Chapter Four
Fundamental Nature of the Mechanism Responsible
for the Advance of the Perihelion of
Mercury.
4.1 Definition of the Absolute Standard
Units [o.s.]. In order to understand
the mechanism responsible for the advance of the perihelion of Mercury, we
need to explain the meaning of quantities such as an absolute standard of
mass, time or length. The meaning of absolute standards is such that each
of them must always represent the same and unique physical quantity in any
frame. This condition is necessary since the absolute length of a rod does
not change because it is measured from a different frame. This also
applies to an absolute time interval and an absolute mass: they do not
change when measured in different frames. However, an absolute length,
time interval or mass can be described using different parameters (e.g.
different units). One must conclude that lengths, time intervals and
masses are absolute and exist independently of the observer. They never
change as long as they remain within one constant frame. However, they
appear to change with respect to an observer who moves to a different
frame because they are then compared with new units located in a different
frame.
In relativity, we always read an expression with respect to a frame "of
reference". The phrase "of reference" gives the illusion that masses,
lengths and clock rates really change as a function of the "reference"
used to measure them. That there could be a real physical change of mass,
length and clock rate because the observer uses a different "reference"
does not make sense. This apparent change of length, clock rate or mass is
simply due to the observer using different units of comparison. In this
book, we avoid the words "of reference" because they are clearly
misleading. We have seen that when
a rod changes frames, its absolute length changes. However, when an
observer carrying his reference meter changes frames, the length of the
rod that remains at rest corresponds to a different number of the
observer's new reference meter. When a rod changes frames, the change of
its length is real as seen in chapters one and three. However, when the
observer changes frames (with his reference meter) and the rod does not,
there is only a change in the number of measured meters; the rod does not
change. Consequently, the change of frame of the rod and the change of
frame of the observer (carrying his reference meter) are not
symmetrical.
4.2 - The Absolute Reference
Meter. The usual definition of
the meter is 1/299 792 458 of the distance traveled by light during one
second. The local clock is used to determine the second. We recall from
section 2.4 that this definition is not absolute because it depends on the
definition of the second which is a function of the local clock rate which
changes from frame to frame. Unfortunately, there is
no direct way to reproduce an absolute meter within a randomly chosen
frame. We have seen that carrying a piece of solid matter from one frame
to another one (in which the potential or kinetic energy is different)
leads to a change of the Bohr radius and consequently to a change in the
dimensions of the piece of matter. However, a local meter can apparently
be reproduced in any other frame using a solid meter previously calibrated
in outer space and brought to the local frame. Of course, the absolute
length of that local meter in the new frame will not be equal to its
absolute length when it was in outer space because the potential and
kinetic energies may change from frame to frame. One can also reproduce
a local meter in any frame by calculating 1/299 792 458 of the distance
traveled by light in one local second. However, the duration
of the local second must be corrected with respect to the reference
clock-rate existing in outer space (with v = 0). It is illusionary to
believe that absolute time and absolute length can be obtained in any
frame just by carrying a reference atomic clock and a reference meter to
the new frame. We define the
absolute reference meter (metero.s.) as the
distance traveled by light during 1/299 792 458 of a second given by a
clock located at rest in outer space away from any mass. The subscript
o.s. defines where the meter is located. This unit of length is equal to a
number Bo.s. times the length of the Bohr radius
ao.s. in outer space. An absolute reference meter must
have the same absolute physical length, independently of the frame where
it is located (and of the frame where the observer is located).
Consequently, an observer must make relevant corrections to his local
meter to reproduce the absolute reference meter. The definition of the
absolute reference meter is then:
metero.s. =
Bo.s.ao.s. |
4.1 |
The absolute meter can
be reproduced in any frame but it is defined with respect to a length in
outer space. The constant Bo.s. (the inverse of the Bohr
radius) is about 1.8897263×1010. Since the
Bohr radius a varies with the electron mass (which changes with
potential and kinetic energies), the constant number Bo.s.
times the outer space Bohr radius a is not an absolute standard
when the meter is not located in outer space. The Earth meter
(meterE) is different from the absolute
reference meter (metero.s.) because the Bohr radius is longer
on Earth. The length of the Earth meter is:
We see that the length
of a meter at a Mercury distance from the Sun is also different from the
length of a meter in outer space or on Earth. Let us study the example of
Mercury since we wish to predict a phenomenon taking place at the distance
from the Sun where Mercury is orbiting. The length of the Mercury meter
(meterM) is:
In order to avoid
useless lengthy repetitions, we will shorten some of the descriptions.
Instead of repeating that we refer to a location at the Mercury distance
from the Sun which has zero orbital velocity, we will simply say "Mercury
location" and the context will provide the supplementary information. The
velocity component of Mercury will be considered separately later. All
other parameters will be taken into account only later because they are
not relevant in this chapter and would bring confusion. An absolute
standard of reference will sometimes be called in short "absolute meter",
"absolute time rate" or "absolute mass" when it corresponds to the
standard established in outer space. In the problems
considered in these first chapters, the relative changes of length, time
rate and mass will always be extremely small. In the case of Mercury,
which is the closest planet to the Sun, these changes will be as small as
about one part per billion. Consequently we will regularly simplify the
calculations by using only the first order. This will be an excellent
approximation. The derivative of the function will then become equal to
the finite difference as used in chapter one. This does not change the
fundamental understanding of the phenomenon as we will see below.
We have seen
in equation 4.1 that the absolute reference meter is a constant number of
times (Bo.s.) the Bohr radius in outer space
(ao.s.). However, the Bohr radius does not change solely
with the gravitational potential. It also changes with velocity. We define
the absolute outer space meter as being a meter in outer space with zero
velocity. From equation 1.22, the relationship giving the Bohr radius
a when there is no change of velocity is (using outer space
units):

