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Solved Examples: Gravitation & Projectile | Mock Tests for JEE Main and Advanced 2025 PDF Download

Question 1: At what initial speed must the basketball player throw the ball, at 55º above the horizontal, to make the foul shot, as shown in below figure? The basketball rim is 18 in. in diameter. Obtain other data from below figure
Solved Examples: Gravitation & Projectile | Mock Tests for JEE Main and Advanced 2025Concept:
The figure below shows the basketball player making a foul shot:
Solved Examples: Gravitation & Projectile | Mock Tests for JEE Main and Advanced 2025It can be seen from the figure that the effective horizontal distance to make that shot is
14ft -1ft=13ft whereas the effective vertical distance travelled by the ball is 10 ft - 7 ft = 3 ft
Assume that the angle at which the ball is released with initial velocity v0 is θ such that the horizontal component of initial velocity is v0x = v0 cosθ and the vertical component of initial velocity is v0y = v0 sinθ.
The time taken by the ball to reach the basket can be written in terms of horizontal component of velocity and the effective horizontal distance travelled by the ball as:
t = 13 ft / v0x
Substitute v0= vcosθ,
t = 13 ft / v0 cosθ    …… (1)
Similarly, one can write the time t in terms of the vertical component on initial velocity and the effective vertical distance travelled by the ball as:
3ft = v0yt – ½ gt2
Substitute v0y = v0 sinθ,
3ft = (v0 sinθ)t – ½ gt2
Substitute t = 13 ft/ vcosθ  from equation (1),
Solved Examples: Gravitation & Projectile | Mock Tests for JEE Main and Advanced 2025
Solved Examples: Gravitation & Projectile | Mock Tests for JEE Main and Advanced 2025
Solved Examples: Gravitation & Projectile | Mock Tests for JEE Main and Advanced 2025
Solved Examples: Gravitation & Projectile | Mock Tests for JEE Main and Advanced 2025
Substitute the value of θ and g to obtain the value of v0.
Solution.
Substitute 55º  for θ and 32.2 ft/s for g in equation
Solved Examples: Gravitation & Projectile | Mock Tests for JEE Main and Advanced 2025
Therefore, the magnitude of initial velocity of the ball is 23 ft/s.

Question 2: A spherical hollow is made in a lead sphere of radius R, such that its surface touches the outside surface of the lead sphere and passes through its center (see below figure). The mass of the sphere before hollowing was M. With what force, according to the law of universal gravitation, will the hollowed lead sphere attract a small sphere of mass m, which lies at a distance d from the center of the lead sphere on the straight line connecting the centers of the spheres and of the follow?  [1946, Olympic, Moscow State University]
Solved Examples: Gravitation & Projectile | Mock Tests for JEE Main and Advanced 2025Concept:
The force of gravity on the small sphere of mass due to the lead sphere after it is made hollow is equal to the force of gravity from a solid lead sphere minus the force which would have been contributed by the smaller lead sphere which would have filled the hole.
Solution:
From the Newton’s law of universal gravitation, the force of attraction between the lead sphere and the small sphere is
F1 = GMm/d2
Here, gravitational constant is G, total mass of the lead sphere is M, mass of the small sphere is m and distance between the centers of the spheres is d.
So, we need to know about the size and mass of the lead which was removed to make the hole.
The density of the lead is given by
ρ = M/[(4/3)(πR3)]
Here, radius of the lead sphere is R.
The spherical sphere has a radius of R/2.
If the density is constant, then the mass of the hole will be the density times the volume of the hollow sphere. Thus, the mass of the hollow sphere is
Solved Examples: Gravitation & Projectile | Mock Tests for JEE Main and Advanced 2025
The hole is closer to the small sphere.  This means the center of the hole is d-(R/2) away from the small sphere.
Now, the gravitational force between the hollow sphere and the small sphere is
Solved Examples: Gravitation & Projectile | Mock Tests for JEE Main and Advanced 2025
The force of attraction with which the lead sphere after it is made hollow and the small sphere is equal to the force of the whole lead sphere before it is made hollow minus the force of the hollow lead sphere. The corresponding force is
Solved Examples: Gravitation & Projectile | Mock Tests for JEE Main and Advanced 2025
Therefore, the required force from the lead sphere which attract the small sphere is
Solved Examples: Gravitation & Projectile | Mock Tests for JEE Main and Advanced 2025

