ES1001 Flashcards

(325 cards)

1
Q

What is Earth’s geographical column?

A

om locality to locality around the world, geologists have pieced together a composite stratigraphic column that represents the entirety of Earth’s visible history

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2
Q

Relative vs. numerical age:

A

The age of one feature relative to another is known as its RELATIVE AGE. The age of a feature given in years is its NUMERICAL AGE

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3
Q

What is radioactive decay?

A

When isotopes undergo a conversion into a different element (Bonus point: In half life)

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4
Q

What is Geochronology?

A

We investigate the what, when, and how of planetary-scale of a process

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5
Q

What is a seismic wave?

A

Rupture of intact rock or frictional slip along a fault produces seismic waves (and earthquakes), these move outward in all directions

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6
Q

What density of rock will make p-waves travel at an increased velocity?

A

Denser rock, such as igneous
(Example: peridotite vs sandstone)

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7
Q

Do seismic waves travel faster or slower in solids? In comparison to liquids

A

They travel faster through solids

(Example: they move more slowly in liquid than solid rock)

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8
Q

Can s-waves go through liquid?

A

both P- and S-waves can travel through solids but only P-waves can travel through liquid

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9
Q

When do seismic waves refract?

A

Seismic energy as waves will reflect and/or refract when reaching the interface between two layers of rock of differing compositions and/or densities

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10
Q

Define a rock
(Like no seriously…)

A

A naturally occurring and consolidated material usually comprised of one or more mineral phases

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11
Q

What rock type is igneous

A

Something which directly crystallised form a liquid rock (melt)

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12
Q

What rock type is sedimentary

A

Bits of other rocks in one place

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13
Q

What rock type is metamorphic

A

Cooked rocks

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14
Q

Why do sedimentary rocks form at or near the Earth’s surface?

A

Cementation of grains and/or fragments derived from pre-existing rocks

Precipitation of minerals from water solutions

Growth of skeletal material in organisms

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15
Q

What is weathering

A

The processes that break up and corrode solid rock, eventually transforming it into sediment

Physical weathering breaks rocks into unconnected grains or chunks

Chemical weathering refers to the chemical reactions that alter or destroy minerals when rock comes into contact with water solutions or air

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16
Q

Fun fact!!
(Lemme have fun jeez… flip!!)

A

Sedimentary Rocks are sometimes made of dead things

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17
Q

How are metamorphic rocks formed?

A

A rock that forms when a pre-existing rock (igneous or sedimentary) is affected by changes in its physical or chemical environment

include variations in temperature (T) and pressure (P), these changes result in the growth of new minerals and textures

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18
Q

What is ‘plate tectonics’

A

The lithosphere is divided into 15-20 plates of varying sizes

The plates move relative to each other

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19
Q

Explain a ‘hot spot’

A

Isolated volcanic centres far away from plate boundaries, many lie at the end of a chain of extinct volcanic islands and seamounts known as a hotspot track

hot spot tracks are thought to be the result of plates moving over stationary plumes

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20
Q

Why do we study minerals?

A

They make up everything, the majority of Earth, any rock is an aggregate of two or more mineral grains.

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21
Q

Definition of a mineral

Aka the web of lies

A

A mineral is a crystalline, homogenous, inorganic solid with a defined chemical composition that occurs naturally

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22
Q

Explain the minerals crystal structure

A

Their building blocks (atoms, ions, molecules) are arranged in an ordered and repeated pattern.

The unit cell is the smallest unit that still has the full symmetry of the crystal structure of a material.

Repeating the unit cell over and over again forms a crystal.

The ordered atomic network within a crystal can be simple or fairly complex.

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23
Q

What is a mineraloid?

A

Some minerals are not (fully) crystalline. These are called mineraloids.

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24
Q

Explain why crystals SHOULD be homogenous

A

Following from the infinitely repeatable unit cell of the crystal structure, minerals should by definition be homogenous

