Distance of the Earth from the Sun, re = 1.5 × 108 km = 1.5×1011 m
Time period of the Earth = Te
Time period of Saturn, Ts = 29. 5 Te
Distance of Saturn from the Sun = rs
From Kepler’s third law of planetary motion, we have
\(T = (\frac{4 \pi^2 r^3 }{ GM})^{\frac{1}{2}}\)
For Saturn and Sun, we can write
\(\frac{rs^3}{ re^3 }= \frac{Ts^2 }{ Te ^2}\)
\(r_s = r_e(\frac{T_s}{ T_e})^{\frac{2}{3}}\)
= 1.5 x 1011 \((\frac{29.5T_e}{T_e})^{\frac{2}{3}}\)
= 1.5 x 1011\( (29.5)^{\frac{2}{3}}\)
= 1.5 x 1011 x 9.55
= 14.32 x 1011 m
Hence, the distance between Saturn and the Sun is 1.432 x 1012 m .
Given below are two statements: one is labelled as Assertion A and the other is labelled as Reason R. Assertion A: The kinetic energy needed to project a body of mass $m$ from earth surface to infinity is $\frac{1}{2} \mathrm{mgR}$, where R is the radius of earth. Reason R: The maximum potential energy of a body is zero when it is projected to infinity from earth surface.
take on sth: | to begin to have a particular quality or appearance; to assume sth |
take sb on: | to employ sb; to engage sb to accept sb as one’s opponent in a game, contest or conflict |
take sb/sth on: | to decide to do sth; to allow sth/sb to enter e.g. a bus, plane or ship; to take sth/sb on board |
In mechanics, the universal force of attraction acting between all matter is known as Gravity, also called gravitation, . It is the weakest known force in nature.
According to Newton’s law of gravitation, “Every particle in the universe attracts every other particle with a force whose magnitude is,
On combining equations (1) and (2) we get,
F ∝ M1M2/r2
F = G × [M1M2]/r2 . . . . (7)
Or, f(r) = GM1M2/r2
The dimension formula of G is [M-1L3T-2].