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Chapter 3 Chemical and Physical Features of Seawater Tides The combined effect of the gravitational pull of the moon and sun and the rotation of the earth, moon and sun. – PowerPoint PPT presentation

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Title: Chemical%20and%20Physical%20Features%20of%20Seawater


1
Chapter 3
  • Chemical and Physical Features of Seawater

2
Atoms and Elements
  • All matter is made of atoms
  • There are 118 types of atoms.
  • Different types of atoms are elements
  • The primary difference in elements is the number
    of protons (atomic number)

3
Molecules
  • Two or more atoms chemically combined
  • Water H20
  • Opposite charges
  • Oxygen is (-)
  • Hydrogen is ()
  • Water is a polar molecule

4
  • Polarity of Water gives it Specific Properties
  • Surface tension
  • Adhesion
  • Cohesion
  • Capillarity

hercules.gcsu.edu/.../hydro/slides/capillary.gif
Cohesion molecules stick to same type of
molecule Adhesion molecules stick to other
types of molecules
http//colin.barschel.net/gallery/d/700-4/floating
_paperclip.jpg
5
Water is unique. Why?
  • Naturally occurs in all three states
  • Solid, liquid, and gas
  • No other substance on earth does this

6
Three States of Water
  • Solid (ice)
  • Liquid
  • Gas (steam)

7
Fig. 3.2
All particles are in motion. Evaporation occurs
when particles break free of hydrogen bonds at
the surface.
8
Fig. 3.3
9
Density and State
  • As liquid water cools, molecules move slower,
    pack closer together and take less space.
  • Density mass / volume
  • As liquid water cools, Mass stays the same, but
    volume decreases, so density increases
  • When liquid turns to solid, the volume increase
    and density decreases
  • Cold water sinks, but ice floats
  • Fresh water is densest at 4oC

10
Why arent solids densest?
  • As liquids cool to solid form, the molecules move
    even less.
  • Hydrogen bonds take over and lock molecules into
    a three-dimensional fixed pattern a crystal
  • Important oceans dont freeze from the bottom up!

11
Energy (heat) is required to break hydrogen bonds.
  • Latent heat of melting the amount of heat
    required to melt a substance
  • Heat capacity the amount of heat needed to
    raise a substances temperature by a given
    amount.
  • One calorie is the amount of energy needed to
    raise one cubic centimeter of water 1oC
  • One food Calorie (kcal) is 1000 calories.

12
  • Latent heat of evaporation the amount of heat
    required to convert a substance from liquid to
    gas.
  • Evaporative cooling As faster moving molecules
    escape, the ones left behind have a lower share
    of kinetic energy, so they are cooler!

13
Fig. 3.4
As water evaporates, the exposed seaweed shrivels
in the sun.
14
Universal Solvent?
  • Universal Solvent - A substance that has the
    ability to dissolve both bases and acids, such as
    water.
  • Water is sometimes called a universal solvent
    because it is extremely common and dissolves more
    things than any other natural substance.

15
Solvents, solutes and solutions.
Solvents dissolve other substances Substances
that are dissolved are solutes. Solvents
solutes solutions
16
Fig. 3.5
Dissociation Polar water molecules cluster
around charged atoms, weakening ionic bonds.
Water molecule
17
Salts
  • Made up of particles with opposite electrical
    charges.
  • Ions charged particles
  • Either or
  • Single atoms or groups of atoms.
  • When ions pull apart, or dissociate, salts
    dissolve.

18
Salt Composition
  • 6 ions compose 99 of the solids dissolved in
    seawater.
  • Sodium and chloride make up
  • 85 of the solids
  • (sodium chloride table salt)

19
Salinity
  • Salinity the total amount of salt dissolved in
    seawater.
  • The number of grams of salt left behind from
    evaporating 100 grams of seawater.
  • If 1000 grams of saltwater leaves 35 g salt, the
    water has a salinity of 35 parts per thousand 35
    o/oo
  • Practical salinity units(psu) are equivalent to
    parts per thousand

20
Rule of Constant Proportion
  • The relative amounts of the various ions in
    seawater are always the same.
  • ie. Chloride ion is always 55.03
  • Water is added by precipitation and removed by
    evaporation or freezing

21
Tab 3.1
22
Fig. 3.6
Ions in seawater mostly come from weathering,
from hydrothermal vents, or volcanoes releasing
ions into the atmosphere
23
Salinity, Temperature and Density
  • Sea water density is determined by salinity and
    temperature.
  • It gets denser as it gets saltier and colder.

