Authors
William Lee Vanderburgh
California State University, San Bernardino
Abstract
When a scientist is the first to perform a difficult type of observation and correctly interprets the result as a significant challenge to then-widely accepted core theories, and the result is later recognized as seminal work in a field of major importance, it is a surprise to find that that work was essentially ignored by the scientific community for thirty years. Such was the fate of the doctoral research on the rotations of the Andromeda Nebula (M31) conducted by Horace Welcome Babcock (1912–2003), who went on to become a very prominent astronomer — in an entirely different sub-field, never working on the subject of his dissertation again. This paper seeks to explain the ‘non-reception’ of Babcock’s work on galactic dynamics and the reasons he did no further work in that sub-field. In particular this paper shows that, contrary to the claims of some commentators, the non-reception of Babcock’s work should not be understood as an example of the unjust treatment of a young scientist by the conservative establishment
Keywords Dark matter  History of Dark Matter  History of Science  History of Astronomy  Galactic Rotation  Philosophy of Science
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References found in this work BETA

A Relation Between Distance and Radial Velocity Among Extra-Galactic Nebulae.E. Hubble - 1929 - Proceedings of the National Academy of Sciences 15:168-173.

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Citations of this work BETA

Quantitative Parsimony, Explanatory Power and Dark Matter.William L. Vanderburgh - 2014 - Journal for General Philosophy of Science / Zeitschrift für Allgemeine Wissenschaftstheorie 45 (2):317-327.

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