Le Pouvoir Mondial aux Peuples

Un article paru dans The Detroit News, en janvier 1981.
L'article n'est pas très lisible mais identifiable quand même :

Extrait du rapport  : 3.6 A distant massive object: Planet X/Nemesis/Tyche
A promising candidate for explaining the anomalous increase of the lunar eccentricity may be, at least in principle, a trans-Plutonian massive body of planetary size located in the remote peripheries of the solar system: Planet X/Nemesis/Tyche (Lykawka & Mukai 2008; Melott & Bambach 2010; Fern´andez 2011; Matese & Whitmire 2011). Indeed, as we will see, the perturbation induced by it would actually cause a nonvanishing long-term variation of e. Moreover, since it depends on the spatial position of X in the sky and on its tidal parameter where mX and dX are the mass and the distance of X, respectively, it may happen that a suitable combination of them is able to reproduce the empirical result of eq. (1).
Let us recall that, in general, the perturbing potential felt by a test particle orbiting a central body due to a very distant, pointlike mass can be cast into the following quadrupolar form (Hogg et al. 1991) UX = KX 2 r2 − 3 r · ˆl 2, (33) where ˆl = {lx, ly, lz} is a unit vector directed towards X determining its position in the sky; its components are not independent since the constraint l2 x + l2 y + l2 z = 1 (34) holds. By introducing the ecliptic latitude X and

On the Anomalous Secular Increase of the Eccentricity of-1102.0212v6

Source originale (anglais) :       http://arxiv.org/abs/1102.0212v6
 
PDF de la thése :
 Lorenzo Iorio