|
4.4 |
which gives:

|
4.5 |
where mgDh is the change of potential energy (Pot.) of a mass m
in a gravitational field across height Dh. In the
case of a central force, Newton's laws say that the gravitational
potential (Pot.) of a body decreases when the distance (R) from the
central body increases. The gravitational potential of a body of mass
M(M) (in the case of Mercury) at a distance
RM from the Sun of mass M(S) with
respect to outer space is:

|
4.6 |
where G is the
Cavendish gravitational constant and g is the gravitational acceleration
where the mass is located (here in the solar gravitational field).
In previous
chapters, we have used the brackets [rest] and [mov] to indicate the
units. From now on, depending on whether we refer to the units of length,
mass, clock rate, etc., located in outer space (free from a gravitational
potential) or units in the gravitational potential of Mercury, we will use
the indices [o.s.] or [M]. The units will always be "translated" in
absolute units (e.g. Mercury second = 1.01 absolute seconds). Using
equations 4.1, 4.3, 4.5 and 4.6, we find that the length of the Mercury
meter (meterM) compared with the absolute
reference meter (metero.s.) is:

|
4.7 |
We recall that the
length of the meter (metero.s.) in outer space is the absolute
standard reference. However, we know that when an observer is located on a
different frame to measure a given length, he finds a different answer
because his unit of comparison (his local meter) is different.
It is useless
here to specify the units of GM(S)/c2RM. Logically, they should be
coherent i.e. either [M] or [o.s.]. Physically, it makes no difference
whether the units of G, M(S) or R are the same or not since the
error brought in this way is of the order of
10-9 on
GM(S)/c2RM which is itself of the order of
10-9 with respect to the
meter.
4.3 - The Absolute Reference
Second. An equivalent
transformation must be taken into account when time is defined. We can
evaluate time on different frames using a local cesium clock. However, one
must recall that the rate of such a clock (or of any other clock) changes
with the electron mass and therefore with the potential and kinetic
energies where the clock is located. Therefore a correction must be made
if we want to know the absolute time. For the case of zero
gravitational potential, we now define an absolute time interval called
the absolute reference second just as in section 3.5.1 where the second
was defined for the case of zero velocity. During one absolute second, a
cesium clock makes N(S) (where the index (S) refers to the definition of a
second) oscillations that are counted from the number of cycles of
electromagnetic radiation emitted. That cesium clock must be located
outside the gravitational potential of the Sun and have zero velocity. By
definition, that absolute time interval will be called the "outer space
second". We have:
absolute ref. second º N(S)
Oscillations (cesium clocko.s.). |
4.8 |
During one absolute
second, a cesium clock in outer space emitting N(S) cycles shows a
difference of clock displays labeled DCDo.s.(S). We must emphasize that DCDo.s.(S) does not correspond to any value
of DCD, it corresponds only to the number of
counts on the outer space clock leading to the absolute second. This is
shown by (S) following the DCD. Consequently,
DCDo.s.(S) representing the absolute
reference second must not be confused with a simple value of DCDframe (without (S))
which can be any number of seconds. We have:
1
abs. sec. º DCDo.s.(S) º
N(S) Oscillations(cesium clocko.s.) |
4.9 |
When an observer on
Mercury observes that his cesium clock has emitted the same number N(S) of
cycles, the absolute time interval elapsed is not the absolute second
since the Mercury clock is slower. That time interval is called the
Mercury second. We have:
1
Mercury sec. º DCDM(S) º N(S) Oscillations(cesium
clockM) |
4.10 |
Therefore we define one
"local second" as the time elapsed when the numerical value shown on a
local frame is equal to DCDframe(S). Of course,
the Mercury second represented by DCDM(S) lasts longer
than the outer space second represented by DCDo.s.(S) because even if the differences
of clock displays DCDo.s.(S) and DCDM(S) are equal, the
