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A body has terminal speed \(V\) when falling in still air. What is its terminal velocity (relative to the ground) when falling in a steady horizontal wind with speed \(U\) ?

Short Answer

Expert verified
The terminal velocity of the body relative to the ground when falling in a steady horizontal wind with speed \(U\) is \(W = \sqrt{V^2 + U^2}\).

Step by step solution

01

Understanding concept of terminal velocity

The terminal velocity is the maximum velocity attainable by an object when it is dropped in a medium (like air). It's called 'terminal velocity' because it is the final, unchanging velocity that the object maintains.
02

Understanding the effect of horizontal wind

Now consider the effect of the steady horizontal wind. The speed of the wind, \(U\), is in the horizontal direction, and it's constant. It doesn't impact the falling object's vertical motion, but it does modify its horizontal movement.
03

Calculating relative terminal velocity

The terminal velocity of the object relative to the ground is the vector sum of its terminal velocity in still air, \(V\), and the steady horizontal wind velocity, \(U\). Since these two velocities are orthogonal, they form a right angled triangle if the result is denoted by \(W\). Using Pythagoras' theorem, \(W = \sqrt{V^2 + U^2}\).

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Key Concepts

These are the key concepts you need to understand to accurately answer the question.

Horizontal Wind Effect
When an object is falling through the air, a horizontal wind can significantly alter its path. The horizontal wind effect modifies the horizontal component of motion, while not affecting the vertical descent. This is because the wind blows across the direction of the fall.

Let's think about it: Imagine you're holding a ball and letting it fall. If there is no wind, the ball simply falls straight down. But now, imagine a steady wind blowing sideways. Although the wind doesn't impact how fast the ball falls downward, it pushes the ball to the side, adding a new dimension to the motion.
  • The horizontal movement of the object is exclusively due to the wind blowing at speed \(U\).
  • It causes the object to drift off course from the purely vertical path.
  • Understanding this effect helps in determining the actual path an object takes as it falls.
These dynamics are crucial for calculating the relative velocity with which the object moves in relation to the ground.
Relative Velocity
Relative velocity refers to the velocity of one object as observed from another. In our scenario, we are concerned with how fast an object, falling with a terminal speed \(V\) in still air, appears to move when accounting for an additional factor like a horizontal wind.

The relative velocity of the object with respect to the ground is essentially how its movement appears to an observer on the ground. This requires accounting for both the vertical and horizontal components of the object's motion.
  • The vertical component is the terminal speed of the object \(V\), which remains unaffected by the wind.
  • The horizontal component is entirely the result of the wind, which contributes \(U\) to the object's velocity along the ground.
Combining these components gives the actual velocity vector, which isn't simply the sum of \(V\) and \(U\), since they act perpendicularly. This combination is described using Pythagorean theorem.
Pythagorean Theorem
The Pythagorean theorem is a mathematical principle that relates the lengths of the sides of a right triangle. In the context of velocity, it helps us calculate the magnitude of the resultant velocity vector when two perpendicular velocities are involved.

When an object falls with terminal speed \(V\) and is acted upon by a horizontal wind speed \(U\), these two vectors create a right triangle. The theorem states for a right triangle with sides \(a\) and \(b\), and hypotenuse \(c\):

\[ c = \sqrt{a^2 + b^2} \]

In our case:
  • \(V\) represents the vertical side of the triangle.
  • \(U\) is the horizontal side.
  • \(W\), the hypotenuse, is the terminal velocity relative to the ground.
Therefore, the effective terminal velocity \(W\) is calculated as:
\[ W = \sqrt{V^2 + U^2} \] By using this equation, we can see how both the falling speed and the wind speed contribute to the overall path of the object.

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Most popular questions from this chapter

A body is projected in a steady horizontal wind and moves under uniform gravity and linear air resistance. Show that the influence of the wind is the same as if the magnitude and direction of gravity were altered. Deduce that it is possible for the body to return to its starting point. What is the shape of the path in this case?

A particle of mass \(m\) can move on a rough horizontal table and is attached to a fixed point on the table by a light inextensible string of length \(b\). The resistance force exerted on the particle is \(-m K v\), where \(v\) is the velocity of the particle. Initially the string is taut and the particle is projected horizontally, at right angles to the string, with speed \(u\). Find the angle turned through by the string before the particle comes to rest. Find also the tension in the string at time \(t\).

A particle \(P\) of mass \(m\) slides on a smooth horizontal table. \(P\) is connected to a second particle \(Q\) of mass \(M\) by a light inextensible string which passes through a small smooth hole \(O\) in the table, so that \(Q\) hangs below the table while \(P\) moves on top. Investigate motions of this system in which \(Q\) remains at rest vertically below \(O\), while \(P\) describes a circle with centre \(O\) and radius \(b\). Show that this is possible provided that \(P\) moves with constant speed \(u\), where \(u^{2}=M g b / m\).

An object is dropped from the top of a building and is in view for time \(\tau\) while passing a window of height \(h\) some distance lower down. How high is the top of the building above the top of the window?

Find a series approximation for the period of the simple pendulum, in powers of the angular amplitude \(\alpha .\) Proceed as follows: The exact period \(\tau\) of the pendulum was found in Example \(4.9\) and is given by the integral (4.9). This integral is not suitable for expansion as it stands. However, if we write \(\cos \theta-\cos \alpha=2\left(\sin ^{2}(\alpha / 2)-\right.\) \(\sin ^{2}(\theta / 2)\) ) and make the sneaky substitution \(\sin (\theta / 2)=\sin (\alpha / 2) \sin \phi\), the formula for \(\tau\) becomes $$\tau=4\left(\frac{b}{g}\right)^{1 / 2} \int_{0}^{\pi / 2}\left(1-\epsilon^{2} \sin ^{2} \phi\right)^{-1 / 2} d \phi$$ where \(\epsilon=\sin (\alpha / 2)\). This new integrand is easy to expand as a power series in the variable \(\epsilon\) and the limits of integration are now constants. Use computer assistance to expand the integrand to the required number of terms and then integrate term by term over the interval \([0, \pi / 2]\). Finally re-expand as a power series in the variable \(\alpha\). The answer to two terms is given by equation (4.10), but it is just as easy to obtain any number of terms.

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