Henrietta Swann
Leavitt (1868 - 1921) made one the great astronomical discoveries of the 20th
Century. Her work enabled the existence of galaxies to be proved and
astronomers realise the scale of our Universe.
Henrietta
graduated from Radcliffe College, USA leaving her with a passion for astronomy, but a long illness had left her deaf. She
recovered to work at Harvard College Observatory. With no chance of actual
theoretical work (only open to men) she still rose to become head of
photographic photometry.
Stars which
changed in brightness were of particular interest to astronomers. By comparing
the astronomer's photographic plates, Henrietta catalogued 2,400 of these stars.
It was a huge painstaking manual effort comparing star fields on thousands of
photographic plates to find ones that 'blinked'. In 1908 she observed a type of star, called a Cephied
Variable, had a link between blinks and luminosity. By timing the period she
could calculate overall brightness. Henrietta had discovered a powerful tool
for astronomers - the standard candle.
The known brightness
of a star indicates its distance. In a similar way that the dimmer a street
light is, the further away it is likely to be. If a Cepheid with a blink of 5
days was fainter than another Cepheid with a blink of 5 days it was further
away. The scale of the universe could now be measured by using these 'standard
candle' stars. In 1923 after finding a Cepheid Variable (V1) in the Andromeda
'spiral nebula' (M31) Edwin Hubble made the astonishing discovery that it was a separate galaxy; 2 million light years away. The first
indication of the true scale of the universe.
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