Saturday, September 21, 2024

Calculate the period of a Planet in another Star System

Time is relative, if you’re standing on earth it takes one day or 24 hours for earth to do a complete rotation in and out of our stars light, while we remain in orbit around our sun.
Earth’s full orbital period around our sun takes 365 earth days.
The earth's spin and orbit are effects of the gravitational pull, as of when our solar system was created.
If you were standing on another planet it would most likely have a different numerical day and year.
To estimate the rotational period or day of a planet in a different solar system you first need to convert the estimated nubmer of days that it takes the planet to orbit it's star into seconds.
Then you can use Newtion and Kepler's Equations to make an estimation of the stars mass by using a standard 24 hour day, then you take your estimated result and divide it by the actual mass. This will let you know roughly what your accuary in math was, and allow you to adjust your hours per day estimation by using mass/math accuracy calculations.

Thursday, September 19, 2024

Solution To Time Dilation

Using Emmy Noether's Symmetry Equation's I estimated the actual mathematical solution to time dilation.
(energy fields enhance time) = space and momentum determine time; is what I derived from interpreting Emmy Noether's Equations.
Space - Time = Speed - // Relativistic Velocity
942477 - Time = e * (v/c^2) -
or
((piVal*3)*1^5) - Time = e * (v/c^2) // Relativistic Velocity
Time Dialation = -e * (v/c^2) + ((piVal*3)*1^5) // To find the answer flip it backwards to find the value of time dilation
Credit: Jennifer Connors, Emmy Noether, Albert Einstein
Similar Idea T0 That Mathematical Approach
New Math Equation to Balance any Two Ratios. Can be used with fractions or decimals.
M a/b = A m/b ex: 4*3/5 = 3*4/5 == 2.4 = 2.4 ==
4*.6 = 3*.8 == 2.4 = 2.4 ==
Credit: Jennifer Connors

New Math Equation to Balance any Two Ratios

M a/b = A m/b ex: 4*3/5 = 3*4/5 == 2.4 = 2.4 ==
4 * .6 = 3 * .8 == 2.4 etc