Physics SL
Physics SL
5
Chapters
329
Notes
Theme A - Space, Time & Motion
Theme A - Space, Time & Motion
Theme B - The Particulate Nature Of Matter
Theme B - The Particulate Nature Of Matter
Discover Matter's Forms: Solids, Liquids & Gases in Physics
Discovering Particles: Evolution of Material Structure Language
Phases Of Matter: Understanding Solid, Liquid, And Gas
Understanding Temperature: From Historical Views To Modern Scales
Internal Energy: Exploring Phases & Particle Movement
Linking KineEnergy & Temperature: Understanding The Boltzmann Constant
Unraveling Energy Transfers: Temperature & Phase Changes
Understanding Specific Heat Capacity: Water vs. Copper
Understanding Specific Latent Heat: From Ice To Vapor
Thermal Energy Transfer: Conduction, Convection & Radiation
Understanding Thermal & Electrical Conduction: A Deep Dive
Understanding Thermal Conductivity: Engineering Design Insights
Unveiling Convection: The Natural Powerhouse Behind Fluid Movement
Sea Breezes: Understanding Day-Night Ocean Wind Changes
Discover Earth's Convection: Shaping Continents Over Time
Understanding Why Winds Blow & The Magic Of Convection
Thermal Radiation & Its Impact on Everyday Objects
Black-Body Radiation: Unraveling The Secrets Of Thermal Energy
Unlocking Black Body Radiation: How Spectrum Varies With Temperature
Unveiling Wien's Displacement Law: The Key To Black-Body Emission
Unlocking the Stefan–Boltzmann Law: The Power of Black Body Radiation
Crucial Astronomy Laws: Stefan–Boltzmann & Wien’s Displacement
Unlocking Stellar Secrets: Apparent Brightness & Galaxy Discoveries
Understanding Earth's Atmosphere: The Vital 0.04% Impact
Unlocking Emissivity: Grey Bodies Vs. Black Bodies Explained
Unlocking The Mysteries: The Solar Constant & Earth's Energy Balance
Unlocking Earth's Energy Balance: Surface & Atmosphere Dynamics
Understanding The Greenhouse Effect: Earth Vs. Moon Temperatures
Why Greenhouse Gases Absorb Energy: The Science Unraveled
Earth's Climate Balance: Unveiling The Secrets Of Surface Temperature
Global Warming: The Undeniable Climate Shift We Face
Understanding The Origin Of Gas Pressure In The Atmosphere
Understanding Pressure: Solids, Liquids, and Gases Explained
Understanding Avogadro's Number & The Significance Of The Mole
Gas Laws: A Deep Dive Into Boyle's, Charles's, And Avogadro's Discoveries
Unlocking the Secrets: A Deep Dive into Gas Molecules and Brownian Motion
Kinetic Model Of Ideal Gas: A Comprehensive Exploration
Linking Temperature to Kinetic Energy: Dive into Ideal Gas Theory
Understanding Real vs. Ideal Gases: Key Insights
Understanding Gas Behavior: Real vs. Ideal Interactions
Thermodynamics Basics: Systems, Surroundings, and Energy Transfer
Unlocking The First Law of Thermodynamics: Insights & Examples
Pressure-Volume Diagrams: Visualizing Gas Work & Processes
Unlocking Gas Behavior: Dive Into P–V Diagrams & Thermodynamics
Isobaric Change: Delve Into Thermodynamics & Gas Laws
Isovolumetric Change: Understanding Constant Gas Volume
Understanding Isothermal Changes: The Basics Explained
Understanding Adiabatic Changes: Insight & Implications
Unlocking The Secrets Of Heat Engines: A Deep Dive
Understanding Refrigerators & Heat Pumps: Energy Transfers Explained
Mastering Thermodynamics: Fun With Physics!
Entropy & Thermodynamics: The Macroscopic Viewpoint Explained
Understanding Entropy: From Microscopic Interpretation To Real-World Implications
Discovering Electrification: From Ancient Greeks To Modern Science
Understanding Metal Conduction: From Atoms To Electrons
Understanding Electric Current: From Electrons To Amperes
Understanding Potential Difference & Its Role in Electrical Circuits
Unraveling The Multifaceted Effects Of Electric Current
Electromotive Force (Emf): Understanding Energy Transfers In Circuits
Understanding Electrical Power: From Basic Concepts To Advanced Applications
Mastering Current & Potential Difference: Analogue Vs. Digital Meters
Understanding Electrical Resistance: From Electron Interactions to Everyday Applications
Understanding Ohm’s Law: From History To Practical Applications
Understanding Non-Ohmic Behavior: Beyond Ohm's Law
Unlocking Resistivity: Key Insights & Practical Explorations
Mastering Resistor Combinations: Series & Parallel Explained
Explore Variable Resistors: How They Adjust To Your Needs
Unraveling Thermistors: NTC's Unique Temperature-Resistance Relation
Unlocking The Secrets Of Light-Dependent Resistors
Understanding Variable Resistors & Potentiometers: A Deep Dive
Master Heating Equations & Energy Conversion Calculations
Unlocking The Secrets Of Electric Cells & Batteries: DC Devices Explored
Chemical Vs. Solar Cells: A Deep Dive Into Energy Sources
Internal Resistance & EMF: Decoding Cell Dynamics
Power Matching in Cells: Maximizing Circuit Efficiency
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 B - The Particulate Nature Of Matter
Physics SL
Physics SL

