Mathematical Model Used to Predict Interplanetary Phenomena

Consider a planet with mass m_1, sidereal rotational period T_1, and north celestial pole unit vector \hat k_1. A sphere, S(r, m_1), of radius r centered on m_1 contains total mass m_1 + m'_1 given r is larger than the planet’s radius. The extra mass m'_1 is mass that lies outside the planet.

The hypotheized intermediary force could manifest as follows:

At position \mathbf{r}, an instantaneous velocity boost occurs every T_1 along the vector:

\bar{V}(m_1 + m'_1)=-C \frac{\gamma sin(\delta )T_1}{m_1 + m'_1} \hat k_1

for some positive constant C, \gamma = \frac{1}{\sqrt{1-v^2/c^2}}, v=\frac{2\pi r }{T_1} cos(\delta):v<c where c is light-speed, and apparent declination \delta of an object at position \mathbf{r} from m_1.

When considering how this velocity boost affects the zonal winds of another planet m_2, we can look at the magnitude of the U-component (west-east) of \bar{V}:

U(m_1 + m'_1) = -C \frac{\gamma sin(\delta )T_1}{m_1 + m'_1} \hat k_1\cdot (\hat k_2 \times \hat{m_1}_2)

where \hat k_2 and \hat{m_1}_2 are the unit vectors representing the north celestial pole of m_2, and the position of m_1 from m_2 respectively. A positive U(m_1 + m'_1) occuring at the nearest point of planet m_2 to planet m_1 would represent a velocity boost in the west-east direction (prograde).

Let’s see how this affects each planetary phenomena listed in the blog sections page.

Venus’s zonal winds

Since the mass term in the velocity boost expression is in the denominator, then smaller planets will exert a stronger force. However, the frequency of velocity boosts is also important. Mercury and Venus have rotational periods of about 58 days and 243 days respectively. This means the effect they have on other planets occurs much less frequently than say Earth and Mars whose rotational periods are about 1 day.

With this in mind, it is clear that Mars has the greatest effect on Venus. The next thing to consider is the mass contained within S(r,Mars), where r is Mars-Venus distance. During their orbits, S will occasionally contain other solar system bodies. In this case, the bodies that significantly reduce the velocity boost expression are the Sun and Earth.

Finally, the mass of Venus is 7.6 times that of Mars. This means that the velocity boost on the near-side of Venus to Mars will be significantly greater than that which occurs on the far side. For simplicity, only the near-side velocity boost is used.

Therefore, given that Mars-Sun and Mars-Earth distances are greater than Mars-Venus distance, and with the gamma term not rising more than about 1.003, the expression we can effectively use to predict zonal winds on Venus is

U(Mars)/C = -\frac{sin(\delta )T}{M} \hat M_{NP}\cdot (\hat V_{NP} \times \hat{M}_V)

where \delta is the apparent declination of Venus from Mars, T is Mars’ sidereal rotational period, M is Mars’ mass, \hat M_{NP} is Mars’ north celestial pole unit vector, \hat V_{NP} is Venus’s north celestial pole unit vector, and \hat{M}_V is the position of Mars from Venus. For the period 1981-2035, the plot looks like this:

This same expression is also used to explore possible connections with Venus’s cloud discontinuities. It should be noted that Venus’ zonal winds are prograde (westward direction given Venus’ retrograde rotation); so a positive U(Mars) will push against the wind, while a negative U(Mars) will accelerate it. It is hypothesized that the friction caused by a positive U(Mars) will create an atmospheric buildup manifesting as a cloud discontinuity.

Earth’s zonal winds

Again, Mars has the greatest effect on Earth. The mass contained within S(r,Mars), where r is Mars-Earth distance, will occasionally contain the Sun and Venus. We can neglect periods when Mars-Sun and Mars-Venus distances are less than Mars-Earth distance.

The mass of Earth is 9.3 times that of Mars, so that only the significantly greater velocity boost on the near-side of Earth to Mars is used.

With the gamma term not rising more than about 1.004, the expression we can effectively use to predict zonal winds on Earth is

U(Mars)/C = -\frac{sin(\delta )T}{M} \hat M_{NP}\cdot (\hat E_{NP} \times \hat M_E)

where \delta is the apparent declination of Earth from Mars, T is Mars’ sidereal rotational period, M is Mars’ mass, \hat M_{NP} is Mars’ north celestial pole unit vector, \hat E_{NP} is Earth’s north celestial pole unit vector, and \hat{M}_E is the position of Mars from Earth. For the period 1981-2035, the plot looks like this:

A positive U(Mars) will push the wind from west to east, and vice versa.

Mars’ zonal winds

Earth has the greatest effect on Mars. The mass contained within S(r,Earth), where r is Earth-Mars distance, will occasionally contain the Sun and Venus. We can neglect periods when Earth-Sun distance is less than Earth-Mars distance. However, when S(r,Earth) contains Venus and not the Sun, the velocity boost is only reduced by a factor of about 1.8. Therefore, it is worth considering in addition to periods when S(r,Earth) does not contain the Sun or Venus.

The mass of Mars is about 0.1 times that of Earth, so the velocity boost on the far side will be only marginally less than on the near side. This could complicate any predictions of overall zonal wind speed changes. We can, however, track the periods when these velocity boosts occur, and compare with instances of Marsquakes and dust storms.

With the gamma term not rising more than about 1.005, then when S(r,Earth) does not contain the Sun or Venus, we can use the expression:

V(Earth)/C = -\frac{sin(\delta )T}{M}

where \delta is the apparent declination of Mars from Earth, T is Earth’s sidereal rotational period, and M is Earth’s mass.

When S(r,Earth) contains Venus but not the Sun, the expression is:

V(Earth)/C = -\frac{sin(\delta )T}{M+m}

where m is Venus’s mass. Assume T is roughly the same as Earth’s sidereal rotational period. For the period 1981-2035, the plot looks like this: