Test 2 Study Guide - Water Chemistry & Physical Properties
Physical and Chemical Properties of Water
Molecular Structure and Bonding:
A water molecule is composed of two hydrogen atoms covalently bonded to one oxygen atom, represented by the chemical formula .
The bonds within an individual water molecule are strong covalent bonds.
Water is a polar molecule, possessing an uneven distribution of electrical charge that creates distinct partial positive and negative poles.
Intermolecular forces between adjacent water molecules consist of hydrogen bonding, where the positively charged hydrogen end of one molecule is electrostatically attracted to the negatively charged oxygen end of another.
Surface Tension Phenomena:
Hydrogen bonding creates high surface tension in liquid water.
Example 1: A metal paper clip can float on the surface of liquid water despite being denser than water, supported entirely by cohesive surface tension forces.
Example 2: Water forms a distinctive rounded bead when dripping from a dropper or surface rather than spreading flat, driven by surface tension minimizing surface area.
Thermodynamic Definitions and Comparison:
Specific Heat: The precise amount of heat energy required to induce a unit change in temperature per unit mass of a given material.
Heat Capacity: The total amount of heat energy required to induce a unit change in temperature for a given mass or body of material.
Comparing heat capacities demonstrates water's exceptional ability to absorb large amounts of heat energy with minimal temperature variation.
Density Dynamics and Thermal Anomalies:
As liquid fresh water cools from higher temperatures down to , its density increases continuously as thermal molecular motion decreases.
Liquid water achieves its absolute maximum density at .
As liquid water cools further from down to , its density counterintuitively decreases as molecules expand into a rigid hydrogen-bonded crystal lattice.
During the phase transition from liquid water to solid ice at , a sharp decrease in density occurs, allowing ice to float on liquid water.
Ocean Salinity, Temperature, and Density Dynamics
Effects of Salt on Thermal Behavior:
As salinity increases, the temperature of maximum density for liquid water continuously decreases (represented visually by the pink line on T-S property diagrams).
As salinity increases, the initial freezing temperature of seawater continuously decreases (represented visually by the black line on T-S property diagrams).
Adding dissolved salt depresses the freezing point of water, requiring colder temperatures for ice formation compared to pure fresh water.
Temperature-Salinity-Density Diagrams:
Seawater density is determined simultaneously by temperature and salinity, plotted on Temperature-Salinity (T-S) diagrams.
Contour lines on a T-S diagram represent lines of equal density (isopycnals).
Cold and salty water masses have the highest density, causing them to sink toward the ocean floor.
Warm and fresh water masses have lower density, causing them to float at or near the surface.
Surface Salinity Variations:
Surface salinity at any given latitude is determined by local hydrological fluxes of evaporation and precipitation.
Evaporation removes pure water molecules into the atmosphere, concentrating salts and increasing surface ocean salinity.
Precipitation adds fresh water to the surface ocean, diluting salt concentrations and decreasing surface ocean salinity.
Oceanic Chemical Inputs and Outputs:
Inputs supplying dissolved constituents to the ocean include:
River runoff carrying weathered continental minerals.
Volcanism releasing gases and compounds into the ocean and atmosphere.
Mid-ocean ridge hydrothermal systems leaching elements from ocean crust.
Organic decay breaking down biological material and releasing dissolved nutrients.
Outputs removing dissolved constituents from the ocean include:
Chemical absorption and mineral precipitation.
Sea spray driving salt particles into the atmosphere.
Biological uptake by organisms constructing tissue and hard structures.
Sediment deposition permanently burying elements on the ocean floor.
Marine Calcium Carbonate and Mineralogy
Calcium Carbonate Polymorphs:
Calcium carbonate () in marine systems primarily forms two mineral polymorphs: Aragonite and Calcite.
Both Aragonite and Calcite are utilized by marine organisms to construct protective shells and structural skeletons.
Magnesium Control:
The presence and concentration of Magnesium () ions in seawater determines whether Aragonite or Calcite is preferentially precipitated by marine calcifiers.
Geological and Ecological Significance:
Calcium carbonate minerals are critical to:
Shell and skeleton synthesis for marine life.
Global biological carbon cycle dynamics.
Ocean buffering capacity.
Accumulation and composition of marine sediments.
Determining depth zones, such as the carbonate compensation depth, which are susceptible to ocean acidification.
Scientific Measurement Methods:
Paleoceanographers measure historical ocean chemistry and mineral conditions by analyzing fluid inclusions trapped inside ancient rock salt (halite) crystals.
The Marine Carbonate System and Ocean Acidification
Chemical Components of the System:
The marine carbonate system consists of four primary dissolved carbon species maintaining chemical equilibrium:
Dissolved carbon dioxide ()
Carbonic acid ()
Bicarbonate ions ()
Carbonate ions ()
Equilibrium Processes:
The species are coupled through air-sea gas exchange, acid-base equilibrium reactions, and relative levels.
Baseline Ocean Chemistry:
A healthy, standard open ocean maintains an alkaline of approximately
Ocean Acidification Drivers and Dynamics:
Ocean acidification is defined as the persistent decrease in ocean caused by the ocean absorbing elevated concentrations of atmospheric
Key human drivers releasing excessive atmospheric include:
Burning of fossil fuels.
Industrial cement production.
Deforestation.
Absorbed reacts with seawater to form carbonic acid (), increasing hydrogen ion concentration and lowering overall .
Biological Impacts on Calcifying Organisms:
Acidification depletes available carbonate ions () in seawater.
Reduced carbonate availability causes diminished skeletal growth in calcifying marine organisms.
Acidification causes structural alterations and changes in skeletal growth patterns, compromising organism shell integrity.
Marine Nutrients, Ocean Ventilation, and Paleoclimate Events
Essential Marine Nutrients:
Primary chemical nutrients necessary for biological productivity include Carbon, Nitrogen, Phosphorus, and Iron.
Nutrient Stratification and Photosynthesis:
Nutrient concentrations are heavily depleted in surface waters due to continuous biological uptake by phytoplankton.
Low surface nutrient levels act as a primary limiting factor that slows down rates of photosynthesis.
Ocean Ventilation Process:
Ventilation is the physical transport process that transfers surface water from the upper mixed layer down into the deeper ocean interior, distributing dissolved gases and regulating ocean chemistry.
Paleocene-Eocene Thermal Maximum (PETM):
The PETM was a major deep-time paleoclimate event that serves as a natural geological analogue for rapid carbon input and rapid global warming.
Sediment core analysis reveals that the onset of rapid input coincides exactly with the appearance of dark-colored sediment layers.
During the PETM, massive carbon input overwhelmed the seawater buffering system, converting dissolved carbon into excessive carbonic acid and driving rapid ocean acidification.