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Motion of Body Under Gravity (Free Fall)

Motion of Body Under Gravity (Free Fall)

Edited By Vishal kumar | Updated on Jul 02, 2025 05:43 PM IST

It is a basic concept in physics, indicating the motion of a body under gravity when the force of gravity acts on that body. This type of motion is commonly referred to as free fall. That is, if the object is dropped from a height, it accelerates towards the Earth on account of gravity, which acts with a constant acceleration of about 9.8 m/s².

This principle applies in a much greater variety of examples—from an apple dropping from a tree to a skydiver diving out of an aeroplane. In each case, the object has a uniform acceleration in the same direction as that due to gravity. The equations of motion enable one to find the time it takes for an object to hit the ground, its velocity at any time, and the distance covered.

Motion of Body Under Gravity (Free Fall)
Motion of Body Under Gravity (Free Fall)

In this article, we will cover the motion of the body under gravity. This concept falls under the broader category of kinematics which is a crucial chapter in Class 11 physics. It is not only essential for board exams but also for competitive exams like the Joint Entrance Examination (JEE Main), National Eligibility Entrance Test (NEET), and other entrance exams such as SRMJEE, BITSAT, WBJEE, BCECE and more. Over the last ten years of the JEE Main exam (from 2013 to 2023), a total of 15 questions have been asked on this concept. And for NEET 4 questions were asked from this concept.

What Is Acceleration Due to Gravity and Sign Convention

The force of attraction of the earth on anybody is called the force of gravity. Acceleration produced on the body by the force of gravity is called acceleration due to gravity. It is represented by the symbol ‘g’.

Upward direction and right direction are taken as positive

The downward direction and left direction is taken as negative

There are Three Cases Basically in This

Case 1: If a body dropped from some height (initial velocity zero)

$\begin{aligned}
& \mathrm{u}=0 \\
& \mathrm{a}=\mathrm{g} \\
& v=g t \\
& h=\frac{1}{2} g t^2 \\
& v^2=2 g h \\
& h_n=\frac{g}{2}(2 n-1)
\end{aligned}$

Case 2: If a body is projected vertically downward with some initial velocity

$ \begin{aligned}
& \text { Equation of motion: } \quad v=u+g t \\
& \begin{array}{ll}
h= & u t+\frac{1}{2} g t^2 \\
v^2 & =u^2+2 g h \\
h_n \quad & =u+\frac{g}{2}(2 n-1)
\end{array}
\end{aligned} $

Case 3: If a body is projected vertically upward.

(i) Apply equation of motion:

Take initial position as origin and the direction of motion (vertically up) as $\mathrm{a}=-\mathrm{g}$ [as acceleration due to gravity is downwards]
So, if the body is projected with velocity $u$, and after time $\mathrm{t}$ it reaches up to height $\mathrm{h}$ then,
$
\mathrm{v}=\mathrm{u}-\mathrm{gt} ; \quad \mathrm{h}=\mathrm{ut}-\frac{1}{2} g \mathrm{t}^2 ; \mathrm{v}^2=u^2-2 \mathrm{gh}
$

(ii) For the case of maximum height $v=0$

So from the above equation

$\begin{gathered}
u=g t \\
h=\frac{1}{2} g t^2 \\
\text { and } u^2=2 g h
\end{gathered}$

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Solved Example Based on Motion of Body Under Gravity

Example 1: A balloon is moving up in the air vertically above point $\mathrm{A}$ on the ground. When it is at a height $h_1$, a girl standing at a distance (point $B$ ) from $A$ (see figure) sees it at an angle $45^{\circ}$ with respect to the vertical. When the balloon climbs up a further height $h_2$, it is seen at an angle $60^{\circ}$ with respect to the vertical if the girl moves further by a distance $2.464 d$ (point $C$ ). Then the height $h_2$ is (given $\tan 30^{\circ}=0.5774$ ) :

1)1.464d
2) $0.732 d$
3) $0.464 d$
4) $d$

Solution:

