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The size of a planet does not have any relevance with its distance from the sun.

They are all dependent on the evolution after big bang which is a reference of their origin

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mass / distance between / orbital velocity / gravity / centripetal force

The (equal) force due to gravity on the planet and the sun is calculated from:

f = (G * m1 * m2) / d2

key:

f = force (newtons)

G = newtons gravity constant

m1 = sun mass (kg)

m2 = planet mass (kg)

d = distance between centres of gravity (metres)

The force due to centripetal action must equal the force of gravity, and only the one orbital velocity will provide this.

orbital velocity (metres per second) = square root ( ( G * m2 ) / d )

Its a fairly remote occurrence where all the (coincident) criteria are met, accounting for the large amount of space and the rarity of planets.

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Dahlia Miller

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3y ago

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