Apes Unit 9: Global Change

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61 Terms

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Which form of light from the sun enters the troposphere from the stratosphere?

l. UV light

ll. Infared light (IV)

lll. visible light

ll & lll (IV, visible)

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Ozone in the stratosphere absorbs what UV light?

UV-C and much of UV-B light

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tropospheric ozone =

respiratory irritant, damaging to plant tissue, precursor to photochemical smog

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human health benefits

  • prevention of skin cancer & cataracts

  • UV-B & C damage DNA (skin cancer) & can cause oxidative stress in eyes
    (cataracts)

  • UV-B &C can also suppress human system

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negative impacts of stratospheric ozone to plants

  • UV-B & C damages plant cells reducing ability to perform photosynthesis

  • Loss of plants/algae can cause breakdown of food web → loss of phytoplankton leads to no fish

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how ozone forms in the stratosphere

UV light splits an oxygen molecule (O₂):
High-energy ultraviolet (UV-C) radiation breaks apart an oxygen molecule:

O2 → (UV-C) → O + O

Free oxygen atoms react with O₂:
Each of those free oxygen atoms (O) can react with another O₂ molecule to form ozone (O₃):

O + O2 → O3

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breakdown of stratospheric ozone

UV light splits an ozone molecule (O)

O3 → (UV-C) → O2 + O

two oxygen atoms bond to form O

O + O → O2

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What is the replacement for HCFC’s?

HFC’s (GHG, but not ozone depleting (no Cl))

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what is the replacement for HFC’s?

HFO’s (HFC’s with C-C double bonds that shorten atm lifetime & GWP)

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HFO

hydrofluoroolefin

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What is the primary anthropologic cause of O3 breakdown?

CFC’s

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Anthropologic ozone depletion

UV radiation separates a chlorine atom from CFCs

highly electronegative chlorine atoms bonds to one of the oxygen atoms of O3 converting it to O2

Free O atom the bonds to O from Cl monoxide to form O2

Free Cl atom breaks down more ozone

Cl + O3 → ClO + O2

ClO + O → Cl + O2

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What circumstances cause polar stratospheric clouds (PSC) to form?

extremely cold temp. unique to the Antarctic stratosphere

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natural ozone depletion

  1. Antarctic winters (June to August)

    • extremely cold stratospheric temps., no sunlight

  2. PSC forms

    • HCI + ClONO2 → Cl2

    • Cl2 → Cl + Cl

  3. during spring (Sep. - Nov.), sunlight returns & breaks down Cl2. Cl atoms destroy O3.

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main way to reduce anthropologic O3 depletion

phasing out and replacing CFC’s

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Montreal protocol (87’)

global agreement to phase CFC’s out of production in refrigerators, aerosols, etc.

  • replaced with HCFC’s (hydrogen with hydrogen added)

  • HCFC’s still deplete O3 and acts a GHG, but to a lesser degree than CFC’s

  • not a Permanant solution, by a temporary transitioning option (phase out

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How much solar radiation is reflected back into space by clouds & atmosphere?

26%

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How much solar radiation is absorbed by atmosphere & clouds & radiated out into space & own to earth?

19%

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the greenhouse effect

Gases in earth’s atmosphere trap heat from the sun & radiate it back down to earth

  • Without greenhouse effect, earth would be too cold to support life

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how does the greenhouse effect work?

  • solar radiation (light waves like UV & visible light) strike earth surface, heating it up

  • earth’s surface releases Infared radiation

    GHGs absorb infrared radiation & radiate it both out into space and back toward earth

  • portion coming back to earth is the greenhouse effect

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Most important GHGs

  • CO2

  • CH4 (methane)

  • N2O (nitrous oxide)

  • CFCs/HCFCs/HFCs

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CO2

FF combustion, decomposition, deforestation

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CH4 (methane)

natural gas extraction & combustion, animal agriculture, anaerobic decomposition (esp. permafrost thaw)

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N2O (nitrous oxide)

agricultural soils (denitrification of nitrate, esp. in overwatered, over fertilized soils)

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global warming potential (GWP)

measure of how much a given molecule of gas can contribute to the warming of the atm. over a 100-year period, relative to CO2

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What is GWP based off of?

  • residence time

  • infrared absorption

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residence time

how long molecule stays in the atmosphere

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infrared absorption

how well the gas absorbs & radiates Infared radiation (IR)

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CO2 GWP

1

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CH4 GWP & residence time

  • 23-84

  • 12 years

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N2O GWP & residence time

  • 300

  • ~ 115 years

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CFCs GWP & residence time

  • 1600 - 13000

  • 50 - 500 years

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Why is sea level rising?

  • thermal expansion

  • melting polar & glacier ice

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thermal expansion

  • water molecules move slightly further apart when they’re heated

  • all the water molecules of ocean moving slightly apart leads to sea level rising

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melting polar and glacial ice

  • increased GHG leads to a warmer climate & more melting of ice sheets (at the poles & glaciers)

  • this water flows into the ocean and leads to sea level rise

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env. impacts of sea level rise

  • flooding of coastal ecosystems like estuaries (mangroves, salt marshes)

  • loss of species that depend on artic & tundra ecosystems (polar bears, penguins, reindeer)

  • loss of thaw-freeze cycle that glaciers go through, depriving surrounding ecosystems and human communities of water source

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human impacts of sea level rise

  • relocation of coastal human pop.