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25
What may be the cause of a non homogenous mineral?
Zonations and crystal defects
26
What are the examples of an organic 'mineral'
Biominerals - formed by a living organism usually inorganic in composition may contain organic material Amber - fossilised tree resin organic composition
27
What is a polymorph?
Minerals with the same composition but different crystal structure
28
What is coordination?
The number of direct neighbours that an atom/ion is bonded to in a crystal structure. Typically we talk about cations and their surrounding anion-neighbours.
29
What is coordination?
the number of direct neighbours that an atom/ion is bonded to in a crystal structure. Typically we talk about cations and their surrounding anion-neighbours.
30
What is a site?
A space in a crystal lattice that can be occupied by an atom/ion. It is typically named by its coordination.
31
What is compatibility?
Atoms/ions in a crystal lattice can be substituted by other elements, as long as their radius is similar. Ideally, their charge would also be the same! If an element fits readily into a crystal structure, it is called compatible
32
Nesosilicates
Island silicates  Consist of isolated “islands” of [SiO4] 4– tetrahedrons.
33
Sorosilicates
Group silicates  Two SiO4-tetrahedrons can share one oxygen and form a group
34
Cyclosilicates
Ring silicates  When a SiO4-tetrahedron shares two of its oxygen corners, we can form rings
35
Inosilicates
Chain silicates Like an unclosed ring, sharing two oxygen corners creates chains
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Phyllosilicates
Sheet silicates Sheets of Inosilicates
37
Tectosilicates
Framework silicates
38
What is ‘plate tectonics’?
The lithosphere is divided into 15-20 plates of varying sizes The plates move relative to each other
39
Hot Spots?
Isolated volcanic centres far away from plate boundaries Many lie at the end of a chain of extinct volcanic islands and seamounts known as a HOT SPOT TRACK Hot spot tracks are thought to be the result of plates moving over stationary plumes
40
Defniton of a mineral?
A mineral is a crystalline, homogenous, inorganic solid with a defined chemical composition that occurs naturally
41
How d minerals have a crystalline structure?
Their building blocks (atoms, ions, molecules) are arranged in an ordered and repeated pattern. Aka repeating he UNIT CELL
42
What a a mineral which isnt fully crystalline?
Mineraloid
43
What is a polymorh?
Polymorphs are minerals with the same composition but different crystal structure.
44
How do minerals form
crystallisation of a magma due to cooling effectively the same as freezing Magma cools below its liquidus, and starts to crystallise minerals. The mix of melt + minerals keeps on crystallising until it ”hits” the solidus, now all melt has solidified
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1. Elements
Pure elements, metals often called “native”... usually bound by metallic (in metals) or covalent bonds
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2. Sulphides
Minerals that have sulphur as anion.
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3. Halides
Minerals with halogens (F, Cl, Br, I) as anion.
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4. Oxides/ Hydroxides
Minerals with oxygen and/or OH as anion.
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5. Carbonates
… with the carbonate ion (CO3) 2- as anion.
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6. Borates
… with the borate ion (BO3) as anion.
51
7. Sulphates
with the sulphate ion (SO4) 2- as anion.
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8. Phosphates
… with the phosphate ion (PO4) 3- as anion.
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9. Silicates
Form 90% of Earths crust Si and O as anions
54
Building silicates
SiO4 tetrahedredreon 1 Si with 4 O- atoms Si4+ (+) 4o^2- makes [siO4]4^4-
55
Neosilicates - Island silicates
consist of isolated “islands” of [SiO4]4– tetrahedrons. Since a mineral cannot be charged, we have to balance the quadruply-negative charge. A charge balance can be achieved by throwing cations in the mix.
56
nesosilicates - island silicates EXAMPLE
Olivine achieves charge balance by adding two divalent cations per [SiO4]4– island. It can be either Mg2+ or Fe2+ → (Mg,Fe)2SiO4
57
Sorosilicaties - group silicates
Two SiO4-tetrahedrons can share one oxygen and form a group: 2 Si4+ + 7 O2- makes [Si2O7]6-
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Sorosilicates-group silicates EXAMPLES
Zoisite
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Cyclosilicates - ring silicates
When a SiO4-tetrahedron shares two of its oxygen corners, we can form rings Depending on the number of rings, we get different molecular anions, with different charges… But always a multiple of Si4+ + 3 O2- → [SiO3]2-
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Cyclosilicates - ring silicates EXAMPLES
Tourmaline, Beryl
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Inoslicates - chain silicates
Like an unclosed ring, sharing two oxygen corners creates chains 2 Si4+ + 6 O2- → [Si2O6]4-
62
Inosiliictes - chain silcates EXAMPLES
Pyroxenes have two slightly different cation-sites in their lattice M2 (larger cation site) M1 (smaller cation site) e.g. Augite Amphiboles … are complicated and have a lot of cation-sites, but are a common mineral
63
phyllosilicates - sheet silicates
Every SiO4-tetrahedron shares three of its corner oxygens Si4+ + 1O2- + 3*½O2- = SiO2.5 = [Si4O10]4-
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phyllosilicates - sheet silicates EXAMPLES
Micas
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Tectosilicates - framework silicates
Every SiO4-tetrahedron shares all four of its corner oxygens Si4+ + 4*½O2- = SiO2 = [SiO2]0 - No charge!
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Tectosilicates - framework silicates EXAMPLES
Quartz is a very happy chappy, doesn’t need any cations to charge balance and therefore usually is very pure. Formula: SiO2
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Composition of a mineral
Heavy element = heavy mineral (duh)
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Packing
More atoms = more dense Like more socks = more dense suitcase Relative estimates
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Colour
colour as a result of interaction with (sun)light (Sunlight = white light contains all wavelengths of the visible spectrum)
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Colour WARNING!
Small changes in a crystal can change the way it interacts with light. (e.g amethyst, quartz, citrine)
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Streak colour?
We can powder” a mineral by grinding it against a hard and rough surface, like an unglazed ceramic tile.
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Transparency
Describes whether a material allows light to pass through.
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Lustre
How a mineral reflects Just make up your own words
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Twinning
Twinning describes the intergrowth of two (or more) crystals of the same mineral through a slight change in orientation of the crystal lattice.
75
Double refraction
Technically the majority of transparent and translucent minerals double-refract light; CALCITE is so very slay that u can see double
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Photo - Luminescence
In some minerals, absorbing (high-energy) light results in the emission of (visible) light.
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Fluorescence
The light emission stops when the high-energy light stops
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Phosphorescence
The light emission can continue for some time after the excitation stops
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Magmatism
Magnetite is magnetic
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Taste
Salty stuffs Halite tastes salty. It is table salt after all. Sylvite tastes salty, too, but has a bitter aftertaste.
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7 crystal system SHAPES (teigan terms dw)
Cube Chip Matchbox Pencil Triangular prism Flattened matchbox sidey-ways Stack of cards pushed askew in two directions
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7 crystal TERMONOLOGY
cubic tetragonal orthorhombic hexagonal trigonal monoclinic
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What is metamorphism
The mineralogical and structural adjustment of solid rocks to physical and chemical conditions that have been imposed at depths below the near surface zones of weathering and which differ from conditions under which the rocks in question originated.
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What are the key factors of metamorphism
The precursor rock Pressure Temp Deformation
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Where does the heatcome from within metamorphism
Conduction (mantel) Advection (magma/hot fluid) Radioactive decay ( U, Th, K etc) Temps of 250 to >1000°C
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Where does pressure come from with metamorphism
Overlying rock mass Horizontal tectonic forces Pressure= fore per unit Lithostatic pressure = density x gravity x height
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Why do newminerals grow?
More stable at better conditions Determined by thermodynamics Thus, thermodynamics determines which collection of minerals have thelowest energy for a particular rock composition, pressure and temp
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Regional metamorphism
Due to burial Occurs with deformation Occurs over large areas Called belts Shows continental collision (therefore mountain ranges) Occurs formulations to 10s of millions of years
