Motion of Body Under Gravity (Free Fall)

Motion of Body Under Gravity (Free Fall)

Vishal kumarUpdated on 02 Jul 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)
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)

Q: How does the concept of free fall apply to tidal forces?
A:
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.
Q: What is the relationship between free fall and the equivalence of gravitational and inertial mass?
A:
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.
Q: How does the concept of free fall apply to the motion of planets around the Sun?
A:
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.
Q: What is the significance of Galileo's leaning tower of Pisa experiment in the context of free fall?
A:
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.
Q: What is the difference between 'g' and 'G' in the context of gravity and free fall?
A:
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.
Q: How does the concept of free fall apply to weightlessness in space?
A:
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.
Q: How does the rotation of the Earth affect free fall motion?
A:
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.
Q: What is the role of the gravitational constant (G) in free fall calculations?
A:
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.
Q: How does air resistance affect the acceleration of a falling object?
A:
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.
Q: How does the mass of a planet affect the free fall acceleration on its surface?
A:
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.