Physics

Earth and Atmospheric Sciences

Fluid Mechanics: Fundamental Concepts, Fluid Properties (1 of 34)

In physics and chemistry, a fluid is a substance that lacks a fixed shape and yields easily to external pressure.1 While we often think of fluids as just liquids, the term technically encompasses liquids, gases, and plasmas.2

The fundamental nature of a fluid is defined by its response to “shear stress”—a force applied parallel to its surface.3 Unlike a solid, which resists such a force by deforming slightly and then stopping, a fluid will deform continuously (flow) for as long as the force is applied.4


1. Classification of Fluids

Fluids are generally categorized by how their molecules interact and how they respond to pressure.

Liquids vs. Gases5

  • Liquids: Have a definite volume but take the shape of their container.6 They are “condensed” phases where molecules are close together and held by cohesive forces.7 They are nearly incompressible.8
  • Gases: Have neither a definite shape nor volume.9 They expand to fill any container they occupy because their molecules are far apart and move independently.10 They are highly compressible.

Newtonian vs. Non-Newtonian11

  • Newtonian Fluids: The “standard” fluids (like water or air) where the resistance to flow (viscosity) remains constant regardless of the force applied.12
  • Non-Newtonian Fluids: Fluids whose viscosity changes based on how hard or fast they are hit or stirred (like Oobleck/cornstarch and water, or ketchup).13

2. Key Physical Properties

Fluid Mechanics: Pascal’s Law, Hydrostatic Pressure Variations, Manometry (2 of 34)

The “nature” of any specific fluid is determined by four primary properties:

PropertyDescriptionScientific Expression
Density (ρ)The mass of the fluid per unit volume.ρ = m / V
ViscosityThe “thickness” or internal friction of a fluid; its resistance to flowing.
Pressure (P)The force exerted by the fluid perpendicular to the surface of its container.P = F / A
Surface TensionThe “skin-like” effect on a liquid’s surface caused by the attraction of molecules to one another.

3. The “Continuum” Hypothesis14

To study fluids, scientists often use the Continuum Hypothesis.15 Even though fluids are made of discrete atoms and molecules with empty space between them, we treat them as a continuous medium.16

Instead of tracking every single molecule, we look at macroscopic properties like temperature and pressure at “points” in space.17 This allow us to use calculus to predict how weather moves, how blood flows through veins, or how air passes over an airplane wing.


4. Fundamental Laws of Fluid Behavior

Fluids follow several core principles that define their “nature” in motion and at rest:

  • Pascal’s Law: Pressure applied to an enclosed fluid is transmitted undiminished to every portion of the fluid and to the walls of the container.18 This is why hydraulic brakes work.
  • Archimedes’ Principle: Any object, wholly or partially immersed in a fluid, is buoyed up by a force equal to the weight of the fluid displaced by the object.
  • Bernoulli’s Principle: In a moving fluid, as the speed of the fluid increases, the internal pressure within that fluid decreases.19 This is a primary factor in how wings generate lift.

What is mass density?

Fluid Mechanics: Forces on Submerged Surfaces I (3 of 34)

Mass density (often simply called density) is a measure of how much matter is packed into a given amount of space.1 It describes the “compactness” of a substance.

In the context of the fluids we discussed, density is what determines whether a liquid will sink or float when mixed with another, or how much pressure a fluid exerts at a certain depth.


1. The Mathematical Formula

Density is defined as the mass per unit volume.2 You can calculate it using the following formula:

ρ = m / V

  • ρ (rho): The mass density.3
  • m: The total mass of the substance.4
  • V: The total volume occupied by the substance.5

2. Units of Measurement

Because density is a ratio, its units always combine a mass unit with a volume unit.6

  • SI Unit (Standard): Kilograms per cubic meter (7 kg/m3).8
  • Common Laboratory Unit: Grams per cubic centimeter (9 g/cm3) or grams per milliliter (10 g/mL).11
  • Imperial Unit: Pounds per cubic foot (12 lb/ft3).13

Note: 14 1 g/cm3 is exactly equal to 15 1,000 kg/m3.16


3. Density of Common Materials

Water is the universal benchmark for density.17 At room temperature, pure water has a density of approximately 1.0 g/cm3 (or 1,000 kg/m3).

