Abstract
Once upon a time philosophers and cosmographers insisted that the motions of the planets must be circular and uniform. An irrelevant aesthetic concept of ‘perfection’ and a more valid mathematical need for simplicity were at the root of this long-held error. Nowadays, theoretical cosmologists insist that the large-scale distribution of galaxies most be homogeneous and isotropic, and most astonomers believe that the expansion of the universe is linear and isotropic and that it proceeds at a uniform rate measured by the Hubble ‘constant’ H.1, 2
In questions of science the authority of a thousand is not worth the humble reasoning of a single individual.
Galileo Galilei
True knowledge can only be acquired piecemeal, by the patient interrogation of nature.
Sir Edmund Whittaker
Reprinted with kind permission from Science 167 (1970) 1203–1213.
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De Vaucouleurs, G. (1974). The Case for a Hierarchical Cosmology. In: Seeger, R.J., Cohen, R.S. (eds) Philosophical Foundations of Science. Boston Studies in the Philosophy of Science, vol 11. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-2126-5_14
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