Mercury clock is slower. Consequently, during one local second, we have
for the outer space clock the same DCD than for
the Mercury clock:
1
local second º DCDframe(S) |
4.11 |
Since the principle of
mass-energy conservation and Bohr equation teach us by how much the rates
of two clocks located in outer space and on Mercury differ, an observer on
Mercury can calculate the absolute time using his Mercury clock and making
suitable corrections due to the gravitational potential at Mercury
location (we will consider the velocity of Mercury later).
Let us
consider that a clock in outer space records a difference of clock
displays equal to the number DCDo.s..
The corresponding absolute time interval elapsed is called Dto.s.[o.s.]. That absolute time interval
can be measured on different locations like Mercury or outer space. For a
phenomenon taking place in outer space, a time interval can be
written:
Dto.s.[o.s.] = DCDo.s.(o.s.)DCDo.s.(S) |
4.12 |
where Dto.s.[o.s.] is the absolute time interval,
DCDo.s.(o.s.) is the
number of seconds shown by the outer space clock and DCDo.s.(S) is the absolute unit of time in
outer space given by the o.s. clock. In equation 4.12, the
symbol [o.s.] after Dto.s. is due to
the units of time DCDo.s.(S). The
parentheses in DCDo.s.(o.s.) indicate
the units used for the measurement. The subscript o.s. of Dto.s.[o.s.] andDCDo.s.(o.s.) refers to the location where
the phenomenon takes place (this is different from what we did in chapter
three). When an outer space phenomenon is observed using a Mercury clock,
the absolute time interval Dto.s. [M]
measured on a clock on Mercury is given by the relationship:
Dto.s.[M] = DCDo.s.(M)DCDM(S) |
4.13 |
where DCDo.s.(M) is the number of
Mercury seconds and DCDM(S) is the unit of time of the clock located on Mercury, as
described in equation 4.10. Of course, a Mercury
second is not equal to one real outer space second. The absolute second is
defined in outer space. Therefore a Mercury second is not a real time
interval. It corresponds to a difference of clock displays which can be
described as an apparent time on Mercury. If a phenomenon taking
place in outer space is measured using a clock located in outer space, its
duration will be represented by the absolute time interval Dto.s.[o.s.] (equation 4.12). If this same
phenomenon is measured using the Mercury clock, the same absolute time
interval will be represented by Dto.s.[M] (equation 4.13). Of course, one
single phenomenon does not last a longer absolute time because it is
observed from a different location using a different clock. The real
absolute duration is the same in any frame. This gives:
Dto.s.[o.s.] = Dto.s.[M] |
4.14 |
Using
equations 4.12 and 4.13 in 4.14, we find:
DCDo.s.(o.s.)DCDo.s.(S) = DCDo.s.(M)DCDM(S) |
4.15 |
4.3.1 - Example. In order to clarify
this description, let us give a numerical example. Let us assume that an
atomic clock located in outer space has emitted 20 times N(S) cycles of
E-M radiation. After N(S) cycles, one more absolute second DCDo.s.(S) has elapsed and this is repeated
DCDo.s.(o.s.) times (with DCDo.s.(o.s.) = 20). Consequently, the
corresponding time interval Dto.s.[o.s.] elapsed is 20 absolute (or
outer space) seconds, as given in equation 4.12. That same clock is moved
to a stationary location (for example Mercury) near a very massive star so
that the relativistic electron mass decreases by 1.0% due to the change of
gravitational potential. Quantum mechanics shows that the atomic clock
will then run at a rate which is 1.0% slower (as explained in chapter
one). Consequently, since the atomic clock on that planet is slower than
when it was in outer space, it will take a longer absolute time to make
the same number N(S) of oscillations. Since the Mercury second is defined
(in equation 4.10) as the time required for the clock on Mercury to emit
N(S) cycles, it is longer than the outer space second. This gives:
1 Mercury second = 1.01 Absolute
second |
4.16 |
Consequently, during the time interval in which the outer space
clock will record an absolute time interval Dto.s.[o.s.] equal to 20 outer space seconds
(DCDo.s.(o.s.)), the Mercury clock
will record a smaller DCDo.s.(M)
because it runs at a slower rate. The DCDo.s.(M) recorded on Mercury will be 1.0%
smaller:

