K
kmarinas86
Guest
Correct:<br />GPE+KE=constant<br />-GMm/r+m*pioneeracceleration*r+.5mV²=C=0<br />-GM+pioneeracceleration*r²+.5V²r=0<br />.5V²=.5*(Escape Velocity)²=(Orbital Velocity)²=v²<br />-GM+pioneeracceleration*r²+v²r=0<br />r=(sqrt(v^4+4*pioneeracceleration*GM)-v²)/(2*pioneeracceleration)<br /><i>Energy is conserved</i><br /><i>Real Distances</i><br /><i>units (m/s)^4 are positive</i><br /><i>units (m/s)² are either negative or postive</i><br /><i>kinetic and potential energy</i><br /><br />Incorrect (Suggests an acceleration of kuiper belt objects that is not observed):<br />Acceleration=GM/r²+pioneeracceleration<br />Acceleration=v²/r<br />If M=0, Acceleration=pioneeracceleration : Acceleration towards sun (contradicts the idea of using the pioneer anomaly for cosmological purposes)<br />v²/r=GM/r²+pioneeracceleration<br />-pioneeracceleration*r²+v²r-GM=0<br />r=(sqrt(v^4-4*pioneeracceleration*GM)-v²)/(2*-1*pioneeracceleration)<br /><i>Energy is not conserved</i><br /><i>Complex Distance</i><br /><i>units (m/s)^4 are "negative"</i><br /><i>units (m/s)² are imaginary</i><br /><i>imaginary energy</i><br /><br />Correct (Suggests that using GM/r² leads to an understimation of the solarsystem's mass):<br />Acceleration=GM/r²-pioneeracceleration<br />If M=0, Acceleration=-pioneeracceleration : Acceleration away from sun (i.e. the Hubble Acceleration which = c*HubbleConstant)<br />Acceleration=v²/r<br />v²/r=GM/r²-pioneeracceleration<br />pioneeracceleration*r²+v²r-GM=0<br />r=(sqrt(v^4+4*pioneeracceleration*GM)-v²)/(2*pioneeracceleration)<br /><i>Energy is conserved</i><br /><i>Real Distances</i><br /><i>units (m/s)^4 are positive</i><br /><i>units (m/s)² are either negative or postive</i><br /><i>kinetic and potential energy</i><br /><br />Conclusions:<br />Pioneer acceleration is due to a change in Gravitational Potential Energy formula.<br />Pioneer acceleration <i>decreases</i> orbital velocity.<br />Pioneer acceleration leads to <i>energy loss</i>, not <i>energy gain</i>.<br />The only way there would be a relative