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Biosphere
Living Things
Geosphere
the solid earth
minerals, rocks and rock cycle
time
tectonic system (earthquakes, volcanos, and plates
Earth Science Observations
many observations are made outdoors in field investigations
however this is less easy to control than lab conditions
scientists must be selective and focus on data relevant to the ideas being tested
Hypotheses
An idea about how observations are related to each other
statement of how observations can be explained
testable by comparing its predictions with future observations or experiment
Theory
a hypothesis that has survived a number of tests and explains more than just one phenomenon
Scientific Law
A theory or part of a theory that explains many observations and has passed many tests may be trusted to the point
Principle of Stratigraphic Superposition
In any succession of sedimentary strata, the order in which strata were deposited is from the bottom to the top
Useful theory but it isn’t always true as there could be magma that flowed through a crack
Model
Simplified version of the natural world
could be physical or a mathematical algorithm
Paradigm
When a whole branch of science is revolutionized by a new theory that is coupled with new ways of making observations and thinking
factors
Uniformitarianism
Features observed in ancient rocks can be explained by processes operating at the present day
was too strict
Principle of Actualism
The natural laws that allowed the formation of ancient features of the Earth are the same as those in operation today
Present is key to the past
System
A portion of the universe that can be separated from the rest for the purpose of observing and understanding changes
eg Atmosphere, Hydrosphere, Biosphere, Geosphere
systems can exist inside one another
Types of Systems
Isolated
Closed
Open
Isolated System
No matter or energy is lost or gained
imaginary concept
the solar system could be treated as one as not much matter escapes or comes in
Closed System
No matter lost or gained; energy may be exchanged with surroundings
Earth is approximately a closed system as only small amount of gas are lost and tiny amounts of material are added
Open System
Matter and energy are exchanged with the surroundings
atmosphere, ruver, island, forest, body, etc
Cycles
We can trace the flow of energy and material through earth systems by looking at cycles
eg energy, water, carbon, rock cycles
quantfied'= on a budget, eg resovior
Reservoir
Location where a quantity of material or energy sits
Flux
the rate at which material moves from one reservoir to another
eg heat from sun evaporating water from oceans
Largest to Smallest Reservoirs of Water
Oceans
Glaciers and other ice
Groundwater
Surface water on land
Water in the atmosphere
Water in the biosphere
Evaporation
heat from the sun evaporating water from oceans, lakes, rivers, etc
Evapo-transpiration
emissions from water vapor from plants
Water Budget
Flow in and out of each reservoir is roughly constant
Residence time of Water
in a reservoir is the average length of time a water molecule spends there
divide volume of reservoir by the rate of flow in or out
Climate Change Impact of Hydrologic Water Cycle
Flow in, and out of some reservoirs is not equal
reservoir may contract or expand
eg glaceirs are melting faster than they are replaced, and the ocean is expanding
What is included in a solar system
A single star
Numerous objects orbiting the sun
Planets, dwarfs and minor planets, asteroids, meteoroids
Comets
Satellites orbiting planets
Origin of the solar system
Entire solar system condensed from gaseous nebula by gravitationalattraction. Central dense body became sun remaining dust and gas formed disk disk eventually condensed to form planets and other bodies “
Gravity
objects in a solar system are maintained in orbit by gravity
Remain in balance between gravity pulling inward and momentum of the object
Orbits are ellipsis
Gravitational pull varies on distance
Shape of orbits
Ellipse
Sun at one focus
Speed varies faster when closer
Comets
Small bodies in highly elliptical orbits
Comet tail always points away from the sun
Compositions similar to Jovian planets
Asteroids and meteoroids
when they strike earth they become meteors as they burn up in the atmosphere
if a meteoroid makes it to the ground, it is called a meteorite
many are remmnants of plants that broke up or collided early in solar system history
samples early solar systems (chondrites)
chondrites
samples of early solar systems
maybe found in meteorites
Jovian Planets
outer 4 planets are similar in size and probable structure
neptune, uranus, Saturn, jupiter
thick hydrogen-rich atmosphere
liquid hydrogen core
denser rock core
Terrestrial planets
inner 4 planets and Earth’s moon are simialr in size and probable structure
mars, earth, venus, mercury,
Metallic core, mostly iron
denser rocky mantle (silicon, oxygen, magnesium, iron)
Mantle
Denser rocky mantle mostly silicon, oxygen, magnesium, iron
thin rocky crust and is vary variable as it depends on the rock cycle affecting each planet
Venus
almost same size as earth but very hard to study the crust, as the atmosphere is CO2 mostly aso the surface temperature just increases
mostly covered in clouds
Mercury
small planet with weak gravity and no atmosphere
Satellites
Orbit around planets
most are very small compared with the parent planet
the moon is the exception as it is similar to a terrestrial planet
Tilts of the Earths axis
the earths axis is tilted and the north and south pole take turns being tilted toward the sun
currently 23.5 degrees
Solstices
poles are tilted towards/away from the sun
Equinoxes
are when tilt is in parallel to the orbit
tilted parallelly
Precession of Equinoxes (Axial Precession)
Tilt direction rotates relative to elliptical orbit
23 000 year period
moves position of solsitices and equinoxes relative to elliptical orbit
Changes in Obliquity
41 000 year period of wobble from 21.5 degrees to 24.5 degrees and back again
Changes in Eccentricity
orbit shape
100 000 period
varies in degree of 6 ish
circular and most elliptical
Tides
The gravity of moon and lesser extent of Sun generates tides on earth

Spring Tide
full or new moon tides mean very high and very low tides when the moon and sun are in line with each other
if it is right angle to sun it makes less intense tides
Sun
sun is a typical star with a 700 00 km radius
109 times the Earth’s diameter
Electromagnetic Radiation
is the represented as waves
wavelength is inversely related to frequency
Solar Spectrum
radio waves, infared light, visible light, ultra-violet

Energy Cycle

atmospheres
gaseous envelopes that surround planets and other large bodies in the solar system
Mixture of gases and aerosols
Aerosols
liquid droplets, solid particles, that are small enough to remain suspended in the atmosphere
Earth’s Atmosphere
Extends above the land and ocean surface and fades into space between 100-1000km depending on criteria used
supports and protects life, stores moisture and solar energy, and moves earths materials
troposphere
lowest part of the earths atmosphere constantly changes from seconds to months which results in weather
longer term changes from months to billions of years are described as climate
30 years is an average time period for calculating climate averages
Temperature
measure of the average kinetic energy of molecules
Heat
Total kinetic of all molecules in a substances
changes with amount of material
Pressure
Gases are compressible
molecules exert a force on the walls of a container due to collisions
force per unit area
Pressure Variation with Altitude
Gases are very compressible
molecules are forced together by the mass of air above so density and pressure of air decrease with altitude
Isobars
contours of constant air pressure
air tends to flow from regions of high pressure to low pressure which drives winds and weather
Adiabatic
no heat is transferred between the gas and its surroundings
as gas rises in the atmosphere and expands, it does work expanding against the pressure of the surrounding gas; therefore, it cools