185’x88’ draft 25’ Sea State 6 Worked example - Here is the electron configuration for a filled fifth shell: ShellSubshellOrbitals Electrons n.

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Presentation transcript:

185’x88’ draft 25’

Sea State 6

Worked example - Here is the electron configuration for a filled fifth shell: ShellSubshellOrbitals Electrons n = 5l = 0m = 0→ 1 type s orbital→ max 2 electrons l = 1m = -1, 0, +1→ 3 type p orbitals→ max 6 electrons l = 2m = -2, -1, 0, +1, +2→ 5 type d orbitals→ max 10 electrons l = 3m = -3, -2, -1, 0, +1, +2, +3→ 7 type f orbitals→ max 14 electrons l = 4m = -4, -3 -2, -1, 0, +1, +2, +3, +4→ 9 type g orbitals→ max 18 electrons Total: max 50 electrons a shell can contain up to 2n² electrons

Igneous rocks – ignis Latin for fire

Locations of world’s volcanoes (on land) What is heat source?

Volcanism is governed by plate tectonics What is the biggest source of new material?

Igneous rocks on Earth #1 – Mid-ocean ridges (divergent) #2 – Subduction zones (convergent)

What causes an eruption….anywhere?

Increasingheat,pressure

Decompression melting

Volatiles decrease melting temperature

What causes an eruption….anywhere? 1. Decompression melting 2. Volatiles decrease melting temperature

So why do we have different volcanic rock types?

4 (common) extrusive igneous rocks Basalt Andesite Rhyolite Komatiite

Where do chemical differences arise?

Magma chamber processes

So why do we have different volcanic rock types? Source material the same: mantle-derived Magma chamber processes: 1. Magmatic differentiation (Bowen’s Reaction Series) 2. … 3. …

TRAIL MIX MODEL OF MAGMA FORMATION Initial composition: 25% M&Ms 25% Raisins 25% Peanuts 25% Almonds

TRAIL MIX MODEL OF MAGMA FORMATION 2nd composition: 25% M&Ms 33% Raisins 33% Peanuts 33% Almonds

TRAIL MIX MODEL OF MAGMA FORMATION 3rd composition: 25% M&Ms 33% Raisins 50% Peanuts 50% Almonds

Magma crystallizes through 200°C+ of temperature Magmatic differentiation

Scenario A: young, hot magma

Initial melt composition: 1. Olivine 2. Pyroxene Ca-rich plagioclase feldspar 3. Amphibole Intermediate plagioclase feldspar 4. Biotite mica Na-rich plagioclase feldspar

Scenario B: magma sits around, cools

2nd melt composition: 1. Olivine 2. Pyroxene Ca-rich plagioclase feldspar 3. Amphibole Intermediate plagioclase feldspar 4. Biotite mica Na-rich plagioclase feldspar

Scenario C: (relatively) old, cold magma

3rd composition: 1. Olivine 2. Pyroxene Ca-rich plagioclase feldspar 3. Amphibole Intermediate plagioclase feldspar 4. Biotite mica Na-rich plagioclase feldspar

So why do we have different volcanic rock types? Source material the same: mantle-derived Magma chamber processes: 1. Magmatic differentiation (Bowen’s Reaction Series) 2. … 3. …

So why do we have different volcanic rock types? Source material the same: mantle-derived Magma chamber processes: 1. Magmatic differentiation (Bowen’s Reaction Series) 2. Assimilation 3. Magma mixing take a long time ~ imply distance from source

How can you predict where you’ll find different rock types?

Which magma sits around longest?

Which magma has to travel farthest?

So why do we have different volcanic rock types? Source material the same: mantle-derived Magma chamber processes: 1. Magmatic differentiation (Bowen’s Reaction Series) 2. Assimilation 3. Magma mixing take a long time ~ imply distance from source

Youngest magma ~ Closest to source Oldest magma ~ Farthest from source

Divergent Boundary Mid-Ocean Ridge Continental rift (Hot spots) Convergent Boundary Continental/ Island Arcs Intra-continentalYellowstoneTaupo

Divergent Boundary Mid-Ocean Ridge Continental rift (Hot spots) Convergent Boundary Continental/ Island Arcs Intra-continentalYellowstoneTaupo Most Explosive Least Explosive

Most Explosive Least Explosive Rhyolite PeridotiteGabbroDioriteGranite AndesiteBasalt Komatiite Extrusive Intrusive