Period–luminosity relation for Cepheid variables (1912)
Brighter Cepheids pulsate more slowly, so the period reveals true brightness and hence distance
Science · Maths, astronomy, medicine & more
1868–1921 · American
Astronomy — variable stars
Henrietta Swan Leavitt was one of the women "computers" employed by Edward Pickering at Harvard College Observatory to study photographic plates. Examining variable stars in the Magellanic Clouds, she discovered that brighter Cepheid variables have longer periods, published in 1912. This period–luminosity relation, now called the Leavitt law, gave astronomers a "standard candle" for measuring cosmic distances and underpinned Hubble's work on galaxies and the expanding universe.
Period–luminosity relation for Cepheid variables (1912)
Brighter Cepheids pulsate more slowly, so the period reveals true brightness and hence distance
1777 Variables in the Magellanic Clouds (1908)
Paper in the Annals of Harvard College Observatory first noting that brighter variables had longer periods
Periods of 25 Variable Stars in the Small Magellanic Cloud (1912)
Harvard College Observatory Circular 173, published under Pickering's name, setting out the relation
Discovery of about 2,400 variable stars (1900s–1910s)
Roughly half of all variable stars known at the time
North Polar Sequence of photographic magnitudes (1913)
A standard scale of stellar brightness on photographic plates, adopted internationally