Curriculum
Course: IB Physics HL
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Curriculum

IB Physics HL

Theme A — Space, Time and Motion

0/125 Dr Dabour Hub Science Diagram and Course Material

Theme B — The Particulate Nature of Matter

0/105 Dr Dabour Hub Science Diagram and Course Material

Theme C — Wave Behaviour

0/73 Dr Dabour Hub Science Diagram and Course Material

Theme D — Fields

0/77 Dr Dabour Hub Science Diagram and Course Material

Theme E — Nuclear and Quantum Physics

0/89 Dr Dabour Hub Science Diagram and Course Material

Tools and Inquiry — IB Physics skills

0/43 Dr Dabour Hub Science Diagram and Course Material
Quiz

B.2.5 Energy Balance Problems – Check yourself

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1.
At equilibrium for a planet, which equation holds?
S = σT4
S(1 − α)/4 = eσT4
S α /4 = σT4
S(1 − α) = 4σT4/e
2.
If the albedo of a planet increases while everything else is unchanged, the equilibrium temperature
rises
stays the same
falls
becomes zero
3.
The solar constant at a planet increases by a factor of 16 with everything else unchanged. The equilibrium temperature increases by a factor of
16
4
8
2
4.
A planet has S = 900 W m−2, α = 0.20 and e = 1. Its equilibrium temperature is approximately
237 K
170 K
330 K
400 K
5.
A greenhouse gas increase lowers the effective emissivity. At the new equilibrium the surface temperature is
zero
lower, because less radiation escapes
unchanged because the Sun's output is constant
higher, because the planet must radiate the same power with a lower emissivity
6.
In the equilibrium equation, why does the planet's radius not affect the temperature?
The radius is always the same
πR2 cancels because power in ∝ πR2 and power out ∝ 4πR2
Large planets have no atmosphere
Emissivity compensates
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