EGCE-571: Hydraulics and Hydrology for Environmental Engineers Lecture 1

EGCE-571: Hydraulics and Hydrology for Environmental Engineers Lecture 1

1. Introduction and Fluid Mechanics

1.1 Introduction: Water

1.1.1 Water Resources Engineering
  • Hydraulic and Hydrologic Components:

    • Key aspects include managing both the supply and excess of water resources.

  • Water Supply Management:

    • Sources:

    • Groundwater

    • Surface water

    • Reuse of water

    • Transmission:

    • Transportation of water from sources to treatment facilities.

    • Water Treatment & Distribution Systems:

    • Methods used to clean and distribute water for use.

    • Wastewater Collection & Treatment:

    • Techniques for gathering, treating, and disposing of used water.

  • Water Excess Management:

    • Collection/Drainage System:

    • Infrastructure for collecting excess water, especially during storms.

    • Storage & Treatment:

    • Techniques for managing excess water safely.

    • Flood Control Components:

    • Implementation of dams, diversions, channels, etc.

1.1.2 Water: Unique Element
  • Chemical Composition:

    • Water is made of two hydrogen atoms (H) and one oxygen atom (O), represented as H2O.

  • Polarity:

    • Water molecules are polar, allowing them to dissolve many substances, which is critical in biological and chemical processes.

  • Phases:

    • Water can exist in three states: solid, liquid, and gas, defining its unique nature as a substance.

  • Surface Tension:

    • This property allows water to form droplets and is essential for plant uptake of water.

  • Solid Phase (Ice):

    • Ice expands upon freezing, increasing its volume by 9%, which is contrary to most liquids.

    • Ice is less dense than liquid water, causing it to float, a phenomenon beneficial for aquatic life.

1.1.3 Water: How Much Do We Have?
  • Origin of Earth's Water:

    • Space origin theories suggest water arrived on Earth via outgassing from the planet's core and meteorite collisions.

  • Distribution of Water on Earth:

    • The Solar System is approximately 4.6 billion years old.

    • Earth is often called the "blue planet", as 70% of its surface is covered with water.

    • Water content in biological systems is significant:

    • 80% of fruits and vegetables are water.

    • Human body composition: 50-70% water and 82% of blood is water.

  • Sustainability Note:

    • Humans can survive without food for several days but not without water, highlighting its critical importance.

1.1.4 Water: How Did It Get Here?
  • Water's presence on Earth is theorized to be due to:

    • Outgassing from the Earth's core.

    • Collisions with meteorites bringing in water.

1.1.5 Earth’s Water Distribution
  • The total quantity of water on the Earth is estimated at about 1386 million cubic kilometers (M km³).

    • Saline Water in Oceans:

    • 96.5% of the Earth's water is found in oceans as saline, making it crucial for understanding freshwater scarcity.

1.2 Units and Dimensions

  • Systems of Units:

    • Two systems primarily in use:

    • BG System (British Gravitational System): Also known as FPS or US customary units.

    • SI System (International System): The metric system used globally.

  • Basic SI Units:

    • There are 7 fundamental SI units:

    • Length [L]

    • Mass [M]

    • Time [T]

    • Electric Current [I]

    • Temperature [Φ]

    • Luminous Intensity [J]

    • Amount of Substance [N]

    • The units we will use in this course include:

    • Length: meter (m)

    • Mass: kilogram (kg)

    • Time: seconds (s)

  • Derived Units:

    • Created by combining basic units:

    • Force: 1 N (Newton) = 1 kg·m/s² [MLT⁻²]

    • Pressure: 1 Pa (Pascal) = 1 kg/(m·s²) [ML⁻¹T⁻²]

  • Dimensional Analysis:

    • Important principle stating that dimensions on both sides of an equation must be the same.