|
4.17 |
giving the numerical
value:

|
4.18 |
Therefore,
in agreement with equation 4.14, since the Mercury second lasts longer, as
seen in equation 4.16, the total absolute time elapsed on Mercury (Dto.s.[M]) is the same as the total absolute
time in outer space. We find in equation 4.12:
Dto.s.[o.s.] = 20×1
absolute second = 20 absolute seconds |
4.19 |
From equations 4.13,
4.16 and 4.18 we have:
Dto.s.[M] =
19.80198×(1.01 abs. seconds) = 20 abs. seconds |
4.20 |
Therefore, Dt is a real absolute time interval in all
frames.
4.3.2 - Relative Clock Displays
between Frames. We have seen that the
clock used in each frame simply counts the number of cycles emitted by the
local atomic clock. In all frames, the local second is equal to the count
of N(S) cycles on the local clock. During one absolute time interval, the
number of cycles is then proportional to the absolute clock rate which is
its absolute frequency as given by equation 1.22 (when v = 0). Therefore,
during one absolute time interval, the ratio of the differences of clock
displays between frames is directly proportional to the ratio of the
natural frequency of each clock. This gives:

|
4.21 |
Equation 4.21 gives the
relative frequencies of clocks located in different frames. Obviously, it
does not matter whether the phenomenon measured is in outer space or on
Mercury, as long as both clocks measure the same phenomenon. This means
that the subscripts of the left hand side of 4.21 could both be M instead
of o.s.. If there is a difference of kinetic energy between the frames,
equation 3.9 must be applied. Any difference of clock rate is caused by
the difference of gravitational potential and/or kinetic energy between an
outer space location and the orbit of Mercury. In the case of pure
potential energy, using equations 1.22 and 4.6, the relative clock rate is
given by the relationship:

|
4.22 |
which gives:

|
4.23 |
Using equation 4.21
with equation 4.23, we see that during the same absolute time interval,
the relative difference of clock displays is:

|
4.24 |
Let us note that these
equations do not take into account a second order that might exist when
the particle moves down in the gravitational potential. Since that second
order effect is quite negligible in the first chapters of this book, we
will consider it only if it becomes significant.
4.4 - The Absolute Reference
Kilogram. The absolute unit of
mass is also defined in outer space. We have seen in chapter one that one
absolute kilogram (kgo.s.) in outer space contains a different
amount of mass after it is carried to Mercury. When we carry a mass of one
kilogram (kgo.s.) from outer space to Mercury location (at
rest), the amount of mass decreases (because it gives up energy during the
transfer). However, the observer on Mercury will still call it one Mercury
kilogram (kgM) since the number of atoms
has not changed. In fact, nothing appears to change for an
observer moving with the kilogram and observing a physical phenomenon on
Mercury. The relationship between two kilograms located in different
potentials is given in equation 1.5. Using equations 1.5 and 4.6, we
find:

