Estimate the mass of the sun, assuming the orbit of the earth round the sun to be a circle. The distance between the sun and earth is `1.49 xx 10^(11) m` and `G = 6.66 × 10^(-11) Nm^(2)//kg^(2)`.

Estimate the mass of the sun, assuning the orbit of Earth round the sun to be a circule. The disatnce between the sun and the Earth is 1.49 xx 10^(11) m , and G = 6.67 xx 10^(-11) Nm^(2) kg^(-2) .

Find the mass of the sun considering the orbit of the earth to be circular. Given , distance of the earth from the sun =1.49xx10^(13) cm and G=6.66xx10^(-8) CGS unit.

Calculate the mass of the sun , given that the sistance between the sum and the earth is 1.5xx 10^(-11) m and G = 6.66 xx 10 ^(-11) SI units and taken a year = 365 days .

Find the magnitude of the gravitational force between the Sun and the earth. (Mass of the Sun =2xx10^(30) kg, mass of the earth =6xx10^(24)kg and the distance between the centres of the Sun and the earth =1.5xx10^(11)m , (G=6.67xx10^(-11)N.m^(2)//kg^(2))

Solve the following examples / numerical problems: Find the magnitude of the gravitational force between the Sun and the earth.( Mass of the Sun =2xx10^30 kg, mass of the earth = 6xx10^24 kg and the distance between the centres of the Sun and the earth = 1.5xx 10^11 m, G =6.67 xx10^-11 N-m^2 /kg^2 ).

Calculate the mass of sun if the mean radius of the earth's orbit is 1.5xx10^(8)km and G=6.67xx10^(-11)Nxxm^(2)//kg^(2)

Calculat the binding energy of the - sum system . Mass of the earth =6xx 10 ^(24) kg , mass of the sun = 2 xx 10^(30) kg, distance between the earth and the sun = 1.5 xx 10^(11) and gravitational constant = 6.6 xx 10 ^(-11) N m^(2) kg^(2)

Calculat the binding energy of the - sum system . Mass of the earth =6xx 10 ^(24) kg , mass of the sun = 2 xx 10^(30) kg, distance between the earth and the sun = 1.5 xx 10^(11) and gravitational constant = 6.6 xx 10 ^(-11) N m^(2) kg^(2)

Assuming that earth's orbit around the sun is a circle of radius R=1.496xx10^(11)m compute the mass of the sun. (G=6.668xx10^(-11)Nm^(2)kg^(-2))

Find the luminous intensity of the sun if it produces the same illuminance on the earth as produced by a bulb of 10000 candela at a distance 0.3 m . The distance between the sun and the earth is 1.5 xx 10^(11) m