Published online by Cambridge University Press: 05 December 2013
In Chapters 7 and 9 we saw how strongly the conclusions we reach about the structure of the Universe can be shaped by intrusions that have no formal role in the philosophy of science. Technological innovations, governmental priorities, economic factors, as well as scientific advisory and oversight boards all play a role in the shaping of astronomy. Astrophysics is continually under pressure from forces pulling in different directions, destabilizing ongoing efforts, and keeping the field off balance.
How astrophysics nevertheless manages to advance is difficult to grasp in the abstract. The present chapter attempts to sketch realistically how modern astronomy is conducted and the vital role a well-coordinated communal approach can play as long as it remains sufficiently flexible to recover from inevitable setbacks. As we shall see, steadfast leadership is the essential ingredient of ultimate success.
A Logical Way to Proceed
By the mid-1970s, it was easy to see how the influx of new detection techniques introduced by the military in World War II and the Cold War had led to undreamed-of discoveries. Earlier theories had given us no inkling to expect the existence of quasars, pulsars, or the detection of cosmic masers, all initially revealed by radio astronomy. Similarly significant discoveries were being made in the gamma-ray, X-ray, and infrared regimes.
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