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Contact deformation
Localised heat sources Occurs around large igneous intrusions (dominated by heating n cooling) Occurs oversmaller areas Area around the intrusion is called the contact aureole Short-lived
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Hydrothermal metamorphism
Ocean floor basalts interact with hot fluids The basalt is metamorphosed
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Impact metamorphism
This occurs when you drop a huge rock from space (meteorite) onto the earth. ¨ Enormous transient pressure and temperature changes ¨ Very short lived - seconds-days ¨ Also called shock metamorphism ¨ Pressure from the impact (force per unit area) ¨ Temperature from friction
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Fault related metamorphism
Related to brittle or ductile deformation in faults and shear-zones Intense deformation allows new minerals to grow ¨ Sometimes friction can provide additional heat Commonly associated with hydrothermal metamorphism
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Metamorphic rocks are classified in general on their appearance ¨ This is controlled by:
Composition P and T conditions Deformation
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Features of metamorphic rocks! Inherited features
Eg bedding in metamorphosed sediments Eg large igneous crystals from metamorphosed igneous rocks
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Features of metamorphic rocks! Metamorphic features
Minerals of different sizes
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Features of metamorphic rocks! Metamorphic and deformation features
Distinct layers Aligned grains (preferred orientation) Folds
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Metamorphic fabric and structure
Layering Alternating layers of different compositions May include inherited features such as bedding Foliation A planar feature in a rock defined by the preferential orientation of mineral grains Lineation A linear feature in a rock defined by the preferential orientation of mineral grains
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Crenulations
Small scale folds
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Porphyroblasts
Metamorphic rocks may have some garians that are much bigger than the average grain size
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Porphyroclasts
In FAULT related rocks they are metamorphic rocks may have some garians that are much bigger than the average grain size
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Phenocrysts
The big grains in igneous rocks
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Matrix
The finer-grained minerals that host the porphyroblasts are collectively referred to as “matrix”
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Matrix minerals
Individual minerals are called “matrix minerals”
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Using structure no foliation
No foliation ¨ Hornfels ¨ Granofels
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Using structure with foliation/lineation
Foliation/lineation ¨ Slate ¨ Phyllite ¨ Schist ¨ Gniess ¨ Layered or banded gneiss & Migmatite
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Using structure- intensely foliated
Intensely foliated and sheared rocks ¨ Mylonite
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What is a metamorphic assemblages
Is those minerals that appear to co-exist stably in a rock ¨ i.e it is a list of minerals AKA Christmas rock Garnet-clinopyroxene(omphacite)-quartz Metamorphic assemblages are important for constraining metamorphic grade (Pressure & Temperature)
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What is a metamorphic facies
any two rocks with the same chemical composition that are metamorphosed at the same P-T conditions will contain the same minerals in the same proportion ¨ This is governed by thermodynamics ¨ We can use common rock types to define broad P-T regions based on the mineral assemblage they contain These broad P-T regions are called metamorphic facies Metamorphic facies can also be determined using other rock types such as metapelites
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What are the 5 main metamorphic facies
¨ Greenschist facies ¨ Amphibolite facies ¨ Granulite facies ¨ Blueschist facies ¨ Eclogite facies
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What is metamorphic evolution
As metamorphic rocks occur at the surface today, they must also experience a period of cooling after metamorphism ¨ We can divide the metamorphic evolution into parts based on whether T is increasing or decreasing T increasing prograde T highest peak T decreasing retrograde
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P-T pathways
The tall, elongated, clockwise path is characterised by deep burial and exhumation with limited heating The shorter, rounder clockwise red path is represents both substantial burial and heating
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What is a metamorphic zone (zonen)
In contact metamorphism there is a strong temperature gradient away from the intrusion ¨ This results in changes in mineral assemblages away from the intrusion
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What is a metamorphic isograd?
Some regional metamorphic belts show a consistent change in minerals across them. ¨ The appearance of a key mineral can be mapped in as an isograd. Each metamorphic zone is separatrated by an isograd
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Whatis continental collision in metamorphism
The most important metamorphic environment If metamorphism occurs when continental plates collide then ancient metamorphic belts show us how and when the continents were assembled into their current configuration
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Ocean subduction I metamorphism
If metamorphism occurs in subduction zone then some metamorphic belt tell us where old subduction zones were
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Metamorphic - Diverent plate boundaries
Plates move apart ¨ This is where new oceans form if the process continues
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Metamorphic - transform plate boundaries
Plates slide laterally ¨ May involve a component of extension (transtension) or compression (transpression)
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Metamorphic- convergentplate boundaries
Plates collide ¨ If one or both of the plates is oceanic then subduction occurs ¨ If both are continental then continental collision occurs
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Orogenesis
Building mountains Mountains represent crust/lithosphere that has been thickened ¨ Sometimes to more than double its normal thickness ¨ Thickened crust is not stable, but occurs because of tectonic forces Mountains are controlled by isostacy (the iceberg effect) ¨ The higher the mountain the thicker the crust/lithosphere
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Examples of continental collision
Alps and himalayas
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Regional metamorphism - With regards to subduction
Here we have subduction causing continental collision. There is defm & thickening due to the applied stresses
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Subduction zones and island arcs
Two types Ocean-ocean ¨ Makes island arcs ¨ Eg Japan Ocean-continent ¨ Makes continental volcanic arcs and mountains on the continental margins ¨ Eg the Andes These may evolve into collision zones
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Subduction metamorphism
Subduction involves high pressures. SO the rocks formed in subduction zones are blueschists and eclogites During burial and heating the rock experiences prograde metamorphism. The prograde reactions release water which enters the hot mantle. This water can initiate melting of the mantle: also melting of the slab can occur
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Metamorphic - volcanic arcs
The large input of magma heats and thickens the arc crust Arcs are very hot environments Get high T at relatively shallow depths Very high temperatures common in the lower half of arc systems High temperature-low pressure metamorphism due to magmatic heat
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Explain the biosphere structure
Living organisms (biota) and non-living (abiotic) factors from which they derive energy and nutrients
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What are the two Geobiological energy sources?
Phototrophy and Chemotrophy
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What is an autotroph
Primary Producers: build organic matter by fixing carbon Provide most organic carbon for the biosphere Cyanobacteria
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What is a Heterotrophs
Cannot fix carbon to form their own organic compounds. Consumes organic compounds/primary producers
129
Energy flow in ecosystems
The biosphere is an open system with regards to energy → energy flow upwards in a food pyramid is inefficient, and relies on continued primary production
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What is the residence time? (Equation)
Mass of substance -------------------------- = residence time (10^12kg/year = GtC) of carbon Flux (in or out of)
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What is a feedback?
A feedback is a self-perpetuating mechanism of chang
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What is negative feedback?
diminishes disequilibrium to maintain a steady state
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What is positive feedback
enhances the effects of perturbation and drives the system further from equilibrium.
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Organic stored carbon
