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267 Terms
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environmental science
the interdisciplinary study of humanity’s relationship with the other organisms and earth; it combines many disciplines such as biology, geography, chemistry, geology, physics, economics, sociology, anthropology, resource management, agriculture, law, politics, engineering, and ethics
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biological environment
encompasses the organic components, organisms (including humans) and their relationships on earth
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physical environment
consists of the incoming radiant energy of the sun, air, water, and soil which is required for life on earth
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social environment
the immediate physical and social setting in which people live or in which something happens or develops, including the culture that the individual was educated or lives in and the people and institutions with whom they interact
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Rachel Carson’s “The Silent Spring”
brought pesticide issue to public view arguing that pesticides, including DDT, were poisoning wildlife, environment, and humans
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DDT (dichlorodiphenyltrichloroethane)
* and organochloride first synthesized in 1874 * insecticidal properties not discovered until 1939 * effective control of malaria and typhus during WWII * Novel Prize in Medicine 1948 to Paul Mueller for discovery that DDT could be used as pesticide * 1950-1980: DDT used worldwide in agriculture as pesticide * US banned its use in 1972
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Scientific method
* recognize problem or unanswered question * develop hypothesis to explain problem * design and perform experiment to test hypothesis * analyze and interpret data to reach conclusions * share new knowledge with other scientists
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hypothesis
* statement, not a question * predicts the outcome of an experiment (testable) * ok to reject
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pseudoscience
trying to prove something or having an agenda
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a modest proposal
satirical essay by Jonathan Swift in 1729; proposal for preventing the children of poor people for being a burden to their parents or country and for making them beneficial to the public; suggests that the Irish might ease their economic troubles by selling their children as food for the rich
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malthusian catastrophe
English economist Thomas Malthus said that it would be impossible to maintain a rapidly multiplying human population on a finite resource base 200 years ago
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Malthus’ 3 premises
1. food is necessary for people to survive 2. passion between sexes is necessary and will remain nearly at its current rate, so children will continue to be born 3. the power of population growth is infinitely greater than the power of earth to produce subsistence
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anthrop
human
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eco
nature
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what sets humans apart
culture and technology
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what makes us a part of the ecosystem
ecological limitations
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s-shaped curve
population initially shows exponential growth, then the population numbers level out as it approaches K
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Carrying capacity (K)
The largest population a particular environment can support sustainable, assuming there are no changes in that environment
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exponential growth
the larger the population gets the faster it grows
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population ecology
a branch of biology that deals with the number of individuals of a particular species found in an area and how and why those numbers increase or decrease over time
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demography
the scientific study of the sum of our individual acts as they affect measurements of the population
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demographers/research
* study population statistics and causes/consequences of changes in population
* can help societies/governments make social, economic, political, resource use decisions for individuals, municipalities, states, and countries * enable us to understand the environmental and cultural consequences of our decisions and can help us implement the decisions necessary for the quality of life we want in the future
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migration
movement from one region/country to another to establish residency
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immigration
migration into a region/country
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emigration
migration out of a region/country
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population increase
(birth+immigration)-(deaths+emigration)
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growth rates
rate the population increases or decreases, predict future population size (cruse birth rate-crude death rate)
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crude birth rate
number of live births per 1,000 people (# of live births/total population x 1,000)
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crude death rate
number of deaths per 1,000 people (# of deaths/total population x 1,000)
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zero population growth
when birth rates=death rates (immigration=emigration)
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negative population growth
death rates outnumbers birth rates (emigration> immigration)
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Less developed countries
countries like high growth rates
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highly developed countries
countries with low growth rates
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general fertility rates
\# of live births per 1,000 women of child-bearing age (15-49
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age-specific fertility rates
\# of live births per 1,000 women of a specific age group
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total fertility rates (TFR)
average # of children a woman will bear in her lifetime (average family size)
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replacement fertility
\# of children a couple must produce to replace each parent
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age distribution
\# of individuals of each sex and age for a population
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population profiles
pyramidal: rapid growth
constructive: slow growth
stationary: no growth
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IPAT (I=PxAxT)
equation that shows the relationship between environmental impacts and the forces that cause them, where I represents impact
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atmosphere
a layer of gases surrounding a material body of sufficient mass that is held in place by the gravity of the body
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what do pressure and oxygen do as altitude increases
decrease
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troposphere
* thinnest layer, but heaviest air mass * where weather occurs (jets fly at top to avoid turbulence) * temperature decreases with altitude
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stratosphere
* in lower region temperature remains constant with altitude * in upper region, temperature increases with altitude * contains the ozone layer surrounding earth
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mesosphere
* temperature decreases with altitude * coldest temperatures in our atmosphere
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thermosphere
* temperature increases with altitude * hottest temperatures in our atmosphere
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ionosphere
* extends from the lower thermosphere into the exosphere * solar wind is deflected by the earth’s magnetic field where its charged particles emit various colors of light- creating the Aurora Borealis or Australis
