Exam 1 Flashcards
What is geology?
The study of Earth including:
composition
behavior
history
Expanding Universe Theory
Hubble observed all light from all galaxies exhibits red shift
Means all galaxies are moving away from the Earth very quickly
Creates the basis for big bang
Universe has been expanding since the big bang
Assumption of the law is that we are a stationary observers
Big Bang Theory
A cataclysmic explosion that scientists suggest represent the formation of the universe
before this, all matter and energy was packed into one volumeless point
There was no big “explosion” from single point, “simultaneous appearance of space everywhere in the universe”
Big Bang theory doesn’t explain what universe expands into
Big Bang theory doesn’t address what caused expansion to begin
during first second= protons and neutrons form
Nebular Theory
The protoplanetary disk was hotter at center, cooler at edges
Thus rings of dust accumulates toward center, rings of ice at outskirts
As disk flattens- separation of volatiles and refractory materials- separates into gaseous planets and rocky planets
formed our solar system
Scientific Theory
group of related observations
based on proven hypotheses
verified multiple times
independent researchers
may be modified
Constant speed of Light
discovered by einstein
300,000 km/sec
Light year
9.5x10^12 km/yr
or 95 trillion kilometers a year
mesaure of distance not time
Doppler Effect
Assuming a stationary observer and moving source of sound or light:
wave frequency increases in direction of motion
Red shift/Blue shift
Blue shift, or higher frequency of light when an object is moving towards, and a red shift, or lower frequency, when an object is moving away from a person
Hubble’s Law
recessional velocity is directly proportional to distance
Means more distant objects move more quickly away from Earth
Law of Conservation of Matter and Energy
Fixed amount of matter and energy in universe
How old is the universe?
13.7 billion years ago
How old is our planet?
the same age as our solar system, 4.6 billion years old
Big Bang Nucleosynthesis
fusion of protons to create elements with low atomic numbers (H, He, Li, Be, B)
aka formation of the lighter elements
Nucleosynthesis–> creation of nuclei by fusion of very close protons –> can create up to boron
Nebula
Gases clump together into a cloud or pillar
Larger nebulae:
more mass
more density
Nebulae–> stars
More mass–> more density–> gravity collapse inward and start to rotate (imagine ice skater spinning and then pulling arms and legs in)
Accretionary disk
spinning mass of gas and dust from which stars and planets form
Hydrogen nuclei at center fuse to make Helium–heat and light create star
See mass start to flatten out after spinning
Stellar Nucleosynthesis
formation of higher atomic number elements within stars by:
- Fusion–small nuclei fuse
- Neutron capture and decay
- neutron sticks to nucleus (so atomic mass goes up
- neutron releases e-, so now p+ (so atomic number goes up)
Need to have stars present before heavier elements become present
Mostly nuetron capture and decay= neutrons that are available stick to nucleus–>higher mass–>decay–> release of electron to it becomes a proton–>change in atomic number
Supernova
A shortlived very bright object in space that results form the cataclysmic explosion marking the death of a very large star
ejects very large quantities of matter into space to form new nebulae
How old is our solar system?
4.6 billion years old (same age as the earth)
Protoplanetary
has ingredients available to create planets
Ex: the accretionary disk of our sun was this
Volatiles
gas or ice (H2, He, CH4, NH3, H2O, CO)
Refractory materials
rocky or metallic materials (heavier elements)
How do we know that layers exist in a planet?