Terrestrial: Coal (land plants in anoxic swamps) Marine: Petroleum in shales (phytoplankton debris)
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Inorganic stored carbon
Carbonates; limestone, aragonite, chalk etc
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What is geobiological weathering
Bicarbonate produced by weathering of both carbonates and silicates
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The Archean (Geobiology)
Single cellular life; chemotrophs and/or non photosynthetic phototrophs Stromatolites: oldest unambiguous fossils at 3.4 Ga. Microbial mats formed of cyanobacteria (modern examples) and interleaved sediments.
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The Proterozoic (Geobiology)
True multicellularity has only ever arisen among the eukaryotes Results in: • Specialised cells • Increase in size • Increased morphological diversity • Sexual reproduction
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Whatis biomineralisation
Largely calcium carbonate plus silica and phosphate Likely as a response to predation→ modern food webs
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What waste Cambrian Explosion
Rapid diversification in body plans, particularly Bilatera • Divergence of nearly all extant phyla • Expansion in mode of life: burrowing, active swimming, pelagic
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Mesozoic Life (Geobiology)
Rapid diversification after the P-T mass extinction Rise and dominance of the dinosaurs! + grass + flowering plants
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Cenozoic life
Loss of dinosaurs following the K-T mass extinction Rapid diversification and dominance of mammals
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The end-Permian “P-T” mass extinction
Largest know mass extinction: occurred in two waves at ~252 Ma ~90 % of marine species and ~70 % of terrestrial vertebrates lost Siberian Traps: giant volcanic eruption coincident with the P-T extinction Dust, volcanic gases (SO2; CO2), intruded into coals → Global Warming Ocean acidification, enhanced weathering and eutrophication-induced “super”anoxia
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The end-Cretaceous (“K-T”) mass extinction
Impact at Chicxulub: resulted in 180 km diameter crater. Iridium (+other PGE) spike, shocked quartz, glassy beads (ejecta spherules) Impacted anhydrite or gypsum → massive sulphur release
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Glaciation for energy resources
Hydroelectric power from glacially fed catchments is a major source of energy in some regions British Columbia, Canada: >85% of electricity from hydropower, and in summer 50% of water supplied by glaciers
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What is an ice sheet
Largest masses of ice, covering huge countries or continents such as Antarctica and Greenland Characterised by a slow-moving interior plateau and fast-moving edges forming outlet glaciers or ice streams 1-3km thick! Melting would cause 70 m of sea level rise
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What is an ice shelf
Large areas of floating ice in embayments or along the margins of an ocean basin, fed by ice streams from a neighbouring ice sheet e.g., Antarctic margin
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What is the cryrosphere
Its the frozen part of Earth and the most susceptible to anthropogenic climate change • Important for controlling global sea level
149
Whatis an ice cap
Smaller accumulations of ice covering high topography or high latitude regions, characterised by radial flow outwards from the centre
150
What is sea ice?
Freezing of sea water at high latitudes Sea ice extent has been declining in recent decades due to climate change
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What is permafrost?
Freeze-thaw activity within the upper “active layer” produces patterned ground structures such as icewedge polygons and pingos
152
What is patterned ground?
regular pattern of circles / polygons formed in active layer due to cyclical freezing and thawing of water in the pore spaces and frost heaving
153
Whatis a pingo?
Small hills of earthcoveredice that form by expansion of pore water through the active layer as a result of pressure from expanding permafrost underneath
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What is a cirque (corrie) glacier
smallest – found in cirque (bowlshaped depression on side of mountain formed by glacial erosion)
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What is a valley glacier?
A cirque glacier that expands outward and downward into a valley
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Whatis a fjord glacier?
When a glacier valley is partly filled by an arm of the sea, the valley is called a fjord, and the glacier is a fjord glacier Bits fall off to cause icebergs
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What's a piedmont glacier
Forms when valley glacier spreads out onto lowlands
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Formation of sea ice
• Air temperature falls below freezing point of salt water • Consists of freshwater as salt is excluded from ice crystals as they form • First ice to form consists of small crystalline needles: frazil ice (pure H2O) • As more crystals form they produce a viscous mixture at the ocean surface, eventually freezing together to make continuous ice cover • Cold air no longer in contact with seawater and so sea-ice growth then proceeds by addition of ice to base • Melting, sublimation removes ice from surface • But loss at surface compensated by ice crystals added to the base
159
Sea ice Zonations Perennial sea ice:
The sea ice that persists for multiple years • In Arctic, just north of Resolute Bay: can be 3-4 m thick and decades old • In Antarctic, confined to semi-enclosed seas (Ross, Weddell): can be 5 m thick, but <5 yr old
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Sea Ice Zonations Seasonal sea ice
sea ice cover that varies annually • Cause of variation in extent varies between Arctic and Antarctic • Arctic: warmer air temperatures is major factor in retreat of the ice margin • Antarctic: warmer ocean temperatures is major factor in retreat of the ice margin
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Glacier formation - from snow to ice
Compaction by overlying snow • Air penetrates pore space and evaporation occurs at points of snowflakes • Moisture freezes between points, near center • Formation of granular snow called FIRN, intermediate stage between snow and glacial ice • Snow gradually loses interstitial air to become glacier ice
162
Glaciers brittle upper layer
Top 50 m of glacier is brittle –does not flow because has relatively little weight on it • Crevasses form in top layer as glacier bends over topography (e.g., an abrupt change in slope) • Provide a conduit for meltwater from surface to get to depth in glacier through englacial channels • Meltwater can also percolate through firn layer
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Glacier surges
Some glaciers undergo periodic surges – rapid advances • Several kilometres per year • May be related to buildup of water at base
164
Glacial erosion
Mechanisms: • freeze-thaw at base of glacier • abrasion • plucking
165
The oceans general knowledge
Cover 70.8% of the Earth’s surface, Contains 97% of the Earth’s water, Have an average depth of 3.6 km.
166
Oceanic crust
Oceanic crust is denser than continental crust, The light thick continental crust floats higher on the mantle than the dense thin oceanic crust
167
Ocean lectures - spreading and subduction
Sea floor spreading creates mid-ocean ridges Subduction creates deep ocean trenches
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What pattern is seen within nutrients in the oceans
Dissolved nutrients to support primary production are low in surface waters and then regenerated at depth.
169
Impacts of ocean stratification
inhibits the vertical mixing of ocean waters, preventing dissolved nutrients being transported back to the sea surface.
170
Effect of mixing within the ocean
Storm mixing and tidal mixing in shelf seas breaks down seasonal stratification
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How are ocean basin formed?
Plate tectonics
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How are continental slopesare shelfs produced
Water overfills the basins and spills onto the continental crust
173
How are shelf seas important in oceanic environments
Shelf seas are important for primary production and carbon storage
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What can affect ocean circulation
Ocean features (seamounts, islands, plateau, trenchs)
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What is Eckman Transport?
Eckman Transport is the deflection of surface waters in the upper 100m of the water column, as a result of the Coriolis Effect. Surface waters are deflected 90° to the right in the northern hemisphere and 90° to the left in the southern hemisphere.
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What is Grye circulation
Winds create drag on the surface waters, setting them in motion The Coriolis effect deflects surface waters to the right in the Northern hemisphere, so oceanic gyres rotate in a clockwise direction. The opposite occurs in the Southern hemisphere.
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The density of surface seawater is sufficient to cause sinking at two general locations:
The North Atlantic The Weddel Sea (Southern Ocean) Together, temperature and salinity drive the thermohaline circulation of the oceans
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How can we detect water masses?
Depth profiles of temperature and salinity
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What can drive surface currents?
