What will be the mass and density of the sun?

Let’s take into account a planet revolving around the sun having mass m and T is its period of revolution. Suppose mass of sun to be M and R its radius.

The equation for the centripetal force is given below:

= mRElectrostatic 4.17 = mR (2 electrostatics 2.67 / T) 2 = 4electrostatics 2.672mR / T2
A force is applied on the planet due to the gravitational force of sun. The equation of force is shown below:
F= GMm / R2
So,
GMm / R2 = 4 electrostatics 2.672 mR / T2
Then the final result will be:

M = 4electrostatics 2.672MmR3 / G T2

According to the formula:
Mass = volume x density
We have supposed earlier that r is the radius of the sun and electrostatic figure 1.43 is the density.
By substituting and solving the values we get:

electrostatic 1.43 = 3electrostatics 2.67 R3/ G T2 R3

From the above equation M and electrostatic 1.43 can be calculated.

Category: Universe

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