Earth Sci 1 S1 Notes
Branches of Earth Science:
Geology: Internal and external changes to the land on Earth (ex. volcanoes)
Meteorology: Study of the atmosphere (properties and composition, weather + climate)
Oceanography: Studies ocean/seas (seafloor, motions, water properties)
Astronomy: Study of space/objects outside of our atmosphere (ex. planets, stars, asteriods, etc)
Steps of the Scientific Method:
State a problem
Gather info
Form a hypothesis
Test your hypothesis
Analyze results
Form a theory or conclusion
Inference: An educated guess based on observations, ex. The tree fell down, so it must have been windy
Observation: Using your eyes or scientific instruments to get information. ex. The ant has two antennae
Prediction: A statement of something that you think is going to happen in the future. ex. There will be an earthquake in San Francisco in 2 years
Doppler Effect:
The change in wave frequency during the relative motion between a wave source and its observer
Example: When a police car with its siren on passes by, the frequency of its waves will increase and it will sound more high pitched
Red-Shifted Spectra: When light is stretched, so it appears a little more to the red side of the spectrum. In astronomy, it means something is moving away from us because the waves are being stretched out.
Types of Spectra:
Continuous, source: incandescent bulb, full rainbow
Bright line, source: element
Absorption, source: star, filtered light
How to determine the composition of a star using its spectra: When you get the spectrum of a star, there will be random black lines in the spectrum, and you have to find elements that match those black lines to determine the stars composition
Converting between units:
1 cm = 0.01 meters, 100 cm = 1 meter, 1000 meters = 1 km, 1 meter = 0.001 km
Electromagnetic Spectrum:
In order from longest to shortest wavelength:
Microwaves
Radio Waves
Infrared
Visible (Red, Orange, Yellow, Green, Blue, Indigo, Violet)
UV Rays
X-Rays
Gamma
In the atmosphere, Short infrared waves are absorbed in the thermosphere and UV rays are absorbed by the ozone layer, and Infrared and Visible light reaches the Earth’s surface.
Nebular Hypothesis:
Nebula (a cloud of dust and gas) spins, contracts, then flattens
Protosun is formed
Nuclear fusion creates the sun
Space Rocks collide to form planets
4 planets that were closest to sun had their gasses heat up and the escape velocity of those gases allowed them to escape, making the 4 planets closer to the sun less gassy, creating the inner and outer planets
Relationships on a HR Diagram:
Color: Darker colors colder and dimmer
Temperature: Lighter colors (blue and white) are hotter than darker colors (red and orange)
Hottest to coldest: blue, white, yellow, orange, red
Brightness: Lighter colors are much brighter than darker colors
Lifespan: Cooler and dimmer stars live the longest (red stars)
Big Bang Theory:
All matter and energy was confined together in one hot, dense body
14 billion years ago matter spreads out
Basic elements form
Clouds of Hydrogen and Helium form
Matter comes together by gravity, forming galaxies and stars
Nuclear reactions in stars create heavier elements
Universe is still expanding
Evidence of the Big Bang:
Cosmic Background Radiation (Microwaves spread out evenly throughout space)
Red-shifted spectra
Hydrogen and Helium make up most of the atmosphere today
Age of Universe: 13.7 billion years old
Age of Solar System: 4.5 billion years old
Age of Earth: 4.5 billion years old
Inner vs. Outer Planets:
Inner:
Denser
Rockier
Smaller
Outer:
Gassy
More Moons
Bigger
Weight: The pull of gravity on an object
Mass: The amount of matter in an object
Volume: How much space an object takes up
Density: How tightly packed the particles in an object are
Density of Water:
Cold and Salty water is the densest water, which is why we have Deep Ocean currents
Warm and fresh water is the least dense and there floats above all other types of water
*Denser objects sink and less dense objects float*
Newton’s Law of Gravitation:
The farther away the object is, the less gravitational pull and the more mass it has the more gravitational pull it has. Distance has more effect than mass.
