Deep time: Lectures 1-8 Flashcards

1
Q

Dates and key events for Hadean, Archean, Proterozoic, Phanerozoic, Cenezoic era and Quaternary period

A

Hadean (4.6-3.8 Ga) - origin of Earth, anoxic atmosphere

Archean (3.8-2.5 Ga) - origin of life in form of single-celled bacterial organisms, lowered CO2

Proterozoic (2.5-0.54 Ga) - The Great Oxidation, Snowball Earths, origin of Eukaryotes, boring billion, and animals by 0.58 Ga

Phaneozoic (0.54-0 Ga) - plants, mass extinctions

Cenezoic (65-0 Ma) - declining and levelling off CO2

Quaternary (Last 2.6 billion years) - Pleistocene and Holocene (11.5 Ka)

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2
Q

Describe the early atmosphere (Kasting, 1993)

A

High amounts of CO2, N2, CH4, H2O

O2 rose naturally and later, whilst greenhouse gases lowered to counter brightening Sun

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3
Q

Describe the Big Bang and formation of the elements

A
  • Occurred 13.7 Ga, taking 9.1 billion years for star formation, and eventually Earth 4.5 Ga
  • Red-shift and CMBR suggest a continually expanding universre
  • Initial cooling after big bang formed neutrons - decay and collide to form H atoms; nuclear synthesis (stops, unstable masses 5/8)
  • Nuclear fusion in large stars produces heavier elements up to Fe
  • Elements heavier than Fe from neutron capture after large stars explode into super novas then cool into neutron stars; elements dispersed
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4
Q

Describe the formation of the solar system i.e. rocky planet formation

A
  1. Coagulation - dust collisions (10^4 yrs)
  2. Runaway accretion - growth by collisions to 1000km planetesimals
  3. Oligarchs - growth by accretion
  4. Embryo planet merging - embryos collide, Earth-sized, v. slow timescale (10^8)
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5
Q

Describe the formation of Earth. Refer to volatiles, the core and the formation of the moon.

A

Earth & core:

  • Non-volatile elements formed by stars assumed to form core of rocky planets e.g. Si and Fe
  • Gravitational energy heated Earth’s inteior as accretion occurred
  • Melting caused dense Fe droplets to form the core
  • Fe and Ni abundant/dominant in core, but Si is not despite not volatile; because Fe and Si are immiscible
  • Si convected upwards in partial melt of mantle = core differentiation

Moon:

  • Anomalously large - from collision with ‘Theia’
  • Moon has less dense, small core
  • Was once closer to Earth, debris ring coalesced into moon - Earth’s spin momentum transferred
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6
Q

How did the oceans and atmosphere form? What evidence is there for liquid water?

A

Oceans & atmosphere:

  1. Out-gassing - some volatiles stored in mantle, out-gassed to surface
  2. Extraterrestrial impacts from water-rich bodies; carbonaceous chondrites

Liquid water:

  • Zircons (4.4 Ga); dated and found within igneous rock
  • Existence of zircons suggests active hydrological cycle for erosional/weathering and tectonic processes
  • Also, enriched in 18^O, suggests water was present (similar to present day isotopes??)

Oldest rocks dated at 4.28 and 4.04 Ga (Quebec and Canada)

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7
Q

When was the first life evidenced; where and how (x5)?

All occurring within 3.8-3.2 Ga…

A
  1. Banded Iron Formations (3.8 Ga) in oldest sedimentary rocks - evidence for existence of some O
  2. Turbidites (3.8 Ga) - oldest reduced carbon, C rich; graphite with 12-C, could have been microorganisms
  3. Stomatolites (3.5 Ga) - odd bunps/dome structures indicating microbial communities
  4. 13-C depleted carbon in oldest fossil cells (3.5 Ga) - although contradicted by Brasier et al., 2002
  5. Dividing cells (3.26 Ga, Swaziland); caught in the act =THE WIDELY ACCEPTED POINT OF ORIGIN

Alternatives - Rare Earth / Transpermia / Deep Hot Biosphere

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8
Q

What is continental drift? What evidence is there for it, sea-floor spreading, and fault lines/boundaries? What is the rate of divergence/convergence?

A

Alfred Wegner (1880-1930) - continents on plates move over time; oceanic (more dense) and continental (less dense); theory of Pangea

Rate of convergence/divergence; 100mm/yr

Pangea evidence:
Biological (fossils matching up), Geological (shelves, cratons) and Climatological (glacial till at tropics)

Boundary evidence:

  • 1960s mapped ocean bathymetry - marine mountain ranges etc.
  • Global distribution of seismicity; fault lines

Sea-floor spreading evidence:

  • Paleomagnetism (aligning and matching ion orientation according to geomagnetic reversal)
  • Sediment depth (deeper further away, dated older too)
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9
Q

Types of plate boundaries? What are cratons?

