Closing in on the Cosmos: Cosmology’s Rebirth and the Rise of the Dark Matter Problem Jaco de Swart Abstract Influenced by the renaissance of general relativity that came to pass in the 1950s, the character of cosmology fundamentally changed in the 1960s as it be- came a well-established empirical science. Although observations went to dominate its practice, extra-theoretical beliefs and principles reminiscent of methodological debates in the 1950s kept playing an important tacit role in cosmological consider- ations. Specifically, belief in cosmologies that modeled a “closed universe” based on Machian insights remained influential. The rise of the dark matter problem in the early 1970s serves to illustrate this hybrid methodological character of cosmological science. Introduction In 1974, two landmark papers were published by independent research groups in the U.S. and Estonia that concluded on the existence of missing mass: a yet-unseen type of matter distributed throughout the universe whose presence could explain several problematic astronomical observations (Einasto et al. 1974a, Ostriker et al. 1974). The publication of these papers indicates the establishment of what is cur- rently known as the ‘dark matter’ problem – one of the most well-known anomalies in the prevailing cosmological model. According to this model, 85% of the uni- verse’s mass budget consists of dark matter. After four decades of multi-wavelength astronomical observations and high-energy particle physics experiments, the nature of this mass is yet to be determined.1 Jaco de Swart Institute of Physics & Vossius Center for the History of Humanities and Sciences University of Amsterdam, Science Park 904, Amsterdam, The Netherlands e-mail:
[email protected] 1 For an overview of the physics, see e.g.