Wind
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Whare does the Coriolis Effect divert current
To the right in the N Hemisphere and the left in the S Hemisphere
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How do deep ocean waters form?
From high density waters
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Wind generated gravity waves:
Wind stress creates small ripples in the water's surface. Now there is a pressure difference between the front and back of the wave. The front face is sheltered from the wind and experiences a lower air pressure than the back face, which faces the wind. This pressure difference pushes the wave along.
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Importance of waves
Water mixing (e.g. shelf sea stratification Sustainable energy source Shipping hazard Erosion/deposition of sediments Sea level changes
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What is an amphidromic point?
Points with no tide
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What is a Guyot?
A flat topped volcanic mountain
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What is a Seamount?
Underwater mountain (usually volcanic)
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Implications of sea level change
Changes in shelf sea area affect primary production, ecosystem distribution, carbon transport etc. Changes in sea level affect tidal dynamics in shelf seas and the global ocean
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What is tidal dissipation
The loss of the energy of tidal i.e. moon generated, waves
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How can we reconstruct sea level?
Using the and age of fossil coral reefs
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What are the common marine pollution issues
Metals Organic chemicals Oil Contaminants of emerging concern Nutrients Plastic Noise
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How are PBCs in the Marianas trench?
These PCBS are probably incorporated into particulate material at the ocean surface which then sinks to the ocean bottom to deliver the contaminant.
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What is a Roche Moutonnee
Rock formation created by the passing of a glacier. The passage of glacier ice over underlying bedrock often results in asymmetric erosional forms as a result of abrasion on the "stoss" (upstream) side of the rock and plucking on the "lee" (downstream) side
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Erosional Glacial features Striations and chatter marks
Striations: Produced by small rock fragments embedded in basal ice that scrape away at the underlying bedrock and produce long parallel scratch marks Chatter marks: A series of often crescent-shaped gauges chipped out of the bedrock as a glacier drags rock fragments underneath it
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Corries!!
Among the most common and distinctive landforms produced by glacial erosion Bowl-shaped valley formed at glacier head Coire Sgorach on Sgurr a’ Mhaim is a classic northfacingcorrie eroded by a small cirque glacier high on the mountain face during successive glaciations of Scotland
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U shaped valleys
Originates in a corrie, U-shaped (duh) Higher geo
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Aretes
Sharp-edged, narrow ridge of rock separating two valleys Formed when two oppositefacing glacial cirques erode headwards towards each other Also formed when two valley glaciers erode parallel Ushaped valleys Edge is sharpened by freezethaw weathering, and slope is steepened through mass wasting events and erosion Svalbard!
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Glacial horns / pyramidal peaks
Pointed pyramidal peaks formed from cirque erosion due to multiple glaciers diverging from a central point A classic example is the Matterhorn in the Swiss/Italian Alps A Scottish example is Carn Mor Dearg
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Hanging valleys
Tributary valley well above main valley floor: typically formed when main valley has been widened and deepened by glacial erosion, leaving the side valley abruptly cut off from main valley Steep drop-off usually creates dramatic cascading waterfalls Coire a’ Mhail and Coire Giubhsachanare both hanging valleys, with steep drops at the end into Glen Nevis below
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Glacial erosion mechanisms
freeze-thaw at base of glacier abrasion plucking
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Till
Sediment deposited directly by a glacier is neither sorted nor stratified Heaps of poorly sorted sediment called till are left as glaciers abate
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Outwash
Till can be then reworked by meltwater streams that transports it beyond terminus of glacier where it is deposited as outwash
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Moraines
Ridge-like accumulations of till are moraines Form as sediment is bulldozed by a glacier advancing across the land End moraines form at the terminus of a glacier, with the terminal moraine marking its furthest advance (Longyear glacier, Svalbard) Lateral moraines form at the sides (Lars, Svalbard) Medial moraines form where two glaciers join Moraines are important tools that scientists use to determine the extent of ice coverage during an ancient glaciation
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Drumlins
Ice sheets mold oval hills called drumlins Drumlins are elongated parallel to the direction of ice flow Formed by glacial ice acting on underlying unconsolidated till Streamlined hills shaped beneath the ice Common in the central lowlands of Scotland, between Glasgow and Edinburgh
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Eskers
Rivers flowing beneath ice (subglacial channels) leave ridges of wellsortedsand and gravel called eskers
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Kettles
Shallow, sediment-filled body of water formed by retreating glaciers or draining floodwaters Form as a result of blocks of ice calving from glaciers becoming submerged in the sediment in outwash plain, which then melt to produce a void filled by a sediment-rich lake Landscapes marked by kettles, now typically occupied by lakes, ponds, or wetlands are clear evidence of previous glaciation
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Kames
Kames are an irregularly shaped hill or mound comprised of piles of sand, gravel, and till that accumulates in a depression on a retreating glacier and is then deposited on the land surface with further melting of the glacier
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Marine ice sheets
The Marine Ice Sheet needs to be heavy (thick) enough to displace the water to be grounded. Ocean warming can melt the ice sheet faster than it moves out to sea thinning the Ice Sheet.
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Marine ice cliff instability
Positive feedback whereby the cliff face can become unstable if not supported by the buttressing effects of ice shelves Leads to rapid ice margin retreat
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Isostatic rebound - mantle movement
Viscous mantle flows away from depressed crust under the huge weight of a mountain chain
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What is a rock?
Crystals of one or more minerals bound together in a mixture
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Pumicevs pyroclastic
pumice –very frothylight-colouredcellular rock, full of interconnected gas bubbles pyroclastic rock formed from fragments of chilled magma pyroclastic = fiery fragments
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Decompression (adiabatic) melting
Mid-ocean ridges Decompression melting forms mid-ocean ridge basalt (MORB) Continental rifts e.g. East Africa Over time, will become an ocean Mantle plumes e.g. Hawaii Both increased heat flow and decompression Forms ocean-island basalt (OIB)
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Volatile-assisted melting
Changing the chemical composition of the system If you add volatiles to Earth’s mantle (H2O, CO2) you lower its melting temperature
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Explain cooling time regarding texture n Grain size
More cooling time means: -coarser -larger grains
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What is a porphyritic
A fine matrix with larger crystals
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Batholith
Huge mass of intrusive rock made of numerous plutons
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Dyke
Vertical igneous intrusions to layering
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Sill
Horizontal igneous intrusions to layering
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What is a felsic rock
High silica content Lighter in colour
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What is a mafic rock
Low silica content Darker rocks
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What is bowens reaction
Mafic minerals crystallise First Felsic are last to Remaining melt becomes more felsic Yet it can also work in reverse
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Mid ocean ridges- constructive margin - igneous
Melting style Opening of plate boundary above mantle creates void = mantle moves up to fill void Melting occurs via decompression
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Subduction zones- destructive margin- igneous
Melting style Hydration of mantle above subducting plate Melting occurs via volatile introduction (flux melting) Mt. Fuji
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Continent - Continent collision - igneous
