麻豆淫院

April 27, 2011

New theory proposed to explain Pioneer probe gravitational anomaly

Schematics of the con铿乬uration of Lambertian sources used to model the lateral walls of the main equipment compartment. Image credit: arXiv:1103.5222v1 [physics.space-ph] http://arxiv.org/abs/1103.5222
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Schematics of the con铿乬uration of Lambertian sources used to model the lateral walls of the main equipment compartment. Image credit: arXiv:1103.5222v1 [physics.space-ph] http://arxiv.org/abs/1103.5222

(麻豆淫院Org.com) -- Portuguese physicists might have finally solved the decades old mystery of why the Pioneer probes, launched in the early 70鈥檚, haven鈥檛 been decelerating from the Sun鈥檚 gravitational pull at the rate expected; it seems it might be something as mundane as adding in the tiny forces that occur when minute traces of heat from the plutonium on board the probes bounce off their receiving dishes, creating a counterforce, which in turn, causes the craft to slow; if ever so slightly.

as it was emitted from the main equipment compartment could emanate outwards, eventually bouncing off the back of the dish, resulting in just enough counterforce to explain the gravitational discrepancy.

Case closed, as far as Francisco et al are concerned, but of course this being science, others will have to replicate the results before any sort of consensus can be found.

More information: Modelling the reflective thermal contribution to the acceleration of the Pioneer spacecraft, arXiv:1103.5222v1 [physics.space-ph]

Abstract
We present an improved method to compute the radiative momentum transfer in the Pioneer 10 & 11 spacecraft that takes into account both diffusive and specular reflection. The method allows for more reliable results regarding the thermal acceleration of the deep-space probes, confirming previous findings. A parametric analysis is performed in order to set an upper and lower-bound for the thermal acceleration and its evolution with time.

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