International Journal of Astronomy
p-ISSN: 2169-8848 e-ISSN: 2169-8856
2013; 2(3): 30-36
doi:10.5923/j.astronomy.20130203.02
P. A. Murad
Morningstar Applied Physics Inc., LLC, Vienna, VA 22182
Correspondence to: P. A. Murad, Morningstar Applied Physics Inc., LLC, Vienna, VA 22182.
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Binary pulsars demonstrate unusual gravitational behaviour that might be a careful balance between orbit performance, companion star and neutron star weights, and most importantly neutron star spin rate. Some binary pulsars are believed to have the same weight for both stars that move in a highly elliptical orbit while some binaries with supposedly vast weight differences, are in near-circular orbits. This is counterintuitive and raises questions outside of the conventional wisdom. Moreover, each neutron star in these binary systems spin at different rates, implying that rotation per Winterberg’s conjecture may induce a repulsive gravitational source analogous to generating dark matter that can negate inertial effects that allows balance. Swirling jets leaving black holes may move either at greater than light speed or also become a repulsive gravitational source. Interactions between the pulsar binary’s two bodies and behaviour of two of Jupiter’s moons may also validate notions from Jefimenko, who claims that gravity induces angular momentum. If true, these findings show that a significant relationship may exist between gravity and angular momentum may suggest angular momentum can be converted to linear momentum after going through an intermediate step to produce repulsive gravitation. Furthermore, these findings may be the prerequisites to devise future starship propulsion drives to explore the cosmos.
Keywords: Binary Pulsar, Neutron Star, Asteroid, Gravity, Jefimenko, Rotation, Angular Momentum, Trajectories
Cite this paper: P. A. Murad, Pulsar Behaviour that may Impact a Future Space Propulsor, International Journal of Astronomy, Vol. 2 No. 3, 2013, pp. 30-36. doi: 10.5923/j.astronomy.20130203.02.
![]() | Figure 1. Scheme of a Herbig-Haro object HH47 and the collimated jets of partially ionized gas claimed as belonging to the accretion disk, taken by the Hubble Space Telescope |
![]() | Figure 2. Some details may indicate a gas dynamic shock may appear in the jet as suggested in this artist rendition |
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![]() | Figure 3. The orbits of the binary pulsar 1913+16 and a comparison of the orbits of the pulsar J1903+0327 with its possible sun-like companion star with the orbit of the Earth around the sun[11] |
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