HTML University
Science Dept.
Geology and Soils GEO 100 Notes
Introduction to Energy and Matter
- Origin of Universe
- Steady State
- Expansion & Contraction
- Element Abundance
- Universe: H = 76%, He = 23%, by Weight or H = 93%, He = 6%
by Atom
- Entire Earth: 90% Fe, O Si, Mg,
by Weight
- Crust: O, Si, Al, Fe, Ca, Na, K, Mg,
by Weight
- Origin of Elements
- Solar System
- Primary Star
- Secondary Star
- Evolution of Atmospheres
- Earth Type Atmosphere
- Energy
- Kinetic Energy
- Gravitational Potential Energy
- Thermal Energy
- Chemical
- Nuclear Transformation & Conservation
- Solar -> Hydrologic
- Solar -> Wind
- Nuclear -> Volcanism
- Matter
- Atomos - Democritus
- Sub - Atomic Particles
- Proton
- Neutron
- Electron
- Elements
- Hydrogen
- Helium
- Isotopes
- Hydrogen
- Deuteruim
- Tritium
- Ions
- Na+
- Cl-
- Ionic Bond: Electrostatic Force of Attraction
- Covalent bond: Sharing of Electrons (H2O)
- States of Matter
- Gases
- Liquid
- Solids
- True Solids vs Amorphous Solids
- Minerals
- Introduction
- General
- 2000 Minerals
- 30 - 40 Rock Forming & Ore Minerals
- Characteristics
- Physical
- Chemical
- X-ray
- Optical
- Definition: A naturally occuring inorganic material with a definite internal order
and arrangement of its constituent atoms having definite chemical and
phyical properties (which may vary within known limits)