Motion of Particles in Uniform Gravitational Field

In summary, two particles with velocities $v_1 = 3 \text{ms}^{-1}$ and $v_2 = 4 \text{ms}^{-1}$ moving horizontally in opposite directions in a uniform gravitational field will have their velocities become mutually perpendicular after a time $t = \frac{\sqrt{v_1 v_2}}{g}$. The distance between the particles at this point will be $7t$ m. This can be determined by setting up a velocity diagram and solving for the vertical component of velocity, which is equal to $2 \sqrt{3}$ m/s. The separation between the particles can then be found by multiplying this value by the time $t$.
  • #1
DrunkenOldFool
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Two particles move in a uniform gravitational field with an acceleration $g$. At the initial moment the particles were located at one point and moved with velocities $v_1 = 3 \text{ms}^{-1}$ and $v_1 = 4 \text{ms}^{-1}$ horizontally in opposite directions. Find distance between the particles when their velocities become mutually perpendicular.
 
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  • #2
DrunkenOldFool said:
Two particles move in a uniform gravitational field with an acceleration $g$. At the initial moment the particles were located at one point and moved with velocities $v_1 = 3 \text{ms}^{-1}$ and $v_1 = 4 \text{ms}^{-1}$ horizontally in opposite directions. Find distance between the particles when their velocities become mutually perpendicular.
The two horizontal components of velocity are constant, and the vertical components are always equal. Now draw a velocity diagram for when the two velocities are perpendicular, and solve the diagram for the vertical component of velocity (it should come to \(2 \sqrt{3}\) m/s if my scratch algebra and arithmetic are correct).

Now you can find the time \(t\) it took the vertical component to reach this value, and the separation is \(7t\) m.

CB
 
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  • #3
Let the velocities of the particles (say $\vec{v_{1}}'$ and $\vec{v_2 }'$) become perpendicular after time $t$. By equation of motion,

$$ \vec{v_{1}'}=\vec{v_{1}}+\vec{g}t \\ \vec{v_{2}'}=\vec{v_{2}}+\vec{g}t$$

As $\vec{v_1 ' }$ and $\vec{v_2 '}$ are perpendicular, we can write

$$ \begin{align*} \vec{v_1 ' } \cdot \vec{v_2 ' } &=0 \\ (\vec{v_{1}}+\vec{g}t) \cdot (\vec{v_{2}}+\vec{g}t) &= 0 \\ -v_1 v_2 +g^2 t^2 &=0 \\ t &= \frac{\sqrt{v_1 v_2}}{g}\end{align*}$$

Let $x_1$ and $x_2$ be the horizontal distances covered by particles 1 and 2 in time $t$ respectively. Note that the acceleration in horizontal direction is zero.

$$x_1 = v_1 t = v_1 \frac{\sqrt{v_1 v_2}}{g} \\ x_2 = v_2 t = v_2 \frac{\sqrt{v_1 v_2}}{g}$$

The total separation between the particles is

$$x_1+x_2= (v_1+v_2)\frac{\sqrt{v_1 v_2}}{g}$$
 
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  • #4
This is my try.

View attachment 277

considering the triangle $ABC$,

$$\begin{align*}
\alpha &=90^\circ - \beta \\
\tan{\alpha} &= \tan (90^\circ -\beta ) \\
\tan{\alpha} &= \cot \beta \\
\frac{gt}{v_1}&=\frac{v_2}{gt}\\
g^2t^2 &=v_1\times v_2\\
\therefore t &= \frac{\sqrt{v_1v_2}}{g} \qquad since \; t>0 \\ \end{align*}

$$

the rest is as same as sbhatnagar's
 

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  • #5
Thank You!:)
 

FAQ: Motion of Particles in Uniform Gravitational Field

What is the definition of "Motion of Particles in Uniform Gravitational Field"?

The motion of particles in a uniform gravitational field refers to the movement of objects under the influence of a constant gravitational force, such as the force of gravity on objects near the surface of the Earth.

What is the equation for calculating the force of gravity on a particle in a uniform gravitational field?

The equation for calculating the force of gravity on a particle in a uniform gravitational field is F = mg, where F is the force of gravity, m is the mass of the particle, and g is the gravitational acceleration.

How does the mass of a particle affect its motion in a uniform gravitational field?

The mass of a particle does not affect its motion in a uniform gravitational field. All objects, regardless of their mass, will experience the same acceleration due to gravity in a uniform gravitational field.

What is the significance of the gravitational constant in the motion of particles in a uniform gravitational field?

The gravitational constant, denoted as G, is a fundamental constant in physics that determines the strength of the gravitational force between two objects with mass. It is a crucial component in the equation for calculating the force of gravity on a particle in a uniform gravitational field.

What are some real-life examples of motion of particles in a uniform gravitational field?

Some real-life examples of motion of particles in a uniform gravitational field include objects falling to the ground, planets orbiting around a star, and satellites orbiting around Earth.

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