|
4.25 |
Equation 4.25 gives the
mass of the outer space kilogram with respect to the Mercury
kilogram.
4.5 - Space and Time Corollaries
within the Action-Reaction Principle. Let us discuss what
happens inside a frame located at the position where Mercury interacts
with the Sun's gravitational field. What is the behavior of Newton's laws
at that location? We believe in the
principle of causality. The cause is the reason for the action. Newton
applied this principle and stated that an action is always accompanied by
a reaction. However, even if this has not been stated specifically, it
becomes obvious that there are two corollaries to that principle. The
first corollary is that both the action and the reaction take place at
exactly the same location where the interaction takes place. The second
corollary is that both the action and the reaction take place at exactly
the same time the interaction takes place. The principle of causality
implies that it is illogical and indefensible to believe that the cause of
a phenomenon does not take place at the same location and at the same time
that the effect does. Let us apply those
corollaries to relativity. When a mass moves in a gravitational field, its
trajectory is modified by the action of the gravitational field. The
interaction between a mass and a gravitational field takes place at the
location of the mass and at the moment the mass is interacting with the
field. Consequently, the relevant parameters during the interaction are
the amount of mass and the intensity of the gravitational field at the
location of the interaction. It would be absurd to calculate an
interaction using quantities that exist somewhere else than where the
interaction takes place. When we study the behavior of Mercury interacting
with the solar gravitational potential, we must logically use the physical
quantities existing where Mercury is located. This means that when we
calculate the behavior of planet Mercury, we must use the units of length,
clock rate and mass existing at Mercury location. This is the only logical
way to be compatible with the principle of causality and with its natural
corollaries leading to the principle of action-reaction. It would not make
sense for the mass of Mercury involved in the interaction with the solar
gravitational field to be the mass it has in outer space rather than its
real mass where it is located at the moment it is interacting near the
Sun.
Therefore the amount of mass, length and clock rate that must be used in
the equations are the ones that appear at Mercury location, since they are
the only relevant parameters logically compatible with the physics taking
place on Mercury. At Mercury location, there is no other physics than the
one using the local mass, length and clock rate. Logically, it must be so
everywhere within any frame in the universe. This point is extremely
important and is fundamental in the calculations below because it is the
basic phenomenon that explains the advance of the Mercury perihelion
around the Sun. 4.6 - Fundamental Mechanism
Taking Place in Planetary Orbits. In classical mechanics,
it is demonstrated that planets revolve around the Sun in a circular or
elliptical orbit. The complete period of an orbit can be defined as the
time taken to complete a full translation of 2p
radians around the Sun or as the time interval taken by the planet to
complete its ellipse between the passages of a pair of perihelions. It is
usually considered that these two definitions of a period of an orbit are
identical. However, if the ellipse is precessing, the angle spanned
between the two passages of a pair of perihelion is larger than for a non
precessing ellipse i.e. larger than 2p radians.
This means that the full translation of 2p
radians is completed before the ellipse reaches the next perihelion.
Therefore we expect the period of that precessing ellipse to be
larger. One of the fundamental
phenomena implied in such an orbital motion is the gravitational potential
decreasing as the inverse of the distance from the Sun where the planet is
orbiting. When the orbit is circular, it is difficult to determine at what
instant one full orbit is completed other than measuring a translation of
2p radians with respect to masses seen in outer
space. However, in an elliptical orbit (as in the case of Mercury around
the Sun), the direction of the major axis can be easily located in space
from the instant Mercury is at its perihelion, i.e. its closest distance
from the Sun.
4.6.1 - Significance of Units
in an Equation. In Galilean mechanics,
when the units are identical in all frames, the pure number that
multiplies the unit is undistinguishable from the quantity that includes
the unit. For example, when someone reports that a rod is ten meters long,
we can assume that either he has in mind that the rod is ten times the
length of the standard meter (in which ten is a pure number separated from
the unit of length), or he means a single global quantity with unit,
corresponding to one single quantity ten times longer than the unit meter.
Of course, the difference brings no consequence at all when we always use
the same standard meter. However, the correct interpretation must be
understood and specified here because the size of the reference meter (and
all other units) changes from frame to frame. If "a" represents the
semi-major axis of the elliptical orbit of Mercury, we have to find
whether "a" represents a pure number (to which a unit is added and
considered separately) or a single global quantity (with units included).
This can be answered if we study the fundamental role of a mathematical
equation. In mathematics, we learn that an equation is a fundamental
relationship between numerical quantities. The same mathematical equation
can relate numbers (or concepts) having different units. This can be
illustrated in the following way. If an apple costs 50
cents, how many apples (N) will we buy with $10.00? We use the following
equation:

