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Mario J. Pinheiro

Mario J. Pinheiro

Universidade de Lisboa
Portugal

Title: The Flyby anomaly in need of new physics?

Biography

Biography: Mario J. Pinheiro

Abstract

The central task of dynamical astronomy is to obtain solutions for equations of satellite motion. This analytic methodology employs Newtonian dynamics with gravitational fields that pulls on matter to get it going. After 100 years the inception of the General Theory of Relativity (GTR) by Einstein, a cornerstone of modern physics, even accomplished theories might have difficulty explaining a certain class of astronomical phenomena - in particular, small astrometric anomalies. At the end of the 19th century, astronomers discovered that the perihelion of Mercury was slowly advancing in a way that could not be explained by Newtonian physics. As it turned out, this small anomaly in Mercury's orbit has found an explanation in GTR. We may point four classes of astrometric anomalies: i) the flyby anomaly, addressed in this work; ii) the slow increase of the astronomical unit (AU), approximately the distance from the Earth to the Sun; iii) the Pioneer anomaly, which is now a  solved puzzle; iv)  the increase in the eccentricity of the Moon's orbit. The flyby anomaly has been a puzzling issue, addressed in the present work and by other numerous authors.

We suggest a possible theoretical explanation for the physical process underlying the unexpected orbital-energy change observed during close planetary flybys based on the new concept of topological torsion current (TTC). This approach is along the line of non-standard physical models used to explain the anomalous velocity increase by means of torsion gravity, the majority based on the Ehlers-Pirani-Schild program of constructive axiomatization of the geometric structure of spacetime. Our theoretical framework is classical and shows that there is an asymmetry when a spacecraft approaches a planet in prograde or retrograde direction, but the anomaly occurring only in retrograde direction.