Embibe Experts Solutions for Chapter: Gravitation, Exercise 4: Exercise - 4

Author:Embibe Experts

Embibe Experts Physics Solutions for Exercise - Embibe Experts Solutions for Chapter: Gravitation, Exercise 4: Exercise - 4

Attempt the free practice questions on Chapter 11: Gravitation, Exercise 4: Exercise - 4 with hints and solutions to strengthen your understanding. Alpha Question Bank for Engineering: Physics solutions are prepared by Experienced Embibe Experts.

Questions from Embibe Experts Solutions for Chapter: Gravitation, Exercise 4: Exercise - 4 with Hints & Solutions

HARD
JEE Main/Advance
IMPORTANT

A sphere of density ρ and radius a has a concentric cavity of radius b, as shown in the figure. 

(a) Sketch the gravitational force F exerted by the sphere on the particle of mass m, located at a distance r from the centre of the sphere as a function of r in the range 0 r  .

(b) Sketch the corresponding curve for the potential energy u (r) of the system.

Question Image

HARD
JEE Main/Advance
IMPORTANT

(a) What is the escape speed for an object in the same orbit as that of earth around sun (take orbital radius R) but far from the earth? (Mass of the sun=Ms

(b) If an object already has a speed equal to the earth’s orbital speed, what minimum additional speed must it be given to escape as in (a)?

HARD
JEE Main/Advance
IMPORTANT

A cosmic body A moves towards the sun with velocity v0 (when far from the sun) and aiming parameter l, the direction of the vector v0 relative to the centre of the sun as shown in the figure. Find the minimum distance by which this body will get to the sun (mass of sun=Ms)

Question Image

HARD
JEE Main/Advance
IMPORTANT

Two stars of mass M1 and M2 are in circular orbits around their centre of mass. The star of mass M1 has an orbit of radius R1, the star of mass M2 has an orbit of radius R2. (Assume that their centre of mass is not accelerating and distance between stars is fixed)

(a) Show that the ratio of the orbital radii of the two stars equals the reciprocal of the ratio of their masses, that is R1/R2 = M2/M1

(b) Explain why the two stars have the same orbital period and show that the period,

              T=2πR1+R232GM1+M2

HARD
JEE Main/Advance
IMPORTANT

A star can be considered as a spherical ball of hot gas of radius R. Inside the star, the density of the gas is ρr at a radius r and mass of the gas within this region is Mr. The correct differential equation for variation of mass with respect to radius dMrdr is (refer to the adjacent figure)

Question Image

MEDIUM
JEE Main/Advance
IMPORTANT

A star can be considered as a spherical ball of hot gas of radius R. Inside the star, the density of the gas is ρr at a radius r and the mass of the gas within this region is Mr. A star in its prime age is said to be under equilibrium due to gravitational pull and outward radiation pressure (p). Consider the shell of thickness dr. If the pressure on this shell is dp then the correct equation is (G is universal gravitational constant

Question Image

HARD
JEE Main/Advance
IMPORTANT

A star can be considered as a spherical ball of hot gas of radius R. Inside the star, the density of the gas is ρr at a radius r and the mass of the gas within this region is Mr. In astronomy order of magnitude, estimation plays an important role. The derivative dpdr be taken difference ratio pr. Consider the star has a radius R, pressure at its centre is PC and pressure at outer layer is zero if the average mass is M2 and average radius R2 then the expression for PC is

Question Image

HARD
JEE Main/Advance
IMPORTANT

The value of mass and radius of sun are given by M0 =2×1030 kg and R0=7×105 km, respectively. The pressure at the centre is about (G=6.67×1011m3 kg1 s2)