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Big Bang
other galaxies are moving away from our own at high speed, in all directions
the entire vastness of the observable universe, was compressed into a hot, dense mass just a few millimeters across.
a massive blast allowed all the universe’s known matter and energy to spring from some ancient and unknown type of energy
Georges Lemaitre
he theorized that the universe began from a single primordial atom
1927
Edwin Hubble
who proposed that galaxies are speeding away from us in all directions, and from the discovery of cosmic microwave radiation by Arno Penzias and Robert Wilson
cosmic microwave background radiation
a tangible remnant of leftover light from the big bang
inflation
gravitational waves rippled through our infant universe during an explosive period of growth
after the universe burst, space itself ripped apart, expanding exponentially
NASA-developed detector technology on the BICEP2 telescope at the South Pole
Planck satellite
European Space Agency mission for which NASA provided detector and cooler technology
B-mode
gravitational waves produced a characteristic swirly pattern in polarized light
Ptolemaic System
arrangement of this geocentric Earth-centered plan
Earth has been assigned the central place in the universe
Nicolaus Copernicus
who proposed the modern heliocentric or sun-centered system of planetary motions in 1543
Immanuel Kant, Laplace
people who postulated the the solar system was derived from the condensation of an enormously dispersed gaseous atmosphere surrounding the sun (1755-1796)
Nebular Hypothesis
solar system started out as a large nebula of gas, dust, and ice which eventually spun out into the shape of a disc
Planetesimal Theory
planetary system was formed from materials removed from the sun by tidal action caused by a passing star
projection became masses of gases that revolved around the sun
Carl Friedrich von Weizacken and Harold C. Urey
proponents of Dust Cloud Theory 1945
Dust Cloud Theory
composition mainly of hydrogen and helium
Interactions of the gas molecules accelerated the lighter ones so that they mostly escaped from the nebula
interactions also produced swirls, forming lumps in the nebula that could grow to become planets and satellites
Protoplanet Hypothesis 1949
the original nebula was so massive that on further contraction and flattening, it broke into separate clouds or protoplanets
Gerald P. Kuoper
proposed protoplanet hypothesis in 1949
crust
mantle
outer core
inner core
layers of earth
crust
brittle outermost layer
thickness ranging from five (5) to 10 km from ocean basins to 25 to 70 km from the continents
mantle
composed of molten silicate rocks
behaving as both solid and liquid, many believe that the mantle might be a non-Newtonian fluid.
100 km cool hard, below is weak and flows slowly like
core
hottest layer
made of iron and nickel
Lithosphere, Hydrosphere, Biosphere, and Atmosphere
parts of the earth
water
energy
time
recycling
bonus features
Characteristics of Earth that are Necessary to Support Life
habitable planets conditions
central star should not be more than 1.5 Mo (Solar mass)
central star should be at least 0.3 Mo to be warm enough to create a large orbital zone which planet could retain liquid water
central star should not flare violently or emit intense x-rays
planet must orbit at the right distance from the star
planet’s orbit must be circular and stable enough
planet’s gravity must be strong enough
geology
study of the earth’s rocky parts found on the crust (lithosphere) and its historical evolution
Physical Geography
study of the physical features of the Earth’s surface
different processes and patterns in the natural environment
Geophysics
studies the shape of the Earth, its reaction to different forces as well as its magnetic and gravitational fields
most vital for mineral and petroleum explorations
Soil Sciences
cover the Earth’s outermost layer which is the crust
Major sub-disciplines of soil sciences include edaphology and pedology
Oceanography/Hydrology
studies the marine and freshwater domains of the hydrosphere
Glaciology
studies the ice and icy parts of the Earth known as the cryosphere
Atmospheric Sciences
study of the gaseous parts of the Earth
Formation of Earth
The creation theory
the big bang
The Creation Theory
biblical in origin asserting that everything in the universe, including humans were created by a supreme being in a span of 7 days
Big Bang Theory
speaks of the Earth's formation in a scientific perspective. It states that the universe is formed sometime between 10 and 20 billion years ago from a cataclysmic explosion.
Continental Drift Theory
Alfred Wegener theorized that there was once a vast supercontinent 200 million years ago which he named Pangaea meaning "All-earth".