Question 3: A certain triple-star system consists of two stars, each of mass m, revolving about a central star; mass M, in the same circular orbit. The two stars stay at opposite ends of a diameter of the circular orbit; see below figure. Derive an expression for the period of revolution of the stars; the radius of the orbit is r.
Solved Examples: Gravitation & Projectile | Mock Tests for JEE Main and Advanced 2025Concept: 
The gravitational force due to the two stars to the central star is
F= GMm/r2 + GMm/r2
= 2 GMm/r2
Here, gravitational constant is G, mass of the central star is M, mass of the orbiting stars is m and radius of the orbit is r.
Also, the gravitational force between the orbiting stars is,
F= Gmm/(2r)2
= Gm2/4r
The net gravitational force acting on the stars is equal to the sum of the gravitational forces acting on the system. It is given as,
Fnet = F1+F2
= 2 GMm/r+ Gm2/4r2
= Gm/r2 [(2M)+m/4]
The centripetal force that makes the stars to orbit around the central star is
F= 4π2mr/T2
Here, period of the stars around the central star is T.
Solution:
The centripetal force is provided by the net gravitational force acting on the system of stars. Thus,
Fnet = Fc
Substitute Gm/r2 [(2M)+m/4] for Fnet  and 4π2mr/T2 for Fin the above equation.
Fnet = Fc
Gm/r2 [(2M)+m/4] = 4π2mr/T2
So, T = √16π2r3/[G(8M+m)]
Therefore, the expression for the period of revolution of the stars is √16π2r3/[G(8M+m)].

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FAQs on Solved Examples: Gravitation & Projectile - Mock Tests for JEE Main and Advanced 2025

1. What is the formula for gravitational force?
Ans. The formula for gravitational force is given by Newton's law of universal gravitation, which states that the force of attraction between two objects is directly proportional to the product of their masses and inversely proportional to the square of the distance between them. Mathematically, it is expressed as F = G * (m1 * m2) / r^2, where F is the gravitational force, G is the gravitational constant, m1 and m2 are the masses of the two objects, and r is the distance between their centers.
2. How does the gravitational force affect the motion of objects?
Ans. The gravitational force affects the motion of objects by acting as an acceleration towards the center of mass of the attracting object. This acceleration is commonly known as the acceleration due to gravity and is approximately 9.8 m/s^2 on the surface of the Earth. It causes objects to fall towards the Earth and determines the trajectory of projectiles. The force of gravity also influences the orbital motion of celestial bodies, such as planets and satellites.
3. What is a projectile and what are its characteristics?
Ans. A projectile is an object that is launched into the air and moves along a curved path under the influence of gravity alone. It has certain characteristics such as a parabolic trajectory, constant horizontal velocity, and a vertical acceleration due to gravity. The horizontal motion of a projectile is independent of its vertical motion, meaning that it follows a straight line at a constant velocity unless acted upon by external forces.
4. How can we calculate the maximum height reached by a projectile?
Ans. The maximum height reached by a projectile can be calculated using the formula H = (V^2 * sin^2θ) / (2g), where H is the maximum height, V is the initial velocity of the projectile, θ is the launch angle, and g is the acceleration due to gravity. This formula represents the vertical motion of the projectile and accounts for the time taken to reach the maximum height and fall back down.
5. What is the range of a projectile and how is it calculated?
Ans. The range of a projectile is the horizontal distance covered by it before hitting the ground. It can be calculated using the formula R = (V^2 * sin(2θ)) / g, where R is the range, V is the initial velocity of the projectile, θ is the launch angle, and g is the acceleration due to gravity. This formula takes into account both the vertical and horizontal motions of the projectile and provides the distance it travels along a horizontal plane.
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