Chapter 11 of 11 · 12 min read
Distances and the cosmic ladder
Parallax, standard candles, geometric methods and the Hubble law, with the IOAA problems that use each rung.
Geometry first
- Parallax: , so 1 mas means 1 kpc. Errors: . Beyond about 20% parallax error, becomes biased, which is why HST and Gaia matter (2017 D1 used HST parallaxes of about 2–3 mas).
- Angular size: . If you know a physical size, an angle gives the distance. Examples: the Moon's radius from the eclipse geometry (2016 D2), eclipsing binaries with surface brightness (2023 DA1).
- Triangulation in the Solar System: the Sun–Earth–Moon triangle at quarter phase (Aristarchus), Venus transits, radar.
Standard candles
A standard candle has a known , so gives the distance.
- Cepheids: the period–luminosity relation , calibrated with parallaxes (2017 D1) and applied to the LMC or other galaxies (2015 P2: IC 342).
- Type Ia supernovae: peak , corrected for light curve width. Slower decliners are brighter (the Phillips relation; the stretch factor in 2016 D3).
- Novae: the maximum-magnitude–rate-of-decline relation, from or (2019 Nova Del 2013).
- Tip of the red giant branch and RR Lyrae: and , respectively.
Each candle's calibration error is a systematic error for every distance it gives.
Physical methods
- Baade–Wesselink: integrate a pulsating star's radial velocity to get , combine with the flux and temperature at two phases to get and then (2015 P1).
- Eclipsing binaries: radii in metres from the light and velocity curves, angular diameters from the surface-brightness–colour relation, so (2023 DA1; the method behind the 1% LMC distance of 2019).
- Microlensing parallax: and together give the lens mass and distance without any luminosity at all (2023 DA2).
The Hubble law
For , , so a distance to a galaxy with a known redshift gives , and the Hubble time
sets the age scale (2016 D3). Peculiar velocities of a few hundred km/s make nearby galaxies unreliable for this, so use galaxies beyond about 50 Mpc.
Key formulas
- Parallax
- Size and distance
- Hubble law
- Einstein radius
Common mistakes
- Using 1/π for a parallax with a 30% error and quoting a symmetric error.
- Forgetting extinction when using a standard candle in the Galactic plane.
- Mixing up apparent and true distance moduli (with and without A).
- Applying the Hubble law to the Local Group.
Practise this chapter
Past IOAA problems that use these skills.
- 2015 P1 | Distance to the Cepheid HV 2257Olympiad
- 2015 P2 | The extinction law and the distance to IC 342Advanced
- 2016 D3 | Stretching Type Ia supernova light curvesAdvanced
- 2017 D1 | Calibrating the distance ladder to the LMCAdvanced
- 2023 DA1 | Distance to the LMC from eclipsing binariesAdvanced
- 2023 DA2 | Weighing an isolated black hole with astrometric microlensingOlympiad
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