25. Astronomy and cosmology
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25.1 Standard candles
25.1.1The term luminosity as the total power of radiation emitted by a star
• understand the term luminosity as the total power of radiation emitted by a star
25.1.2The inverse square law for radiant flux intensity F
• recall and use the inverse square law for radiant flux intensity F in terms of the luminosity L of the source F = L / (4πd 2)
25.1.3An object of known luminosity is called a standard candle
• understand that an object of known luminosity is called a standard candle
25.1.4The use of standard candles to determine distances to galaxies
• understand the use of standard candles to determine distances to galaxies
25.2 Stellar radii
25.2.1Wien’s displacement law λmax ∝ 1 / T to estimate the peak surface
• recall and use Wien’s displacement law λmax ∝ 1 / T to estimate the peak surface temperature of a star
25.2.2The Stefan–Boltzmann law L = 4 πσr 2 T 4
• use the Stefan–Boltzmann law L = 4 πσr 2 T 4
25.2.3Wien’s displacement law and the Stefan–Boltzmann law to estimate the radius
• use Wien’s displacement law and the Stefan–Boltzmann law to estimate the radius of a star
25.3 Hubble’s law and the Big Bang theory
25.3.1The lines in the emission and absorption spectra
• understand that the lines in the emission and absorption spectra from distant objects show an increase in wavelength from their known values
25.3.2Redshift of electromagnetic radiation
• use ∆λ / λ ≈ ∆f / f ≈ v / c for the redshift of electromagnetic radiation from a source moving relative to an observer
25.3.3Why redshift leads to the idea that the universe is expanding
• explain why redshift leads to the idea that the universe is expanding
25.3.4Hubble’s law v ≈ H0d and explain how this leads to the Big Bang theory
• recall and use Hubble’s law v ≈ H0d and explain how this leads to the Big Bang theory (candidates will only be required to use SI units)