Source of (original) melt: crust Sediments, metamorphic rocks, igneous rocks Often melt is too viscous and deep enough in crust, so it does not escape Forms granite plutons/batholiths
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Continental rift - igneous
Melting style: decompression Source of (original) melt: mantle Majority of melt is mafic Some remelting of crust produces felsic volcanoes –BIMODAL volcanism
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Flood basalts
Vast eruptions of basaltic lava Associated with the initial impingement of a mantle plume under a plate – often continental Can start the breakup of continents – start rifting by weakening/thinning the plate HUGE fissure eruptions of basalt
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What is a lava flow
molten rock that moves over the ground
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What is a pyroclastic debris
fragments blown out of a volcano
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What is volcanic gases
Expelled vapor and aerosols
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What determines magmatic flows
1. Composition of melt 2. Crystal content 3. Gas content 4. Temperature
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Physical properties of magma
Temperature Increasing temperature decreases the viscosity Crystal content The present of crystals in a melt acts to increase the viscosity of a melt Gas content If the gases are dissolved, the will act as network modifiers (decrease viscosity) If the gases exsolve, they will form bubbles which act against the flow
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Volcanic gas
Magma composition often controls gas content. • Felsic magmas have more gas; mafic magmas less. • Gases are expelled as magma rises (P drops). • Style of gas escape controls eruption violence. • Low viscosity (basalt)—easy escape; effusive eruption • High viscosity (rhyolite)—difficult escape; explosive release • Gas bubbles in rock are called vesicles.
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Lava flow (viscosity) depends on:
• Composition, especially silica (SiO2) content. • Temperature. • Gas content. • Crystal content
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Effusive lava flows
Mafic magma – low viscosity, efficient degassing Andesitic magma – medium viscosity Rhyolitic magma – high viscosity, does not flow – forms domes
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Basaltic lava flows
Mafic lava—very hot, low silica, and low viscosity • Basalt flows are often thin and fluid. • They can flow rapidly (up to 30 km per hour). • They can flow for long distances (up to several hundred km). • Most flows measure less than 10 km. • Long-distance flow facilitated by lava tubes.
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Andesitic lava flows
Higher SiO2content makes andesitic lavas viscous. • Unlike basalt, they do not flow rapidly. • Instead, they mound around the vent and flow slowly. • The crust fractures into rubble, called blocky lava. • Andesitic lava flows remain close to the vent.
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Rhyolitic lava flows
Rhyolite has the highest SiO2; is the most viscous lava. • Rhyolitic lava rarely flows. • Rather, lava plugs the vent as a lava dome. • Sometimes, lava domes are blown to smithereens.
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Volcaniclastic deposits
Volcanoes often erupt large quantities of fragments. Volcaniclastic deposits include: • Pyroclastic debris—lava fragments (of all sizes) that freeze in air. • Preexisting rock—blasted apart by eruption. • Landslide debris—blocks that have rolled downslope. • Lahars—transported as water-rich slurries.
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Pyroclastic debris
Explosive eruption: Melt, crystals and ‘country’ rock (lithic) fragments are fragmented fragmented = blasted apart …and blown from the vent
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Explosive eruptions - felsic
Andesitic or rhyolitic eruptions • More viscous magmas; more volcanic gases • Less easy to de-gas = more prone to explode • Explosive eruptions generate huge volumes of debris. • Pumice—frothy volcanic glass • Ash—fragments less than 2 mm in diameter • Pumice lapilli—angular pumice fragments • Accretionary lapilli— rounded clumps of ash forming in moist air
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Pyroclastic eruptions Different eruptive styles
Pyroclastic fall (ash or tephra deposit) Pyroclastic flows Pyroclastic surges
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Pyroclastic eruptions Fall
Fallout from an eruptive column/cloud Falls like snow – mantles topography
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Pyroclastic eruptions Flow
Avalanches of hot ash (200oC to 450oC) that race downslope. Moving up to 300 km per hour, they incinerate all in their path. Immediately deadly; they kill everything quickly. Many historic examples: Mt. Vesuvius, Mt. Pelee, Mt. St Helens Block and ash flows - Ignimbrites welded by heat of flow
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Pyroclastic eruptions Surges
Like a pyroclastic flow, but denser (wetter) Very energetic eruptions Generally colder, lots of water
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Incoming energy flux
Earth receives more energy from sun (electromagnetic waves) Seasons due to Earth's xis rotation causing a tilt 30% of solar energy is affected by albedo effect
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Outgoing energy flux
Earh has an approximate energy balance, energy is returned as blackbody radiation Stefano- Boltzman law: ōT⁴ W/m² (ō is a constant)
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Earth's energy budget
Atmosphere and ocean move because equator receives more energy from sun than it emits
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Combining incoming and outgoing radiation
To close earth's energy budget, the atmosphere and ocean need to move energy from low latitudes to high lattitudes
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Energy/heat transport
We must transport polewardsas we receive more at equator
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What does hydrostatic balance tell us
Pressure decreases with altitude at a rate dependant on temperature
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What does geopotential height depend on
Depends on the temperature integrated between the surface and that level
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Air density with temp
Warm air is less dense
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Chemical composition of the atmosphere
78% N2, 21% O2, 0.93% Ar and others
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Ideal gas law
p = pRT
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Water saturation in atmosphere
When air cannot hold any more water vapor, its saturated , to get air to condense and firm mist, fog, clods and rain, it must cool to saturation
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Atmospheric phenomena
We want to understand this for fundamental scientific discoveries and practical purposes
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What is an easterlies wind??
Comes from east
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What is an westerlies wind??
Comes from west
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What is an notherlies wind??
Comes from north
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Volcanic rock types at the rock and spindle
1. Intrusive - igneous, fine grained basalts 2. Bedded tuffs - pyroclastic deposits, fallen back into vent 3. Tuffisite, ash rich veins that never got to the surface
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Sedimentary rocks
formed on or near Earth’s surface via erosion, deposition and lithification of sediment transported by water, ice and wind or precipitated out-of-solution by biotic and abiotic processes
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Classification of sedimentary rocks
clastic: composed of fragments (clasts) of pre-existing minerals/rocks (i.e. a source area or provenance) non-clastic: (bio)chemically precipitated clastic rocks and non-clastic rocks commonly occur together
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Classifying clastic sedimentary rocks
conglomerate versus breccia: both consist of gravel-sized sediment but their grain shapes are different, rounded vs angular, respectively weathering and erosion of ‘parent’ rocks determines composition of resulting sediment intensity, duration and ‘style’ of sediment transport processes determines the texture of the sediment
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Concept of 'maturity'
As sediment undergoes increasing intensities and durations of weathering and transport, it begins to ‘mature’: •mafic minerals and feldspars breakdown into finer particles and clays •quartz becomes more and more enriched •sediment becomes better sorted and grains more rounded
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Evolution of sedimentary rocks
Source (provenance) Weathering and transport Site of deposition Lithification occurs and the resulting sedimentary rock is classified based on its composition and texture
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Non clastic sedimentary rocks
non-clastic sedimentary rocks are precipitated by organisms or abiotically temperature, salinity, water chemistry and sediment flux (needs to be low) influence precipitation chemical sediments are good indicators of environmental conditions there are numerous types of (bio)chemical sediments: coal, carbonates, evaporites and siliceous precipitates
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The order that mineral salts precipitated by (increasing) evaporation
Calcite Gypsum Halite Potassium