$\begin{aligned}
& \frac{\mathrm{h}_1}{\mathrm{~d}}=\tan 45^{\circ} \Rightarrow \mathrm{h}_1=\mathrm{d} \ldots \\
& \frac{h_1+h_2}{d+2.464 d}=\tan 30^{\circ} \\
& \Rightarrow\left(h_1+h_2\right) \times \sqrt{3}=3.46 \mathrm{~d} \\
& \left(\mathrm{~h}_1+\mathrm{h}_2\right)=\frac{3.46 \mathrm{~d}}{\sqrt{3}} \\
& \Rightarrow \mathrm{d}+\mathrm{h}_2=\frac{3.46 \mathrm{~d}}{\sqrt{3}} \\
& \mathrm{~h}_2=\mathrm{d}
\end{aligned}$

Hence, the answer is option (4).

Example 2: When a ball is dropped anto a lake from a height $4.9 \mathrm{~m}$ above the water level, it hits the water with a velocity $v$ and then sinks to the bottom with the constant velocity $v$. It reaches the bottom of the lake 4.0 safter it is dropped. The approximate depth of the lake is :
1) $19.6 \mathrm{~m}$
2) $29.4 \mathrm{~m}$
3) $39.2 \mathrm{~m}$
4) $73.5 \mathrm{~m}$

Solution:


$\mathrm{v= \sqrt{2gh}= \sqrt{2\times 9.8 \times 4.9}= 9.8\, m/s}$
$\mathrm{\text{time for A to B}= \sqrt{\frac{2h}{g}}= \sqrt{\frac{2\times4.9}{9.8}}= 1\, sec}$
distance travelled by ball in 3 sec in lake $\mathrm{= 9.8\times 3}$
$\mathrm{\therefore }$ depth of lake $\mathrm{= 29.4\, m}$

The correct answer is (2)

Example 3: A tennis ball is released from a height $h$ and after freely falling on a wooden floor, it rebounds and reaches height $h$ $\overline{2}$. The velocity versus height of the ball during its motion may be represented graphically by:
(graphs are drawn schematically and not to the scale)

1)

2)

3)

4)

Solution:

Velocity at the ground (means zero height) is non-zero therefore the option 4 is incorrect.

The velocity versus height curve will be parabolic as for motion under gravity.
i.e The velocity versus height curve is non-linear therefore option 1 is also incorrect.
$
\begin{aligned}
& \mathrm{v}^2=2 \mathrm{gh} \\
& \mathrm{v} \frac{\mathrm{dv}}{\mathrm{dh}}=2 \mathrm{~g}=\mathrm{const} \\
& \Rightarrow \frac{\mathrm{dv}}{\mathrm{dh}}=\frac{\text { constant }}{\mathrm{v}}
\end{aligned}
$

Here we can see the slope is very high when velocity is low therefore at the maximum height the slope should be very large which is in option 3 and as velocity increases slope must decrease therefore option 3 is correct.

Example 4: An NCC parade is going at a uniform speed of $9 \mathrm{~km} / \mathrm{h}$ under a mango tree on which a monkey is sitting at a height of $19.6 \mathrm{~m}$. At any particular instant, the monkey drops a mango. A cadet will receive the mango whose distance from the tree at time of drop is : (Given $\mathrm{g}=9.8 \mathrm{~m} / \mathrm{s}^2$ )

1)$5 \mathrm{~m}$

2)$10 \mathrm{~m}$

3)$19.8 \mathrm{~m}$

4)$24.5 \mathrm{~m}$

Solution:

$
\begin{aligned}
& \text { Time to fall }=\sqrt{\frac{2 \mathrm{~h}}{\mathrm{~g}}}=2 \mathrm{~s} \\
& \begin{aligned}
& \text { Velocity at parade }=9 \frac{\mathrm{km}}{\mathrm{hr}} \\
&=9 \times \frac{5}{18} \mathrm{~m} / \mathrm{s} \\
&=2.5 \mathrm{~m} / \mathrm{s}
\end{aligned}
\end{aligned}
$

Cadet will receive mango at a distance $\mathrm{x}$
$
\mathrm{x}=\mathrm{v}_{\mathrm{x}} \mathrm{t}=2.5 \times 2=5 \mathrm{~m}
$

Hence 1 is correct option.

