl – under shelf! • Methane = natural gas! 17 Where is Gas Hydrate? • ‘imaged’ seismically on most shelves and in arctic tundra How abundant is gas hydrate? • Estimated Carbon abundance >2x all other fossil fuels • Possible future source of fuel??? 18 Gas Hydrate and Climate Change • Could Release of methane into atmosphere cause global warming? • We don’t know yet. • But, estimated methane in GH is 3000x atmosphere Gas Hydrate and Turbidity Currents: • ‘melt’ G-H and ‘weaken’ sediment on shelf/slope and cause failure (avalanche) • Turbidity trigger?? – Many slump scars on the shelf are at the depth of GH stability. 19