Theme B - The Particulate Nature Of Matter

Thermal Radiation & Its Impact on Everyday Objects

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

Table of content

Thermal radiation basics 🌟

  • What is it? Thermal radiation is how energy is transferred using electromagnetic radiation.
  • Special Power: Unlike other forms of heat transfer (like conduction & convection), it doesn't need a material to move through. It's like a superhero that doesn't need air to fly!
  • Sun's Radiance: Think about it – the Sun's energy travels through a whopping 150 million km of the vacuum to give us that warm, sunny day!

Real-world Example: Ever stood outside on a sunny day? Even if it's cold out, the sun's rays can still make you feel warm. That’s thermal radiation in action!

Science behind it 🔬

  • Thermal Motion: Atoms move around randomly due to heat. Inside these atoms are charged particles.
  • Electromagnetic Radiation: When these charged particles speed up (or are accelerated), they emit electromagnetic radiation.

(For those super keen, there's even more info on page 401.)

Black vs. ⚪ white surfaces 🖤

Let's Do an Experiment! Ever wonder why some objects feel hotter than others?

  • The Setup: Two tin cans (twins!). One painted matt black, the other shiny white.
  • Heat 'em up: Fill them with equal amounts of hot water.
  • Watch & Record: Place the thermometers in. Observe how the temperature changes over time.
  • Graph Time: Plot a graph (cooling curve) to visualize the results.

Flip the Experiment!

  • Start with cold water and warm them up with a radiant heater.

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

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IB Resources
Theme B - The Particulate Nature Of Matter
Physics SL
Physics SL

Theme B - The Particulate Nature Of Matter

Thermal Radiation & Its Impact on Everyday Objects

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

Table of content

Thermal radiation basics 🌟

  • What is it? Thermal radiation is how energy is transferred using electromagnetic radiation.
  • Special Power: Unlike other forms of heat transfer (like conduction & convection), it doesn't need a material to move through. It's like a superhero that doesn't need air to fly!
  • Sun's Radiance: Think about it – the Sun's energy travels through a whopping 150 million km of the vacuum to give us that warm, sunny day!

Real-world Example: Ever stood outside on a sunny day? Even if it's cold out, the sun's rays can still make you feel warm. That’s thermal radiation in action!

Science behind it 🔬

  • Thermal Motion: Atoms move around randomly due to heat. Inside these atoms are charged particles.
  • Electromagnetic Radiation: When these charged particles speed up (or are accelerated), they emit electromagnetic radiation.

(For those super keen, there's even more info on page 401.)

Black vs. ⚪ white surfaces 🖤

Let's Do an Experiment! Ever wonder why some objects feel hotter than others?

  • The Setup: Two tin cans (twins!). One painted matt black, the other shiny white.
  • Heat 'em up: Fill them with equal amounts of hot water.
  • Watch & Record: Place the thermometers in. Observe how the temperature changes over time.
  • Graph Time: Plot a graph (cooling curve) to visualize the results.

Flip the Experiment!

  • Start with cold water and warm them up with a radiant heater.

Unlock the Full Content! File Is Locked Emoji

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

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