Chapter 8: Problem 27
Show that the system $$ \frac{d x}{d t}=-2 y, \quad \frac{d y}{d t}=x-5, $$ has closed elliptical orbits. (Hint: Consider first transforming \(x\) to \(x-5\) and \(y\) to \(y / 2\) and then using a polar transformation.)
Short Answer
Expert verified
The system has closed elliptical orbits centered at (5, 0).
Step by step solution
01
- Transform the system
Transform the variables: let \(x' = x - 5\) and \(y' = \frac{y}{2}\). Substitute these into the original differential equations.
02
- Substitution into original equations
For \(dx\) with the transformation, we have \(dx' = dx\), so \(\frac{dx'}{dt} = \frac{dx}{dt}\). For \(dy\), we have \(dy' = \frac{1}{2}dy\), hence \(\frac{dy'}{dt} = \frac{1}{2} \frac{dy}{dt}\). Substituting these into the original system gives: \[\frac{dx'}{dt} = -4y', \quad \frac{dy'}{dt} = x'\].
03
- Use polar coordinates
Consider the polar transformation with \(x' = r \cos(\theta)\) and \(y' = r \sin(\theta)\). This changes our equations to polar form.
04
- Transform the differential equations
Using the chain rule for polar coordinates, \(\frac{dx'}{dt} = \cos(\theta) \frac{dr}{dt} - r \sin(\theta) \frac{d\theta}{dt}\) and similarly for \(y'\). Substituting these into our transformed system:\[-4r \sin(\theta) = \cos(\theta) \frac{dr}{dt} - r \sin(\theta) \frac{d\theta}{dt}\] \[r \cos(\theta) = \sin(\theta) \frac{dr}{dt} + r \cos(\theta) \frac{d\theta}{dt}\].
05
- Solve for \(\frac{dr}{dt}\) and \(\frac{d\theta}{dt}\)
By equating coefficients for \(\sin(\theta)\) and \(\cos(\theta)\) we get: \(\frac{dr}{dt} = 0\) (so \(r\) is constant) and \(\frac{d\theta}{dt} = -4\). Recall that \(r\) constant implies a circular motion in polar coordinates.
06
- Verify elliptical shape
Returning to Cartesian coordinates with \(x' = x - 5\) and \(y' = \frac{y}{2}\), and recognizing we have a proportional relationship, the curves are ellipses centered at (5, 0).
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Key Concepts
These are the key concepts you need to understand to accurately answer the question.
polar coordinates transformation
To better understand elliptical orbits, we first transform the system's coordinates from Cartesian to polar. Polar coordinates describe a point in terms of its distance from a reference point (called the radius, \( r \)) and the angle formed with a reference direction (called the angle, \( \theta \)).
This transformation simplifies the analysis of problems where symmetry and rotation are involved. By converting the variables \( x \) and \( y \) into polar coordinates, we can leverage trigonometric relationships to further simplify the differential equations. For our problem, the new transformed coordinates become \( x' = r \cos(\theta) \) and \( y' = r \sin(\theta) \).
This helps us deal with the motion and behavior of the system more intuitively.
This transformation simplifies the analysis of problems where symmetry and rotation are involved. By converting the variables \( x \) and \( y \) into polar coordinates, we can leverage trigonometric relationships to further simplify the differential equations. For our problem, the new transformed coordinates become \( x' = r \cos(\theta) \) and \( y' = r \sin(\theta) \).
This helps us deal with the motion and behavior of the system more intuitively.
closed orbits
A key element to recognize in this problem is the presence of closed orbits. Closed orbits imply that the motion of the system repeats itself in a cyclical pattern, forming closed loops.
For the system \( \frac{dx}{dt} = -2y \) and \( \frac{dy}{dt} = x - 5 \), transforming to a new set of variables allows us to see these closed orbits more clearly. The transformation \( x' = x - 5 \) and \( y' = \frac{y}{2} \) is used to shift and scale the original variables.
Through this transformation, it becomes easier to analyze the phase space of the system and identify the elliptical paths that represent the closed orbits.
For the system \( \frac{dx}{dt} = -2y \) and \( \frac{dy}{dt} = x - 5 \), transforming to a new set of variables allows us to see these closed orbits more clearly. The transformation \( x' = x - 5 \) and \( y' = \frac{y}{2} \) is used to shift and scale the original variables.
Through this transformation, it becomes easier to analyze the phase space of the system and identify the elliptical paths that represent the closed orbits.
differential system transformation
Transforming a differential system is often necessary to make complicated systems more tractable. For our system, we start by redefining \( x \) and \( y \) as \( x' = x - 5 \) and \( y' = \frac{y}{2} \).
Next, we substitute these new variables into the original differential equations. This gives us a transformed system: \( \frac{dx'}{dt} = -4y' \) and \( \frac{dy'}{dt} = x' \).
The goal is to simplify the equations, making them easier to solve or analyze. By choosing appropriate transformations, we can often reduce the complexity of the system, revealing underlying structures or symmetries.
Next, we substitute these new variables into the original differential equations. This gives us a transformed system: \( \frac{dx'}{dt} = -4y' \) and \( \frac{dy'}{dt} = x' \).
The goal is to simplify the equations, making them easier to solve or analyze. By choosing appropriate transformations, we can often reduce the complexity of the system, revealing underlying structures or symmetries.
chain rule
The chain rule is essential when dealing with transformations, particularly in differential equations. It relates the rate of change of a function to the rates of change of its variables.
For instance, when we transform our variables to polar coordinates, we need the chain rule to express how derivatives like \( \frac{dx'}{dt} \) and \( \frac{dy'}{dt} \) change according to \( \frac{dr}{dt} \) and \( \frac{d\theta}{dt} \).
For instance, when we transform our variables to polar coordinates, we need the chain rule to express how derivatives like \( \frac{dx'}{dt} \) and \( \frac{dy'}{dt} \) change according to \( \frac{dr}{dt} \) and \( \frac{d\theta}{dt} \).
- For \( x' \), we have \( \frac{dx'}{dt} = \cos(\theta) \frac{dr}{dt} - r \sin(\theta) \frac{d\theta}{dt} \).
- Similarly, for \( y' \), we have \( \frac{dy'}{dt} = \sin(\theta) \frac{dr}{dt} + r \cos(\theta) \frac{d\theta}{dt} \).
constant radius in polar coordinates
Understanding the concept of constant radius in polar coordinates is crucial, especially when dealing with closed orbits. In a system where the radius \( r \) does not change over time \( \left( \frac{dr}{dt} = 0 \right) \), the motion is constrained to a circle in the polar plane.
In our problem, we found that \( \frac{dr}{dt} = 0 \), indicating that \( r \) remains constant. This simplifies the analysis and shows that the closed orbits are circles, which in this transformed context translate to ellipses in the original coordinates.
This insight helps us conclude that the original system features elliptical orbits, providing a clear visualization of the motion dynamics.
In our problem, we found that \( \frac{dr}{dt} = 0 \), indicating that \( r \) remains constant. This simplifies the analysis and shows that the closed orbits are circles, which in this transformed context translate to ellipses in the original coordinates.
This insight helps us conclude that the original system features elliptical orbits, providing a clear visualization of the motion dynamics.