|
4.26 |
With a = $10.00, and b
= $0.50 each, we find
Now, if we also find
that an orange costs 50 cents, how many oranges will we have for $10.00?
Using again equation 4.26 with a = $10.00 and b = $0.50 each, we
find:
We also want to buy
peas. They cost 1 cent each. How many peas do we get for $10.00? Using
again equation 4.26, we find that the number of peas is:
Equations 4.27, 4.28
and 4.29 illustrate that the mathematical parameter N does not represent
apples, oranges or peas. It represents only the numerical value of the
unit. The unit must be specified separately. One must know that the units
also follow a separate mathematical relationships. This is called a
dimensional analysis which requires an analysis separate from the
numerical analysis. Therefore, "a"
represents the number of units of length. The same remark
must be applied to all physical quantities that are pure numbers obtained
from a previous definition of other standard units. Furthermore, in order
to be compatible with the principle of causality given above, the units of
length, mass and clock rate must necessarily be the ones existing on
Mercury where the phenomenon takes place. We will see below how this description leads to a perfect coherence. In the solar system,
the orbit of Mercury is very elongated and is an excellent example to
study Kepler's laws. However, since there are several other planets moving
around the Sun, there are other classical corrections due to the
interactions between these other planets that need to be taken into
account. Extensive classical calculations show that the interaction of the
other planets of the solar system also produces an important advance of
the perihelion of Mercury. After accurate calculations, data show that the
advance of the perihelion of Mercury is larger than the value predicted by
classical mechanics. The advance of the perihelion is observed to be 43
arcsec per century larger than expected from all classical interactions by
all planets. In order to solve this
problem, we have to examine in more detail the conditions in which the
equations must be applied. As we will see in chapter five, the
number of seconds giving the period P is a function of the
parameters a, G, M(S) and M(M). However, due to mass-energy
conservation we have seen that the units of length, time and mass are
different at Mercury distance from the Sun than in outer space. In section
4.5, we have also seen that the action of the gravitational potential on
Mercury must be calculated using the number of units of mass (and all
other parameters) that Mercury has at that location.
4.7 - Transformations of
Units.
4.7.1 -
aM(o.s.) versus aM(M). When we measure the
number of meters that constitute a given length, we find
that this number depends on the length of the unit used in conjunction
with it. We call aM(o.s.), the
number of outer space meters that represents the length of
the semi-major axis of the orbit of Mercury when we use outer space
meters. The absolute physical length LM[o.s.] being measured using outer space meters is then:
LM[o.s.] =
aM(o.s.)metero.s. |
4.30 |
The value of the
absolute length LM[o.s.] of the semi-major
axis of the orbit of Mercury corresponds to measuring the number
aM(o.s.) of meters in the orbit times the
outer space meter (metero.s.). We now have to determine the
number aM(M) of Mercury
meters (meterM) found in conjunction with
Mercury units. aM(M) represents the
corresponding number of Mercury meters to measure the same
length when we use Mercury meters. We find that the absolute physical
length LM[M] of the semi-major axis, is
given by:
Since a physical length
does not change because we use a different reference meter to measure it,
we must understand that the absolute physical length of the semi-major
axis is the same whether it is measured using outer space or Mercury
units. Therefore, the absolute length LM[frame] of the semi-major axis of the orbit of Mercury is the same
independently of the units used to measure it. Therefore, equations 4.30
and 4.31 are identical:
LM[M] =
LM[o.s.] = aM(o.s.)metero.s. = aM(M)meterM. |
4.32 |
Equation 4.32 gives us
the relationship between the number aM(o.s.) of outer space meters and the number
aM(M) of Mercury meters to measure the
same length. This gives:

|
4.33 |
Combining equations 4.7
and 4.33 gives:

