Igneous Petrology Course Lecturer: Matt Genge, Meteorite Researcher, Previously worked at The...

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Igneous Petrology Course Lecturer: Matt Genge, Meteorite Researcher, Previously worked at The Natural History Museum. Lectures: Part I (4 weeks) Igneous Processes at the Atomic Scale. Part II (4 weeks) Igneous Processes at Large Scales. Practicals: How to recognise and describe igneous rocks in hand specimen and thin section (see list on handout sheet). Coursework (20%): Five coursework pieces focused on each major group of igneous rocks. 1.5 hour Exam (80%):

Transcript of Igneous Petrology Course Lecturer: Matt Genge, Meteorite Researcher, Previously worked at The...

Page 1: Igneous Petrology Course Lecturer: Matt Genge, Meteorite Researcher, Previously worked at The Natural History Museum. Lectures: Part I (4 weeks) Igneous.

Igneous Petrology Course

Lecturer: Matt Genge, Meteorite Researcher, Previously worked at The Natural History Museum.

Lectures: Part I (4 weeks) Igneous Processes at the Atomic Scale.Part II (4 weeks) Igneous Processes at Large Scales.

Practicals:How to recognise and describe igneous rocks in hand specimen and thin section (see list on handout sheet).

Coursework (20%):Five coursework pieces focused on each major group of igneous rocks.1.5 hour Exam (80%):Straight after christmas! Special revision session last practical.

Page 2: Igneous Petrology Course Lecturer: Matt Genge, Meteorite Researcher, Previously worked at The Natural History Museum. Lectures: Part I (4 weeks) Igneous.

Hot Under the Collar (part I)

Melting and the Phases of Matter

Pacaya Volcano - Guatemala

Igneous Rocks: formed by cooling of a magma.

Page 3: Igneous Petrology Course Lecturer: Matt Genge, Meteorite Researcher, Previously worked at The Natural History Museum. Lectures: Part I (4 weeks) Igneous.

The Four Phases of Matter

Liquid

Solid Gas

Plasma

Page 4: Igneous Petrology Course Lecturer: Matt Genge, Meteorite Researcher, Previously worked at The Natural History Museum. Lectures: Part I (4 weeks) Igneous.

Structural Differences

Configurational entropy (disorder)

Page 5: Igneous Petrology Course Lecturer: Matt Genge, Meteorite Researcher, Previously worked at The Natural History Museum. Lectures: Part I (4 weeks) Igneous.

Kinetic Differences

Vibrational entropy (disorder)

Page 6: Igneous Petrology Course Lecturer: Matt Genge, Meteorite Researcher, Previously worked at The Natural History Museum. Lectures: Part I (4 weeks) Igneous.

Entropy

The entropy of a mixture is higher than a pure material

Page 7: Igneous Petrology Course Lecturer: Matt Genge, Meteorite Researcher, Previously worked at The Natural History Museum. Lectures: Part I (4 weeks) Igneous.

Entropy

Entropy increases with temperature due to the magnitude of atomic vibrations

Page 8: Igneous Petrology Course Lecturer: Matt Genge, Meteorite Researcher, Previously worked at The Natural History Museum. Lectures: Part I (4 weeks) Igneous.

Entropy

Entropy is “wasted” or unavailable energy

Page 9: Igneous Petrology Course Lecturer: Matt Genge, Meteorite Researcher, Previously worked at The Natural History Museum. Lectures: Part I (4 weeks) Igneous.

Total Thermodynamic Energy in Matter

+Potential Energy Kinetic Energy

Total Energy (Enthalphy H) = PE + KE

Page 10: Igneous Petrology Course Lecturer: Matt Genge, Meteorite Researcher, Previously worked at The Natural History Museum. Lectures: Part I (4 weeks) Igneous.

Gibbs Free Energy

G – Gibbs Free Energy (energy available for chemical work)

H – Enthalpy (total energy)

S – Entropy (energy locked up in disorder – wasted energy)

G = H – T.S

First Law of Thermodynamics

Page 11: Igneous Petrology Course Lecturer: Matt Genge, Meteorite Researcher, Previously worked at The Natural History Museum. Lectures: Part I (4 weeks) Igneous.

Extrinsic and Intrinsic Properties

Extrinsic properties depend on the mass of the system.

Page 12: Igneous Petrology Course Lecturer: Matt Genge, Meteorite Researcher, Previously worked at The Natural History Museum. Lectures: Part I (4 weeks) Igneous.

Extrinsic and Intrinsic Properties

Intrinsic

Taste

Colour

Specific Gravity

Temperature

Extrinsic

Volume

Amount of Alcohol

Attractiveness

Page 13: Igneous Petrology Course Lecturer: Matt Genge, Meteorite Researcher, Previously worked at The Natural History Museum. Lectures: Part I (4 weeks) Igneous.

Extrinsic and Intrinsic Properties

Intrinsic

Composition

Temperature

Pressure

Extrinsic

Volume/mass

Enthalpy

Entropy

Gibbs Free Energy

Page 14: Igneous Petrology Course Lecturer: Matt Genge, Meteorite Researcher, Previously worked at The Natural History Museum. Lectures: Part I (4 weeks) Igneous.

Temperature

2

2

1

3

2mv

kT

• Temperature is the effect of the motions of atoms within a material (the vibrations, translations and rotations of molecules).

• Temperature is proportional to the average kinetic energy of the atoms or molecules within a material.

Page 15: Igneous Petrology Course Lecturer: Matt Genge, Meteorite Researcher, Previously worked at The Natural History Museum. Lectures: Part I (4 weeks) Igneous.

Pressure

V

NmvP

3

2

Pressure is the force applied by rebounding atoms and is related to the change in momentum.

Page 16: Igneous Petrology Course Lecturer: Matt Genge, Meteorite Researcher, Previously worked at The Natural History Museum. Lectures: Part I (4 weeks) Igneous.

Transitions between the Phases of Matter

Page 17: Igneous Petrology Course Lecturer: Matt Genge, Meteorite Researcher, Previously worked at The Natural History Museum. Lectures: Part I (4 weeks) Igneous.

Transitions and Gibbs Free Energy

•The phase with the lowest Gibbs Free Energy at equilibrium is the stable phase.

•Two coexisting phases have the same Gibbs Free Energy

Page 18: Igneous Petrology Course Lecturer: Matt Genge, Meteorite Researcher, Previously worked at The Natural History Museum. Lectures: Part I (4 weeks) Igneous.

Melting

Sudden increase in disorder on melting. A discontinuous increase in entropy S.

Page 19: Igneous Petrology Course Lecturer: Matt Genge, Meteorite Researcher, Previously worked at The Natural History Museum. Lectures: Part I (4 weeks) Igneous.

First & Second Order Phase Transitions

G = H – T.S• H is the latent heat of fusion

• Temperature stays constant until all the material has melted.