24
How Salty is the Ocean?
  • Seawater has a salinity of 35 parts per thousand
    (ppt)
  • For every 1000 g of seawater --gt 35 g of salt
  • Exactly how salty is 35 ppt?

25
Thats a lot of salt . . .
  • If salt were removed from ocean and spread evenly
    over earths land surface, it would form a layer
    about 500 feet thick (the height of a 40-story
    office building)
  • How do the seas get so salty?
  • How did the seas get here in the first place?

26
Origin of the Oceans
  • 4 bya earth was large, hot rock w/out a trace of
    water
  • Outgassing
  • Releasing of gasses from mantle through volcanic
    activity
  • Comets and meteorites brought gasses as well
  • Methane, ammonia, water vapor, carbon dioxide
  • 3.8 bya, earths surface cooled below 100C --gt
    water condensed into rain and poured onto land
    for centuries
  • Water filled basins and gravity kept it there

27
Fig. 3.7
Niskin bottles are used to sample sea water and
to test temperature
28
Fig. 3.8
29
Profile
  • A profile is a plot that shows temperature,
    salinity, or any other characteristic of seawater
    at various depths in the water column.
  • Thermoclines are sudden changes in temperature
    over a small depth interval

30
Fig. 3.9
CTDs conductivity temperature depth meters
a rosette of sampling bottles and electronic
instruments
31
Dissolved gases
  • There are gases dissolved in seawater
  • oxygen (O2)
  • 0-8 ml/l seawater (air is 21 oxygen)
  • carbon dioxide (CO2)
  • 80 of the dissolved gas in the ocean (.04 of
    the air)
  • nitrogen (N2)
  • Gas exchange Gases dissolve into the seawater at
    the surface and are released back
  • Gases dissolve better in cold than warm water.

32
Fig. 3.12
Transparency is vital for photosynthesis.
33
Fig. 3.10
Ocean surface temperature red 29.5oC, 85.1oF
(Arrow at NewGuinea)
34
Fig. 3.11
Blue light generally penetrates deepest. Coastal
waters may contain materials that absorb blue
light, making the water appear green.
All light is absorbed by 1,000 meters.
35
Fig. 3.13
A Secchi disk measures water clarity
36
Pressure
At surface, how much pressure? 1 ATM or 14.7
lbs/in2 Every 10m (33ft) of increased depth --gt 1
ATM How much pressure on a organisms that dives
to 100m? 14.7psi x 11 161 psi What happens if
that organisms surfaces too quickly?
37
Fig. 3.15
The internal air sac (swim bladder) of the
longfin grouper.
38
Ocean Circulation
39
Coriolis effect
  • Deflects large-scale motions like wind and
    current to the right in the Northern hemisphere
    and to the left in the Southern Hemisphere.

40
Fig. 3.16
Coriolis effect How would an object shot in a
straight line from the North Pole move in
relation to the earth in 2.5 hours? The earth
would rotate under it.
41
Wind
  • Wind are driven by heat energy from the sun.
  • Air is warmer at the equator than the poles.
  • warm air is less dense and rises
  • adjacent air gets sucked in to replace rising
    equatorial air, creates wind
  • winds move and are bent by Coriolis effect
  • trade winds approach the equator at 45o angle

42
Fig. 3.17
43
Fig. 3.18
44
Wind Patterns
  • What happens to the warm, rising air after it
    releases its moisture?
  • It becomes dry and cold and descends towards
    earth N S of equator.
  • Where does this happen (in terms of latitude)?
  • 30 N and S.
  • What type of environment do we usually see here?

45
Global Vegetation.
Where are the deserts located?
46
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47
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48
Low vs. High Pressure
  • Whats the relationship?
  • Low pressure
  • Hot, moist, rising air
  • Clouds and rain
  • High Pressure
  • Cool, dry, sinking air
  • Sunny
  • Notice the flow from high to low pressure---This
    is convection!!!
  • Explanation (Fig. 7o-3)

49
Ekman transport
  • Atmospheric winds push the sea surface creating
    currents.
  • The upper water layer moves at a 45o angle to the
    wind due to Coriolis effect. (Ekman layer)
  • The moving top water layer pushes the layer below
    that moves slower and to the right of the top
    layer (also Coriolis effect.)
  • Continues down the water column causing the Ekman
    spiral.