MaterialDensity (approx. kg/m3)Why it matters
Air1.2Very low; why bubbles rise in water.
Oak Wood600 – 900Less than water; why it floats.
Water1,000The standard reference point.
Steel7,850Much denser than water; sinks rapidly.
Gold1819,300Extremely dense; one of the heaviest metals.19

4. What Affects Density?

Density is not always a “fixed” number; it changes based on the environment:

  • Temperature: For most substances, increasing the temperature makes molecules move faster and spread out, decreasing density. (Water is a famous exception; it actually becomes less dense when it freezes into ice, which is why ice floats).
  • Pressure: Increasing pressure squeezes molecules closer together, increasing density.20 This is very noticeable in gases (like air) but barely affects liquids (like water).21

5. Density vs. Specific Gravity

You might also encounter the term Specific Gravity. This is simply the ratio of a material’s density to the density of water.22

  • If an object has a Specific Gravity 23 > 1, it is denser than water and will sink.24
  • If it is 25 < 1, it is less dense and will float.26

What is pressure?

Fluid Mechanics: Forces on Submerged Surfaces II (4 of 34)

In physics, pressure is defined as the amount of force applied perpendicular to the surface of an object per unit of area over which that force is distributed.1

While force is a vector (it has a specific direction), pressure itself is a scalar quantity.2 This means that at any given point in a fluid, the pressure acts equally in all directions.3


1. The Mathematical Formula

The relationship between pressure, force, and area is expressed by the equation:

P = F / A

  • P: Pressure
  • F: The perpendicular force (Normal force)4
  • A: The area of the surface in contact5

2. Units of Pressure

  • Pascal (Pa): The standard SI unit, where 6 1 Pa = 1 Newton per square meter (N/m²).7
  • Atmosphere (atm): The average pressure of the Earth’s atmosphere at sea level (8 1 atm ≈ 101,325 Pa).9
  • PSI (Pounds per square inch): Commonly used in the US for tire pressure and industrial applications.10
  • Bar: Often used in meteorology; 11 1 bar = 100,000 Pa.12

3. Understanding the Relationship

Pressure is inversely proportional to the area.13 This explains many everyday phenomena:

  • The Bed of Nails: A person can lie on a bed of hundreds of nails because their weight (force) is distributed over a large total area, making the pressure at each individual nail point too low to puncture the skin.14
  • Snowshoes: By increasing the surface area of your feet, snowshoes reduce the pressure you exert on the snow, preventing you from sinking.15
  • Sharp Knives: A sharp knife has a very thin edge (tiny area).16 Even a small force creates enough pressure to cut through material easily.

4. Pressure in Fluids (Hydrostatic Pressure)

In a static fluid (a liquid or gas at rest), pressure increases with depth because of the weight of the fluid above.17 This is calculated as:

P = ρgh

  • ρ (rho): Density of the fluid18
  • g: Acceleration due to gravity19
  • h: Depth (height of the fluid column)20

5. Types of Pressure Measurements

Fluid Mechanics: Buoyancy & the Bernoulli Equation (5 of 34)
  • Atmospheric Pressure: The pressure exerted by the weight of the air in the Earth’s atmosphere.21
  • Gauge Pressure: The pressure relative to the local atmospheric pressure (e.g., what a tire gauge reads).22
  • Absolute Pressure: The total pressure, including atmospheric pressure (23 Pabs = Pgauge + Patm).24

Understanding Fluid Pressure

This video provides a visual explanation of how pressure works within fluids and the principles that govern it.

What is the relationship between pressure and depth in a static fluid?

