3.0 Kepler's Laws of Planetary Motion - Relativistic Domain Theory Applicability.3.1 Kepler's First Law.In [1], Kepler's first law is stated as follows,
In [1], after analysis, this is slightly extended, to show that the planets describe conic sections about the Sun at one focus. It is well known that all gravitationally generated central orbits, in non-relativistic form, open or closed, describe conic sections given by,
Where
In the Relativistic Domain D1, it is shown in [2] Section 5, that a central orbit is also a conic section described thus, [2], Eq.(5.11),
In (3.2), (3.3), (3.4) and (3.5) the terms are defined thus,
The derivation of (3.2), (3.3), (3.4) and (3.5) is shown in [2] and in [3] it is shown that (3.4) is a relativistic effect within the gravitational source. Because W is a variable, a precise re-statement of Kepler's first law, specifically for relativistic effects would therefore need to be as follows,
3.2 Kepler's Second Law.In [1], Kepler's second law is stated as follows,
Mathematically this is stated as,
Where,
In [2] it is shown, [2], Eq.(5.4), that the relativistic version of the
parameter h is given by,
and thus the relativistic version of (3.6) becomes,
Where,
and other terms are as defined above. Kepler's second law therefore holds in Relativistic Domain Theory with the relationship modification as shown in (3.8). 3.3 Kepler's Third Law.In [1], Kepler's third law is stated as follows,
In [1] the mathematical relationship for this law is derived and quoted as,
Where,
In the Relativistic Domain D1, to determine whether this law holds, the equation of motion applicable to a central orbit is used as the starting
point. This is given by [2]. Eq. (3.17), viz.
Where
From [2], Eqs. (4.6) and (4.7)
So that in (3.10)
as derived in [2], Eq. (4.4) and where
Inserting (3.12) into (3.10) gives,
so that (3.13) then becomes,
uOR is determined simply thus. The temporal rate at s is given by [2], Eq. (4.6), viz,
wOR is determined as follows. In one complete orbit the angle rotated through is
Where
From (3.5) this is given by
and therefore the mean value of the angular rate over one orbit is,
Where
Here m0 is as defined in this series of papers. Substitution of (3.16) and (3.19) into (3.14) then gives
Re-arrangement into Kepler's format then yields,
Eq.(3.21) shows that, irrespective of the actual value of sOR, Kepler's third law does not quite hold under relativistic conditions. The reason being the presence of the -2a term on the LHS of (3.21) and the -3am0 term on the RHS. Compounding this, there is a difference in the mean value of the radius vector, sOR. This is shown as follows. In erting the classical value for L into (3.2) and re-arranging gives,
Where,
Now, when f = 0, W = 0 and (3.22) reduces to,
and so (3.22) becomes
Therefore, from (3.23) and (3.24)
As both halves of the orbit are identical, (3.25) also applies over the complete orbit. Eq.(3.25) shows that the difference between the mean values of the radius vectors in Kepler's original third law and the relativistic version is solely due to the orbit precession angle. Approximation to the non-relativistic version, Kepler's original, is obtained by allowing c ® ¥ so that both a and WOR become zero, which results in (3.25) becoming
so that (3.21) then becomes
as in (3.9). The combination of Eqs.(3.21) and (3.25), although not equivalent to Kepler's third law is very close to it and represents the relationship for an elliptic orbit. Putting e = 0 produces the relationship for a circular orbit. In view of the smallness of the discrepancy of (3.21) and (3.25) from (3.9), a re-statement of this law for a relativistic planetary orbit is unnecessary provided the modified relationships are used as appropriate
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P.G.Bass, November 2008
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