Planets:
Closest to Farthest from Sun: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune
Mercury: Biggest temperature swings between day and night because it has a very thin atmosphere
Venus: hottest planet and has acid rain
Earth: only planet known to support life and have fresh water
Mars: Red from iron and oxygen forming rust on its surface
Jupiter: Largest planet, has huge storms, wind patters somewhat similar to those of Earth
Saturn: Only planet with visible rings
Uranus: Tilts sideways on its axis
Neptune: Coldest planet, farthest from sun
Kepler’s Laws
Law of Ellipses: All objects that orbit the Sun follow elliptical paths
Formula for Eccentricity: Eccentricity = F (the distance between the foci) Ă· A (Length of line that passes through both foci and goes from one end of the ellipse to the other)
Law of Equal Areas: A line drawn from the Sun to a planet sweeps equal areas in equal time. A planets orbital velocity (speed at which the planet travels around the sun) changes as its position in its orbit changes
Law of Periods: Relates a planets period of revolution (time it takes to go around the Sun once) to its average distance from the Sun
Formula: T² = R³, where T is the planet’s period of revolution in Earth years and R is the planets mean/average distance from the sun in astronomical units (1 AU = Earths average distance to the sun, which is 150 million km)
Seasons:
Caused by Earth’s tilt as well as direct and indirect rays
Equinox: When Direct Rays hit the equator
12 hour day and night everywhere
Mar and Sep 21st or 22nd
Solstice: When Direct Rays hit one of the Tropics
Summer Solstice (Jun 21st or 22nd): Direct Rays hit Tropic of Cancer (23.5N) and North Pole has 24 hours of daylight, South Pole has 0 hours of daylight. Northern Hemisphere is in Summer, Southern is in Winter
Winter Solstice (Dec 21st or 22nd): Direct Rays hit Tropic of Capricorn (23.5S) and South Pole has 24 hours of daylight, North Pole has 0 hours of daylight. Southern Hemisphere is in Summer, Northern in Winter
Perihelion (Jan 4): When Earth is closest to the sun
Aphelion (Jun 4): When Earth is farthest from the sun
Rotation: Rotating on an axis, the time it takes to complete one rotation is 1 day
Revolution: Earth (or any object) orbiting the Sun (or any other object), time it takes to complete 1 revolution is a year
Cause of Direct and Indirect Rays:
Due to Earth’s shape, direct rays hit the area between the Tropics at a 90 degree angle, but the farther you get away from them, the more indirect rays you get, and the poles have the most indirect rays.
Places that receive indirect rays are generally cooler
Heat Transfer:
Conduction: When heat is transferred through solids by direct contact. Ex. Walking on sand.
Radiation: Transfer of heat through empty spaces in the form of waves. Ex. The Sun’s heat.
Convection: Density driven, particles move as a current, in liquids and gases due to uneven heating.
Heating and Cooling of Land vs. Water:
Water needs a lot more heat to warm up and cool down, which is why coastal areas have milder climates than landlocked areas
Water needs more heat to warm up and more time to cool down because it has a low specific heat
Milankovitch Cycles:
Eccentricity: How Elliptical the Earth’s orbit is. Changes every 100,000 years
Axial Tilt: The tilt of the Earth’s axis changes between 21.5 and 24.5 degrees every 41,000 years
Precession: Earth’s “wobble” on its axis as it orbits around the sun, changes every 26,000 years
For Milder Climate:
Less Eccentricity: Less difference between Perihelion and Aphelion means more milder seasons
Less Axial Tilt: So each Hemisphere does not get much more radiation in the summer than it does in the winter
Less Precession: Less Direct Rays in Summer means milder summers and More Direct Rays in winter means warmer winters
Convection Currents:
Uneven heating
Direct vs. Indirect Rays
Absorbers & Reflectors
Wind is a portion of the convection current
Low Pressure —> Low density
High Pressure —> High density
Land and Sea Breezes
Uneven heating
Specific Heat of land vs. water
Mountain and Valley Breezes
Differences in Elevation
Thunderstorms:
Air rises to form a cloud
Downdraft forms from precipitation
Downdrafts take over and storm dies
Lightning:
+ charged particles build at top of cloud at base, where - charged particles
Changes in ground get repelled and + are attracted
A step leader made of - charged particles heads towards the ground to meet with a + streamer. When the 2 meet, you get lightning
Thunder:
Caused by warm air rapidly expanding and cold air rushing in to replace
Low vs. High Pressure Centers:
Low: Air rises, wind rushes inwards towards L and turns counter clockwise. Cyclones, clouds and storms near fronts
High: Air sinks, wind rushes outwards and clockwise in Northern Hemisphere. Anticyclones, clear skies and dry, at the center of an air mass.
Hurricanes:
Late summer to early fall, when ocean is warmest
Fuel = warm, moist, rising, air
Stages of Development
Tropical Depression (Series of thunderstorms)
Tropical Storm (35+ mph)
Hurricane (75+ mph or 64 knots)
Trade Winds push them towards US, then the Westerlies move them along the eastern coast of the US
Storm dies if:
If it makes landfall —> No moist air to keep it going
If it goes over colder areas —> Air can’t rise
Eye: calm, eyewall has the worst winds
Damage most from storm surge
Water expands upwards from low pressure. Winds also help with this.