Fluid Mechanics: Bernoulli Equation Examples (6 of 34) – YouTube

In a static fluid (a fluid at rest), pressure increases linearly with depth.1 This happens because as you go deeper, there is a greater weight of fluid resting on the area below.2

1. The Hydrostatic Pressure Equation

The relationship is defined by the Hydrostatic Equation:

P = P0 + ρgh

Where:

  • P: The total pressure at a specific depth.
  • P0: The pressure at the surface (usually atmospheric pressure, 3 ≈ 101,325 Pa).4
  • ρ (rho): The density of the fluid.5
  • g: The acceleration due to gravity (6 9.81 m/s2).7
  • h: The depth below the surface.8

If you are only looking for the gauge pressure (the pressure caused only by the fluid itself), the formula simplifies to 9 P = ρgh.10


2. Why Does This Happen?

Imagine a column of water. Each layer of water has to support the weight of all the layers above it.11

  • At the surface, there is no water above you, so you only feel the weight of the atmosphere (P0).
  • At 1 meter deep, you feel the atmosphere plus the weight of that 1 meter of water.12
  • At 10 meters deep, the pressure has roughly doubled because 10 meters of water weighs approximately as much as the entire column of air above it.13

3. Key Characteristics

  • Independent of Shape: The pressure at a certain depth depends only on the vertical height (14 h), not the width or shape of the container.15 A skinny pipe 10 meters tall exerts the same pressure at the bottom as a massive lake 10 meters deep.
  • Acts in All Directions: Pressure doesn’t just push “down.”16 Because fluids can flow, the pressure at any given point is exerted equally in all directions (up, down, and sideways).17
  • Density Matters: Denser fluids create higher pressure at the same depth. For example, because mercury is 13.6 times denser than water, you would only need to go 76 cm deep in mercury to feel the same pressure you’d feel 10 meters deep in water.

4. Real-World Examples

Fluid Mechanics: Fluid Statics Examples (7 of 34)
  • Dams: Dams are built much thicker at the base than at the top because they must withstand the significantly higher pressure at the bottom of the reservoir.18
  • Submarines: Submarines have “crush depths”—the point where the hydrostatic pressure of the ocean exceeds the structural strength of the hull.
  • Ear Popping: When you dive to the bottom of a pool, the increased pressure pushes on your eardrums, causing discomfort until you “equalize” the pressure.19

Understanding Pressure at a depth in a fluid

This video provides a clear visual demonstration of how the weight of a fluid column generates pressure and how that pressure increases as you move deeper.

What are pressure gauges?

Fluid Mechanics: Fluid Kinematics (8 of 34)

A pressure gauge is a mechanical or electronic instrument used to measure the internal force of a fluid (liquid or gas) within a closed system.1

These devices are essential for safety and performance in everything from household water heaters and car tires to industrial power plants and oil refineries.2


1. How Do They Work?

Most pressure gauges operate on the principle of elastic deformation.3 When a fluid exerts force on a flexible component inside the gauge, that component moves or changes shape.4 This movement is then converted into a readable measurement on a dial or digital screen.5

The most common mechanical design is the Bourdon Tube Gauge.6

  • The Component: A curved, hollow metal tube (shaped like a “C” or a spiral) that is closed at one end.7
  • The Action: As fluid enters the tube under pressure, the tube tries to straighten out—much like a party horn unfurls when you blow into it.8
  • The Result: This slight movement pulls a mechanical linkage that turns a gear, moving the needle on the display dial.9

2. Types of Pressure Gauges

Different applications require different ways of sensing pressure:

TypeSensing ElementBest For…
Bourdon TubeCurved hollow tubeGeneral purpose; medium to high pressures.
DiaphragmFlexible membraneCorrosive fluids or low-pressure gases.
CapsuleTwo circular diaphragmsVery low-pressure air or gas monitoring.
BellowsAccordion-like metal tubeHigh sensitivity; often used for leak testing.
DigitalElectronic transducerHigh precision; resistant to vibration.

3. Analog vs. Digital Gauges

Choosing between a traditional “dial” gauge and a modern digital one depends on the environment:

  • Analog Gauges:
    • Pros: Inexpensive, requires no power, easy to read from a distance.
    • Cons: Can be damaged by heavy vibration; prone to “parallax error” (reading the needle wrong from an angle).
  • Digital Gauges:
    • Pros: Extremely accurate, easier to read, can store data or change units (PSI to Bar) with a button.
    • Cons: Requires batteries/power; usually more expensive.10

[Image comparing an analog dial gauge and a digital pressure gauge]


4. Important Considerations

When using a pressure gauge, you’ll often see two different types of readings:

  • Gauge Pressure (psig): Measures pressure relative to the surrounding atmosphere.11 If your tire gauge says 32 PSI, it means 32 PSI above the outside air pressure.12
  • Absolute Pressure (psia): Measures pressure relative to a perfect vacuum.13 This is used in scientific applications and meteorology.

