IB Physics SL Topic 3 — Oscillations & Waves Paper 1 & 2 Expanding universe ~7 min read

Redshift of Galaxies

Point a telescope at almost any galaxy and its spectral-line barcode is slid towards the red. Not some galaxies — almost all of them. That one stubborn observation, plus a little Doppler physics, leads to one of the biggest conclusions in science: the universe is expanding.

📘 What you need to know

Red and Blue Shifts in the Sky

Everything from the last two pages now goes to work on the night sky. Compare the spectrum of a distant galaxy with a reference spectrum from a close, well-understood source — the Sun, or a lamp in the laboratory:

The exam definition of redshift is worth learning word for word:

Redshift is the fractional increase in wavelength (or decrease in frequency) due to the source and observer receding from each other.

“Fractional” is doing real work there — redshift is the ratio Δλ/λ, so it’s a pure number with no units.

Positive and Negative Velocities

When you calculate a speed from Δf = f0f, the sign that pops out isn’t clutter — it’s the answer to “towards or away?”:

f0 > f
Δf positive
velocity positive
blueshift
moving TOWARDS Earth
f0 < f
Δf negative
velocity negative
redshift
moving AWAY — receding

An Expanding Universe

When astronomers surveyed the sky after discovering Doppler redshift, the result was startling: almost every galaxy is redshifted — almost everything is receding from us. The explanation isn’t that galaxies happen to be fleeing Earth; it’s that the space between the galaxies is expanding, and the expansion stretches the light waves as they travel through it, shifting them towards the red end of the spectrum.

The classic picture is dots on an inflating balloon:

before inflate after — every dot is further from every other dot
Dots on an inflating balloon: as the rubber stretches, every dot moves away from every other dot — yet no dot moves across the rubber. In the same way, space itself stretches between galaxies; the galaxies themselves do not move through space.

The analogy carries three exam-ready points:

The Further, the Faster

One more observation seals the argument. Comparing spectra from galaxies at different distances shows that the greater the distance to a galaxy, the greater its redshift — and since a bigger redshift means a bigger recession speed, the furthest galaxies are receding the fastest. Exactly what you’d expect if all of space is expanding uniformly.

redshift distance the furthest galaxies are redshifted the most — so they are receding the fastest
Redshift against distance for many galaxies: the points follow a straight line through the origin. Double the distance, double the redshift — the signature of uniformly expanding space.

🧭 Making the “expanding universe” argument in an exam

  1. Observation 1: the spectral lines of almost all galaxies are shifted towards the red end — nearly every galaxy is receding
  2. Observation 2: the greater the distance to a galaxy, the greater its redshift — the furthest galaxies recede fastest
  3. Conclusion: the space between the galaxies must be expanding, stretching light waves in transit towards the red
  4. Polish: add the balloon analogy — like dots on inflating rubber, galaxies separate without moving through space, and no galaxy is the centre
Quick recap: redshift (λ up, f down) = receding; blueshift = approaching. Nearly all galaxies are redshifted, and the further they are, the bigger the shift — evidence that space itself is expanding.
WE 1

A spectral line from a source in the laboratory has a frequency of 6.170 × 10¹⁴ Hz. The same line in the light from a distant galaxy is measured at 6.130 × 10¹⁴ Hz. Calculate the velocity of the galaxy relative to the Earth and state whether it is moving towards or away from the Earth.

Find the frequency shift (observed minus reference) Δf = f₀ − f = (6.130 − 6.170) × 10¹⁴ = −4.0 × 10¹² Hz Apply the Doppler equation v = cΔf/f = (3.0 × 10⁸ × −4.0 × 10¹²) ÷ (6.170 × 10¹⁴) v ≈ −1.9 × 10⁶ m s⁻¹ Interpret the sign The velocity is negative (the observed frequency is less than the reference), so the light is redshifted the galaxy is receding at 1.9 × 10⁶ m s⁻¹
WE 2

State two observations about the light from distant galaxies and explain how they lead to the conclusion that the universe is expanding.

Observation 1 The spectral lines of almost all galaxies are redshifted compared with laboratory references — so almost all galaxies are moving away from Earth Observation 2 The greater the distance to a galaxy, the greater its redshift — so more distant galaxies are receding faster Conclusion Both observations follow if the space between galaxies is expanding, stretching the light waves as they travel — like dots on an inflating balloon, every galaxy separates from every other without moving through space the universe is expanding

💡 Top tips

⚠ Common mistakes

And that completes the Doppler Effect — from squashed wavefronts, through Δλ/λ ≈ v/c, to the expanding universe. These same ideas come straight back whenever spectra, stars, or moving sources appear in an exam question.

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