Physics Gravitation
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8.11 For the above problem, the direction of the gravitational intensity at an arbitrary point P is indicated by the arrow (i) d (ii) e (iii) f (iv) g
8.11 For the above problem, the direction of the gravitational intensity at an arbitrary point P is indicated by the arrow (i) d (ii) e (iii) f (iv) g
If the upper half of the spherical shell is cut out, then the net gravitational force acting on a particle at an arbitrary point P will be in the downward direction. Since gravitational intensity at a point is defined as the gravitational force per unit mass at that point, it will also act in the do
8.10 In the following two exercises, choose the correct answer from among the given ones:
The gravitational intensity at the centre of a hemispherical shell of uniform mass density has the direction indicated by the arrow (see Fig 8.12) (i) a (ii) b (iii) c (iv) 0

8.10 In the following two exercises, choose the correct answer from among the given ones:
The gravitational intensity at the centre of a hemispherical shell of uniform mass density has the direction indicated by the arrow (see Fig 8.12) (i) a (ii) b (iii) c (iv) 0

Gravitational potential (V) is constant at all points in a spherical shell. Hence the gravitational gradient ( is zero everywhere inside the spherical shell. The gravitational potential gradient is equal to the negative of gravitational intensity. Hence intensity is also zero at all points ins
8.9 Which of the following symptoms is likely to afflict an astronaut in space
(a) Swollen feet
(b) Swollen face
(c) Headache
(d) Orientational problem
8.9 Which of the following symptoms is likely to afflict an astronaut in space
(a) Swollen feet
(b) Swollen face
(c) Headache
(d) Orientational problem
(a) Legs hold the entire mass of a body in standing position due to gravitational pull. In space, an astronaut feels weightlessness because of the absence of gravity. Therefore swollen feet of an astronaut do not affect him/her in space
(b) A swollen face is caused generally because of appare
8.8 A comet orbits the sun in a highly elliptical orbit. Does the comet have a constant
(a) Linear speed
(b) Angular speed
(c) Angular momentum
(d) Kinetic energy
(e) Potential energy
(f) Total energy throughout its orbit?
Neglect any mass loss of the comet when it comes very close to the Sun
8.8 A comet orbits the sun in a highly elliptical orbit. Does the comet have a constant
(a) Linear speed
(b) Angular speed
(c) Angular momentum
(d) Kinetic energy
(e) Potential energy
(f) Total energy throughout its orbit?
Neglect any mass loss of the comet when it comes very close to the Sun
Angular momentum and total energy at all points of the orbit of a comet moving in a highly elliptical orbit around the Sun are constant. Is linear speed, angular speed, kinetic and potential energy varies from point to point in the orbit.
(a) No
(b) No
(c) Yes
(d) No
(e) No
(f) Yes
8.7 Does the escape speed of a body from the earth depend on
(a) The mass of the body
(b) The location from where it is projected
(c) The direction of projection
(d) The height of the location from where the body is launched?
8.7 Does the escape speed of a body from the earth depend on
(a) The mass of the body
(b) The location from where it is projected
(c) The direction of projection
(d) The height of the location from where the body is launched?
(a) Escape velocity of a body from the Earth is given by the relation:
= …. (1)
Where g = acceleration due to gravity and R = radius of the Earth
So escape velocity is independent of the mass of the body.
(b) It does not depend on the location from where it is projected.
(c) Does not
8.6 Choose the correct alternative:
(a) If the zero of potential energy is at infinity, the total energy of an orbiting satellite is negative of its kinetic/potential energy
(b) The energy required to launch an orbiting satellite out of earth’s gravitational influence is more/less than the energy required to project a stationary object at the same height (as the satellite) out of earth’s influence
8.6 Choose the correct alternative:
(a) If the zero of potential energy is at infinity, the total energy of an orbiting satellite is negative of its kinetic/potential energy
(b) The energy required to launch an orbiting satellite out of earth’s gravitational influence is more/less than the energy required to project a stationary object at the same height (as the satellite) out of earth’s influence
(a) Total mechanical energy of a satellite is the sum of its kinetic energy (always positive) and potential energy (can be either positive or negative). At infinity, the gravitational potential energy of the satellite is zero. As the Earth-Satellite system is a bound system, the total energy of the
8.5 Let us assume that our galaxy consists of 2.5 × 1011 stars each of one solar mass. How long will a star at a distance of 50,000 ly from the galactic centre take to complete one revolution ? Take the diameter of the Milk Way to be 105 ly.
8.5 Let us assume that our galaxy consists of 2.5 × 1011 stars each of one solar mass. How long will a star at a distance of 50,000 ly from the galactic centre take to complete one revolution ? Take the diameter of the Milk Way to be 105 ly.
Mass of our galaxy Milky Way, M = 2.5 solar mass
Solar mass = Mass of the Sun = 2.0 kg
Mass of our galaxy = 2.5 2.0 = 5 kg
Diameter of the Milky Way, d = 105 ly
Radius of the Milky Way = 5 ly
1 ly = 9.46 m
r = 5 9.46&n
8.4 IO, one of the satellites of Jupiter, has an orbital period of 1.769 days and the radius of the orbit is 4.22 × 108 m. Show that the mass of Jupiter is about one-thousandth that of the sun.
8.4 IO, one of the satellites of Jupiter, has an orbital period of 1.769 days and the radius of the orbit is 4.22 × 108 m. Show that the mass of Jupiter is about one-thousandth that of the sun.
The rotation period of the satellite Io, = 1.769 days = 1.769 x 24 x 60 x 60s
Radius of the Orbit is given by the relation, = 4.22 m
Mass is given by the relation: = ……(i)
Where = mass of Jupiter and G = Universal gravitational constant
O
8.3 Suppose there existed a planet that went around the Sun twice as fast as the earth. What would be its orbital size as compared to that of the earth?
8.3 Suppose there existed a planet that went around the Sun twice as fast as the earth. What would be its orbital size as compared to that of the earth?
Time taken by the Earth to complete one revolution around the Sun, = 1 year
Orbital radius of the Earth in its orbit, = 1 AU
Time taken by the planet to complete one revolution around the Sun, = = year
Orbital radius of the planet =
From Ke
8.2 Choose the correct alternative:
(a) Acceleration due to gravity increases/decreases with increasing altitude
(b) Acceleration due to gravity increases/decreases with increasing depth (assume the earth to be a sphere of uniform density)
(c) Acceleration due to gravity is independent of mass of the earth/mass of the body
(d) The formula –G Mm(1/r2 – 1/r1) is more/less accurate than the formula mg(r2 – r1) for the difference of potential energy between two points r2 and r1 distance away from the centre of the earth
8.2 Choose the correct alternative:
(a) Acceleration due to gravity increases/decreases with increasing altitude
(b) Acceleration due to gravity increases/decreases with increasing depth (assume the earth to be a sphere of uniform density)
(c) Acceleration due to gravity is independent of mass of the earth/mass of the body
(d) The formula –G Mm(1/r2 – 1/r1) is more/less accurate than the formula mg(r2 – r1) for the difference of potential energy between two points r2 and r1 distance away from the centre of the earth
(a) Decreases - Acceleration due to gravity at depth h is given by = (1 – )g, where g = acceleration due to gravity on the surface of the Earth. From this equation, it is clear that acceleration due to gravity decreases with increase in height
(b) Decreases – Acceler