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First teaching 2023

First exams 2025

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Albedo & Emissivity (HL IB Physics)

Revision Note

Katie M

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Katie M

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Emissivity

  • Stars are good approximations to a black body, whereas planets are not
    • This can be quantified using the emissivity
  • Emissivity, e, is defined as

The the ratio of the power radiated per unit area by a surface compared to that of a black body at the same temperature

  • It can be calculated using the equation

e = fraction numerator power space radiated space by space an space object over denominator power space emitted space by space straight a space black space body end fraction

  • Calculations of the emissivity assume that the black body:
    • Is at the same temperature as the object
    • Has the same dimensions as the object
  • For a perfect black body, emissivity is equal to 1
  • When using the Stefan-Boltzmann law for an object which is not a black body, the equation becomes:

P = eσAT4

  • Where:
    • P = total power emitted by the object (W)
    • e = emissivity of the object
    • σ = the Stefan-Boltzmann constant
    • A = total surface area of the object black body (m2)
    • T = absolute temperature of the body (K)

Examiner Tip

You will be expected to remember that a perfect black body has an emissivity of 1 - this information is not included in the data booklet!

Albedo

  • Albedo, a, is defined as

The ratio of the total scattered power to the total incident power of radiation that is reflected by a given surface

  • It can be calculated using the equation

a = fraction numerator total space scattered space power over denominator total space incident space power end fraction

  • More specifically, the albedo of a planet is defined as

The ratio between the total scattered, or reflected, radiation and the total incident radiation of that planet

  • Earth’s albedo is generally taken to be 0.3, which means 30% of the Sun’s rays that reach the ground are reflected, or scattered, back into the atmosphere
  • An albedo of 1 represents a surface that scatters all the incident radiation
  • Earth’s albedo varies daily and depends on:
    • Cloud formations and season – the thicker the cloud cover, the higher the degree of reflection
    • Latitude
    • Terrain – different materials reflect light to different degrees
    • Incident angle of radiation
  • It is useful to know the albedo of common materials: 
    • Fresh asphalt = 0.04
    • Bare soil = 0.17
    • Green grass = 0.25
    • Desert sand = 0.40
    • New concrete = 0.55
    • Ocean ice = 0.50 - 0.70 
    • Fresh snow = 0.85
  • Albedo has no units because it is a ratio (or fraction) of power

8-2-3-ib-sl-rn-albedo

Worked example

The average albedo of fresh snow is 0.85

Calculate the ratio fraction numerator energy space absorbed space by space fresh space snow over denominator energy space reflected space by space fresh space snow end fraction

 

Answer:
Step 1: Define albedo 
    • Albedo = the proportion of radiation that is reflected
    • Therefore, the energy reflected by fresh snow = 0.85
Step 2: Identify the proportion of radiation that is absorbed
    • If 85% of the radiation is reflected, we can assume that 15% is absorbed
    • Therefore, the energy absorbed by fresh snow = 1 – 0.85 = 0.15
Step 3: Calculate the ratio

fraction numerator energy space absorbed space by space fresh space snow over denominator energy space reflected space by space fresh space snow end fraction equals fraction numerator 0.15 over denominator 0.85 end fraction equals 0.18

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Katie M

Author: Katie M

Expertise: Physics

Katie has always been passionate about the sciences, and completed a degree in Astrophysics at Sheffield University. She decided that she wanted to inspire other young people, so moved to Bristol to complete a PGCE in Secondary Science. She particularly loves creating fun and absorbing materials to help students achieve their exam potential.