A planet moves around the sun in nearly circular orbit. Its period of revolution 'T' depends upon :
(i) radius 'r' or orbit (ii) mass 'M' of the sum and
(iii) the gravitational constant G.
Show dimensionally that `T^(2) prop r^(2)`.

A planet moves around the sun in nearly circular orbit. Its period of revolution 'T' depends upon. (i) radius 'r' or orbit, (ii) mass 'm' of the sun and. (iii) The gravitational constant G show dimensionally that T^(2) prop r^(3) .

A planet moves around the sun in nearly circular orbit. Its period of revolution 'T' depends upon. (i) radius 'r' or orbit, (ii) mass 'm' of the sun and. (iii) The gravitational constant G show dimensionally that T^(2) prop r^(3) .

The period of revolution (T) of a planet around the sun depends upon (i) radius (r ) of obit (ii) mass M of the sun and (iii) gravi-tational constant G. Prove that T^2 prop r^3

Consider a planet of mass (m), revolving round the sun. The time period (T) of revolution of the planet depends upon the radius of the orbit (r), mass of the sun (M) and the gravitational constant (G). Using dimensional analysis, verify Kepler' third law of planetary motion.

If a planet revolves around the sun in a circular orbit of radius a with a speed of revolution T, then (K being a positive constant

The period T of revolution of the earth around the sun depends upon (1) Orbital radius R (2) mass M of the sun and (3) gravitational that T^2ooR^3 .

The period of revolution(T) of a planet moving round the sun in a circular orbit depends upon the radius (r) of the orbit, mass (M) of the sun and the gravitation constant (G). Then T is proportioni of r^(a) . The value of a is

When a satellite revolves around the sun in a circular orbit of radius a with a period of revolution T, and if K is a positive constant, then