krit.club logo

Gravitation - Acceleration due to Gravity

Grade 11ICSEPhysics

Review the key concepts, formulae, and examples before starting your quiz.

πŸ”‘Concepts

β€’

Acceleration due to gravity (gg) is the acceleration produced in a body due to the Earth's gravitational pull.

β€’

The value of gg on the surface of the Earth is approximately 9.8Β m/s29.8 \text{ m/s}^2 or 980Β cm/s2980 \text{ cm/s}^2.

β€’

Variation with Altitude: As height (hh) above the Earth's surface increases, the value of gg decreases. For hβ‰ͺRh \ll R, gβ€²β‰ˆg(1βˆ’2hR)g' \approx g(1 - \frac{2h}{R}).

β€’

Variation with Depth: As depth (dd) below the Earth's surface increases, the value of gg decreases linearly. At the center of the Earth (d=Rd=R), gg becomes zero.

β€’

Effect of Earth's Shape: Earth is an oblate spheroid. The radius at the equator (ReR_e) is greater than the radius at the poles (RpR_p). Consequently, gg is maximum at the poles and minimum at the equator.

β€’

Effect of Rotation: The centrifugal force due to Earth's rotation reduces the effective value of gg. This effect is maximum at the equator and zero at the poles.

πŸ“Formulae

g=GMR2g = \frac{GM}{R^2}

g=43Ο€GRρg = \frac{4}{3} \pi G R \rho

gβ€²=g(RR+h)2g' = g \left( \frac{R}{R+h} \right)^2

gβ€²β‰ˆg(1βˆ’2hR)Β (forΒ hβ‰ͺR)g' \approx g \left( 1 - \frac{2h}{R} \right) \text{ (for } h \ll R \text{)}

gβ€²=g(1βˆ’dR)g' = g \left( 1 - \frac{d}{R} \right)

gΟ•=gβˆ’RΟ‰2cos⁑2Ο•g_{\phi} = g - R\omega^2 \cos^2 \phi

πŸ’‘Examples

Problem 1:

At what height hh above the Earth's surface will the acceleration due to gravity be 25%25\% of its value on the surface? (Let RR be the radius of Earth)

Solution:

Given gβ€²=g4g' = \frac{g}{4}. Using the formula gβ€²=g(RR+h)2g' = g \left( \frac{R}{R+h} \right)^2, we have: g4=g(RR+h)2\frac{g}{4} = g \left( \frac{R}{R+h} \right)^2 14=(RR+h)2\frac{1}{4} = \left( \frac{R}{R+h} \right)^2 Taking the square root on both sides: 12=RR+h\frac{1}{2} = \frac{R}{R+h} R+h=2Rβ€…β€ŠβŸΉβ€…β€Šh=RR + h = 2R \implies h = R

Explanation:

Since the value of gg decreases with the square of the distance from the center, to reduce gg to a quarter, the distance must be doubled. Thus, hh must equal the radius of the Earth.

Problem 2:

Calculate the depth dd below the Earth's surface where the weight of a body becomes 13\frac{1}{3} of its weight on the surface.

Solution:

Weight W=mgW = mg. If weight becomes 13\frac{1}{3}, then gβ€²=g3g' = \frac{g}{3}. Using the depth formula: gβ€²=g(1βˆ’dR)g' = g \left( 1 - \frac{d}{R} \right) g3=g(1βˆ’dR)\frac{g}{3} = g \left( 1 - \frac{d}{R} \right) 13=1βˆ’dR\frac{1}{3} = 1 - \frac{d}{R} dR=1βˆ’13=23\frac{d}{R} = 1 - \frac{1}{3} = \frac{2}{3} d=2R3d = \frac{2R}{3}

Explanation:

Acceleration due to gravity decreases linearly with depth. At a depth of two-thirds the radius, gg is reduced by two-thirds, leaving only one-third of the surface value.

Acceleration due to Gravity - Revision Notes & Key Formulas | ICSE Class 11 Physics