|
4.34 |
Equation 4.34 shows
that the number aM(M) of
Mercury meters required to equal the semi-major axis of Mercury is smaller
than the number aM(o.s.) of outer space
meters since the outer space meter is shorter. Therefore the outer space
observer will record a larger number
aM(o.s.) of meters than the Mercury
observer even if both observers are measuring the very same semi-major
axis.
4.7.2 - M(S)(o.s.) and
M(M)M(o.s.)
versus M(S)(M) and M(M)M(M). The symbols (S)
and (M) represent respectively the Sun and Mercury.
M(S)(o.s.) and M(M)M(o.s.)
represent the numbers of absolute outer space kilograms
(kgo.s.) for the Sun and Mercury
respectively. The subscript M of M(M)M(o.s.) indicates that the planet is at Mercury location. The
numbers of Mercury units that give the same masses are represented by
M(S)(M) and M(M)M(M). The
absolute solar mass m(S)[o.s.] using outer
space units is:
m(S)[o.s.] =
M(S)(o.s.)kgo.s. |
4.35 |
Using Mercury units,
the same absolute solar mass is given by:
m(S)[M] =
M(S)(M)kgM |
4.36 |
Since the solar mass
does not change because we measure it using Mercury units instead of outer
space units, we have:
m(S)[o.s.] = m(S)[M] |
4.37 |
Similarly, the mass of
Mercury measured with outer space units is:
m(M)M[o.s.] = M(M)M(o.s.)kgo.s. |
4.38 |
When the measurement is
done with Mercury units, the same mass is given by:
m(M)M[M] = M(M)M(M)kgM |
4.39 |
Since it is the same
absolute mass of Mercury described using different units, we have:
m(M)M[o.s.] = m(M)M[M] |
4.40 |
Due to mass-energy
conservation, the amount of mass contained in one local Mercury kilogram
is different from the one in one outer space kilogram. From equations
4.35, 4.36 and 4.37 we have:

|
4.41 |
The left hand side of
equation 4.41 gives the ratio between the number of outer
space kilograms and the number of Mercury kilograms needed
to measure the same solar mass. From equation 4.25, we get:

|
4.42 |
Combining equations
4.41 and 4.42 gives:

|
4.43 |
Equation 4.43 shows
that the number of kilograms M(S)(o.s.) found in the
measurement of the solar mass is smaller when measured in conjunction with
the outer space kilogram than when measured in conjunction with the
Mercury kilogram. Combining equations 4.38, 4.39 and 4.40 with 4.42, we
get for the case of the mass of Mercury:

|
4.44 |
Consequently, the
number M(M)M of kilograms giving
the mass of Mercury is smaller using outer space kilograms than using
Mercury kilograms.
4.7.3 - PM(o.s.) versus PM(M). In equations 4.12 and
4.13, we have calculated absolute time intervals Dt as measured from outer space location (Dto.s.[o.s.]) and Mercury location (Dto.s.[M]). Let us consider now that the time interval
Dt is the period of translation of Mercury to
complete an ellipse around the Sun. The number of seconds
PM(o.s.) giving the period of Mercury when measured with an outer space
clock is given by the relationship:
DtM[o.s.] = PM(o.s.) DCDo.s.(S) |
4.45 |
and the period
PM(M) measured on Mercury using a Mercury
clock (with Mercury units) refers to the relationship:
DtM[M] = PM(M) DCDM(S) |
4.46 |
The time intervals
DtM[o.s.] and
DtM[M] in
equations 4.45 and 4.46 represent the absolute time interval for the
period P of translation of Mercury around the Sun. An absolute time
interval is not different because it is measured with a Mercury clock
instead of an outer space clock:
DtM[o.s.] = DtM[M] = PM(M) DCDM(S) = PM(o.s.) DCDo.s.(S) |
4.47 |
We have seen in
equation 4.24 the ratio of the numbers DCDM(o.s.)
and DCDM(M)
between two frames in different gravitational potentials. We see that the
numbers PM(o.s.) and
PM(M) displayed by the clocks correspond
to DCDM(o.s.) and
DCDM(M) during
one period of translation. Therefore,

|
4.48 |
Combining equation 4.48
with 4.24 gives:

|
4.49 |
Equation 4.49 shows
that even if the absolute time interval Dt for
the period is the same in both frames, the differences of clock displays
are different because the clocks run at different rates.
4.7.4 - G(o.s.) versus G(M)
.
Since lengths, clock rates and masses are not the same in different
frames, we see now that the gravitational constant G is different when
measured using Mercury units. The number of outer space
units of the gravitational constant is called G(o.s.) and the
number of Mercury units of the same gravitational constant
is called G(M). The fundamental units corresponding to the gravitational
constant G are called respectively Uo.s. and
UM. The total gravitational constant G is
called J[o.s.] when measured from outer space and J[M] when measured from
Mercury orbit. Therefore we have:
J[o.s.] = G(o.s.)Uo.s. |
4.50 |
and
Since the absolute
gravitational constant does not change because we measure it from a
different location, we have:
The relative number of
units between G(o.s.) and G(M) is found using a dimensional analysis. The
units of G can be obtained from Newton's well known gravitational
law:

