Laws of compression

Laws of compression (new physics?)
Physical laws proposed by the Swedish hobby-astronomer Carl van den Swaerdenheem.
First law of compression
m / (4 x π x r2 x g) = C
Example: The mass of the Sun is 1.9891 x 10^30 kg. The radius of the Sun is 6.955 x 10^8 m. The gravity of the Sun is 274.0 m/s^2. The value for C is thus 1.1942 x 10^9 kgs^2/m^3.
Second law of compression
m / (4 x π x v2 x d) = C
Example: The mass of the Sun is 1.9891 x 10^30 kg. The average orbital speed of Venus is 35020 m/s. The semi-major axis of Venus is 1.0820893 x 10^11 m. The value for C is thus 1.1927 x 10^9 kgs^2/m^3.
Third law of compression
1 / (4 x π x G) = C
Example: The value for G is 6.67428 x 10^-11. The value for C is thus 1.1923 x 10^9 kgs^2/m^3.
m = mass of a body
r2 = square of the radius of the body
g = gravity of the body
C = constant of compression
v2 = velocity of a body in orbit
d = distance between two bodies
G = constant of gravitation
Source of data: all physical data from .

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