Pro-Tip: If you see a gauge filled with a clear liquid (like glycerin), it isn’t broken! The liquid is there to dampen vibrations, making the needle stay steady and protecting the internal gears from wear.14

What is Pascal’s Principle?

Fluid Mechanics: Reynolds Transport Theorem, Conservation of Mass, Kinematics Examples (9 of 34)

Pascal’s Principle (also known as Pascal’s Law) is a fundamental rule in fluid mechanics.1 It states that when pressure is applied to a confined, incompressible fluid, that pressure change is transmitted undiminished to every part of the fluid and to the walls of its container.2

In simpler terms: if you squeeze one part of a sealed bottle of water, the pressure increases by the exact same amount everywhere inside that bottle instantly.3


1. The Mathematical Foundation

Because the pressure (4 P) is the same throughout the system, we can relate two different points in a connected fluid system (like a hydraulic lift) using the formula:5

P1 = P2

Since pressure is Force (F) divided by Area (A), this becomes:

F1 / A1 = F2 / A2

This formula shows that if you have a small area (A1) on one side and a large area (A2) on the other, a small input force can be magnified into a massive output force.


2. How Hydraulics Work (Force Multiplication)

Pascal’s Principle is the “secret sauce” behind hydraulic systems.6 It allows a human to lift a 2,000 kg car with just one hand using a hydraulic jack.

  • The Setup: You push down on a small piston (small area).7
  • The Transmission: The pressure you create travels through the oil to a much larger piston.8
  • The Result: Because the second piston has a much larger surface area, the same pressure creates a much larger total force.9

The Trade-off: You don’t get “free” energy. While you multiply the force, you have to push the small piston a much longer distance to move the large piston just a few centimeters.10 This is the law of conservation of energy: 11 Workin = Workout.12


3. Real-World Applications

You encounter Pascal’s Principle every time you travel or use machinery:

  • Car Brakes: When you tap the brake pedal, you move a small piston.13 The pressure is transmitted through the brake fluid to the larger pistons at each wheel, which clamp the heavy brake pads onto the rotors.
  • Heavy Machinery: Excavators and bulldozers use high-pressure hydraulic fluid to move massive metal arms with incredible precision and strength.14
  • Medical Syringes: When a nurse pushes the plunger of a syringe, the pressure is transmitted through the liquid to push the medicine through the tiny needle.
  • The “Barrel Buster” Experiment: Legend says Pascal proved his law by inserting a long, thin tube into a sealed wine barrel. By pouring just a small amount of water into the tall tube, the pressure at the bottom increased so much—due to the height—that the barrel burst open.15

4. Necessary Conditions

For Pascal’s Principle to work perfectly, the system must be:

  1. Enclosed: If there is a leak, the pressure will escape rather than transmit.
  2. Incompressible: This is why liquids (like oil or water) are used.16 Gases (like air) compress when squeezed, which “absorbs” some of the pressure and makes the system spongy or inefficient.

Pascal’s Principle and Hydraulics

This video explains the mechanics of Pascal’s Principle and demonstrates how hydraulic systems use fluid pressure to multiply force.

What is Archimedes’ Principle?

Fluid Mechanics: Continuity Equation, Bernoulli Equation, & Kinematics Examples (10 of 34)

Archimedes’ Principle is a physical law of buoyancy that explains why some objects float and others sink.1 It states that any object, whether completely or partially submerged in a fluid, is acted upon by an upward force called the buoyant force (or upthrust), which is equal to the weight of the fluid that the object displaces.2

In simple terms: if you push a 1-liter bottle underwater, it displaces 1 liter of water. Because 1 liter of water weighs about 1 kilogram (9.8 N), the water pushes back up on the bottle with exactly 9.8 Newtons of force.


1. The Mathematical Formula

The buoyant force (3 Fb) can be calculated by finding the weight of the displaced fluid:4

Fb = ρ • g • V

  • ρ (rho): The density of the fluid (not the object).5
  • g: Acceleration due to gravity (6 9.81 m/s2).7
  • V: The volume of the submerged part of the object (which equals the volume of the displaced fluid).8

2. Sinking, Floating, and Neutral Buoyancy

An object’s behavior in a fluid depends on the battle between its weight (pulling down) and the buoyant force (pushing up).

