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Chemical and Physical Features of Seawater

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1 Chemical and Physical Features of Seawater
Chapter 3 Chemical and Physical Features of Seawater

2 Properties of Water Low Density of Ice Temperature Moderation
Dissolves Substances Cohesion and Adhesion*

3 Low Density of Ice As temperature rises, hydrogen bonds break and evaporate Seawater Fresh water Colder = denser until frozen Cold water sinks Colder = denser only to 4°C Below 4°C = less dense

4 Heat and Water In ice, hydrogen bonds must be broken before molecules can move around No hydrogen bonds = melt at -90°C (-130F) Latent heat of melting: the amount of heat required to melt Higher than any common substance Heat capacity: amount of heat needed to raise temperature by a certain amount Latent heat of evaporation: the amount of heat required to evaporate Evaporative cooling: fastest molecules leave liquid *Water does not change temp easily.

5 Water as a Solvent Universal solvent Dissolves salts well
Salt ions are attracted to polar water molecules Ability to transport minerals easily

6 Seawater Volcanoes: gases released into atmosphere and then into water as precipitation Substances come from various sources Weathering: chemical breakdown from rocks into rivers Hydrothermal vents: minerals from Earth’s interior

7 Seawater Salt Composition
Only 6 ions compose over 99% of solids dissolved in seawater 85% = Sodium and Chlorine Salinity: total amount of salt dissolved in seawater # grams left when 1,000g evaporated psu = practical salinity units Average = 35 0/00 Open ocean =33 to 37 Red Sea = 40 0/00 Baltic Sea surface = 7 0/00

8 Composition of Seawater
Rule of constant proportions: relative amounts of the various ions ins seawater are always the same Salinity can change

9 Salinity, Temperature, Density
Saltier/colder= denser Salt water freezes at lower temps than fresh Density is controlled more by temperature Temp varies

10 Dissolved Gases Oxygen Carbon dioxide Nitrogen
0 – 8 mL dissolved per L of seawater Avg= 4-6 ml/l Air = 210 mL Carbon dioxide 80% of dis gases Nitrogen Gases dissolve better in cold water

11 Transparency Sunlight needs to penetrate
Clear water most transparent to BLUE Most colors get filtered out

12 Pressure Land = 1 atmosphere (14.7 psi) Water Each 10m of depth =1 ATM
Pressure increase = gases compress Air bladders shrink

13 “The Bends”: Decompression Sickness

14 Ocean Circulation

15 Surface Circulation Most intense ocean currents are near the surface
Driven by the wind Influenced by the Coriolis Effect

16 Coriolis Effect Anything that moves over the earth’s surface tends to turn instead of moving in a straight line Earth is round and rotating Important for wind and ocean currents Northern hemisphere = deflects to the right Southern = left

17 Wind Patterns Trade winds: near equator Westerlies: middle latitudes
Blow west Westerlies: middle latitudes Blow east Polar easterlies: high latitudes Driven by heat energy from the sun Equator: heated air is less dense and rises Air gets sucked in areas to replace rising air = wind

18 Surface Currents Driven by wind Moves in a 45° angle Ekman Spiral:
Top layer pushes on bottom Moves at a 45° angle again Each layer looses speed Ekman Layer: layer affected by wind Water moves at a 90° angle from wind

19 Movement of Warm Currents
Equitorial currents: move parallel to equator Result of trade winds moved toward equator Create gyres: circular systems of current Warm water moves away from equator; cooler water moves toward it El Niño: large-scale fluctuation

20 Currents Affect Surface Temp
Eastern coasts are usually warmer Western = cooler

21 Layers of the Ocean Densest water sinks, least dense toward the surface Stratified : layers Surface layer 100 to 200m thick Mixed layer: wind, waves, currents Thermocline: sudden changes in temp Intermediate Layer 1,000 to 1,500m Main Thermocline Only open ocean Deep and Bottom Layers Below 1,500m (5,000 ft) Less than 4°C

22 Thermohaline Circulation
Form of circulation driven by changes in density Determined by temp and salinity Circulation over great distances

23 The Great Ocean Conveyor
Global thermohaline circulation Rise and fall of water throughout oceans 4,000 years Critical in regulating climate Brings oxygen to deep sea

24 Waves and Tides

25 Waves Caused by wind Crest: highest part Trough: lowest part
Height = distance between wave and trough Wavelength: distance between waves Period: time it takes for a wave to go by at one point

26 Wave Movement Water particles move in circles
Not transported Fetch: span of open water over which the wind blows Contributes to wave size Swells: smoothly rounded crests waves move away faster than the wind is blowing

27 Surf Surf: waves fall forward and break
Happens as the water becomes shallower Waves behind catch up Rogue waves: crests of two waves collide

28 Tides Rising and falling of sea surface Expose/submerge shore life
Drive circulation of bays and estuaries Trigger spawning

29 Cause of Tides Gravitational pull of moon and sun
Moon’s pull is strongest on the closest side of the earth

30 Daily Tides 2 High and 2 Low tides per day
Bulges are on opposite sides of the earth at one point in the day Full tidal cycle is 24 Hours and 50 minutes

31 Monthly Tides Sun’s affect on tides is only ½ of moon’s
Spring Tides: Tidal range increases Full and new moons: sun and moon are in line and their affects add together Nothing to do with season Neap tides: tidal range is small First and 3rd quarters

32 Variance on Earth Not all places are the same
Semidiurnal tides: 2 high and 2 low tides a day East coast, most of Europe and Africa Mixed Semidiurnal: higher 2nd tide of the day West coast Diurnal: 1 high and 1 low tide per day Uncommon Antarctica, parts of Gulf of Mexico, Caribbean, Pacific


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