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compositional classification of (bio)chemical sedimentary rocks is typically based on the major anion carbonates (CO3-)
CaCO3 – calcite (aragonite polymorph is metastable); forms limestone*^ (Ca)Mg(CO3)2 – dolomite; forms dolostone* Fe2CO3 – siderite *can form abiotically or biotically ^fizzes with weak HCl (acid)
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compositional classification of (bio)chemical sedimentary rocks is typically based on the major anion sulphates (SO4-2); commonly termed evaporites
CaSO4•2(H2O) – gypsum CaSO4 – anhydrite
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compositional classification of (bio)chemical sedimentary rocks is typically based on the major anion Others include:
Fe2O3 – ironstone (iron oxide) SiO2 – chert (flint; opal is SiO2•nH2O)* NaCl – halite *can form abiotically or biotically
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limestones and dolostones: textural classification
characterised by their allochems (grains) • bioclasts (fpieces of fossils) • ooids – small spheres • peloids – fecal pellets • intraclasts – eroded clasts and their interstitial autochem material (kinda like matrix) • lime mud or micrite (micro-crystalline calcite) • cement as coarse carbonate crystals (spar) Ooids are an allochem
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Graded bedding (sedimentary)
deposition due to decreasing flow energy results in graded bedding: coarser grains at the base of beds and finer grains upwards (Reverse grading is also a thing)
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Bedding scale (sedimentary)
layering <1 cm thick is termed laminated layering 1 – 10 cm is termed thin bedded layering 10 – 50 cm thick is termed medium bedded layering 50 – >100 cm thick is termed thick to very-thick bedded
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Bedform (sedimentary)
a morphological feature formed by the interaction between a flowing fluid (water, air) and sediment on a bed bedforms inform about flow energy and transport direction
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Ripples n' dunes
ripples have h <4 cm, dunes have h > 4 cm ripples and dunes inform on direction of sediment transport ripples and dunes often occur together
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Fluid flow and bedforms
sediment is carried up the stoss side of a ripple by the flow at the crest, the flow separates from the bed and grains cascades down the lee side flow ‘reattaches’ in the trough causing erosion and that sediment is transported up the stoss-side of the next ripple the progressive cascade and migration of grains forms cross-bedding
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Bedform stability and flow energy
when sediment is transported, it becomes organised into stable bedforms (e.g. ripples, dunes) that reflect flow ‘energy’ (velocity) acting on a particular grain size distribution generally, as flow velocity increases, the stable bedforms are: flat beds --> ripples --> dunes --> plane beds --> antidunes by recognising bedforms, and changes in bedforms through a sedimentary sequence, you can reconstruct past flow conditions and sediment transport direction
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Types of flow n ripple symmetry
unidirectional flow generates asymmetric/current ripples oscillatory flow generates symmetric/wave ripples
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Formation of wave ripples
wind shear generates waves waves on the surface generate a circular motion (‘orbitals’) of water molecules orbitals decrease in size downward; in shallow water these can intersect the seafloor and friction causes the circular motion to become elliptical the horizontal motion of the ellipse at the bed can move sediment and generate symmetric ripples
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Imbrication
a depositional fabric in which clasts align and overlap one another, much like a run of toppled dominoes
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Soft sediment deformation
these form due to gravitational instabilities via loading and by excessive shear stress
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sedimentary environments: fluvial
characteristic features of fluvial deposits: • point bars (m-scale lateral accretion surfaces) • crevasse splay sands (flat, tabular beds) • overbank or floodplain mud and fine sand • fining-upward trend from gravel in channel, sand in point bar to mud in floodplain/overbank
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sedimentary environments: shorelines and deltas
• coastal zones are the interface between marine and non-marine settings • areas where wave, tide and storm energies are dissipated • sinks for products of physical (sediment) and chemical (ions) weathering • zones of mixing between fresh and saline waters
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foreshore or swashface
• cm- to dm-thick sets of low-angle laminae • symmetric (wave) and flat-topped ripples • bioturbation (burrowing)
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sedimentary environments: marine settings (focus on carbonates)
controls on patterns and characteristics of deposition in marine settings include: • physical processes such as waves, storms and tides • oceanic conditions such as bathymetry (shelf, slope, abyssal plain), salinity and water temperature (the latter two are latitudinal or ‘climatic’) • tectonic setting such as passive vs active margins
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Carbonate reef distribution
low to no siliciclastic flux • warm temperature (20˚- 30˚ C) • shallow water depth (<10 - 20 m) • average to high salinity (34.4 ppm)
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Components of the climate system
The greenhouse effect The carbon cycle Forcing mechanisms and feedback Climate variation
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The atmosphere is made up of:
Troposphere Stratosphere Outer atmosphere
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Drivers of climate change
Geological time-scales – millions of years Movement of the solar system through the galaxy ~ changes in cosmic ray flux and galactic dust Influence cloud formations - Plate tectonics – movement of continental plates Affects on ocean currents - Mountain building etc etc Affects on atmospheric circulation Weathering Presence/absence of sea ice/ice sheets at poles Albedo affects Multiple feedbacks in the system
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The hadean eon
Formation of Earth: 4.6 Gya 50-70 Mya later, a Mars-sized object collides with the Earth and the Moon is formed first 600 My of Earth’s history Sun was 30% fainter than at present formed with no “primary” atmosphere, but outgassing resulted in an atmosphere which was likely water vapour, CO2, ammonia, methane, hydrogen sulphide, sulphur dioxide + others no O2 at that time zircons show oceans and continental material had formed by 4.4Gya (0.1Gya after formation)
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A planet under seige
Impacts occurred from formation through until the Late Heavy Bombardment (about 3.9Gya) Sterilizing impacts probably occurred 6-12 times during the Hadean No real idea what the “temperature” of the planet was at this time
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The Archean
3.9 to 2.5 Gya Oldest rocks on Earth from this period Evidence for lack of Oxygen Witwatersrand gold ore (~3 Gya) Detrital Pyrite (FeS2) Was not oxidized during weathering Evolution of life: 3.7 – 3.5 Gya Evolution of methanogens (prokaryotes) [cannot survive with free oxygen] CO2 + 4 H2 → CH4 + 2 H2O Archean ends with rise in global oxygen levels Evolution of cyanobacteria (eukaryotes) – 2.8 Gya (earlier??) Tectonics different to today Higher heat flow Smaller plates (proto-continents) and many hot spots Temperatures likely warmer than today Oxygen isotopes in Archean rocks suggest oceans twice as warm as today’s tropical oceans (~50oC). This is contentious – but climate was WARM But this is odd as the Sun was less bright!
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The Faint sun paradox
No Atmosphere? - The Earth should have been “frozen” for the first two billion years 3.8 Gya: Sun’s luminosity 75% of present value Yet – during the Archean liquid water was prevalent on the surface In fact the geological and palaeoclimatic record strongly suggests Earth has maintained a “moderate” climate throughout its history – BUT WITH WOBBLES The Greenhouse Effect!!! CO2 - supplied by volcanoes CH4 - Also from volcanoes - but also requires life - Methanogens!!
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Hydrolysis
Main chemical weathering mechanism that removes atmospheric CO2 Reaction of silicate minerals (CaSiO3) with carbonic acid (H2CO3) to form clay minerals and dissolved ions CaSiO3 + H2CO3 --> CaCO3 + SiO2 + H2O Atmospheric CO2 combines with water = H2CO3 This process accounts for 80% of the CO2 removal CO2 also dissolves in sea water etc Later life – photosynthesis etc etc
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Controls on weathering reactions
Chemical weathering influenced by -Temperature Weathering rates double / 10oC rise -Precipitation H2O – required for hydrolysis H2O increases as temperature increases Vegetation [not relevant for Archean] Respiration in soil increases CO2 CO2 in soils 100-1000x higher than atmospheric CO2 Other factors land formation, mountain building, latitude location etc
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Organic haze
If CH4 becomes more abundant than CO2, an organic haze begins to form Haze from UV photolysis (decomposition) of CH4 Creates an anti-greenhouse effect Haze absorbs sunlight in the stratosphere and radiates energy back to space E.g. Titan
