Physics HL
Physics HL
5
Chapters
329
Notes
Theme A - Space, Time & Motion
Theme A - Space, Time & Motion
Mastering Motion: Scalars Vs. Vectors Explained
Scalar Vs. Vector: Dive Into Speed & Velocity Insights
Master Distance-Time Graphs: A Student’s Journey Explained!
Understanding Instantaneous & Average Speed: A Student's Journey Explained
Understanding Acceleration: Dive Into Physics & Spreadsheets
Mastering Distance-Time Graphs: Speed, Velocity & Acceleration Insights
Mastering Kinematic Equations: Dive Into Distance-Time & Speed-Time Graphs
Unveiling Kinematic Equations: Dive into Motion Analysis
Incredible Dog Catch Explained: Dive Into Physics!
Gravity's Grip: Understanding Earth’s Acceleration Variances
Understanding 2D Projectile Motion: Beyond Basics
Understanding Horizontal & Vertical Motion in Physics
The Unrealistic Nature of Neglecting Air Resistance
Understanding Air Resistance's Impact on Vertical Motion
Comparing Trajectories: Vacuum Vs. Air Resistance (Figure 24)
Unveiling The Mystery Of Forces: From Aristotle To Modern Physics
Unraveling Newton's Laws of Motion: The Ultimate Guide to Force and Acceleration
Unveil The Science Of Motion: Master Free-Body Force Diagrams Easily!
Unraveling The Mysteries of Translational Equilibrium
Unlocking The Secrets Of Hooke's Law And Elastic Forces
Master The Physics Of Springs: Series Vs Parallel!
Uncover The Secrets of Buoyancy Forces!
Unraveling the slippery secrets of friction
Uncover The Mysteries Of Friction Forces
Understanding Air Resistance: The Record-Breaking Skydive Of Alan Eustace
Stokes' Law: Dive Deep Into Fluid Dynamics & Viscosity
Understanding Force & Momentum: From Sports To Physics
Newton's Cradle: Visualizing Momentum Transfer and Collisions
Unraveling Newton's Third Law: Momentum Conservation Explored
Understanding Momentum Conservation: The Recoil of Guns & Water Hoses
Helicopter Physics & Momentum: Understanding Motion & Force
Unlocking The Secrets Of Circular Motion In Theme-Park Rides
Centripetal Acceleration: Exploring Forces & Circular Motion
Centripetal Forces: Unraveling The Secrets Of Satellites & Rides
Banked Tracks Explained: Maximizing Racing Safety & Performance
Vertical Circle Motion: Unraveling The Physics Behind Thrilling Rides
Unveiling The Physics Of Energy Transfer: A Historical Dive
Understanding Energy: Transfers, Forms, and Applications
Unlocking Energy Conservation: Noether's Pioneering Principle
Coriolis' Insight: Understanding Work Done & Energy Transfer
Understanding Force-Distance Graphs: Unlock Energy Calculations
Unraveling Power: Renee vs. Phillipe's Climb Explained
Key Factors Determining a Car's Maximum Speed
Unlocking Kinetic Energy: Equations & Real-Life Examples
Unveiling The Secrets of Mechanical Energy
Unlocking Gravitational Potential Energy: Earth's Conservative Force
Unlock The Secrets Of Elastic Potential Energy
Unlock The Secrets Of Energy Flow With Sankey Diagrams
Unlock The Power Of Energy Density!
Unveiling The Truth Behind Fossil Fuels Extraction
Master The Concept Of Moment Of Inertia!
Unlock The Secrets Of Angular Acceleration!
Unlock Rotational Motion Secrets: Essential Guide & Examples
Unravel Rotational Mechanics: From Graphs To Equations!
Unleash The Secrets Of Rotational Motion!
Unveiling The Secrets of Forces and Torque
Unveiling Newton’s Third Law of Rotational Motion
Unlock The Secrets of Angular Momentum in Sports & Universe!
Unlocking Angular Impulse: Rotational Dynamics Simplified
Unlock The Secrets Of Angular Momentum Change!
Master The Art Of Motion: Rolling Vs. Sliding
Unlocking the Mysteries of Rolling and Slipping: An Energy Perspective
Unraveling Einstein's Relativity: Maxwell's Revolutionary Theory
Unlock The Mysteries Of Spacetime!
Unlock The Secrets Of The Universe With IB Diploma Physics
Unlock The Mysteries Of The Universe With Galilean Relativity
Unlock The Mysteries Of Time Dilation And Special Relativity
Unlocking Einstein's Special Relativity With Lorentz Transformation
Unlocking Proper Length & Relativity: Deep Dive Into Lorentz Transformations
Understanding Relativistic Velocity Addition: Lorentz vs. Galilean
Invariant Spacetime Intervals: Einstein's Revelations
Muon Decay Mysteries: Unraveling Time Dilation & GPS Insights
Unraveling Spacetime: Minkowski's Visionary Diagrams and Worldlines
Unlocking Spacetime Secrets: The Invariant Hyperbola Explained
Theme B - The Particulate Nature Of Matter
Theme B - The Particulate Nature Of Matter
Theme C - Wave Behaviour
Theme C - Wave Behaviour
Theme D - Fields
Theme D - Fields
Theme E - Nuclear & Quantum Physics
Theme E - Nuclear & Quantum Physics
IB Resources
Theme A - Space, Time & Motion
Physics HL
Physics HL

Theme A - Space, Time & Motion

Stokes' Law: Dive Deep Into Fluid Dynamics & Viscosity

Word Count Emoji
690 words
Reading Time Emoji
4 mins read
Updated at Emoji
Last edited on 5th Nov 2024

Table of content

Hey Future Physicist! 🎓 Grab a drink (but not too viscous!) and let's dive into the cool world of fluids, drag, and spheres moving through them. We're talking about George Stokes' law, who was a cool Irish scientist from way back in 1851. Ready? Let's get moving!

