Gravitational Explanation of the Glacial Periods and Calculation of the Precession of
Mercury's Orbit
According to the gravitorelative theory, the
gravitational acceleration that a reference body experiences due to a mass
which moves at a velocity
in relation to it is:
|
(1) |
|
|
and
are the
components, perpendicular and parallel to the velocity, of the gravitostatic
acceleration
.
This formula, which may be considered as the
generalization of Newton's Law, is deduced supposing that the gravitational interaction is
produced by means of a flux of particles which spread at velocity c.
That is to say, a mass creates a flux of particles and the reference body
experiences an acceleration depending on the density of the flux (by unit of
volume) that it perceives. Due to the Lorentz contraction of the length, the reference body perceives a greater
density if the velocity of the mass is perpendicular to the line of centres and
less if is parallel. In the general case where the velocity forms an angle
with the line of centres, formula (1) is deduced, in which
and
.
Following the same model of interaction (by
means of flux of particles) for the electric case, a similar formula to (1) is deduced which may be considered as the
generalization of Coulomb's Law. The magnetic forces are deduced from this formula as shown in.
It must be pointed out that the method used in
this theory to describe the interaction is not the usual method of
"laboratory reference frame" but rather that of "relation".
In the book (*)
"Diálogos sobre Física" the possible
mechanism of gravitational interaction is described.
Gravitorelative Effects
The formula (1) is made up of three terms. The first term represents the
Newtonian or gravitostatic acceleration. The other two terms are the components
(perpendicular and parallel to the velocity) of the so called gravitorelative
acceleration
which arises when the mass moves in
relation to the reference body. Moreover, it turns out that the gravitorelative
acceleration component parallel to the velocity is of opposite direction to the
component parallel to the velocity of the Newtonian acceleration ( fig 1).
|
( fig 1) |
|
|
The radial component of the gravitorelative
acceleration contributes to the determination of the average radius of the
orbit of a planet.
When the
eccentricity varies the radial gravitorelative acceleration also varies. This
is, on one hand, because the radial projections of
and
have
opposite directions (the first increases the gravitostatic acceleration while
the second decreases it) and, on the other hand, because when the eccentricity
decreases,
increases and
decreases, while when the eccentriciy increases, exactly the
opposite occurs. In a circular orbit
= 0 and the gravitorelative acceleration
coincides with the direction of the gravitostatic acceleration.![]()
The gravitorelative component parallel to the
velocity
produces a small lengthening of the major axis (near 4 km in the
earth's orbit) because as the planet moves away the deceleration of the
velocity is less than in the Newtonian case and as it moves nearer the
acceleration is less in the same measure so both acceleration and deceleration
are balanced but they nevertheless cause this small effect.
The perpendicular gravitorelative component
, which
in circular orbits coincides in direction with the Newtonian acceleration, in
elliptic orbits produces a precession of the orbit.
The Precession of Mercury's Orbit
In elliptic orbits the gravitorelative
acceleration perpendicular to the velocity does not change its
magnitude, instead it simply changes its direction and with it the trajectory
of the planet.
To understand what the trajectory of the
planet is, we are going to place ourselves in the Newtonian frame which corresponds
to that of a planet that moves in relation to the Sun in a Newtonian elliptic
orbit. Now if the planet not only shares the movement of the Newtonian frame
but is also affected by the perpendicular component of the gravitorelative
acceleration then we will see it moving away continuously from our Newtonian
reference frame with the said acceleration (fig 2a). If we place ourselves in the Sun frame the movement of both
would be as seen in (fig 2b). (as the
factor
comes into the gravitorelative acceleration
it is very small and must always be taken as a first approximation).
|
|
|
|
(fig 2a) |
(fig 2b) |
We will calculate the separation S
produced at the end of a period T between the Newtonian frame and the
planet on which the gravitorelative acceleration acts.
The separation produced in the interval of
time
is:
![]()
where
is the average acceleration which is
approximately equal to
, where a is the length of the major
semiaxis of the orbit. The value of
is calculated in the
data section.
In a complete period T, the separation S from
the Newtonian orbit is:
![]()
this separation represents a displacement of
the perihelion which corresponds to a deviation angle equal to:
![]()
where
is
the radius of the perihelion. The velocity of spin of the perihelion is
therefore
so in one century the perihelion covers the
following angle:
![]()
K is the product of the number of seconds in a
century by the radian conversion factor in angular seconds, and e is the
eccentricity of the orbit. Therefore, in one century the perihelion moves at an
angle equal to:
![]()
This result admits only a slight error of a
few angular seconds due to the use of average values to obtain it. Therefore,
the precession of elliptic orbit can also be gathered from the gravitorelative
theory. The value obtained in 1973 for the "general precession" of
Mercury is approximately 41.4". Whilst the value obtained from the G R
theory is 43".
|
|
|
|
Data: |
|
|
|
|
100 000-year Glacial Periods
Recently it has been possble to establish quite
a reliable chronology of the glaciations using various methods, the most
important of which is based on the isotopic analysis of the oxygen in marine
sediments. It is known that in the last million years some 10 glaciations have
taken place, the last of which occurred some 18 000 years ago. The average
temperature then was about 5 ºC lower than the present average and ice
covered a third of the Earth's surface.