A

Divergent/Constructive - move apart; crust created = rift valleys, mid-ocean ridges e.g. East African

Convergent/Destructive - plates collide; denser crust subduct beneath other, melting, volatiles and pressure, magma rises = trenches and volanoes (oceanic-continental) or island arcs (ocean-ocean) or buckling and mountains (continent-continent) e.g. Andes, Himalayas

Passive - innactive boundaries

Cratons = continental shield

  • Oldest rock found on surface since most mountain ranges conain “young” rock because of erosion
  • E.g. Canada, Greenland, Australia up to 3 Ga
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10
Q

What are supercontinent cycles? How many have occurred since formation of Earth and how many years dows a cycle take to complete?

A

Movement of supercontinents; broken up, move, then join again in THE WILSON CYCLE

Estimated 8-10 cycles in Earth’s history; complete in 500x10^6 years

3 currently proposed supercontients:

  1. Nuna (1.3 Ga)
  2. Rodinia (750 Ma)
  3. Pangaea (225 Ma)
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11
Q

What is the equation for Silicate Weathering including Carbonate deposition?

A

CaSiO3 + CO2 –> CaCO3 + SiO2

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12
Q

What is the FYSP, HZ, and H-R Diagram? Whilst your at it, describe star lifecycles…

A

Faint Young Sun Puzzle - when Earth formed 4.6 Ga Sun was 30% dimmer, so Earth should have been frozen. BUT there is evidence for liquid water at this time (zircons) - so how was the Earth kept warm despite the lack of solar irradiation

Habitable Zone - zone in which liquid water can exist on planet based on distance from star and how bright it is; temps of 0-70C; not fixed, HZ will move further as star brightens

Herzprung-Russell Diagram - categorises stars based on luminosity (brightness) and temp (colour); shows evolution of stars

Bigger than Sun = main sequence –> produce Fe -> super red giant –> supernova –> neutron star/black hole
Same/smaller than Sun = red giant –> white dwarf

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13
Q

How is the solution to the puzzle proposed? What is the role of silicate weathering and then what role does life play?

A

GHG:

  • Greenhouse gas effect must have been greater
  • High levels of certain GH gases; many suggest CO2 or ammonia

Carbon cycle/weathering:

  • Largest C store = buried oxidized carbonate
  • Smallest C store = surface
  • Input (volcanoes & heterotrophs) balanced by organic carbon burial (dead animals) and silicate weathering
  • CO2 dissolves in rainwater, produces carbonic acid, reacts with Ca or Mg in rocks, ions washed into ocean, carbonate used by organisms (shells)
  • FEEDBACK; temp increases from brightening Sun, Si weathering speeds up, more C buried, less CO2 = less heat trapping…

Climate regulation:

  • Plant amplification of Si weathering (e.g. fungus breaking rocks to reach minerals)
  • Also increase phosphorus cycle which increases burial of also (since it increases ocean productivity)
  • Plants caused CO2 to decline and level out
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14
Q

How many snowball events have been thought to have occurred; give their dates.

A

3 within the proterozoic and neoproterozoic eon

  1. Makganyene, 2.22 Ga
  2. Sturnian, 710 Ma
  3. Marinoan, 640 Ma
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15
Q

How does a Snowball Earth occur - what triggered it (x2)? How would it ‘get out’ of one? How did complex life ancestors survive?

A

Causes/triggers:
- Runaway feedback; cooling causes ice sheet expansion, if reaches 30 degree latitude tipping point, albedo so high that ice sheets ‘snap shut’ - what drove a reduction in CO2 then?
GEOLOGICAL = Rodinia supercontinent breaking up, continents dispersed at tropics = rapid weathering, increased C burial AND Large Igenous Province = increased basalt weathering
BIOLOGICAL = colonisation by fungi, cyanobacteria, algae and lichens (1430-600 Ma) = x10 faster weathering = increased C burial

Escape?

  • Accumulation of CO2 in atmosphere since output inhibited (dry, arid, no rain, no Si weathering)
  • Increased greenhouse effect; volcanic areas melting ice, degassing of ocean floor, cracks in ice etc.
  • Dark ocean reduces albedo, runaway feedback enables global melt

Survival?
Warm refuges by hot springs

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16
Q

What evidence is there for the first photosynthesis?

A

Simultaneous with first life 3.7 Ga (oxygenic at 2.7 Ga)
Firstly ANOXYGENIC; didn’t use H2O or produceO
- Early types of photosynthesis far simpler - one photosystem - requiring less energy

OXYGENIC; rips water molecules to get sugars, requires more energy (2.7 Ga)

  • First performed by cyanobacteria - release O, rapidly consumed by reactive elements, reducing atmosphere…
  • Now part of eukaryote cells
  • Rock record with oxidised compounts

= atmosphere less reducing, surface ocean becomes oxygenated

17
Q

Outline the 4 main phases through which oxygen rises.

A
  1. Reducing atmosphere, anoxic surface and deep ocean (>2.7 Ga)
    - ->FIRST OXYGENIC PHOTOSYNTHESIS
  2. Reducing atmosphere, oxygenated surface, anoxic deep (2.7-2.4 Ga)
    - -> GREAT OXIDATION
  3. Oxidising atmosphere, oxygenated surface, anoxic deep (2.3-0.6 Ga)
    - -> LESSER OXYGENATION
  4. Oxidising, oxygenated surface and deep ocean (0.6-0.4 Ga)
18
Q

What was the LHB?

