Journal of High Energy Physics, Gravitation and Cosmology

Volume 9, Issue 4 (October 2023)

ISSN Print: 2380-4327   ISSN Online: 2380-4335

Google-based Impact Factor: 1.31  Citations  

NASA’s Pioneer Spacecraft Anomaly, Heat, Dark Matter and a Probable Persuasive Genesis

HTML  XML Download Download as PDF (Size: 2494KB)  PP. 1356-1373  
DOI: 10.4236/jhepgc.2023.94091    76 Downloads   336 Views  

ABSTRACT

An analysis is performed on what is known as the anomaly of NASA’s probe spacecraft. It explains why this additional acceleration can hardly be caused by the heat emitted by the electronic equipment of the spacecraft or by the dark matter that the Solar System could contain. Additionally, the correct stellar dynamics are mathematically demonstrated to explain the high speed of stellar rotation directly in galaxies and to show that this dynamics governing galaxies is very different from the dynamics of the Solar System. This also demonstrates the superfluity of postulating the existence of Dark Matter at the galactic level. It is concluded that the anomaly of the Pioneer spacecraft is relatively feasible as a product of an explainable difference between the modeling of the 70s and the real sources of the gravitational field of the Solar System. Therefore, it is claimed that there were sources of gravitational field that were not included in the original modeling because they were unknown at the time. Finally, a particular distribution of the disperse Solar System mass is proposed that could represent the sources of the field that give a plausible explanation for the NASA spacecraft anomaly.

Share and Cite:

Lugo, L. and Alarcón, E. (2023) NASA’s Pioneer Spacecraft Anomaly, Heat, Dark Matter and a Probable Persuasive Genesis. Journal of High Energy Physics, Gravitation and Cosmology, 9, 1356-1373. doi: 10.4236/jhepgc.2023.94091.

Cited by

No relevant information.

Copyright © 2024 by authors and Scientific Research Publishing Inc.

Creative Commons License

This work and the related PDF file are licensed under a Creative Commons Attribution 4.0 International License.