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Archean/Proterozoic transition
A time of significant change Change from “small plates” to modern large plate tectonics Significant rise in O2 due to [evolution] increase of cyanobacteria (blue green algae) Photosynthesis Cyanobacteria: 2.8 Gya (possibly evolved 3.8Gya) Stromatolites Layered Cyanobacteria accretionary structures
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Implications of increased oxygen
Disrupted the balance Solar luminosity – low but increasing! CO2 CH4 + water vapour Increased weathering - oxidation Decrease CO2 Methanogens outcompeted (?) by cyanobacteria – decrease CH4 1st major glaciation 2.3 – 2.2 Gya It did not take much to shift the planet into a glaciation
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2.2 Gya to 750 Mya
Tectonic style changed Small to large plates First supercontinent Rodinia: 1 Gya – 750 Mya Bulk of land: mid-latitudes Related Grenville Orogeny
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750 - 580 Mya
Neoproterozoic Snowball Earth: Cryogenian Multiple periods of severe “global” glaciation Lots of geologic evidence of low latitude glaciation Global temperatures plunged and the whole planet was encased in ice Or in “Slushball” alternative – tropics were ice free
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Mechanics to a snowball state
Neoproterozoic Snowball Earth: Cryogenian Multiple periods of severe “global” glaciation Lots of geologic evidence of low latitude glaciation Global temperatures plunged and the whole planet was encased in ice Or in “Slushball” alternative – tropics were ice free
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How to get out the icehouse
It’s the Greenhouse Effect again Volcanic activity and carbon dioxide release would NOT have ceased during Snowball periods Due to cold conditions, weathering rates were low so hydrolysis rates low and therefore little “scrubbing” of CO2 from atmosphere
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Phanerozoic consists of 3 eras
Paleeozoic Mesozoic Cenozoic
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Early Phanerozoic
Started with the Cambrian Explosion A direct response to the late Proterozoic Snowball Earth Quick evolution from “Ediacaran” fauna Initially marine Rapid evolution “empty planet” - many open ecological niches driven by predation competition for “food” resources
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Phanerozoic climate
Large swings from “greenhouse” to “icehouse” conditions Understanding this long-term variability in global temperatures is not straightforward Underlying hypothesis CO2 is the main driver of global climate change Faint sun less of an issue now Myriad of feedbacks Presence/absence of continents at poles Presence/absence of ICE at poles Hydrolysis: carbonate-silicate cycle
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Cambrian
540 - 490 mya CO2 ~ 4500 ppm, 16x pre-Industrial Snowball build up O2 ~ 63% of present Temp ~ 21°, 7° above present Sea level 30-90m above present No ice cover No terrestrial life Trilobites dominant in oceans (became extinct at end of Permian) Slow removal of CO2 through Hydrolysis
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Devonian
415 - 360 mya CO2 ~ 2200 ppm, 8x pre-Ind. O2 ~, 75% of present Temp ~ 20°, 6° above present Sea level 180-120m above present No ice cover Land has some plants and animals Continued removal of CO2 through Hydrolysis
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Carboniferous
360 - 300 mya CO2 ~ 800 ppm, 3x pre-Industrial O2 ~ 163% of present Temp ~ 14°, 0° above present Sea level 80-120m above present Land is dominated by swamps and forests Some ice cover – south pole
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Permo-Carboniferorous glaciation
Since the “Snowballs” of the late pre-Cambrian, one of the most extensive glacial periods in earth history until “recent” glaciations of the Cenozoic Devonian to Carboniferous Super continent at poles: Pangea/Gondwana Tropical mountain range Decreasing CO2
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Permian
300-250 mya CO2 ~ 900 ppm, 3x pre-Industrial O2 ~ 115% of present Temp ~ 16°, 2° above present Sea level >60m to <20m present Pangaea diverse climate states Cold dry at southern polar latitudes North – intense and great seasonal variation Worst extinction event in Earth’s history 95% of species disappeared
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Permian- triassic extinction
The boundary of the Permian and Triassic ~90% of all species died out 95% of species in oceans Marine invertebrates – worst hit! Took place over a 5-10 million year period Slow start – rapid by end Impact event (Nickel-rich Layers From impact or heavy-metal rich mantle-derived lavas) Volcanism (Flood basalt events The Siberian Traps (also another in China) ) Final complete state of Pangaea – extreme climate states Climate Change – hot or cold (or both?)
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Mesozoic era
The emergence of the dinosaurs Predatory reptiles Amphibians living on land and in water Reef Building corals Climate and CO2 levels relatively constant
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Triassic
250 - 200 mya CO2 ~ 1750 ppm, 6x pre-Industrial O2 ~ 80% of present Temp ~ 17°, 3° above present Desert conditions prevail, leads to success of reptiles Late Triassic – emergence of dinosaurs
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Jurassic
200 - 145 mya CO2 ~ 1950 ppm, 7x pre-Industrial O2 ~ 130% of present Temp ~ 16.5°, 3° above present High CO2, largest terrestrial animals ever Landscape dominated by coniferous forests and fern plains
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Cretaceous
145 - 65 mya CO2 ~ 1700 ppm, 6x pre-Industrial O2 ~ 150% of present Temp ~ 18°, 4° above present By end of Cretaceous CO2 levels are approaching Cenozoic levels Another extinction event which wiped out the dinosaurs Emergence of flowers and associated insects Diversification of mammals
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Cenozoic era
Mammals increased in numbers and diversity Grasses and flowering plants expanded on land Ocean life remained relatively unchanged however The Eocene-Paleocene is the last “warm” period in Earth history Early Eocene seen as a “worst case” analogue for where today’s change in climate, as influenced by anthropogenic CO2 emissions, could go………….!!
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Eocene
55 - 35 mya CO2 ~ 385 ppm, 1.5x pre-Industrial O2 ~ 100% of present Temp ~ 19°, 5° above present BUT within this period were some significantly extreme climate states Paleocene-Eocene Thermal Maximum End of Eocene marked beginning of current icehouse climate
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Drivers of climate change
External and Internal External to climate system Orbital variations, tectonic effects, sun’s variations Internal to climate system Feedback mechanisms Ocean/atmospherics interactions Ocean conveyor belt El Nino-southern oscillation, Monsoons etc
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Milankovitch cycles
- obliquity (tilt) It is this tilt that results in the planet having seasons. The larger the angle, the larger the difference between summer and winter - eccentricity How oval it is - pressession The spinning of the earth its self All whilst spinning around the sun
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Ice sheet changes with climate change
As ice sheets form, global albedo increases Results in a further temperature drop and ice expansion Expanding ice sheets result in a fall in global eustatic sea-level Makes it easier for ice to flow out from the land Further increasing albedo These mechanisms could explain some of the added cooling not explained by Milankovitch theory But still not enough
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CO2 and the role of thermohaline circulation
Acts as a pump transferring CO2 and nutrients from the surface to the deep ocean Carbon–plankton relationship Phytoplankton take up CO2, falls to ocean bottom when dead Released through oxidation – BUT deep oceans are anoxic returned to the surface when the thermohaline circulation is on If circulation slows – carbon is not returned to the surface – global cooling Changes in strength of circulation would also alter energy transfer from equator to poles – especially in N Atlantic (Gulf Stream looses energy)
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Self regulating negative feedback loops within climate change
Extra ice at poles should cause more downwelling exclusion of salt from water in ice formation Increased sea salinity – therefore denser Causing strong thermohaline circulation Colder climate means less terrestrial biological activity – therefore more atmospheric CO2 Colder climate means less moisture vapour in atmosphere less precipitation to feed glaciers Moisture vapour also a greenhouse gas
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Ice cores
Ice cores High resolution palaeo archives Greenland ~130,000 yrs Antarctic ~800,000 yrs Greenland data Shows very rapid climate change
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The youngest dryas
The last short major cold event During the transition from the last glacial into the present Holocene Occurred from 12,800 and 11,500 yrs ago General warming trend interrupted by cold reversal
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The late holocene
Good quality high resolution proxy data e.g. tree-rings, ice cores, corals, speleothems, historical archives “reasonable” knowledge of the climate over this period Reasonable records of solar and volcanic forcing as input parameters in climate models Last 150 years – anthropogenic period So called “Anthropocene”