Example 5: Two balls $\mathrm{A}$ and $\mathrm{B}$ are placed at the top of $180 \mathrm{~m}$ tall tower. Ball $A$ is released from the top at $t=0 \mathrm{~s}$. Ball $\mathrm{B}$ is thrown vertically down with an initial velocity' $\mathrm{u}^{\prime}$ at $\mathrm{t}=2 \mathrm{~s}$. After a certain time, both balls meet $100 \mathrm{~m}$ above the ground. Find the value of ' $\mathrm{u}$ ' in $\mathrm{ms}^{-1}$. [use $g=10 \mathrm{~ms}^{-2}$ ]:

1)$10$

2)$15$

3)$20$

4) $30$

Solution:

Let they meet $t=t_{\circ}$
For A
$
80=\frac{1}{2} g t_0^2
$

For B
$
80=u\left(t_0-2\right)+\frac{1}{2} g\left(t_0-2\right)^2
$

From (i)
$
\mathrm{t}_0=4
$
$
\begin{aligned}
& 80=\mathrm{u} \times 2+5 \times 2^2 \\
& \mathrm{u}=30 \mathrm{~m} / \mathrm{s}
\end{aligned}
$

The correct answer is Option (4)

Summary

Understanding the motion of a body under gravity means being able to explain very many daily phenomena, such as why objects fall when dropped and how projectiles travel.

It is a universal theory that has broad use, ranging from the prediction of a path a basketball will take when it is thrown to explaining how satellites orbit. Consequently, all objects should respond equally to the force of gravity, thus having uniform acceleration while in motion, which makes the motion of the falling objects predictable and consistent.

Frequently Asked Questions (FAQs)

