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The Asteroid Belt as the Consequence of Resonance Density Convergence From Solar Velocity Around the Galaxy and Universal Dynamic Pressure

Treść / Zawartość
Identyfikatory
Warianty tytułu
Języki publikacji
EN
Abstrakty
EN
The velocity of the solar system around the galaxy as it moves through universal dynamic pressure of about 0.15 nPa results in a critical mass density of 1.5 protons per cc. Interplanetary measurements indicate this density occurs within the space occupied by asteroids. Quantitative evidence is offered that the matter in asteroid space failed to accrete into a planet because of the disruptive resonance between universal dynamic pressure and the velocity of the system. The model may accommodate the chemical characteristics of the different regions of the asteroid belt and the marked difference in planetary characteristics above (the inner planets) and below (the “gas giants”) the critical density. The energy accumulated within the functional toroidal space between Mars and Jupiter since the formation of the solar system is equivalent to the total mass of asteroids. If energy is still emerging within this region then the probability of non-traditional disruption of orbits for certain masses of asteroids may have significant impact. Specific frequencies that should show enhanced power based upon these calculations are derived.
Rocznik
Tom
Strony
73--79
Opis fizyczny
Bibliogr. 10 poz., rys., wz.
Twórcy
  • Laurentian University, Sudbury, Ontario P3E 2C6, Canada
  • Laurentian University, Sudbury, Ontario P3E 2C6, Canada
Bibliografia
  • [1] M. A. Persinger, International Letters of Chemistry, Physics and Astronomy 11 (2014) 18-23.
  • [2] M. A. Persinger, Journal of Physics, Astrophysics and Physical Cosmology 3 (2009) 1-3.
  • [3] M. A. Persinger, International Letters of Chemistry, Physics and Astronomy 4 (2013) 387-396.
  • [4] H. S. Bridge, J. W. Belscher, R. J. Butler, A.J. Lazarus, A. M. Mavretic, J. D. Sullivan, G. L. Siscoe, V. M. Vasyliunas, Space Science Reviews 21 (1977) 259-287. [5] A. N. Kolmogorov, Journal of Fluid Mechanics 13 (1962) 82-85.
  • [6] B. E. Clark, Lunar and Planetary Institute Science Conference Abstracts 27 (1996) 225.
  • [7] J. C. Brandt, Introduction to the Solar Wind. W. H. Freeman & Company, San Francisco, 1970.
  • [8] M. Bordag, U. Mohideen, W. M. Mostepanenko, Physics Reports 353 (2001) 1-205.
  • [9] H. E. Puthoff, Physical Review A 39 (1989) 2333-2342.
  • [10] D. A. E. Vares, M. A. Persinger, International Journal of Geosciences 4 (2013) 1321-1325.
Typ dokumentu
Bibliografia
Identyfikator YADDA
bwmeta1.element.baztech-dd488967-a7b3-4d1e-9efe-b44f15d06772
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