Article ID: CBB000741578

A “Large and Graceful Sinuosity”: John Herschel's Graphical Method (2006)

unapi

In 1833 John Herschel published a graphical method for determining the orbits of double stars. He argued that his method, which depended on human judgment rather than mathematical analysis, gave better results than computation, given the uncertainty in the data. Herschel found that astronomy and terrestrial physics were especially suitable for graphical treatment, and he expected that graphs would soon become important in all areas of science. He argued with William Whewell and James D. Forbes over the process of induction, over the application of probability, and over the moral content of science. Graphs entered into all these debates; but because they constituted a method, not a metaphysics, they were acceptable to most practicing scientists and became increasingly popular throughout the nineteenth century.

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Description On Herschel's graphical method for determining the orbits of double stars.


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Authors & Contributors
Case, Stephen
Charles Kostelnick
Belteki, Daniel
Cristalli, Claudia
Miles A. Kimball
Case, Stephen R.
Journals
Journal for the History of Astronomy
Vistas in Astronomy
Victorian Studies
Studies in History and Philosophy of Science
Statistical Science
Leonardo
Publishers
Washington State University
University of Notre Dame
Routledge
Books on Demand
Concepts
Astronomy
Visual representation; visual communication
Graphic methods
Solar system; planets
Stars; stellar astronomy
Statistics
People
Herschel, John Frederick William
Herschel, William
Herschel, Caroline
Merz, Georg
Somerville, Mary Fairfax
Simms, William
Time Periods
19th century
18th century
21st century
20th century
Places
United States
British Isles
Great Britain
Institutions
British Geological Survey
Leeds Astronomical Society
Royal Observatory Greenwich
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