Earthquakes generate seismic waves
Energy from waves reflected or refracted at boundaries between different materials
Seismic waves travel at different speeds in different materials
Differences in density–> different speeds of seismic waves
Some waves can only go through some materials
Less dense material= slower wave
More dense/homogenous material= faster wave
Seismic Waves
waves of energy emitted from the focus of an earthquake
Differences in density–>different speeds of seismic waves
Some waves can only go through some materials
Less dense material= slower wave
More dense/homogenous material= faster wave
Physical Differentiation
Earth has 4 layers based on physical characteristics like density and the material’s ability to flow:
Lithosphere (rigid solid)
Asthenosphere (plastic solid)
Outer core (liquid)
Inner core (solid)
Chemical Differentiation
core, mantle, and crust
Core= iron
mantle= iron, silicon, oxygen
Crust= silicon and oxygen
Mantle is a blend of both- b/c the core is recycled over time through plate tectonics and mix in the mantle
Felsic
lighter in color
higher silicon content
melts at lower temperatures
Mafic
darker color
higher magnesium and iron content
melts at higher temperatures
Continental Crust
Average thickness = 35 – 40 km
Continental crust has felsic composition
Oceanic Crust
Average thickness = 7-10 km
Oceanic crust has a mafic composition
Lithosphere
rigid outer shell including crust and uppermost mantle
Two types of crust- oceanic crust and continental crust
Asthenosphere
portion of mantle where mafic rock flows (very slowly)
Convection occurs here
Outer Core
Liquid iron-nickel alloy
Fe, Ni, Si, O, S
Convective flow generates Earth’s magnetic field
Inner Core
Boundary between outer and inner core separates
Solid Fe-Ni alloy
Solid because of high pressure
Minerals
- Naturally occurring
- Solid
- Formed by geologic processes
- Crystalline structure
- Definite chemical composition
- Inorganic
Identified by
color, streak, luster, hardness, specific gravity, fracture vs. cleavage,
Crystal Structure
how atoms are arranged in organized pattern (crystal lattice)
Polymorphs
Minerals with same chemical composition, but different chemical structure
ex: graphite and diamond
Calcite
CaCO3
nonmetallic
clear
white streak
cleavage
soft
normal specific gravity
reacts with HCl
Quartz
SiO2
nonmetallic
white
no streak
fracture
hard
normal gravity
Covalent Bond
shared electrons
Ionic Bond
transfer of electrons
Oxides
mineral class
Metal cation bonded to oxygen anion
very common on earth
hematite, magnetite
Sulfides
Mineral class
Metal cation bonded to sulfide anion (S2-)
pyrite, galena
Sulfates
mineral class
Metal cation bonded to (SO4 )2-
gypsum
Halides
mineral class
Anion is a halogen ion (Cl-, F-)
halite
Carbonates
mineral class
Anionic group (CO3)2-
calcite
Native Metals
Mineral class
Atoms of one metal (metallic bonds)
Ex: gold, copper
Silicates
most importatn mineral class
Si and O most abundant elements in crust
Silicate minerals = 95% of crust
Diversity due to how tetrahedra link and share oxygen atoms
Anion (SiO4)4-
Silicon-oxygen tetrahedron
Ionic bond to cations
Covalent bond to oxygens
Amazing diversity
Ex: isolated tetrahedra (olivine), chains (amphibole and pyroxene), sheets (micas), frameworks (feldspars)
Plagioclase Feldspar
nonmetallic
grey, cream, brown
white streak
cleavage
hard
K-Feldspar
nonmetallic
brown, cream, orange, pink
no streak
cleavage
hard
normal gravity
Amphibole
nonmetallic
black
grey streak
fracture
hard
Pyroxene
mineral
nonmetallic
green to black
hard
cleavage
streak varies by type
Olivine
hard
fracture
nonmetallic
green
makes up the earth’s mantle
no streak
Hematite
nonmetallic
soft
fracture
earthy color
distinct red brown streak
The Rock Cycle
Igneous Rocks
for classification condsider setting of crystallization, mineral composition, and texture
formed by the freezing of molten rock
Magma
molten rock below the earths surface
LAva
molten rock at Earth’s surface
primarily stuff coming out of volcanoes
Intrusive
If crystallization occurs below surface
Magma intrudes into pre-existing country rock
Creates baked zone (where magma bakes other rock)
Extrusive
If crystallization occurs at surface
Decompression
one way to get magma
Hot mantle rock rises to shallower depths
Pressure decreases, magma forms
Addition of volitiles to rock
one way to get magma
hot, dry rock–> H2O or other gases diffuse through rock–> rock begins to melt
Mixing of volatiles (H2O, CO2) with rock breaks chemical bonds to cause melting
adding water decreases the melting point
Heat Transfer
Rising magma melts rock it intrudes
Why does magma composition vary?
Source rocks
Mixing
Assimilation–country rock from walls of magma chamber incorporated into magma