1. What is free fall motion?
Free fall motion refers to the movement of an object under the influence of gravity alone, without any other forces acting on it. In this state, the object accelerates towards the Earth's center at a constant rate, typically about 9.8 m/s² near the Earth's surface. This acceleration is the same for all objects, regardless of their mass, in the absence of air resistance.
2. Why do all objects fall at the same rate in a vacuum, regardless of their mass?
All objects fall at the same rate in a vacuum because the gravitational force acting on an object is directly proportional to its mass, while the object's resistance to acceleration (inertia) is also proportional to its mass. These two effects cancel out, resulting in the same acceleration for all objects, regardless of their mass. This principle is known as the equivalence of gravitational and inertial mass.
3. What is the acceleration due to gravity, and why is it important?
The acceleration due to gravity, often denoted as 'g', is the rate at which an object's velocity changes during free fall. Near the Earth's surface, it's approximately 9.8 m/s². This value is crucial in physics because it allows us to predict the motion of objects under the influence of gravity, calculate the time and distance of falls, and understand the behavior of projectiles.
4. How does the value of 'g' change with altitude?
The value of 'g' decreases as altitude increases because gravitational force weakens with distance from the Earth's center. The relationship follows an inverse square law: as the distance from the Earth's center doubles, the gravitational force (and thus 'g') decreases by a factor of four. This variation is negligible for most everyday situations but becomes significant for high-altitude applications like satellite orbits.
5. What is the difference between weight and mass in the context of free fall?
Mass is a measure of an object's amount of matter and remains constant regardless of location. Weight, however, is the force exerted on an object due to gravity and can change based on the local gravitational field strength. In free fall, an object's weight is what causes it to accelerate, but its mass determines how much it resists this acceleration. The relationship between weight (W) and mass (m) is given by W = mg, where g is the local acceleration due to gravity.
6. How does air resistance affect free fall motion?
Air resistance opposes the motion of falling objects, causing them to reach a terminal velocity instead of continuously accelerating. The effect of air resistance depends on an object's shape, size, and speed. Objects with a larger surface area relative to their mass experience more air resistance and reach lower terminal velocities. In contrast, denser objects with smaller surface areas are less affected by air resistance and fall more closely to true free fall motion.
7. What is terminal velocity, and how is it related to free fall?
Terminal velocity is the maximum speed an object can reach when falling through a fluid (like air) under the force of gravity. It occurs when the downward force of gravity equals the upward drag force exerted by the fluid. At this point, the net force on the object becomes zero, and it no longer accelerates. Terminal velocity is related to free fall because it represents the limit of a falling object's speed due to air resistance, deviating from the continuous acceleration of true free fall motion.
8. How does the shape of an object affect its motion during a fall?
An object's shape significantly influences its fall through air due to air resistance. Objects with a larger surface area relative to their mass (like feathers or parachutes) experience more air resistance and fall more slowly. Streamlined shapes (like arrows or droplets) experience less air resistance and fall faster. In a vacuum, however, shape doesn't matter, and all objects fall at the same rate regardless of their shape or mass.
9. What is the relationship between potential energy and kinetic energy during free fall?
During free fall, there's a continuous conversion between potential energy and kinetic energy. At the start of the fall, an object has maximum gravitational potential energy and zero kinetic energy. As it falls, potential energy decreases while kinetic energy increases. At any point during the fall, the sum of potential and kinetic energy remains constant (ignoring air resistance), demonstrating the principle of conservation of mechanical energy.
10. What is the difference between free fall and projectile motion?
Free fall refers to motion under the influence of gravity alone, typically in a vertical direction. Projectile motion, on the other hand, involves both vertical and horizontal components. In projectile motion, the vertical component behaves like free fall (affected by gravity), while the horizontal component maintains constant velocity (assuming no air resistance). Free fall can be considered a special case of projectile motion where the initial horizontal velocity is zero.
11. What is the importance of free fall in the context of orbital mechanics?
Free fall is crucial in orbital mechanics because objects in orbit are essentially in a continuous state of free fall around the Earth (or other celestial body). The circular or elliptical path of an orbiting object results from its tangential velocity combined with the continuous free fall towards the Earth's center. Understanding free fall is key to calculating orbital parameters, predicting satellite trajectories, and planning space missions.
12. How does the concept of free fall relate to Einstein's equivalence principle?
Einstein's equivalence principle states that the effects of gravity are indistinguishable from the effects of acceleration in a small region of spacetime. This means that an observer in free fall cannot distinguish between being in a gravitational field and being in an accelerating reference frame in empty space. This principle was crucial in developing general relativity and understanding gravity as a curvature of spacetime rather than a force.
