Binary Pulsar Orbits and New Ephemeris Based on The Precession Factor x

Feed: Dr. Myron Evans
Posted on: Monday, April 23, 2012 11:30 PM
Author: metric345
Subject: Binary Pulsar Orbits and New Ephemeris Based on The Precession Factor x

It would be very interesting to make a very careful graphical study with a range of x values for the precessing elliptical orbit to see if the orbit behaves at some point as in the binary pulsars, where it decreases by a few millimetres per orbit. The old interpretation of this was gravitational radiation from the Einstein theory, but it is now known that that is completely wrong. At some value of x close to unity the orbit will start to deviate slightly from a precessing ellipse, the type of deviations might be different for x less than one and greater than one, but very close to one. The orbit may cease to become a closed orbit and may start to behave like a binary pulsar orbit – a “shrinking precessing ellipse”, the true curve being given by x. There is no experimental evidence that a binary pulsar orbit will eventually collapse. The only experimental evidence is that the orbit decreases by a few millimetres an orbit, and a huge amount of horse hair was brushed away from this observation, revealing a wooden construction bearing Greek gifts. Gravitational radiation has never been observed, LIGOS has been a complete failure, covered up of course. I suspect that the true orbit of a binary pulsar will be given by varying x very carefully. A catalogue of orbits needs to be built up by varying x in order to classify the new information for mathematics and as well as physics. Our graphics experts here are Horst Eckardt, Robert Cheshire and Ray Delaforce, and it would be really interesting if they could build up such a catalogue or ephemeris, classifying the orbits or conical sections. We were going to do this for a new CISP book. The entire book could be lavishly illustrated in colour and orbits compared from known objects and the new theory. For example Halton Arp’s peculiar galaxies book. It is delightful to be able to work with such a simple equation as:

r = alpha / (1 + epsilon cos (x theta))

As my old Viking Uncle Olaf used to say, there’s a lot of finding to do, in the nicest way of course. I admit he could be a little cutting on occasions until he heard about cynghanedd.

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