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

Unlocking Gravitational Potential Energy: Earth's Conservative Force

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

Table of content

What's the big idea?

Energy can't be created or destroyed, only transformed! Specifically, kinetic energy (KE) and gravitational potential energy (GPE) can swap places in a process known as energy transfer, but the total energy, called mechanical energy, stays the same. In an ideal, frictionless world, the energy exchange between KE and GPE is perfect - the energy loss from one is the exact gain for the other.

Transferring the energy, no net change

Imagine a satellite whizzing around a planet in the vacuum of space. The satellite's speed isn't constant - it speeds up and slows down, changing its kinetic energy. But the mechanical energy of the satellite stays the same, because as it gains kinetic energy, it loses gravitational potential energy, and vice versa.

Making it real - the snowboarding example

Imagine a snowboarder at the top of a 50m hill (start from rest, so initial KE = 0). As they go down the slope, they trade GPE for KE. We can't use kinematic equations (suvat) here because the acceleration isn't constant. Using energy conservation, we can find the snowboarder's speed at the bottom: v = √(2 × 9.8 × 50) = 31 m/s (that's roughly 110 km/hr!). However, this doesn't account for air resistance and friction.

 

Fun Fact: Regardless of the snowboarder's mass, the speed at the bottom remains the same, as the mass cancels out in the equations.

Practical examples

  • A ball thrown upwards: The ball's initial KE is converted into GPE at the highest point of its trajectory. Using KE = 0.5mv² and GPE = mgh, we can calculate the maximum height the ball will reach.
  • A pendulum bob: If the bob is released from a certain height, we can calculate its speed as it passes through the lowest point using conservation of energy principles (KE at the lowest point = GPE at the highest point).
  • Ski jumping: A ski jumper loses some GPE as they descend down the ramp, which is transferred into KE, but not all of it because of resistive forces (like air resistance).

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

Theme A - Space, Time & Motion

Unlocking Gravitational Potential Energy: Earth's Conservative Force

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

Table of content

What's the big idea?

Energy can't be created or destroyed, only transformed! Specifically, kinetic energy (KE) and gravitational potential energy (GPE) can swap places in a process known as energy transfer, but the total energy, called mechanical energy, stays the same. In an ideal, frictionless world, the energy exchange between KE and GPE is perfect - the energy loss from one is the exact gain for the other.

Transferring the energy, no net change

Imagine a satellite whizzing around a planet in the vacuum of space. The satellite's speed isn't constant - it speeds up and slows down, changing its kinetic energy. But the mechanical energy of the satellite stays the same, because as it gains kinetic energy, it loses gravitational potential energy, and vice versa.

Making it real - the snowboarding example

Imagine a snowboarder at the top of a 50m hill (start from rest, so initial KE = 0). As they go down the slope, they trade GPE for KE. We can't use kinematic equations (suvat) here because the acceleration isn't constant. Using energy conservation, we can find the snowboarder's speed at the bottom: v = √(2 × 9.8 × 50) = 31 m/s (that's roughly 110 km/hr!). However, this doesn't account for air resistance and friction.

 

Fun Fact: Regardless of the snowboarder's mass, the speed at the bottom remains the same, as the mass cancels out in the equations.

Practical examples

  • A ball thrown upwards: The ball's initial KE is converted into GPE at the highest point of its trajectory. Using KE = 0.5mv² and GPE = mgh, we can calculate the maximum height the ball will reach.
  • A pendulum bob: If the bob is released from a certain height, we can calculate its speed as it passes through the lowest point using conservation of energy principles (KE at the lowest point = GPE at the highest point).
  • Ski jumping: A ski jumper loses some GPE as they descend down the ramp, which is transferred into KE, but not all of it because of resistive forces (like air resistance).

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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