13. What is the role of free fall in determining the shape of large celestial bodies?
Free fall plays a crucial role in determining the shape of large celestial bodies like planets and stars. The mutual gravitational attraction between particles in these bodies causes them to "fall" towards their common center of mass. For sufficiently massive bodies, this process results in a nearly spherical shape as gravity pulls material equally from all directions. This is why planets and large moons are roughly spherical, while smaller bodies can have irregular shapes.
14. How does the concept of escape velocity relate to free fall?
Escape velocity is the minimum speed an object needs to escape a planet's gravitational field without further propulsion. It's directly related to free fall because it represents the velocity needed to counteract the entire potential energy of the object in the planet's gravitational field. An object launched at escape velocity will continue moving away from the planet, its speed asymptotically approaching zero as it moves to infinity. The escape velocity from Earth's surface is about 11.2 km/s.
15. What is the role of free fall in understanding black holes?
Free fall is crucial in understanding black holes. As an object falls towards a black hole, it accelerates due to the intense gravitational field, similar to free fall near Earth but much more extreme. At the event horizon, the velocity required to escape the black hole's gravity equals the speed of light. Beyond this point, even light is in an inescapable free fall towards the singularity. The concept of free fall helps explain phenomena like tidal forces and time dilation near black holes.
16. How does the concept of free fall relate to the principle of equivalence in general relativity?
The principle of equivalence in general relativity states that the effects of gravity are indistinguishable from the effects of acceleration in a small region of spacetime. This principle is intimately related to free fall. An observer in free fall experiences no local gravitational effects and is equivalent to an observer in an inertial frame in empty space. This equivalence led Einstein to describe gravity not as a force, but as a curvature of spacetime, forming the basis of general relativity.
17. What is the significance of Eötvös experiments in the context of free fall?
Eötvös experiments, named after Hungarian physicist Loránd Eötvös, are high-precision tests of the equivalence principle. These experiments compare the gravitational acceleration of different materials to verify that all objects fall at the same rate regardless of their composition. The extreme precision of these experiments (currently to parts in 10^-14) provides strong support for the equivalence principle and, by extension, for general relativity.
18. How does the concept of free fall apply to the formation of raindrops?
The formation of raindrops involves free fall, but with significant influence from air resistance. Water droplets initially fall freely, accelerating due to gravity. However, as they fall, air resistance increases, causing larger droplets to reach terminal velocity sooner. This interplay between gravity and air resistance affects the size and shape of raindrops. Very large drops tend to break apart due to air resistance, while smaller drops coalesce as they collide during their fall, demonstrating the complex application of free fall principles in meteorology.
19. What is the relationship between free fall and the concept of gravitational time dilation?
Gravitational time dilation, a prediction of general relativity, is closely related to free fall. In a gravitational field, time passes more slowly closer to the source of gravity compared to farther away. An object in free fall experiences proper time (its own time) that differs from the coordinate time of a stationary observer. This effect is negligible in everyday life but becomes significant in strong gravitational fields or precise timekeeping, such as in GPS satellites.
20. How do we calculate the distance traveled by an object in free fall?
To calculate the distance traveled by an object in free fall, we use the equation: d = ½gt², where 'd' is the distance, 'g' is the acceleration due to gravity, and 't' is the time of fall. This equation assumes the initial velocity is zero and neglects air resistance. It's derived from the general kinematic equation for constant acceleration: d = v₀t + ½at², where v₀ (initial velocity) is zero and 'a' is replaced by 'g'.
21. What is the equation for velocity in free fall, and how is it derived?
The equation for velocity in free fall is v = gt, where 'v' is the velocity, 'g' is the acceleration due to gravity, and 't' is the time of fall. This equation assumes the initial velocity is zero and neglects air resistance. It's derived from the general kinematic equation for constant acceleration: v = v₀ + at, where v₀ (initial velocity) is zero and 'a' is replaced by 'g'. This linear relationship between velocity and time is a key characteristic of free fall motion.
22. How does the concept of free fall apply to objects thrown upward?
When an object is thrown upward, it's still in free fall, just with an initial upward velocity. The object slows down at a rate of 9.8 m/s² (neglecting air resistance) until it reaches its peak height, where its velocity becomes zero momentarily. Then it begins falling back down, accelerating at 9.8 m/s². The entire journey, both up and down, is considered free fall because gravity is the only force acting on the object (ignoring air resistance).
23. What is the significance of the negative sign in the equation y = -½gt²?
The negative sign in the equation y = -½gt² indicates that the displacement (y) is in the opposite direction of the positive y-axis. In physics, we often define the upward direction as positive and the downward direction as negative. Since objects in free fall move downward, their displacement is negative. The negative sign ensures that the calculated displacement correctly represents the object's downward motion.
