John
Goodricke who was deaf was on one the fathers of variable star
astronomy. He worked with Edward Pigott in the city of York between
1781 and 1786 when he died at the tragically young age of 21.
Goodricke
and Pigott explored the sky they explained that the variations of the
star Algol in the constellation of Perseus were caused by an unseen
body eclipsing Algol. The same principal is used by astronomers today
to look for planets orbiting other stars. They then went on to both
discover a new variable star on the same night, the 10th
September 1784, Pigott discovered eta Aquila and Goodricke discovered
beta Lyra. I described this as a night to remember in York.
The
indefatigable Goodricke then went onto to discover the variability of
the star delta Cephei in the constellation of Cepheus the King on the
night of October 23rd 1784. This was to prove to be one of
the most important astronomical discoveries.
Delta
Cepheus is of tremendous value to astronomers today, Goodricke could
not know the importance of his discovery. Cepheid variable stars are
used to work out the distance to other galaxies. It was in 1912 that
Henrietta Leavitt working at Harvard realised that there is a
relationship between the Cepheid variable stars a pattern was seen
that the brighter ones seem to have longer periods and that cepheids
were very luminous stars and there was a relationship between the
periods and distance.
If cepheids could be found in other galaxies the distances could be
worked out. They were and this allowed astronomers to work out how
far away the galaxies were. This was down to the discovery of delta
Cepheus in 1784 by the deaf astronomer John Goodricke the discovery
of this relation with the cepheids in 1912 by Henrietta Leavitt who
was also partially deaf. This relationship is known today as the
Period Luminosity Relationship.