50
Fig. 3.19
Net transport is 90o from the wind direction.
Ekman Transport
51
Fig. 3.20
Net effect Trade winds move toward the Equator,
but equatorial currents move parallel to the
Equator This forms large circular systems called
gyres
Water currents bring warm water to poles, cool
water to tropics to regulate the Earths climate.
52
Fig. 3.21
Tropical organisms prefer high latitudes on west
sides of oceans. Kelp (cold-loving) occur closer
to the Equator near Eastern shores of oceans
53
Fig. 3.24
3-layered Ocean
stratified in layers or strata
54
The 3-layered ocean
  • Surface layer (or mixed layer)
  • mixed by wind, waves, and currents
  • 100-200 m thick
  • may have sharp transitions to cooler water below
    (seasonal thermoclines)
  • Intermediate layer to a depth of 1,000 to 1,500
    m.
  • main thermocline is in the intermediate layer
  • rarely breaks down
  • feature of the open ocean
  • Deep and bottom layers are below 1,500m
  • Uniformly cold, less than 4oC

55
Fig. 3.22
TYPICAL OPEN OCEAN PROFILES
b. temperature varies with latitude c. seasonal
thermoclines develop during the summer
Variation at the surface due to evaporation,
precipitation, and runoff.
56
Fig. 3.23
A high density difference results in a stable
water column.
Surface water may become more dense and less
energy is needed to mix with water below.
Downwelling occurs when the upper layers becomes
denser and displaces and mixes with deeper water.
57
Overturn
  • When surface water downwells, becoming denser
    than water below.
  • Surface water sinks, displacing lower water.
  • Occurs in temperate and polar regions during the
    winter when the surface cools.

58
Water Mass
  • Once surface water sinks, it maintains its
    salinity and temperature.
  • That volume of water (the water mass) has a
    fingerprint or characteristic identification
    based on salinity and temperature.
  • Oceanographers follow the movement of the water
    mass circulation
  • Thermohaline circulation density driven
    circulation (thus saline and temperature driven)

59
Fig. 3.25
Global thermohaline circulation critical in
regulating the Earths climate
The Great Ocean Conveyor starts with cold, salty
water in Greenland sinking and spreading.
60
Waves
  • Crest
  • Highest point
  • Trough
  • Lowest point
  • Wavelength
  • Distance between crests
  • Period
  • Average time interval (seconds) between
    successive crests or troughs of a wave

61
Fig. 3.27
Waves move energy, but not matter. The water
moves in circles, up with the crest, and down
with the trough.
62
  • The size of waves depends on
  • Speed of wind
  • Length of time wind blows
  • Fetch
  • Span of open water over which wind blows

63
Fig. 3.29
Seas Wind pushes wave crests into sharp peaks
and stretches out troughs. Swells Away from the
wind, waves settle into swells with smoothly
rounded crests and troughs.
Surf near the shore, the bottom forces the water
into elongated ellipses, slowing the wave. Waves
pile up getting higher and steeper. High and
steep enough to fall forward and break surf
64
Waves entering shallow water
  • Wave feels ocean bottom --gt friction --gt 3 things
    happen
  • Wave speed decreases
  • Wavelength decreases
  • Wave height increases
  • Whats this called?

65
  • Wave cancellation when one wave crest lines up
    with another wave trough
  • Wave reinforcement multiple waves line up crest
    to crest.
  • creates rogue waves that may be as high as a
    ten story building

66
Tides
  • The combined effect of the gravitational pull of
    the moon and sun and the rotation of the earth,
    moon and sun.
  • Centrifugal force arises because the moon doesnt
    rotate evenly around the center of the earth.
  • rotates around the earth/moon center of mass.

67
Fig. 3.30
Grunion spawn with the peak of the highest tide.
The fish climb to the highest part of the beach.
Eggs hatch a month later. High tides help the
young swim away.
68
Fig. 3.31
69
Tides Bulges
  • Why the bulge on the side opposite of the moon?
  • Centrifugal force
  • Caused by earth and moon system rotating around
    common center of mass
  • You have two bulges (high tide)
  • Whats happening at the other two places?
  • Low tide!

70
Tides Spinning
  • Because the earth spins, the place where high and
    low tides occur are constantly changing
  • Notice the red flag
  • About every 6 hours

71
Tides Spring and Neap
  • When are tidal bulges the largest?
  • When sun and moon are in line, acting
    togetherspring tides

72
Tides Types
  • Semidiurnal two high, two low
  • Mixed semidiurnal successive high tides of
    different height
  • Diurnal one high and one low

73
Tides Vary
  • Based on continents, islands and bottom
    topography
  • Continents block westward passage of tidal bulges

74
Tidal Bores
  • A high wave caused by an extreme incoming tidal
    flow
  • Shape of estuary must be shallow and uniform
  • Only occur in about 100 rivers in the world

75
Page 52
Bering Sea Current Patterns
76
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77
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78
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