A-LEVEL 9702 · A2 · TOPIC 25

Astronomy and cosmology

The chain of the topic: a star's luminosity plus the inverse-square law turns a standard candle into a distance; its spectrum, through Wien's law and Stefan-Boltzmann, fixes its radius; and the redshift of distant galaxies feeds Hubble's law, the expanding Universe and the Big Bang. Around the hexagon are the three ideas; above is what it builds on, below is where it leads.

TOPIC 25: ASTRONOMY AND COSMOLOGY CAMBRIDGE A-LEVEL PHYSICS 9702 · PATHWAYS TheLucidSTEM · thelucidstem.com BUILDS ON T22Photons & spectra T7Waves & the Doppler shift T13Gravitation & stellar mass 25.1 25.2 25.3 apply TOPIC 25 ASTRONOMY & COSMOLOGY 1 · STANDARD CANDLES Known brightness gives distance. Luminosity L: total power radiated by a star (W). Radiant flux F: power per unit area reaching us. A standard candle has a known L, so measuring F fixes the distance d to its galaxy. F = L / (4πd²) inverse-square law L power spreads over a sphere 4πd² so flux F falls as 1 / d² with distance d 2 · STELLAR RADII The spectrum reveals temperature, then size. A star radiates as a black body; the peak shifts to shorter λ as the surface gets hotter. Wien fixes T; Stefan-Boltzmann links L, r and T. Knowing L and T then yields the radius r. λmax ∝ 1 / T L = 4πσr²T⁴ intensity λ hotter cooler peak λ moves left as T rises 3 · HUBBLE'S LAW & THE BIG BANG Galaxies recede; the Universe expands. Spectral lines from galaxies are redshifted: λ is stretched, so the galaxy is moving away. Recession speed v rises with distance d (Hubble). Reverse the expansion: a hot, dense origin, the Big Bang, of age ≈ 1 / H₀. Δλ/λ ≈ Δf/f ≈ v/c v = H₀d v d gradient = H₀ 4 · MEASURING THE UNIVERSE Chain the relations to reach cosmic scales. From F and a known L get distance d (candle). From the spectrum get T (Wien), then r (Stefan). From redshift get v, then far d via v = H₀d. Invert the constant for the age of the Universe. d → r → v → H₀ → age candle radius redshift a distance ladder out to cosmic scales LEADS TO T23Nuclear physics: fusion that powers a star's L T13Gravitation: dark matter from orbital dynamics T22Quantum: spectral lines identify the elements One thread runs through: light carries the numbers, luminosity, spectrum and redshift, that measure the Universe.

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