|
4.53 |
where the force F is in
newtons, M and m are in kilograms and the radius R is in meters. From
equation 4.53 and recalling that the units of G(o.s.) are called
Uo.s., we find:

|
4.54 |
From the
relationship
where a is the acceleration, we find that the units of F
are:

|
4.56 |
Combining 4.54 with
4.56 we get:

|
4.57 |
From the definition of
velocity, the units of v are:

|
4.58 |
Equation 4.58 in 4.57
gives:

|
4.59 |
We have seen in
sections 3.5.3 and 3.6 that a velocity is represented by the same number
within any frame. This means that the number representing a
velocity is the same within any frame when it is measured using any
coherent system of local units. Since a velocity is the quotient between a
length and a time interval, this quotient stays constant even when
switching between frames because the same correction is made on both
lengths and clock displays. Consequently, we have:
Equations 4.7, 4.42 and
4.60 in equation 4.59 give:

|
4.61 |
The first order
expansion of equation 4.61 gives:

|
4.62 |
By analogy with 4.59
for UM, we have:

|
4.63 |
Equation 4.63 in 4.62
gives:

|
4.64 |
Equations 4.50, 4.51,
4.52 and 4.64 give the relationship between the number of
units of G:

|
4.65 |
Equation 4.65 shows
that the gravitational constant G is represented by different numbers when
measured with the units existing on Mercury and in outer space.
4.7.5 - F(o.s.) versus
F(M). From equation 4.56 we
have:

|
4.66 |
Using equations 4.7,
4.15, 4.24 and 4.25, we find:

|
4.67 |
To the first order,
this is equal to:

|
4.68 |
and:

|
4.69 |
Consequently, the
relationship between the number of Mercury newtons and the number of outer
space newtons is given by:

|
4.70 |
4.8 - Symbols and Variables.
aframe[o.s.] |
length of the local Bohr radius in absolute
units |
aM(M) |
number of Mercury meters for the semi-major axis
of Mercury |
aM(o.s.) |
number of outer space meters for the semi-major
axis of Mercury |
DCDM(M) |
DCD for the period of
Mercury measured by a Mercury clock |
DCDM(o.s.) |
DCD for the period of
Mercury measured by an outer space clock |
DCDM(S) |
apparent second on Mercury |
DCDo.s.(M) |
DCD in outer space
measured by a Mercury clock |
DCDo.s.(o.s.) |
DCD in outer space
measured by an outer space clock |
DCDo.s.(S) |
absolute second in outer space |
DtM[M] |
period of Mercury in Mercury units |
DtM[o.s.] |
period of Mercury in outer space
units |
Dto.s.[M] |
time interval in outer space in Mercury
units |
Dto.s.[o.s.] |
time interval in outer space in outer space
units |
G(M) |
number of Mercury units for the gravitational
constant |
G(o.s.) |
number of outer space units for the gravitational
constant |
J[M] |
gravitational constant in Mercury
units |
J[o.s.] |
gravitational constant in outer space
units |
kgframe |
mass of the local kilogram in absolute
units |
LM[M] |
length of the semi-major axis of the orbit of
Mercury in Mercury units |
LM[o.s.] |
length of the semi-major axis of the orbit of
Mercury in outer space units |
meterframe |
length of the local meter in absolute
units |
M(M)M(M) |
number of Mercury units for the mass of Mercury at
Mercury location |
m(M)M[M] |
mass of Mercury in Mercury units at Mercury
location |
M(M)M(o.s.) |
number of outer space units for the mass of
Mercury at Mercury location |
m(M)M[o.s.] |
mass of Mercury in outer space units at Mercury
location |
M(S)(M) |
number of Mercury units for the mass of the
Sun |
M(S)(o.s.) |
number of outer space units for the mass of the
Sun |
m(S)[M] |
mass of the Sun in Mercury units |
m(S)[o.s.] |
mass of the Sun in outer space units |
N(S) |
number of oscillations of an atomic clock for one
local second |
PM(M) |
DCD for the period of
Mercury measured by a Mercury clock |
PM(o.s.) |
DCD for the period of
Mercury measured by an outer space clock |
RM |
distance between Mercury and the Sun |
Uframe |
unit of the gravitational constant in the local
frame |
|