A

Late Heavy Bombardment, 3.9 Ga:

Late ‘flourish’ of rocks, identified by dating of moon rocks and craters

19
Q

What evidence is there for the great oxidation?

A

Sudden oxidation of atmosphere, never reversed (2.45-2.32 Ga)

Paleosols - ancient soil record; lack of iron to sudden abundance

Red beds - oxidised iron deposits in sedimentary beds

Banded Iron Formations - soluble reduced iron in rocks reacting with oxygen in bands; sudden disappearance by 1.8 Ga (removal of Fe from oceans = O!)

20
Q

What other mechanism for O rise is there?

What evidence to we use to understand the history of atmospheric oxygen? (P, MIF, O3)

A

Further O rise 600-400 Ma - phosphorus weathering accelerated by eukaryotes and lichen at 470 Ma - more nutrients for ocean = consumption and burial of CO2 increases, production of O increases (evidenced by P-rich deposits)

Reduction in MIF of sulphur isotopes in record suggests increase in O (O3 enabled by abundant O!)

Stable states and Bi-Stability:
LOW O = CH4 rapidly consuming O, lack of O3, high energy UV
HIGH O = O3 reduces UV, slowing CH4 consumption of Oxygen

Bi-stability meaning O never reverses not fully understood yet

21
Q

Can oxygen explain complex life?

A

No….but…

Proterozoic Eon saw origin of eukaryotes and aerobic respiration (2 Ga). Really slow evolution from this point (boring billion), until O rose enough?

Complex life associated with Edicarans (0.58-0.54 Ga) and then the Cambrian Explosion and the hard-shelled organisms (0.54-0.5 Ga)

22
Q

What evidence do we have for the Sturnian and Marinoan?

A

In theory, expect planet to be very hot and wet in the aftermath of a snowball event, lots of CO2

Oxygen levels:
Jump up during glacial events = C cycle disruption, increased CO2 consumption resulting in cooling

Sedimentary rocks - paleomagnetism, glacial deposition, Cap carbonates & dropstones:

  • Preserved ‘compass’ in striations/dropstones suggest deposited at the equator
  • Large depositions of carbonate rocks following snowball events e.g. 1km thick platforms
  • Glacial dropstones alongside carbonate deposits
  • Large amounts of Si weathering = huge removal of CO2

BIFs

  • Only form in anoxic oceans (small oxidation = bands)
  • Rare re-appearance of BIFs suggests sealed-off ocean for a period of time = ice sheets everywhere!
23
Q

What is the Gaia Hypothesis - basic tenets; who proposed it?

A

Lovelock & Margulis (1972); life controls greenhouse gases, control climate to an extent

  1. Atmosphere is far from equilibrium, but is largely stable
  2. Environment and dominant organisms within narrow tolerance bounds
  3. Persistently habitable climate
  4. Acidity of Earth’s surface anomalous compaired to other planets but is tolerable to life

Margulis added to the hypothesis by suggesting the role of homeostasis; ‘self-regulation to a fixed stable state’

24
Q

What is proposed as the signature of life?

A

Comparing Earth to Mars’ atmosphere - identifying the presence of gases at disequilibrium e.g. CH4 and O (abundant oxygen is abnormal)

25
Q

What scientific validity did the Gaia Hypothesis have? What criticisms did it bring?

A

Increased scientific validity:

  • Questioned function of atmospheric, oceanic and soil composition, surface temp, pH - how maintained
  • Through this, Dimethyl Sulphide and Methyl Iodide discovered; an essential compound exclusive to life!

Criticism:

  • Mythical naming of the hypothesis ‘Gaia’, Greek Goddess of life
  • Teleology; bacteria would require a sense of consciousness, foresight
  • Natural selection; biological perception that life progresses only through this process, and the planet is not a biological single entity in competition with anything else - not a unit of selection
26
Q

How did Lovelock respond to criticism?

A

Daisyworld (1981):
Environment reduced to temp and single life type of black and white daisies; forced by solar luminosity…
- Black = absorb heat, warm surroundings, rapid growth, runaway positive feedback, but then exceeds 22.5C, reaches 40C maximum, eventual decline in population
- White = lag time for sun to get brighter since they reflect radiation, steady cool period, eventually too hot from luminosity, daisies die, increased dark patches, reduces albedo, temp increases further

If both species present =

Conclusion = life can automatically alter its surroundings without conscious foresight - temporary stable periods

27
Q

What other examples are there of Earth’s self-regulation?

A

Ocean saltiness and nutrients

  • Ocean should be saltier since Na Cl washed into it with little output
  • Life helps regulate salinity by lagoons = net evaporation = halite depositions?
  • Other outputs e.g. ‘black smokers’; transferred to crust
Redfield Ratio (1934)
- Proportion of nitrate and phosphorus in world's oceans match levels required for animals and plants in seas