SLíдτ2: (TRC3:SS)...P3.1...Balance & Separating...1.Main Line

The Road

Chapter 3 : Solar Separating

Page 3.1 : Balance & Separating

1. Separating's Main Line

We can find by 2 types of the movement as follow

1 Using Sun as a center
2 Using planets that orbit around as a center.

1.1 Using Sun As A Center

Suppose that

- There are only 2 planets's clashing (A, B) that orbit around the Sun

- Planets A, B was clashing by the Sun with in order.

1.1.1. The 1st clashing with A as shown in Pic 1

Discription :

While Sun is at position 1 (Step1).

Sun and A are moving towards position 2 (Step2).

When Sun and A reach at position 2, A will be pushed out to position 3

And sun is replaced at position 2 (Step3)

We can replace the values of movement into an equation like in Pic 2

And the equation is

tan θ1= h1/(r1-e1)
or
h1= tan θ1 * (r1-e1)

And we can get from this equation is

1. The height of the sun when it hits planet A = h1 = tan θ1 * (r1-e1)

2. Rightward motion of the Sun or length along the X axis = r1-e1

3. Main motion of the Sun or length along the Z axis = r1

1.1.2. The 2nd clashing with B as shown in Pic 3

Discription :

While Sun is in the 2nd position (Step 1)

Sun and B are moving towards position 4 (Step2).

When Sun and B reach at position 4, B will be pushed out to position 5

And sun is replaced at position 4 (Step3)

We can replace the values of movement into an equation like in Pic4

And the equation is

tan θ2= h2/(r2-e2)
or
h2= tan θ2 * (r2-e2)

And we can get from this equation is

1. The height of the sun when it hits planet B = h2 = tan θ2 * (r2-e2)

2. Rightward motion of the Sun or length along the X axis = r2-e2

3. Main motion of the Sun or length along the Z axis = r2

1.1.3 Collision's Merging

From Pic 5

When the sun is at position 1 and has two collisions occur,

At position 4, we will get

height (Y axis) = h1+h2

Length along the X axis = (r1-e1)+(r2-e2)

Length along the Z axis = r1+r2

We can get the coordinates (Y, X, Z ) From collision's merging like below

(Y, X, Z ) = h1+h2, (r1-e1)+(r2-e2), r1+r2

And this coordinates will made us to get a distance (height of the Sun's movement from position 1st to 4th) and brifely in pic 6

2. Using Planets That Orbit Around As A Center.

Suppose that

- Sun has a main direction to the right and planet A is orbiting around (Pic 7)
- The main path (Step1, 3 in Pic 7) is used to creat a beam

- Planet A is the center of the beam

Processing :

From Pic 8.1

If Sun is thrown along the main path of separating (Big Green Arrow).....And this will gives a result (beam) with Planet A as the center as shown in step 3

From Pic 8.2

Pic 8.2 is a step 2 from Pic 8.1,and it is shown that

Sun's Main Direction Line is not the same as Separating's Line

From Pic 9

If there are 3 planets (A, B, C) with the Sun's road

Resulting from a collision on the main path is formed as a beam, it is shown like below

And when separating the beams of each planets, it will be shown in Pic 10.

And when brought together (merge horizontally) This will be the main separating's line that sun travels (Pic 11). The values of h1, h2, h3 are the same values obtained by calculating the coordinates above in pic 6

From Pic 12 shown that

Sun will travel from 1, 2, 3 (Blue Arrow) with respectively and it has used more distance than h1

10/27/2020

(TRC3:SS)...P3.1...Balance & Separating...1.Main Line