Hurricane Watch: 24-36 hours
Hurricane Warning: Within 24 hours
Climate:
Reasons that some places are hotter than others:
Latitude
Elevation
Costal vs. Landlocked
Direct and Indirect Rays
Reasons that some places get more precipitation than others:
Costal vs. Landlocked
Elevation
- Latitude
Direct and Indirect Rays
Coastal areas have milder climates because water absorbs a lot of sunlight and has a low specific heat and albedo
Atmospheric Terms:
Albedo —> The amount of light that a surface can reflect
Scattering —> When moving particles or radiation are forced to change paths when heading towards or away from Earth
Greenhouse effect —> The process by which heat is trapped in the atmosphere and re emitted by greenhouse gases (Carbon Dioxide, Methane, Water Vapor, etc.)
Atmospheric Pressure: The weight on top of you in the atmosphere, decreases with altitude.
Layers of the Atmosphere:
Troposphere - Thinnest layer, Gets colder with altitude as pressure decreases and it gets away from the heat of the Earth’s surface; also responsible for weather
Stratosphere - Contains the ozone layer, Gets warmer by absorbing UV rays
Mesosphere - Coldest layer, temperature and pressure decrease as the layer gets away from the warmth of the ozone layer, also where meteors burn up
Thermosphere - Warmest layer, Nitrogen and Oxygen in it absorb short wave radiation, also where auroras form
Moisture Vocabulary:
Dew point: The temperature at which the air is saturated. Needed for clouds to form
Relative humidity: The amount of water vapor currently in the air compared to the amount that can be in the air; expressed as a percent
Specific humidity: The maximum amount of water vapor that can be in a certain amount of air at one time
Saturated air: Air that is at the dew point and its relative humidity is 100%
Psychrometer: Instrument used to measure the humidity of air
Latent Heat: The heat used by a substance to change between states of matter
Temp stays the same during a phase change because the heat is being used to change phases
Evaporation: The process by which liquid water is turned into a gas (water vapor)
Condensation: The process by which water vapor becomes liquid water
Sublimation: The process by which a substance goes straight from a solid to a gas
Adiabatic cooling: Cooling caused by a change in air pressure
Requirements for Clouds to Form:
Rising, moist, warm air
Condensation nuclei
Low Pressure (so air rises)
Expanding air
Adiabatic Cooling
Relative Humidity Formula:
(Relative Humidity Ă· Specific Humidity) * 100 = Relative Humidity (%)
Air Masses:
Maritime Polar —> cold, wet, cloudy
Maritime Tropical —> warm, wet, cloudy
Continental Polar —> cold, dry, clear
Continental Tropical —> warm, dry, clear
Types of Fronts:
Warm Fronts
Slow moving
Brings cirrus clouds followed by stratus-type clouds
Brings steady precipitation followed by warmer temps
Cold Fronts
Faster
Bring cumulus-type clouds
Brings heavy precipitation followed by colder temps
Stationary Fronts
When a warm and cold front collide
Similar weather to warm fronts
Occluded Fronts
Cold front overtakes a warm front until the warm front is not in contact with the ground
Similar weather to cold fronts
Deep Ocean Currents:
Caused by differences in density from salinity and temperature differences
North Atlantic Deep Water, Antarctic Bottom Water
Start at the poles and eventually the North Atlantic Deep Water and Antarctic Bottom Water upwells and allows surface currents to travel from the equator northward bringing warm water along our coast (The Gulf Stream)
These start the Great Ocean Conveyor a giant convection current in the ocean that transfers heat, oxygen, and nutrients
Surface Currents (Gyres):
Affected by winds and Coriolis effect and location of continents
Spin Clockwise in Northern Hemisphere, Counter clockwise in Southern Hemisphere
Named for what they border
Currents from the Equator are Warm, currents from the poles are cold
Ex. California (cold), Brazil (warm), Canary (warm), etc.
CO2 and Temperature:
As CO2 levels increase, climates get warmer because CO2 is a greenhouse gas, so its a positive feedback loop that helps accelerate the greenhouse effect, allowing for more energy to be re emitted back towards Earth
Climate Change over the past 800,000 years:
CO2 levels have increased during interglacial periods and decreased during glacial periods
Climate Change Indicators:
Rising sea levels
More ocean acidification
Increased CO2 levels
Increased methane levels