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Revision Notes

Edexcel IAL Physics: Astrophysics and Cosmology — Revision Notes

Condensed recall notes on luminosity, Wien and Stefan laws, the HR diagram, stellar evolution and Hubble law for Edexcel International A Level Physics WPH15.

Subject
Physics
Level
A LEVELS
Topic
Unit 5: Thermodynamics, Radiation, Oscillations and Cosmology
Updated

Aligned to Pearson Edexcel A Level Physics (YPH11), Issue 3. Official specification .

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Condensed for the final weeks. For the full explanation, use the Astrophysics and Cosmology study guide.

Gravitational fields

g = F / m
F = G m1 m2 / r^2      (Newton's law of universal gravitation)
g = G m / r^2           (field of a point mass)
Vgrav = -G m / r         (gravitational potential, radial field)

Gravitational field strength, g = F/m, is the force per unit mass on a small test mass. Gravitational fields are structurally like electric fields — both inverse-square, both with radial and uniform forms — but gravity is always attractive (never repulsive) and Vgrav is always negative, rising towards zero at infinity, whereas electric potential can be positive or negative.

Orbital motion: gravity supplies the centripetal force, so GMm/r² = mv²/r, giving orbital speed v = √(GM/r) for a satellite in circular orbit.

Luminosity, flux and distance

F = L / (4 pi d^2)

Luminosity is total power emitted; radiant flux is power received per unit area. Confusing the two is the commonest error in the topic.

Standard candles have known luminosity, so measuring flux gives distance. Type Ia supernovae qualify because they detonate at a fixed critical mass and so reach a consistent peak luminosity. For relatively close stars, trigonometric parallax — the apparent shift in a star’s position against distant background stars as Earth orbits the Sun — provides an independent distance measurement, useful for calibrating standard candles.

Stellar temperature and size

Wien:    lambda_max T = 2.898 x 10^-3 m K
Stefan:  L = 4 pi r^2 sigma T^4

Wien first, then Stefan. Peak wavelength gives temperature; temperature plus luminosity gives radius. Attempting Stefan first leaves two unknowns.

Because L ∝ T⁴, a small rise in temperature produces a very large rise in luminosity.

Worked example. A star has a surface temperature of 5800 K. Find the wavelength at which it emits most strongly.

lambda_max = (2.898 x 10^-3) / T = (2.898 x 10^-3) / 5800 = 5.00 x 10^-7 m

500 nm, in the visible spectrum — consistent with a Sun-like star.

The Hertzsprung–Russell diagram

Luminosity (vertical) against temperature (horizontal), with temperature increasing to the left — the reversed axis is a standard trap.

Regions: main sequence (diagonal band), red giants (top right — cool but luminous, so they must be very large), white dwarfs (bottom left — hot but dim, so very small).

The HR diagram’s power is that position implies size. A cool star that is nonetheless highly luminous must have an enormous surface area, which is what identifies it as a giant.

Stellar evolution

Sun-like star: nebula → protostar → main sequence → red giant → planetary nebula → white dwarf.

Massive star: nebula → protostar → main sequence → red supergiant → supernova → neutron star or black hole.

The fate is determined by mass. The Chandrasekhar limit (~1.4 solar masses) is the maximum mass of a white dwarf; above it, electron degeneracy pressure cannot resist gravity and collapse continues.

Main-sequence lifetime is shorter for more massive stars, despite their greater fuel supply, because luminosity rises far faster than mass — they burn through it disproportionately quickly, so a massive star’s greater reserves are exhausted sooner rather than later.

Redshift and cosmology

Doppler:  delta-lambda / lambda = v / c
Hubble:   v = H0 d
age  ~  1 / H0

There is ongoing scientific controversy over the precise value of the Hubble constant, and what this implies for the age and ultimate fate of the universe.

Almost all galaxies are redshifted, and redshift increases with distance, so the universe is expanding.

This does not place us at the centre. Space itself is expanding, so every observer everywhere would see the same relationship — a point worth stating explicitly, since it is a common misreading of the redshift-distance evidence.

Big Bang evidence, with what each shows:

  1. Galactic redshift → the universe is expanding and was once smaller and denser.
  2. Cosmic microwave background → the cooled remnant of a hot early universe, black-body at ~2.7 K.
  3. Hydrogen and helium abundances → match the ratio predicted by Big Bang nucleosynthesis.

Dark matter is inferred from galactic rotation curves — outer stars orbit faster than visible mass can account for, implying unseen mass exerting additional gravitational pull. Dark energy is inferred from supernova observations showing the expansion is accelerating rather than slowing under gravity’s pull, as would otherwise be expected.

Exam traps

  • Confusing luminosity with flux.
  • Applying Stefan’s law before Wien’s.
  • Forgetting the HR diagram’s reversed temperature axis.
  • Saying massive stars live longer because they have more fuel.
  • Claiming redshift shows Earth is at the centre.
  • Using °C in Wien’s or Stefan’s law.
  • Forgetting that gravitational potential is always negative, unlike electric potential.

Self-test

  1. Distinguish luminosity from radiant flux.
  2. In what order are Wien’s and Stefan’s laws applied, and why?
  3. Why must a cool, highly luminous star be very large?
  4. Why do massive stars have shorter main-sequence lifetimes?
  5. What is the evidence for dark matter?
  6. A star has a surface temperature of 5800 K. Find its peak emission wavelength.
  7. How does trigonometric parallax measure stellar distance, and what is it used for?
  8. State the equation for gravitational field strength due to a point mass, and give one similarity and one difference between gravitational and electric fields.

Answers: 1. Luminosity is the total power radiated by the star; radiant flux is the power received per unit area at the observer. 2. Wien first, because peak wavelength gives temperature; Stefan then uses that temperature with the luminosity to find the radius — reversing the order leaves two unknowns. 3. Luminosity depends on both temperature and surface area, so a low temperature can only give high luminosity if the surface area, and hence the radius, is very large. 4. Luminosity increases much faster than mass, so they consume their larger fuel supply disproportionately quickly. 5. Galactic rotation curves show that stars in the outer regions orbit far faster than the visible mass distribution can explain. 6. λmax = (2.898×10⁻³) ÷ 5800 = 5.00×10⁻⁷ m (500 nm). 7. It measures the apparent shift in a nearby star’s position against distant background stars as Earth orbits the Sun; it is used to calibrate standard candles for larger distances. 8. g = Gm/r²; both fields are inverse-square with radial and uniform forms, but gravitational forces are always attractive while electric forces can attract or repel.

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