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6 - Moving in the inner circle

Published online by Cambridge University Press:  03 May 2011

Barbara J. Becker
Affiliation:
University of California, Irvine
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Summary

I saw … the creation of a great method of astronomical observation which could not fail in future to have a powerful influence on the progress of astronomy …

William Huggins

Huggins could have set himself the arduous task of examining the spectrum of every known nebular object, or systematically cataloguing the spectra of northern hemisphere stars. Instead, he pursued a varied and opportunistic research programme like many other amateur astronomers of his day, devoting considerable time and serious attention to research problems generated by others, and to the exotic rather than the mundane. As an independent observer he was free of the obligations and commitments that restricted his institution-bound contemporaries. Driven by broad interests and an insatiable curiosity, he explored a number of different subjects in innovative and often technically demanding ways. His challenge was to maximise his exposure to opportunities for new discoveries without becoming identified as a speculative or impulsive dilettante.

It was a challenge his years as an entrepreneur had prepared him well to meet. He developed a reputation for care in making observations and caution in suggesting explanations for the phenomena he observed. His successes led to more opportunities for success, and he became recognised as one upon whom colleagues could rely for advice on spectroscopic matters.

Cultivating advantageous alliances

In June 1865, the Royal Society called on Huggins to verify a discovery recently announced by Father Angelo Secchi, director of the Vatican observatory.

Type
Chapter
Information
Unravelling Starlight
William and Margaret Huggins and the Rise of the New Astronomy
, pp. 82 - 103
Publisher: Cambridge University Press
Print publication year: 2011

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References

AR 2 (1864), pp. 4–6 and pp. 98–101
Discussion on the willow-leaved structure of the Sun's photosphere’, MNRAS 24 (1864), pp. 140–2; p. 141
Sixth meeting, April 13, 1866’, AR 4 (1866), pp. 139–40
AR 4 (1866), p. 268 and pp. 310–11
Joseph Baxendell’, MNRAS 48 (1888), pp. 157–60CrossRef
AR 4 (1866), p. 97
MNRAS 26 (1866), p. 214
AR 4 (1866), pp. 97–8
Mr. Huggins, at the president's request …’, AR 4 (1866), p. 181
γ Cassiopeiae’, MNRAS 27 (1867), p. 135
MNRAS 28 (1868), p. 87
On a possible method of viewing the red flames without an eclipse’, AR 7 (1868), pp. 263–5; p. 264
A letter from Professor Chevallier’, MNRAS 5 (1842), pp. 186–7
The president announced …’, MNRAS 5 (1843), p. 264
Third meeting, January 11, 1867’, AR 5 (1867), pp. 25–8
On the radiation of heat from the Moon’, AR 6 (1868), pp. 92–3
Heating power of the stars’, MNRAS 30 (1870), pp. 107–9
On the radiation of heat from the Moon’, AR 6 (1868), pp. 39–41
On the radiation of heat from the Moon’, AR 6 (1868), pp. 39–41
On the radiation of heat from the Moon’, AR 6 (1868), pp. 92–3

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