  Christopher Nolan's latest blockbuster, Interstellar, has supposed a
revolution not only from a cinematographically viewpoint, but also in the
relation between current spectators and science. The aim of this report is to
analyze some features presented in Interstellar. Basic Newtonian Physics shows
how a planet orbiting a supermassive black hole like Gargantua must travel at
0.25 the speed of light in order to be in a stable orbit. Thus, this orbit is
too far from the black hole to explain the time dilatation observed in Miller's
Planet and an the orbit that could explain such a time dilatation is much more
smaller that Roche's limit. Furthermore, I explain how enormous waves as
Miller's Planet ones could appear by studying the tidal potential created by
Gargantua, obtaining a wave of 200 kilometers high, but better results are
obtained by considering a series of tsunamis in Miller's Planet. Finally, I
present an explanation to Mann's Planet ice-covered landscape in which Snowball
Earth Theory plays a fundamental role. No difficult General Relativity formulas
will be used in order to make easier the comprehension of the research.
  Supervisors: M. L. Osete & J. Gorgas