(fig 3)
Variation of the temperature in the last 500 000 years which
corresponds to the volume of ice in the glaciars in accordance with the
relation of the two oxygen isotopes in marine sediments. (The heavy oxygen
isotope O-l8 is more resistent to evaporation so it appears less in glacial ice
water than in ocean water. Therefore when continental ice layers are formed,
the ocean water and the shells of marine organisms which fall in the ocean
sediments appear enriched in oxygen-18).
On the other hand, it is known that due to the
small gravitational attraction of the Moon and the other planets, the orbital
parametres of the Earth change with time. The inclination of the Earth's axis
varies between 22.1 and 24.5 degrees with a period of some 40 000 years. The
eccentricity of the orbit varies between 0.005 and 0.006 approximately, with a
period of some 100 000 years. The terrestrial axis takes some 26 000 years to
describe a complete precession circunference.
The spectral analysis of figure 3 shows a
certain number of fundamental frequencies. The frequency of greatest intensity
corresponds to a cycle of some 100 000 years, then there are three notable
cycles, one of 40 000 and two others of 24 000 and 19 000 years each. The
climatic variation of the last three frequencies may be explained from the
variations in the inclination of the Earth's axis which produce a variation in
average sunshine in the high latitudes of the northern hemisphere (where there
is more continental area) in the different seasons (this explanation was given
by the Yugoslavian astronomer Milutin Milancovitch and verified by Gerard R.
North and his colleagues at NASA with experiments carried out with models of
energetic balance). What continues to be an enigma is the main cycle of 100 000
years in the glacial periods. It is thought that this cycle must be linked to
the variation of the eccentricity of the terrestrial orbit, but it is not known
how .
According to the gravitorelative theory, when
the eccentricity of the orbit is increased, the component of radial gravitorelative acceleration is
increased in the opposite direction to the gravitostatic acceleration, which
makes the radius of the orbit increase. While when the eccentricity is
decreased the radial gravitorelative
acceleration increases in the same direction as the gravitostatic acceleration,
which makes the radius decrease.
For an eccentricity e given the average value
of the radial gravitorelative acceleration is equal to:
![]()
The two terms of the addition correspond to
the radial components of the perpendicular and parallel gravitorelative
accelerations respectively, while
is the average value of the angle
, which
varies between the maximum value
and the minimum value arccos e, that
is to say:
, and
is the average
gravitorelative acceleration for an eccentricity e given, in which r
and v are the average values of the orbital radius and velocity (
is
practically equal to 1 as the eccentricity in all cases is small).
From the data that we possess we can see that
the curve of variation in time of the ice layers is slanting towards the right
which means that ice takes more time in forming that in melting. This can be
due to the elastic properties of the bed-rocks over which the ice acumulates,
since the weigth of the ice layers causes the collapse (sinks) of the bed-rocks
through thousands years, which makes easier the melting of the ice. Afterwards
the bed-roks raises again. Thus, the solar irradiation that the Earth recives
does not determine the volume of ice in the glaciars but it is, however, the
main cause, and the explanation of the great intensity of the 100 000-year
glacial periods.
Let us calculate the distance
r = rmax - rmin travelled by the Earth in its fall, (rmax and rmin are the average radii that correspond
to the maximun and minimum orbits).
In order to simplify this calculation, we are
going to consider that the gravito-relative force change in a linear way in
time (this is a good aproximation since it changes very slowly), and that there
are two phases in the Earth fall: one of acceleration and another of
deceleration.
This distance is appoximately equal to:

where tc is the fall time and
is the increase
in the radial gravitorelative acceleration (or deceleration) which is equal to:
![]()
is the average gravitorelative acceleration
in the whole cycle which in turn is equal to:
![]()
where v and r are the average
velocity and the average radius of the orbit in the whole cycle, that we can
take with a good approximation equal to the present average values.
On the other hand, the average sunshine is
inversely proportional to the square of the distance, while the temperature is
proportional to the average sunshine, that is to say:

where E(rmin ) is the average
sunshine in the orbit of minimum average radius, while E(rmax ) is average
sunshine in the orbit of maximun average radius, T(rmin ) y T(rmax ) are the
respective average temperatures.
Developing the square in brackets we will
obtain that the total increase in the temperature
T
= T(rmin ) - T(rmax ) is
approximately equal to:
![]()
Then the total variation of temperature is
about 21 ºC.
The variation of temperature in the last 18 000 years can be obtained changing
the minimal eccentricity by the actual one, taking the fall time tc
equal to 18 000 years, and only considering
the acceleration phase, that is to say:
. We obtain a variation of
temperature of about 5.5 ºC. So, in the last 18 000 years the average
temperature of the Earth is increased about 5º C which agrees with the
estimates made by geologists, which demonstrates Milutin Milancovitch
hypothesis that the glacial periods are linked to orbital variations.
|