Stokes' law 🌊

Stokes' law helps us understand how things move in fluids like water, honey, or even air. Imagine trying to swim through a pool of honey; it's going to be a sticky situation. That's what this law explains!

 

Key Concepts

  • Viscosity: It's like the "thickness" of the fluid. Honey has high viscosity (pours slowly) and water has low viscosity (pours quickly).
  • Drag Force: Imagine wearing a parachute and trying to run. The air pulls you back, and that's drag. Stokes calculated the drag force (Fd) on a sphere in a fluid as Fd=6πηrv, where:
  • r: radius of the sphere
  • v: speed of the sphere
  • η: dynamic viscosity of the fluid (e.g., 1×10−3 Pa s1×10−3Pa s for water and up to 20 Pa s20Pa s for honey).
  • Temperature Dependence: Just like how butter melts on a hot pan, viscosity changes with temperature too!
  • Laminar vs. Turbulent Flow: Imagine a calm river vs. wild rapids. Stokes' law only applies to calm, smooth flow (laminar). Real life is often more turbulent (swirly)!

Assumptions of stokes' law

  • Flow is calm and smooth (laminar).
  • Particles are perfect smooth spheres.
  • The fluid is the same all the way through (homogeneous).
  • Particles don't interact.

Moving through fluids - a tennis ball in water 🎾

Think of dropping a tennis ball in a giant glass of water. Here are the forces at play:

  • Weight (W): Gravity pulling down on the ball.
  • Buoyancy (B): The "floaty" force pushing up. Given by B = ρf​gV, where ρf​ is the fluid's density and V is the sphere's volume.
  • Drag (D): The sticky, slow-down force going up, calculated using Stokes' law.

The net force is W−B−DW−B−D, and it can also be expressed as (ρs​ − ρf​)gV−6πηrv, where ρs​ is the sphere's density.

 

The ball will keep speeding up until drag and buoyancy balance the weight. Then it reaches a constant speed called terminal speed, given by vt = 6πηr (ρs​−ρf​)gV​.

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IB Resources
Theme A - Space, Time & Motion
Physics HL
Physics HL

Theme A - Space, Time & Motion

Stokes' Law: Dive Deep Into Fluid Dynamics & Viscosity

Word Count Emoji
690 words
Reading Time Emoji
4 mins read
Updated at Emoji
Last edited on 5th Nov 2024

Table of content

Hey Future Physicist! 🎓 Grab a drink (but not too viscous!) and let's dive into the cool world of fluids, drag, and spheres moving through them. We're talking about George Stokes' law, who was a cool Irish scientist from way back in 1851. Ready? Let's get moving!

Stokes' law 🌊

Stokes' law helps us understand how things move in fluids like water, honey, or even air. Imagine trying to swim through a pool of honey; it's going to be a sticky situation. That's what this law explains!

 

Key Concepts

  • Viscosity: It's like the "thickness" of the fluid. Honey has high viscosity (pours slowly) and water has low viscosity (pours quickly).
  • Drag Force: Imagine wearing a parachute and trying to run. The air pulls you back, and that's drag. Stokes calculated the drag force (Fd) on a sphere in a fluid as Fd=6πηrv, where:
  • r: radius of the sphere
  • v: speed of the sphere
  • η: dynamic viscosity of the fluid (e.g., 1×10−3 Pa s1×10−3Pa s for water and up to 20 Pa s20Pa s for honey).
  • Temperature Dependence: Just like how butter melts on a hot pan, viscosity changes with temperature too!
  • Laminar vs. Turbulent Flow: Imagine a calm river vs. wild rapids. Stokes' law only applies to calm, smooth flow (laminar). Real life is often more turbulent (swirly)!

Assumptions of stokes' law

  • Flow is calm and smooth (laminar).
  • Particles are perfect smooth spheres.
  • The fluid is the same all the way through (homogeneous).
  • Particles don't interact.

Moving through fluids - a tennis ball in water 🎾

Think of dropping a tennis ball in a giant glass of water. Here are the forces at play:

  • Weight (W): Gravity pulling down on the ball.
  • Buoyancy (B): The "floaty" force pushing up. Given by B = ρf​gV, where ρf​ is the fluid's density and V is the sphere's volume.
  • Drag (D): The sticky, slow-down force going up, calculated using Stokes' law.

The net force is W−B−DW−B−D, and it can also be expressed as (ρs​ − ρf​)gV−6πηrv, where ρs​ is the sphere's density.

 

The ball will keep speeding up until drag and buoyancy balance the weight. Then it reaches a constant speed called terminal speed, given by vt = 6πηr (ρs​−ρf​)gV​.

Unlock the Full Content! File Is Locked Emoji

Dive deeper and gain exclusive access to premium files of Physics HL. Subscribe now and get closer to that 45 🌟

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