    • Example Formula: s = v × t

  • Unit Conversion Examples:

    • 1 m = 3.28 ft

    • 1 liter = 0.001 m³

    • 1 bar = 10⁵ Pa

Example 1.1: Units Determination

  • Calculate the units of coefficients c, k, and f(t) in the equation:
    m rac{d^{2}y}{dt^{2}} + c rac{dy}{dt} + ky = f(t)
    Where:

  • m is in kilograms,

  • y is in meters,

  • t is in seconds.

1.3 Introduction: Fluid Mechanics

1.3.1 Mechanics
  • Focuses on the behavior of physical bodies under the influence of forces.

  • Two main branches:

    • Statically equilibrium: Objects at rest.

    • Dynamic behavior: Objects in motion.

  • Classical Mechanics:

    • Newtonian Mechanics: Applies from projectiles to galaxies.

    • Relativistic Mechanics: Deals with velocities close to the speed of light (v ≈ c).

  • Quantum Mechanics:

    • Considers phenomena at the microscopic level.

Example 1.2: Force Calculation

  • Determine the net force in Newtons (N) required to accelerate a 10 kg mass at a rate of 40 m/s² (ignoring friction):

    • (a) Horizontally

    • (b) Vertically upward

1.3.2 States of Matter
  • Three Main States of Matter:

    • Solid:

    • Retains its shape and volume, does not flow easily.

    • Liquid:

    • Assumes the shape of its container but has a fixed volume, flows easily.

    • Gas:

    • Takes the shape and volume of its container, flows easily.

  • Classification of Liquid and Gas:

    • Both classified as fluids, not maintaining a fixed shape nor resisting shear forces.

Example 1.3: Comparison of Liquids and Gases

  • Similarities:

    • Both are made up of molecules and classified as fluids.

    • Molecules in both states are free to move compared to solids.

    • Molecules in each phase are in continuous random motion.

  • Differences:

    • Inter-molecular Forces:

    • Liquids exhibit strong attractive and repulsive forces, while gases demonstrate minimal forces, only strong during close interactions (collisions).

    • Viscosity:

    • Liquids have significantly higher viscosity than gases.

    • Volume:

    • Liquids maintain a definite volume, whereas gases expand to fill their container.

    • Molecular Exchange:

    • Gases exchange molecules with ambient air while liquids do not.

    • Surface:

    • Liquids form a free surface, unlike gases, which do not have a defined upper boundary.

    • Evaporation:

    • Specific to liquids, gases do not exhibit this phenomenon.

1.4 Properties of Fluid

  • Density:

    • Defined as \rho = \frac{m}{V}, with units kg/m³.

  • Specific Weight:

    • Given by \gamma = \frac{W}{V}, or \gamma = \rho g, in units of N/m³, representing weight per unit volume.

  • Temperature Dependency:

    • Density of water can be approximated by the formula:
      \rho_{water} = 1000 - \frac{(T - 4)^{2}}{180}

  • Specific Volume:

    • Defined as V_s = \frac{1}{\rho}

  • Specific Gravity:

    • Definition: s{liq} = \frac{\rho{liq}}{\rho_{water}} at 4°C

    • Reference for water: \rho_{water} = 1.0 g/cm³ = 1000 kg/m³ at 4°C

    • Example for mercury: s_{Hg} = 13.6 - 0.0024T

Example 1.4: Specific Weight, Density, and Specific Gravity Calculation

  • Given 6 m³ of oil weighing 47 kN, compute:

    • Specific weight, density, and specific gravity.

Example 1.5: Water Spill Calculation from Tank

  • Consider a cylindrical tank with:

    • Diameter = 8 m

    • Depth = 5 m

  • Water at 15°C heated to 60°C results in spillage.

  • Given:

    • \gamma_{15°C} = 9.798 kN/m³

    • \gamma_{60°C} = 9.642 kN/m³

  • Problem-solving requires analysis under constant tank volume and temperature effect.

Example 1.6: Thermal Expansion Impact on Water Spill

  • Analyze spillage in a previously discussed tank, under conditions where the tank itself has a thermal expansion coefficient of 4.6 \times 10^{-6}\frac{mm}{mm} /°C.