24. How does the initial velocity affect the motion of a falling object?
The initial velocity of a falling object affects its total travel time and maximum height reached. An object thrown downward (positive initial velocity) will reach the ground faster than one dropped from rest. An object thrown upward (negative initial velocity) will first rise to a maximum height before falling back down. The initial velocity is incorporated into the kinematic equations: y = y₀ + v₀t - ½gt² for displacement, and v = v₀ - gt for velocity, where v₀ is the initial velocity.
25. How does the mass of a planet affect the free fall acceleration on its surface?
The mass of a planet directly affects the free fall acceleration on its surface. The gravitational acceleration (g) is given by the equation g = GM/R², where G is the gravitational constant, M is the mass of the planet, and R is the planet's radius. A planet with greater mass will have a stronger gravitational field and thus a higher value of 'g'. For example, on Jupiter, g ≈ 24.8 m/s², while on Mars, g ≈ 3.7 m/s².
26. How does air resistance affect the acceleration of a falling object?
Air resistance opposes the motion of a falling object, reducing its acceleration. Unlike the constant acceleration of true free fall, the acceleration of an object falling through air decreases over time. As the object's speed increases, so does the air resistance, until it eventually balances the gravitational force. At this point, the object reaches terminal velocity and stops accelerating. The effect of air resistance is more pronounced for objects with a large surface area relative to their mass.
27. What is the role of the gravitational constant (G) in free fall calculations?
The gravitational constant (G) is a fundamental physical constant that appears in Newton's law of universal gravitation. While it's not directly used in most free fall calculations near Earth's surface, it's crucial for understanding the origin of the acceleration due to gravity (g). The value of g on Earth's surface can be derived using G: g = GM/R², where M is Earth's mass and R is Earth's radius. G allows us to calculate gravitational effects for any two masses at any distance.
28. How does the rotation of the Earth affect free fall motion?
The Earth's rotation affects free fall motion through the Coriolis effect, which causes moving objects to appear to deflect from their path when viewed from a rotating reference frame. This effect is negligible for small-scale, short-duration falls but becomes significant for long-range projectiles or very tall structures. Additionally, the Earth's rotation slightly reduces the effective gravitational acceleration at the equator due to the centrifugal force, making g about 0.3% less than at the poles.
29. How does the concept of free fall apply to weightlessness in space?
Weightlessness in space is actually a state of continuous free fall. Astronauts in orbit around Earth are falling towards the planet at the same rate as their spacecraft. They appear weightless because both they and their surroundings are falling at the same rate, so there's no force of the floor pushing up against them. This state is more accurately called "microgravity" because small gravitational effects are still present.
30. What is the difference between 'g' and 'G' in the context of gravity and free fall?
g' and 'G' are distinct but related concepts in gravity and free fall. 'g' represents the acceleration due to gravity, typically about 9.8 m/s² near Earth's surface. It's used in free fall calculations and varies depending on location. 'G', on the other hand, is the gravitational constant, a fundamental physical constant with a value of about 6.674 × 10⁻¹¹ N(m/kg)². 'G' is used in Newton's law of universal gravitation and doesn't change with location.
31. What is the significance of Galileo's leaning tower of Pisa experiment in the context of free fall?
Galileo's leaning tower of Pisa experiment (whether actually performed or thought experiment) was crucial in disproving Aristotle's theory that heavier objects fall faster than lighter ones. By demonstrating that objects of different masses fall at the same rate (neglecting air resistance), Galileo laid the groundwork for understanding that acceleration due to gravity is independent of mass. This insight was fundamental to the development of classical mechanics and our modern understanding of free fall.
32. How does the concept of free fall apply to the motion of planets around the Sun?
The motion of planets around the Sun can be understood as a form of free fall. Each planet is continuously "falling" towards the Sun due to gravitational attraction, but its tangential velocity prevents it from spiraling inward. The balance between this "falling" motion and the planet's velocity results in an elliptical orbit. This perspective, first proposed by Newton, demonstrates that the same principles governing the fall of an apple also govern the motion of celestial bodies.
33. What is the relationship between free fall and the equivalence of gravitational and inertial mass?
The equivalence of gravitational and inertial mass is demonstrated by the fact that all objects fall at the same rate in free fall (in a vacuum). Gravitational mass determines the force of gravity on an object, while inertial mass determines its resistance to acceleration. If these were different, objects would fall at different rates. The fact that they don't supports Einstein's equivalence principle and is a cornerstone of general relativity.
34. How does the concept of free fall apply to tidal forces?
Tidal forces arise from the difference in gravitational acceleration across an extended body. In essence, different parts of the body are in slightly different states of free fall. For example, the side of the Earth facing the Moon experiences a stronger gravitational pull (and thus a different free fall condition) than the side facing away. This differential in free fall conditions causes the stretching effect we observe as tides.

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