Biography:William Hyde Wollaston: Difference between revisions
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{{Short description|English scientist associated with early observations of solar spectrum lines}} | {{Short description|English scientist associated with early observations of solar spectrum lines}} | ||
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{{Infobox scientist | {{Infobox scientist | ||
| name = William Hyde Wollaston | | name = William Hyde Wollaston | ||
Revision as of 17:35, 24 May 2026
| William Hyde Wollaston | |
|---|---|
| |
| Wollaston | |
| Born | 6 August 1766 East Dereham, Norfolk, England |
| Died | 22 December 1828 London, England
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| Known for | Early observation of solar dark lines; discovery of palladium and rhodium |
William Hyde Wollaston (1766-1828) was an English scientist whose work ranged across chemistry, optics, and physics. In 1802 he observed dark lines in the solar spectrum, an important early step in the history of spectroscopy.
Solar spectrum
Wollaston observed dark lines in sunlight using a prism and a narrow slit. He interpreted them as boundaries between colors rather than as absorption features. Joseph von Fraunhofer later mapped many more of these lines with greater precision, and they became known as Fraunhofer lines.
Although Wollaston's observation came before quantum mechanics, spectral lines later became central evidence for discrete atomic energy levels and quantum transitions.
Quantum Collection links
- Physics:Quantum Spectral lines and series
- Physics:Quantum atoms/transition
- Physics:Quantum atoms/energy level
- Physics:Quantum photon
References
- "William Hyde Wollaston". https://www.britannica.com/biography/William-Hyde-Wollaston.
- "William Hyde Wollaston". https://mathshistory.st-andrews.ac.uk/Biographies/Wollaston/.
Author: Harold Foppele