Animated Solution for Mathematics - Conic Sections: Two stones are projected from the top of a cliff h metres high, with the same speed u, so as to hit the ground at the same spot. If one of the stones is projected horizontally and the other is projected at an angle θ to the horizontal then tanθ equals
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Visualized Solution
Visualizing the Setup
Cliff height: h
Initial speed for both stones: u
Stone 1: Projected horizontally (θ=0)
Stone 2: Projected at an angle θ upwards
Both hit the same spot, so their horizontal range R is identical.
Trajectory of Stone 1
For Stone 1 (horizontal projection):
Initial vertical velocity uy=0
It follows a parabolic path under gravity.
Calculating Range R
Time of flight: t=g2h
Horizontal range R=u×t
R=ug2h
Squaring both sides: R2=g2hu2
Trajectory of Stone 2
For Stone 2 (projection at angle θ):
It travels higher and longer.
But it lands at the exact same horizontal distance R.
Equation of Trajectory
General equation of trajectory:
y=xtanθ−2u2cos2θgx2
Taking the launch point as origin (0,0).
The landing coordinates are (R,−h).
Applying Boundary Conditions
Substitute x=R and y=−h:
−h=Rtanθ−2u2cos2θgR2
Eliminating u and g
From Step 2, we know 2u2gR2=h
Substitute this into the trajectory equation:
−h=Rtanθ−cos2θh
Algebraic Simplification
Rearrange to isolate Rtanθ:
Rtanθ=cos2θh−h
Factor out h:
Rtanθ=h(cos2θ1−1)
Applying Trigonometry
Use the trigonometric identity cos2θ1=sec2θ
Rtanθ=h(sec2θ−1)
Since sec2θ−1=tan2θ:
Rtanθ=htan2θ
Isolating tanθ
Assuming θ=0, divide by tanθ:
R=htanθ
Isolate tanθ:
tanθ=hR
Final Answer
Substitute R=ug2h:
tanθ=hug2h
Simplify by bringing h inside the square root:
tanθ=ugh22h
Final Answer:tanθ=ugh2
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The Sigma Insight: Standard Equations of Parabola, Ellipse, and Hyperbola
Solution Diagram
The Dance of Two Stones
A Journey Through Projectile Motion
Imagine you are standing on the edge of a sheer cliff, the wind whipping past you, looking down at the ground h meters below. You hold two stones. You are about to perform a feat of physics.
You throw the first stone perfectly horizontally with speed u. It doesn't just fall; it traces a graceful parabolic arc until it kisses the ground at a specific spot.
Now, you throw the second stone with the same speed u, but this time, you aim it upwards at an angle θ. It soars higher, spends more time in the air, and yet, in a moment of pure mathematical harmony, it lands at the exact same spot as the first.
Phase 1
The Horizontal Stone
Let us begin with the first stone. Because it is thrown horizontally, its initial vertical velocity is zero. It is purely a victim of gravity.
The time it takes to fall a vertical distance h is governed by the kinematic equation:
h=21gt2
Solving for time, we get t=g2h. Since the horizontal velocity u remains constant throughout the flight, the horizontal range R is simply R=u×t.
Thus, we find our first crucial relationship:
R=ug2h
If we square this, we get:
R2=g2hu2
Keep this in your mind; it is the key that will unlock the entire problem.
Phase 2
The Angled Stone
Now, consider the second stone. It is launched at an angle θ. Its path is governed by the trajectory equation:
y=xtanθ−2u2cos2θgx2
If we set our origin at the launch point, the landing spot is at coordinates (R,−h). We use −h because the ground is below our launch point.
Substituting these coordinates into our trajectory equation, we get:
−h=Rtanθ−2u2cos2θgR2
Phase 3
The Mathematical Bridge
Here is where the magic happens. Look at the term 2u2gR2 in our equation.
From our first stone, we know that R2=g2hu2, which implies:
2u2gR2=h
We can substitute this directly into our trajectory equation. The equation transforms into:
−h=Rtanθ−cos2θh
Phase 4
The Elegant Simplification
Now, let us rearrange the terms to isolate our target, tanθ. Moving the terms around, we get:
Rtanθ=cos2θh−h
Factoring out h, we have:
Rtanθ=h(cos2θ1−1)
Recall your trigonometric identities: cos2θ1 is simply sec2θ, and sec2θ−1=tan2θ. The equation becomes:
Rtanθ=htan2θ
Since $\theta
eq 0$, we can divide both sides by tanθ to get:
R=htanθ
The Final Reveal
We are almost there. We know R=ug2h. Substituting this back into our simplified equation, we get:
ug2h=htanθ
Solving for tanθ, we find:
tanθ=hug2h
Bringing the h inside the square root as h2, we get tanθ=ugh22h, which simplifies to:
tanθ=ugh2
And there it is! The answer emerges from the algebra, clean and elegant. You have just mastered the physics of two stones, proving that even the most complex motions are governed by simple, beautiful laws.