SituationComparisonResult
Weight > Buoyant ForceObject is denser than the fluid.The object sinks.
Weight < Buoyant ForceObject is less dense than the fluid.The object rises until it floats on the surface.
Weight = Buoyant ForceObject has the same density as the fluid.Neutral Buoyancy: The object stays suspended at its current depth.9

3. The “Eureka!” Story10

According to legend, the Greek mathematician Archimedes discovered this while stepping into a bathtub.11 He noticed the water level rose as he sat down and realized he could use water displacement to measure the volume of an irregular object—specifically, a golden crown.12

King Hiero II suspected a goldsmith had replaced some gold with cheaper, less dense silver.13 Archimedes realized that if the crown was a mixture, it would have a larger volume than a pure gold bar of the same weight, thus displacing more water.14 He was so excited he allegedly ran through the streets naked shouting “Eureka!” (I have found it!).15


4. Real-World Applications

  • Ships and Boats: A massive steel ship can float because its hollow shape displaces a volume of water that weighs more than the ship itself.16
  • Submarines: They use “ballast tanks” to change their density.17 By filling the tanks with water, the sub becomes heavier and sinks; by blowing the water out with compressed air, it becomes lighter and rises.
  • Hot Air Balloons: The hot air inside the balloon is less dense than the cool air outside.18 The balloon rises because the weight of the air it displaces is greater than the weight of the balloon and its basket.19https://youtu.be/Qgl_l0H7Qgc

Archimedes Principle and Buoyancy

This video provides a helpful introduction to calculating buoyant forces and explains the core mechanics behind why objects float or sink.

What is the relationship between fluids in motion and streamlines?

Fluid Mechanics: Linear Momentum Equation and Bernoulli Equation Examples (11 of 34)

Streamlines are the “visual language” of fluid dynamics. They are imaginary lines drawn through a flowing fluid to represent its velocity and direction at a specific instant.

The relationship between fluids and streamlines is defined by how these lines map the movement, speed, and stability of the flow.


1. Velocity and Direction

By definition, a streamline is a curve where every point’s tangent is parallel to the local velocity vector of the fluid.

  • Direction: If you place a particle on a streamline, its instantaneous motion will always be along the path of that line.
  • Speed: The spacing between streamlines indicates the fluid’s speed.
    • Converging (closer) streamlines indicate the fluid is speeding up (high velocity).
    • Diverging (wider) streamlines indicate the fluid is slowing down (low velocity).

2. The “No-Crossing” Rule

A fundamental property of streamlines is that they can never cross. If two streamlines intersected, a fluid particle at the point of intersection would have two different velocities at the same time, which is physically impossible. This rule ensures that streamline flow is orderly.


3. Steady vs. Unsteady Flow

The nature of the relationship changes depending on whether the flow changes over time:

  • Steady Flow: The velocity at any given point in space does not change with time. In this case, streamlines are fixed in space. A particle entering the flow will follow the same path as the particle before it. Here, streamlines, pathlines (the actual trail of a particle), and streaklines (dye injected at a point) are all identical.
  • Unsteady Flow: The velocity at points in space changes over time (like a gusty wind). In this scenario, streamlines are just “snapshots” that change from moment to moment, and they no longer match the actual path a particle takes.

4. Laminar vs. Turbulent Flow

Streamlines help us distinguish between the two primary “moods” of a fluid in motion:

  • Laminar (Streamline) Flow: The fluid moves in smooth, parallel layers. Streamlines are clearly defined, stable, and do not mix. This typically happens at low speeds or with highly viscous fluids (like honey).
  • Turbulent Flow: The flow becomes chaotic. Streamlines break apart into swirls called eddies and vortices. In true turbulence, it is nearly impossible to draw traditional streamlines because the velocity vectors are changing so rapidly and irregularly.

5. Streamtubes

When you take a bundle of neighboring streamlines, they form an imaginary “pipe” called a streamtube. Since streamlines are always parallel to the velocity, no fluid can ever cross the “walls” of a streamtube. This allows engineers to treat a section of open air (like air entering a jet engine) as if it were contained within a solid pipe for mathematical calculations.

