APS March Meeting 2010
Volume 55, Number 2
Monday–Friday, March 15–19, 2010;
Portland, Oregon
Session D5: Pais Prize Talk; Sam Goudsmit: Physics, Editor, and More
2:30 PM–5:30 PM,
Monday, March 15, 2010
Room: Portland Ballroom 256
Sponsoring
Unit:
FHP
Chair: Gloria Lubkin, Physics Today, Editor Emerita
Abstract ID: BAPS.2010.MAR.D5.1
Abstract: D5.00001 : Abraham Pais Prize for History of Physics Talk: Henry Cavendish, John Michell, Weighing the Stars
2:30 PM–3:06 PM
Preview Abstract
Abstract
Author:
Russell McCormmach
This talk is about an interaction between two 18th-century
natural philosophers (physical scientists), Henry Cavendish and
John Michell, and its most important outcome, the experiment of
weighing the world (their name for it) using a torsion balance
(our name for it). Michell was the most inventive of the 18th
century English natural philosophers, and Cavendish was the first
of his countrymen to possess abilities at all comparable with
Newton's. By their interests and skills, they were drawn to one
another. Both were universal natural philosophers, equally adept
at building scientific instruments, performing experiments,
constructing theory, and using mathematics; both had a penchant
for exacting, quantitative work. Both also had fitful habits of
publication, which did not begin to reveal the range of their
work, to the mystification of later scientists and historians.
Late in life, Cavendish and Michell turned their attention to the
force that Newton had examined most completely, a singular
triumph of his natural philosophy, the force of universal
gravitation. Over the course of the 18th century, abundant
evidence of attraction had been gathered from the motions of the
earth, moon, planets, and comets, phenomena which span the
intermediate range of masses, sizes, and distances. But in three
domains of experience, involving the extreme upper and lower
limits of masses and dimensions, the universality of gravitation
remained an article of faith. These were the gravity of the
``fixed'' stars, the mutual attraction of terrestrial bodies, and the
gravitation of light and other special substances. Michell took
on himself the task of deducing observable consequences from each
of these prospective instances of universal gravitation.
Cavendish encouraged Michell, and he followed up the resulting
observational and experimental questions. The experiment of
weighing the world was the last experiment Mitchell planned and
the last experiment Cavendish published. The capstone of two
distinguished careers, the experiment outlived the world in which
it was conceived and carried out. Today gravitation is at the
center of the physics of the very small and the very large, and
experiments that followed in Michell and Cavendish's footsteps
find a place in it. The ``most important advance in experiments
on gravitation,'' to quote an authority, ``was the introduction of
the torsion balance'' by Michell and Cavendish and independently by
Coulomb; ``it has been the basis of all the most significant
experiments on gravitation ever since.'' Another authority traces
the ``noble tradition of precision measurement to which we are
heirs'' to Cavendish's experiment, which he calls the ``first
modern physics experiment.''
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2010.MAR.D5.1