  • increase in flood frequency = higher insurance and repair costs, lost property

  • saltwater intrusion (saltwater pushing into ground water & contaminating wells)

  • refugees forced to move inland

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vectors

living organisms (usually mosquitos, ticks, fleas) that can transmit diseases from human to human or animal to human

Ex. malaria, zika, west Nile, dengue fever

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historic climate change

earth’s climate has varied over geologic time, largely due to variations in earth’s orbit around the sun

  • varies in obliquity (~40,000 yrs.) exposing northern latitudes to higher insolation at different times

  • varies in eccentricity (~100,000 yrs.) bringing it closer to and further from the sun at different times

    • more eccentric = further from sun

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Milankovitch cycles

predictable variation in Earth’s climate

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how have scientists been measuring/estimating earth’s historical temperature & CO2 levels?

  • foraminifera shells in ocean sediments - different species have different temp. tolerance

  • air bubbles in ice cores that contain ancient atmospheric gas (CO2 levels)

  • 16 vs 18O isotope concentration in ancient ice

    • increased 18O = higher temp.)

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effects of climate change

  • rising temp. → habitat/species loss, drought, soil desiccation (drying), heat waves, increased precipitation in some regions

  • rising sea levels → due to glacial, polar ice melt + thermal expansion

  • melting of permafrost → permanent frozen tundra soils that begins to thaw & release methane & CO2 from anaerobic decomposition

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impact of climate change on coastal communities

  • Property loss, damage, potential relocation: Coastal communities, especially poorer ones that can’t build up may need to relocate inland

    • Seawalls or other barriers can be built higher, but this just delays eventual flooding

  • Loss of barrier islands: islands that buffer coastal communities/ecosystems from wind & waves may be lost as sea level rises

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impact of climate change on atmospheric currents

  • Widening & weakening of Hadley cell: as temperature difference between equator and poles decreases, air ascending and expanding from equator travels further before sinking

    • This shifts subtropical zones (dry, desert biomes) toward the poles and expands the tropics

    • Regions between 300 and 60o may experience drier climate as cool, dry, descending air from Hadley cell shifts north & south

  • Weakened, destabilized Jet Stream: as arctic warms faster than other areas of earth, temperature difference between equator & poles weakens

    • Because temperature & pressure difference between polar & subtropical regions is what drives the polar jet stream, less difference between them means weaker, wobblier jet stream

      • Leads to extreme cold spells in eastern US & dry spells in western US

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impact of climate change on marine ecosystems

  • Altered range of marine ecosystems: some new marine habitats will be formed by rising sea level flooding coastline 

    • Some areas of ocean will become too deep to receive sunlight & photic zone will shift up, further from ocean floor

  • Altered ranges for organisms: warm water holds less O2, so many fish populations have declined, or migrated to cooler waters

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impact of climate change on ocean circulation

  • Suppression of thermohaline circulation: global ocean current that redistributes heat from the equator, salt, and nutrients by mixing ocean waters could slow or stop altogether

    • ice melt from Greenland → especially cold, freshwater buildup in north Atlantic

    • Freshwater is less dense than salt, preventing it from sinking

    • This cold north Atlantic slows warmer Gulf Stream waters, cooling Europe & slowing global thermohaline circulation

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unequal global warming

polar regions of earth are warming faster than other regions (polar amplification)

  • especially the arctic (N. pole) because there is more land & less water to absorb heat

    • melting sea ice = more expose ocean water, absorbs more sunlight than ice & snow, leading to more ice melting (P feedback loop)

  • distribution of tropical heat to poles by thermohaline circulation also warms poles

  • melting of permafrost

    • air pollution, adds soot/other PM to atm, distributed to poles by atm. circulation

      • darker, soot/PM covered in ice absorbs even more heat due to low albedo

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impact of climate change on polar ecosystems

artic sea ice loss = habitat loss

  • seals use it for resting & finding holes for breathing

  • algae grow on ice, forming base of artic food web

  • polar bears use ice for hunting seals at breathing holes

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9.6

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9.7

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9.8

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9.9

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HIPPCO

  • habitat fragmentation/loss

  • invasive species

  • population growth

  • pollution (pollutants)

  • climate change

  • over-exploitation

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habitat fragmentation/loss

Breaking of larger, continuous habitats into smaller, isolated patches; disrupts breeding, hunting, migration

  • Deforestation/logging (lumber, cities, roads), Wetland draining (ag, urbanization), River water level decreased by dams

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metapopulations

mostly isolated, subpopulations connected by habitat corridors; this can allow some gene flow (mating between populations) and improve genetic diversity 

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invasive species

Invasives such as z. mussel and kudzu vine outcompete native species for food/space, lowering populations

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population growth

Human pop. growth drives hab. loss, Urbanization, ag. expansion to feed more people remove/fragment hab.

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pollution (pollutants)

Oil spills reduce marine org. pop. size, Pesticides (glyphosate, atrazine) kill non-target species

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climate change

Shifts biomes & therefore species habitat ranges can change temp. & precip. patterns too rapidly for a species to adapt or migrate, causing pop. decline or extinction

sea level rise

precipitation change

  • Warming global. temp. will decrease precipitation in some areas, leading to soil desiccation and desertification

    • Will increase in some areas, expanding tropical ecosystems

temp. change

  • Warming temp. can shift biomes

    • Boreal forest & temperate coniferous forests may shift northward; tundra may decrease

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over-exploitation

Excessive hunting or poaching (faster than reproductive rate) leads to pop. decline & potential extinction

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edge effect

where two ecosystems such as forest-grassland or ocean-river (estuaries) meet have diff. characteristics than the middle of each ecosystem

  • Some species thrive in the edge habitat & biodiversity is often higher in edge habitats due to diversity of food, shelter, and nutrient resources

  • Edge habitats can expand range of potentially disruptive species (ex: brown headed cowbird) that thrive in grassland-forest edge

    • Brood parasite that leaves its eggs in the nests of songbirds for them to raise, unknowingly