Would you like me to explain the Reynolds Number, which scientists use to predict exactly when smooth streamlines will break down into turbulence?

Laminar and Turbulent Flow

This video provides a visual demonstration of how streamlines behave in different flow regimes, helping you see the transition from smooth to chaotic motion.

Streamlines – YouTube

What is the equation of continuity?

Fluid Mechanics: Linear Momentum Equation Examples (12 of 34)

The Equation of Continuity is a mathematical expression of the law of conservation of mass.1 In fluid dynamics, it states that for a continuous flow, the mass of fluid entering a system must equal the mass of fluid leaving it, provided there are no sources or sinks.2

Essentially, if you squeeze a fluid through a smaller opening, it must speed up to ensure the same amount of mass passes through every second.3


1. The General Formula (Incompressible Fluids)

For most liquids (which are incompressible), the density remains constant.4 The equation relates the cross-sectional area (5 A) and the velocity (6 v) at two different points in a pipe or stream:7

A1v1 = A2v2

  • A: The cross-sectional area of the flow.8
  • v: The velocity of the fluid at that section.9
  • A • v: This product is known as the Volume Flow Rate (10 Q), typically measured in cubic meters per second (11 m3/s).12

2. Physical Implications

The equation shows an inverse relationship between area and velocity:

  • Wider Area (A increases): The fluid slows down (v decreases).
  • Narrower Area (13 A decreases): The fluid speeds up (14 v increases).15

Common Example: Think of a garden hose. When you place your thumb over the end, you are decreasing the area (A2). To maintain the same flow rate, the water must exit at a much higher velocity (v2), allowing it to spray much further.


3. General Form (Compressible Fluids)

If the fluid is a gas (where density ρ can change), the mass flow rate must be used. The conservation of mass requires:

ρ1A1v1 = ρ2A2v2

This ensures that the Mass Flow Rate (ṁ), measured in kg/s, remains constant throughout the tube.


4. Differential Form

In advanced fluid mechanics, the continuity equation is written as a partial differential equation to describe flow at a specific point in space:16

∂ρ / ∂t + ∇ • (ρu) = 0

  • ρ / t: The rate of change of density over time at a fixed point.
  • ∇ • (ρu): The divergence of the mass flux (how much mass is spreading out from or converging at that point).17
  • For steady, incompressible flow, this simplifies to $\nabla \cdot \mathbf{u} = 0$, meaning the velocity field has no “sources” or “sinks.”

Would you like me to walk through a calculation example, such as finding the exit speed of water in a narrowing pipe?

The Continuity Equation for an Ideal Fluid

This video provides a detailed derivation of the continuity equation and explains how it relates to the conservation of mass in various fluid systems.

What is Bernoulli’s Equation?

Fluid Mechanics: Energy Equation and Kinematics Examples (13 of 34)

Bernoulli’s Equation is essentially the law of conservation of energy specifically adapted for flowing fluids.1 It states that for a steady, incompressible, and frictionless (inviscid) flow, the total mechanical energy along a streamline remains constant.2

In practical terms, it describes the trade-off between a fluid’s speed, its pressure, and its height.3


1. The Mathematical Equation4

The equation is written as the sum of three distinct types of energy (expressed as pressure):5

P + 1/2ρv2 + ρgh = constant

To compare two points (1 and 2) along a streamline, we use:

P1 + 1/2ρv12 + ρgh1 = P2 + 1/2v22 + ρgh2

  • P (Static Pressure): The actual thermodynamic pressure of the fluid.
  • 1/2ρv2 (Dynamic Pressure): Represents the kinetic energy per unit volume.6
  • ρgh (Hydrostatic Pressure): Represents the potential energy per unit volume due to height (7 h).8

2. The Bernoulli Effect

The most famous takeaway from this equation is the Bernoulli Effect: as the velocity of a fluid increases, its pressure decreases (assuming the height stays the same).9

This happens because the total “energy budget” is fixed. If the kinetic energy (speed) goes up, the pressure energy must go down to compensate.10