Laurasia and Gondwana
pangaea broke into 2 smaller supercontinent
luster penetrability color streak
optical characteristics of minerals
luster
property of a mineral to reflect light; describes how brilliant or dull it is
penetrability
optical property of minerals to allow light to pass through
transparent, translucent, opaque
types of penetrability
color
optical perception described through certain color categories; considered to be unreliable due to impurities affecting color quality
streak
mineral's color in powdered form; minerals with higher hardness cannot leave streak marks on the porcelain
mineral strength tenacity hardness cleavage fracture
types of mineral strength
mineral strength
determines how easy minerals break or deform when exposed to stress
Tenacity (or toughness)
refers to the mineral's resistance to breaking or deforming
Hardness (or strength)
is the measure of a mineral's resistance to abrasions (or scratches)
Cleavage
is the tendency of minerals to break along the planes of weakness
Fracture
form of splitting where a mineral is split despite not having any cleavage plane due to its strong chemical bonds between the mineral's atoms
Specific Gravity
is the measure of a mineral's density
by slow cooling
by rapid cooling
by pyroclastics
formation of igneous rock
by cementation
by chemical precipitation
formation of sedimentary rock
through pressure
through temperature
formation of metamorphic rocks
clastic
bioclastic
chemical crystalline
identifying sedimentary rocks
foliated non foliated
identifying metamorphic rocks
exogenic
any process that includes geological phenomena and processes originating externally to the Earth’s surface
Weathering
gradual on-site breakdown of rocks into sediments
exfoliation
thermal
expansion
wedging
types of mechanical weathering
exfoliation
splitting of intrusive rock sheets from its original formation
thermal expansion
breakup of rocks due to being heated
wedging
forcefully breaking rocks apart via external factors
oxidation
hydrolysis
carbonation
acid precipitation
erosion
types of chemical weathering
erosion
weathered and unweathered materials from its substrate due to gravity or agents of transportation
gravity
wind
water
glaciers
agents of erosion
Traction
Saltation
Suspension
Solution
types of water erosion
traction
movement caused by rolling or dragging large sediment grains aided by smaller grains pushing against them
saltation
movement caused by repeated bouncing of sand grains as they are transported by water
suspension
movement observed in fine particles such as silt and clay
solution
Movement found in soluble materials such as salts
relief
slope stability
fragmentation and weathering
types of mass wasting (gravity)
deposition
where sediments settle out of the transporting medium, usually associated with water
endogenic
process that includes geological phenomena and processes originating within the Earth’s surface
decompression melting
flux melting
heat transfer melting
partial melting
generation of magma
decompression melting
temp is constant thruout while pressure decreases
flux melting
volatiles (gaseous substance) are added to the magma
burial metamorphism
type of metamorphism pressure from compaction within the affected sediments exceeds the natural limits
cataclistic
type of metamorphism rocks affected by lateral motion earthquake
dip slip
strike slip
oblique slip
types of fault
relative dating
absolute dating
fossils
geologic time scale
earth’s history
Uniformitarianism
states that all geological processes known today also occured in the past, operating slowly thru out the ages
Original Horizontality
materials forming any stratum were continuous on the earth’s surface unless some other bodies stood in the way
superposition
at the time when any stratum is formed, all matter resting upon it was fluid and none upper strata exists
oldest layer - bottom
youngest - top
Cross-Cutting Relationships
any rock that cuts thru established rock strata is the youngest
Inclusions and Components
any foreign material found in another material
faunal succession
strata that have been known to hold fossils
chronostatic time
any physical subdivision and the time they represent
unconformities
a missing stratum
angular unconformity
nonconformity
disconformity
paraconformity
types of unconformity
angular unconformity
originally deposited horizontal layer that has been folded, weathered and eroded
nonconformity
rocks come in contact with sedimentary beds indicating period of uplift and erosion of previous rocks
disconformity
sediment layers are uplifted without folding but exposed to weathering and erosion creating an irregular surface
paraconformity
strata are parallel with each other
alpha ++
beta plus +-
beta minus --
electron capture
gamma
radioactive decay types
half life
time radioactive material takes to lose half of its mass
tree rings
display alternating bands which when counted, its possible to find the number of years tree lived
ice cores
formation of snow-dust strata
varves
alternating sedimentary bed found at the bottom of lakes especially at the end of glaciers
stratigraphy
ordering and analysis of earth’s layers
hadean eon
the burning earth
earliest iteration
how solar system came into existence
earth is devoid of life and still made of molten material
archaean eon
the first rain
newly formed crust after iron catastrophe began to cool down
Vaalbara was formed
protorozoic eon
the first glacier
life began to dominate earth
arctica
atlantica and columbia
rodinia
pannotia
supercontinents that formed during protorozoic eon