Y13 Oceans Flashcards
Reasons why oceans are important
Produces 70% atm oxygen (phytoplankton carrying out photosynthesis)
Absorbs CO2 from atm
Regulate earth temp
Distribute heat from equator to poles
Influences climate and weather
85% water added to the atmosphere comes from ocean evaporation, regulating temp
Formation of the ocean
Earth formed from dust and ice
GPE of dust and ice converted to KE, friction, hence molten surface to earth
Steam released into atm
Surface cooled, clouds formed, rain —> oceans
Comets and meteors entering earths atm add the other half of water
Properties of water
Absorb a lot of heat (high specific heat capacity)
Universal solvent - dissolves a lot of substances
Polar, so it forms a lattice when it freezes
So ice less dense than water
Strong intermolecular attraction - hydrogen bonding
Created surface tension
What is hydrogen bonding?
Strong intermolecular attraction between hydrogen and oxygen on another molecule
Define latent heat
The energy needed to change states
Latent heat of fusion - energy needed to change from solid to liquid
Latent head of vaporisation
Energy needed to change from liquid to gas
Define specific heat capacity
Amount of energy needed to raise the temperature of 1kg of water by 1C
Water has high heat capacity
So the ocean is slow to warm
Transports a huge amount of heat with only a small temperature change
Three main layers of the ocean
Mixed layer: surface
EUPHOTIC ZONE
Warmed by sunlight
Wind, waves, tides, convection currents mix this layer
Depth varies with seasons
Transition layer:
DISPHOTIC ZONE
Temp; salinity and density rapidly change
Deep layer:
APHOTIC ZONE
Fairly constant in temp and salinity
Parts of the transition layer
200m-1000m
Based on physical properties:
Thermocline - rapid temperature changes
Halocline - rapid salinity changes
Pycnocline - rapid density changes occur
Layers of the ocean in terms of light
Light is absorbed, reflected and scattered by the ocean
6% reflected at surface
65% absorbed in the first meter
Top 200m = euphotic or Protic zone = sunlight zone
200m-1000m = disphotic = twilight zone
Below 1000m = aphotic = midnight zone
Euphotic zone
Depth 50-200m, depending on turbulence and water clarity
The depth at which light drops to 1%
90% of all marine life lives here
Photosynthesis zone
Describe the temperature at different layers of the ocean
Mixed layer distributes heat, consistent
Transition layer
Thermocline, where heat energy is conducted slowly downwards, creating a temperature gradient
Temperature decreases rapidly
Deep layer: stays cold
How does the thermocline vary depending on latitude?
Upper seasonal thermocline and lower permanent thermocline
Seasonal thermocline depends on latitude
High latitude
No thermocline - low solar heating of surface layer
Mid latitudes - winter no thermocline
Summer strong thermocline. Direct sunlight and low winds so less mixing
Low latitudes - strong thermocline due to direct heating and low winds
Define salinity
The amount of dissolved salts in the ocean
Average salinity is 35ppt (parts per thousand)
How does salinity vary with layers of the ocean?
Mixed layer: similar due to mixing
Transition layer: the HALOCLINE
Deep: similar due to limited mixing
How is salinity reduced and increased
Reduced by rainfall (tropics and mid latitudes) and river runoff
Increased by evaporation (tropics) and ice formation (polar regions)
Seawater freezes, salt left behind, forming dense water which sinks
How does salinity vary with latitude
Poles: high rainfall, runoff and melting reducing salinity
Equator:
High evaporation, with rainfall reducing the effect
Tropics: Mid latitudes
Low rainfall with high evaporation, so high surface salinity
Low to high: poles, equator, tropics
What does density of the ocean depend on?
Temperature
Colder = denser
Salinity
Saltier = denser
Pressure
Deeper = denser