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Question: A body is projected at \(t = 0\) with a velocity of \(10m{s^{ - 1}}\) at an angle of \({60^ \circ }\...

A body is projected at t=0t = 0 with a velocity of 10ms110m{s^{ - 1}} at an angle of 60{60^ \circ } with the horizontal. The radius of curvature of its trajectory at t=1st = 1s is RR. Neglecting air resistance and taking acceleration due to gravity g=10ms2g = 10m{s^{ - 2}}, the value of RR is:
(A) 2.4m2.4m
(B) 10.3m10.3m
(C) 2.8m2.8m
(D) 5.1m5.1m

Explanation

Solution

Hint
For solving this question, we need to use the concept of centripetal acceleration and find its value. From there, we can easily find the radius of curvature of the trajectory.
Formula Used: The formulae used in solving this question are:
-v=u+atv = u + at, vv is the final velocity, uu is the initial velocity, aa is the acceleration, and tt is the time elapsed.
-ac=v2R{a_c} = \dfrac{{{v^2}}}{R}, ac{a_c} is the centripetal acceleration, vv is the velocity, and RR is the radius of the circle.

Complete step by step answer
We begin by finding the velocity of the body at t=1st = 1s.
According to the question the initial velocity of the body, u=10ms1u = 10m{s^{ - 1}}
Also, the angle of projection θ=60\theta = {60^ \circ }
Horizontal direction:
Let uh{u_h}andvh{v_h} be the horizontal component of the initial and the final velocity of the body respectively.
uh=ucosθ\Rightarrow {u_h} = u\cos \theta
uh=10cos60\Rightarrow {u_h} = 10\cos {60^ \circ }
On solving, we get
uh=10(0.5)=50ms1\Rightarrow {u_h} = 10(0.5) = 50m{s^{ - 1}}
The acceleration in the horizontal direction is zero as there is no horizontal force on the body, i.e.
ah=0\Rightarrow {a_h} = 0
By the first equation of motion
vh=uh+aht\Rightarrow {v_h} = {u_h} + {a_h}t
vh=5+(0)1\Rightarrow {v_h} = 5 + (0)1
On solving, we get
vh=5ms1\Rightarrow {v_h} = 5m{s^{ - 1}} (1)
Vertical direction:
Let uv{u_v} andvv{v_v} be the horizontal component of the initial and the final velocity of the body respectively.
uv=usinθ\Rightarrow {u_v} = u\sin \theta
uv=10sin60\Rightarrow {u_v} = 10\sin {60^ \circ }
On solving, we get
uv=1032=53ms1\Rightarrow {u_v} = 10\dfrac{{\sqrt 3 }}{2} = 5\sqrt 3 m{s^{ - 1}}
As the only force which acts on the body is the gravitational force, which is downwards, so the acceleration of the body is in the vertical direction, i.e.
av=g=10ms2\Rightarrow {a_v} = g = - 10m{s^{ - 2}}
By the first equation of motion, we have
vv=uv+avt\Rightarrow {v_v} = {u_v} + {a_v}t
vv=53+(10)1\Rightarrow {v_v} = 5\sqrt 3 + ( - 10)1
On solving, we get
vv=5(32)ms1\Rightarrow {v_v} = 5\left( {\sqrt 3 - 2} \right)m{s^{ - 1}} (2)
Now, the total final velocity vv of the body is given by
v2=vh2+vv2\Rightarrow {v^2} = {v_h}^2 + {v_v}^2
Substituting from (1) and (2), we get
v2=52+[5(32)]2\Rightarrow {v^2} = {5^2} + {\left[ {5\left( {\sqrt 3 - 2} \right)} \right]^2}
v2=26.79m2s2\Rightarrow {v^2} = 26.79{m^2}{s^{ - 2}} (3)
Also, the angle φ\varphi with the vertical made by the final velocity vector is given by
tanφ=vhvv\Rightarrow \tan \varphi = \dfrac{{{v_h}}}{{{v_v}}}
tanφ=55(32)\Rightarrow \tan \varphi = \dfrac{5}{{5\left( {\sqrt 3 - 2} \right)}}
On solving, we get
tanφ=1(32)\Rightarrow \tan \varphi = \dfrac{1}{{\left( {\sqrt 3 - 2} \right)}}
Taking tangent inverse both the sides, we get
φ=tan1(1(32))\Rightarrow \varphi = {\tan ^{ - 1}}\left( {\dfrac{1}{{\left( {\sqrt 3 - 2} \right)}}} \right)
φ=75\Rightarrow \varphi = - {75^ \circ }
Now, we find the component of the acceleration perpendicular to the velocity, that is, the centripetal acceleration of the body.
As the acceleration is vertically downwards, the centripetal acceleration is given by
ac=avsinφ\Rightarrow {a_c} = {a_v}\sin \varphi
ac=10sin(75)\Rightarrow {a_c} = - 10\sin \left( { - {{75}^ \circ }} \right)
On solving, we get
ac=9.66ms2\Rightarrow {a_c} = 9.66m{s^{ - 2}} (4)
We know that the centripetal acceleration is given by
ac=v2R\Rightarrow {a_c} = \dfrac{{{v^2}}}{R}
Substituting from (3) and (4), we get
9.66=26.79R\Rightarrow 9.66 = \dfrac{{26.79}}{R}
By cross multiplication, we get
R=26.799.66\Rightarrow R = \dfrac{{26.79}}{{9.66}}
R=2.77m\Rightarrow R = 2.77m
R2.8m\Rightarrow R \approx 2.8m
So the radius of curvature of its trajectory at t=1st = 1sis2.8m2.8m
Hence, the correct answer is option (C), 2.8m2.8m

Note
Do not forget to find out the perpendicular component of the acceleration along the velocity of the body. As we know that the centripetal force acts perpendicular to the motion of the body, so the centripetal acceleration is the component of the acceleration perpendicular to the body.