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auroras
lights are always present, as close to the poles as possible, winter is usually the best time to view them, peaks every 11 years
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rotation
24 hrs
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revolution
365\.25 days
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elliptical
shape of earth’s orbit
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aphelion
july 4th, 94 million miles from earth to sun
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perihelion
jan 3rd, 91 million miles from earth to sun
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summer solstice
furthest north the sun appears to travel to those of us in the northern hemisphere (longest day of the year)
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tropic of cancer
latitude where the sun is directly overhead on the summer solstice
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winter solstice
furthest south the sun appears to travel to those of us in the northern hemisphere (shortest day of the year)
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tropic of capricorn
latitude where the sun is directly overhead on the winter solstice
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autumnal equinox
day the sun is directly overhead of the equator in the autumn
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vernal equinox
day the sun is directly overhead of the equator in the spring
internal molecular energy that flows from hot objects to cold objects
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conduction
transfer of heat through electron and molecular collisions
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convection
transfer of heat through actual movement or circulation
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thermal convection
rising warm air in the atmosphere
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advection
horizontal air currents (wind)
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radiation
transfer of heat through space from one object to another
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solar radiation
energy from the sun
* 20% absorbed by gases and clouds * 30% reflected or scattered back into space * 50% reaches earth
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4 basic principles of radiation
1. all objects emit and absorb radiant energy over a range of wavelengths 2. good absorbers are good emitters (blackbody) 3. Hot objects radiate more energy than cold object 4. hotter objects emit shorter wavelengths and higher frequencies
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electromagnetic radiation
* waves travel through space at the speed of light 300,000km/sec * solar radiation: shorter wavelength (higher frequency) emits more energy * terrestrial radiation: longer wavelength (lower frequency) emits less energy * sunlight is: 43% visible light, 49% IR, 7% UV, >1% other
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how radiation may be
absorbed, transmitted, redirected, reflected, and scattered
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diffused light
scattering of light by dust particles and gas molecules
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blue skies
scattering of blue light by nitrogen gas molecules
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red skies
scattering of red light by dust particles
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why sunsets/sunrises appear red
sunlight travels a longer path through the atmosphere at that time causing more scattering, removing shorter wavelengths (blue, violet) and leaving sunlight consisting of longer (red) wavelength
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greenhouse gases
gases that absorb infrared radiation in the atmosphere
* in the absence of GHGs, Earth’s average surface temperature, which is currently 14 C would be as low as -18 C
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special properties of water
* only liquid found in large quantities at the Earth’s surface * found in all three states at earth’s surface * great capacity to store heat * solid phase is less dense than its liquid phase (ice floats) * forms hydrogen bonds * dissolves more substances than any other solvent
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albedo effect
warmer temperatures→ less snow and ice→more sunlight absorbed by land and sea → warmer temperatures
* surface without snow or ice absorbs more heat * surface with snow and ice reflects more heat
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why water heats and cools faster than land
* water is highly mobile (heat penetrates more than surface) * water is transparent, allowing radiation to penetrate deeper than land which is opaque * evaporation more pronounced over water (cooling process is more pronounced) * specific heat of water is 3x that of land
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specific heat
amount of heat required to raise the temperature of a substance by 1 degree
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thermal inertia
resistance to a change in temperature
(a large body of water exhibits a greater resistance to temperature change than land because of difference in specific heat)
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ocean currents
transfer warm water from the equator to polar regions, and cold water to equatorial regions
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latent heat
latent heat is he energy released or absorbed by a chemical substance during a change of state that occurs without changing its temperature, meaning a phase transition such as the melting of ice or the boiling of water
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calorie
the amount of heat requires to raise the temp of 1 gram of water by 1 degree C
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melting
solid to liquid
absorbs heat from the environment
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freezing
liquid to solid
releases heat to the environment
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evaporation
liquid to vapor
absorbs heat from the environment
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condensation
vapor to liquid
releases heat from the environment
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sublimation
solid to vapor
absorbs heat from the environment
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deposition
vapor to solid
releases heat to the environment
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humidity
a general term that refers to the amount of water vapor in the atmosphere
* depending on the temp of the air, there is a certain ratio of gaseous water to liquid water * water will either evaporate or condense until this equilibrium is met
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relative humidity
percentage tells how close the air is to saturation
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saturation
100% relative humidity
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how is relative humidity changed
* adding (evaporating) or subtracting (condensing) H20 vapor * changing the temp (drop in temp, relative humidity increases)(rise in temperature, relative humidity decreases)
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dew point temp
temperature at which air capacity shrinks to cause saturation (100% humidity) and then condensation (dew)
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low dew point temp
dry air
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high dew point temperature
moist air
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clouds
visible aggregate of minute droplets of water, or tiny crystals of ice (or both)
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precipitation
when the condensation droplets get big enough, gravity takes over and this occurs
* two conditions must be met: saturation or surface
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cirrus
* clouds are high, white, and thin * they are separated or detached and form delicate veil-like patches or extended wispy fibers and often have a feathery appearance
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cumulus
* consist of globular individual cloud masses * normally they exhibit flat base and appear as rising domes or towers * cauliflower-like structure