3. Real-World Applications

  • Airplane Wings (Lift): The top of a wing is curved, forcing air to move faster over the top than the bottom.11 According to Bernoulli, this higher speed creates lower pressure on top, while the slower air underneath maintains higher pressure, pushing the wing upward.12
  • Venturi Meters: These devices measure fluid flow by narrowing a pipe.13 The fluid speeds up in the narrow section, causing a measurable drop in pressure that tells engineers how fast the fluid is moving.14
  • Chimneys: Wind blowing across the top of a chimney creates a low-pressure zone. The higher pressure inside the house then “pushes” the smoke up and out.
  • Atomizers/Perfume Sprayers: When you squeeze the bulb, air moves quickly across the top of a tube dipped in liquid.15 This creates low pressure at the top, which sucks the liquid up the tube and sprays it out.

4. Necessary Assumptions (The “Ideal” Fluid)16

Fluid Mechanics: Energy Equation Examples, Differential Continuity Equation (14 of 34)

For Bernoulli’s Equation to be perfectly accurate, the fluid must meet these criteria:

  1. Incompressible: The density (17$\rho$) must remain constant (mostly true for liquids, less so for high-speed gases).18
  2. Inviscid (Frictionless):19 No energy is lost to “thickness” or internal friction.20
  3. Steady Flow: The velocity at any point doesn’t change over time.21
  4. Along a Streamline: You are comparing points along the same path of flow.22

Bernoulli’s Equation and the Conservation of Energy

This video provides a visual derivation of the equation from the perspective of energy and work, making the relationship between pressure and speed much clearer.

Bernoulli’s Equation: Energy Conservation for Fluids | Fluid Mechanics

What are some applications of Bernoulli’s Equation?

Bernoulli’s Equation is one of the most practical tools in physics because it explains how a fluid’s speed relates to its pressure. While we often think of it in terms of massive airplanes, it also explains small “everyday mysteries.”

Here are the most common applications across various fields:


1. Aviation: Lift and Airspeed

The most famous application is the airfoil (the shape of an airplane wing).

  • Generating Lift: The top of a wing is curved, while the bottom is flatter. Air traveling over the top must move faster to meet the air underneath. According to Bernoulli, this higher speed creates lower pressure on top, while the slower air underneath maintains higher pressure, pushing the wing upward.
  • Pitot Tubes: These are the small, L-shaped probes you see on the front of airplanes. They measure “stagnation pressure” (where air stops) and “static pressure” (normal air pressure). By using Bernoulli’s equation to compare these two, the plane’s computer can calculate exactly how fast it is flying through the air.

2. Automotive: Downforce and Carburetors

  • Formula 1 Racing: Racing cars use “inverted wings” (spoilers). By using the Bernoulli effect in reverse, they create high pressure above the car and low pressure below it. This “downforce” glues the car to the track, allowing it to take corners at incredible speeds without flipping.
  • Carburetors: In older engines, air is forced through a narrow pipe (a Venturi). As the air speeds up, its pressure drops, creating a vacuum that sucks fuel into the airstream to be burned in the engine.

3. Sports: The Magnus Effect

Fluid Mechanics: Navier-Stokes Equations, Conservation of Energy Examples (15 of 34)

When a ball spins, it drags a layer of air around with it.

  • Curveballs: On one side of a spinning baseball, the spin move in the same direction as the wind, speeding the air up (low pressure). On the other side, the spin moves against the wind, slowing it down (high pressure). This pressure difference pushes the ball to the side, making it “curve.”
  • Soccer and Tennis: This same principle allows players to “bend” a soccer ball into the goal or hit a tennis ball with “topspin” so it dives back onto the court.

4. Household and Medical

  • Perfume Sprayers/Atomizers: When you squeeze the bulb, air rushes over a straw. This creates low pressure at the top of the straw, drawing the liquid up and turning it into a fine mist.
  • Shower Curtains: Have you ever noticed the curtain blowing inward when you take a hot shower? The fast-moving water and steam create a low-pressure zone inside the tub. The higher pressure outside the curtain pushes it toward you.
  • Aneurysms: In medicine, if a blood vessel develops a bulge (aneurysm), the cross-sectional area increases and the blood slows down. According to Bernoulli, slower speed means higher pressure, which pushes even harder on the weakened wall, potentially making the bulge worse.

