Computing possible worlds in the history of modern astronomy

Authors

  • Osvaldo Pessoa Jr. Depto. de Filosofia, FFLCH, Universidade de São Paulo
  • Rafaela Gesing Institute of Mathematics and Statictics University of São Paulo
  • Mariana Jó de Souza Undergraduate student Institute of Physics University of São Paulo
  • Daniel Carlos de Melo Marcílio Undergraduate student Polytechnic School University of São Paulo

DOI:

https://doi.org/10.5007/1808-1711.2016v20n1p117

Keywords:

Causal model, possible worlds, linking advance, history of the telescope, computational philosophy of science.

Abstract

As part of an ongoing study of causal models in the history of science, a counterfactual scenario in the history of modern astronomy is explored with the aid of computer simulations. After the definition of “linking advance”, a possible world involving technological antecedence is described, branching out in 1510, in which the telescope is invented 70 years before its actual construction, at the time in which Fracastoro actually built the first prototelescope. By using the principle of the closest possible world (PCP), we estimate that in this scenario the discovery of the elliptical orbit of Mars would by anticipated by only 28 years. The second part of the paper involves an estimate of the probability of the previous scenario, guided by the principle that the actual world is the mean (PAM) and using computer simulations to create possible worlds in which the time spans between advances is varied according to a gamma distribution function. Taking into account the importance of the use of the diaphragm for the invention of the telescope, the probability that the telescope were built by 1538 for a branching time at 1510 is found to be smaller than 1%. The work shows that one of the important features of computational simulations in philosophy of science is to serve as a consistency check for the intuitions and speculations of the philosopher.

Author Biography

Osvaldo Pessoa Jr., Depto. de Filosofia, FFLCH, Universidade de São Paulo

Possui graduação em Física (1982) e em Filosofia (1984) pela USP, mestrado em Física Experimental pela Unicamp (1985), e doutorado em História e Filosofia da Ciência pela Indiana University (1990).

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Published

2016-09-22

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Section

Articles