5. Engineering: Flow Measurement

Fluid Mechanics: Viscous Flow in Pipes, Laminar Pipe Flow Characteristics (16 of 34)
  • Venturi Meters: Engineers use these to measure how much liquid is flowing through a pipe without opening it. By narrowing the pipe and measuring the pressure drop at the “throat,” they can calculate the exact flow rate using Bernoulli’s formula.

Would you like to see the math behind one of these examples, such as how much lift an airplane wing actually generates?

The Physics of the Curveball

This video explains how the Bernoulli principle combines with ball spin to create the pressure differences that make a baseball curve in mid-air.

https://youtu.be/0gEBNyBDonQ
How Does Bernoulli’s Principle Explain Curveballs? – Civil Engineering Explained

What is viscous flow?

Fluid Mechanics: Laminar & Turbulent Pipe Flow, The Moody Diagram (17 of 34)

In previous sections, we looked at “ideal” fluids where we assumed no energy was lost to friction. However, in the real world, all fluids have some degree of viscosity—a measure of a fluid’s resistance to flow or deformation.1

Viscous flow is the movement of a fluid where internal friction (viscosity) plays a significant role in its behavior.2 You can think of viscosity as “fluid friction.”


1. The Cause of Viscosity

Viscosity arises from the cohesive forces between molecules and the collisions between them as they slide past each other.3

  • In Liquids: It is primarily caused by the attractive forces between molecules. As you heat a liquid, these forces weaken, and the viscosity decreases (e.g., warm syrup flows faster than cold syrup).
  • In Gases: It is caused by the collision of molecules. As you heat a gas, molecules collide more frequently, and the viscosity actually increases.4

2. The Velocity Profile (No-Slip Condition)

Fluid Mechanics: Minor Losses in Pipe Flow (18 of 34)

In viscous flow, the fluid does not move at a uniform speed across a pipe or channel.5

  • The No-Slip Condition: Fluid molecules directly touching a solid surface (like the wall of a pipe) stick to it and have a velocity of zero.6
  • The Profile: The velocity increases as you move toward the center of the flow.7 This creates a parabolic “velocity profile,” where the fastest-moving fluid is in the very middle.8

3. Newton’s Law of Viscosity

For many common fluids (Newtonian fluids), the shear stress (9 τ) is directly proportional to the velocity gradient.10

τ = η dv/dy

  • τ (tau): Shear stress (the force per unit area applied to the fluid).
  • η (eta): The dynamic viscosity coefficient.11
  • dv/dy: The velocity gradient (how fast the speed changes as you move away from the wall).12

4. Poiseuille’s Law

Viscosity significantly impacts how much pressure is required to push a fluid through a pipe.13 According to Poiseuille’s Law, the flow rate (14 Q) is heavily dependent on the radius of the pipe (15 r) and the viscosity (16 η):17

Q = (πr4ΔP) / (8ηL)

The most critical takeaway here is the r4 term. If you reduce the radius of a pipe by half, you don’t just lose half the flow—the flow rate drops to 1/16th of its original value unless you massively increase the pressure.


5. Laminar vs. Turbulent Viscous Flow

Viscosity acts as a stabilizing force.18

  • High Viscosity: Tends to keep flow Laminar (smooth and layered). The internal friction “dampens” small disturbances.19
  • Low Viscosity / High Speed: Tends to become Turbulent. The fluid’s momentum overcomes the viscous “glue,” leading to chaotic swirls and eddies.

6. Real-World Impact

  • Blood Flow: Our hearts must exert significant pressure to push viscous blood through tiny capillaries.
  • Lubrication: Motor oil is designed with a specific viscosity to create a thin film that prevents metal-to-metal contact in engines.
  • Volcanoes: The “runniness” of lava (its viscosity) determines whether a volcano erupts explosively or flows slowly like a river.20

Solved Problems

In the traditional academic world, we are told to ‘pick a lane.’ But the atmosphere doesn’t care about academic silos. A modern hurricane is a physics problem, a data problem, and a communication crisis all at once.

Learn how we bridge these gaps: [The Starline Philosophy: The Modern Polymath]

Physics

Earth and Atmospheric Sciences