Warning: foreach() argument must be of type array|object, bool given in /var/www/html/web/app/themes/studypress-core-theme/template-parts/header/mobile-offcanvas.php on line 20

Compute velocity and acceleration from position data; one dimension. Let \(x(t)\) be the position of an object moving along the \(x\) axis. The velocity \(v(t)\) and acceleration \(a(t)\) can be approximately computed by the formulas $$ v(t) \approx \frac{x(t+\Delta t)-x(t-\Delta t)}{2 \Delta t}, \quad a(t) \approx \frac{x(t+\Delta t)-2 x(t)+x(t-\Delta t)}{\Delta t^{2}} $$ where \(\Delta t\) is a small time interval. As \(\Delta t \rightarrow 0\), the above formulas approach the first and second derivative of \(x(t)\), which coincide with the well-known definitions of velocity and acceleration. Write a function kinematics \((x, t, d t=1 E-4)\) for computing \(x, v\), and \(a\) time \(t\), using the above formulas for \(v\) and \(a\) with \(\Delta t\) corresponding to dt. Let the function return \(x, v\), and \(a\). Test the function with the position function \(x(t)=e^{-(t-4)^{2}}\) and the time point \(t=5\) (use \(\left.\Delta t=10^{-5}\right)\). Name of program: kinematics 1.py.

Short Answer

Expert verified
Write a Python function using given formulas to compute velocity and acceleration for a position function at a specific time point.

Step by step solution

01

Understand the Problem

We need to compute velocity and acceleration given position data using finite difference approximations. Position, velocity, and acceleration of an object are relevant to one dimension, specifically the x-axis.
02

Use the Given Formulas

We are provided with the general formulas for approximating velocity and acceleration:\[ v(t) \approx \frac{x(t+\Delta t) - x(t-\Delta t)}{2 \Delta t} \]\[ a(t) \approx \frac{x(t+\Delta t) - 2x(t) + x(t-\Delta t)}{\Delta t^2} \]
03

Define the Position Function

We test the formulas with the position function \(x(t) = e^{-(t-4)^2}\). This function describes the position of the object at any time \(t\).
04

Python Implementation

Write a function named `kinematics` that takes as input: position function \(x\), time \(t\), and a small time interval \(dt\). It should return \(x(t)\), \(v(t)\), and \(a(t)\).```pythonimport mathdef kinematics(x, t, dt=1e-4): position = x(t) velocity = (x(t + dt) - x(t - dt)) / (2 * dt) acceleration = (x(t + dt) - 2 * x(t) + x(t - dt)) / (dt ** 2) return position, velocity, acceleration```
05

Test the Function

Test the `kinematics` function at time \(t=5\) with \(x(t) = e^{-(t-4)^2}\) and \(dt=10^{-5}\).```pythondef position_function(t): return math.exp(-(t-4)**2)# Testingposition, velocity, acceleration = kinematics(position_function, 5, 1e-5)print("Position:", position)print("Velocity:", velocity)print("Acceleration:", acceleration)```
06

Verify the Results

Upon running the test, you should see the computed values for position, velocity, and acceleration at \(t=5\). Ensure these results are consistent with expectations for this Gaussian position function.

Unlock Step-by-Step Solutions & Ace Your Exams!

  • Full Textbook Solutions

    Get detailed explanations and key concepts

  • Unlimited Al creation

    Al flashcards, explanations, exams and more...

  • Ads-free access

    To over 500 millions flashcards

  • Money-back guarantee

    We refund you if you fail your exam.

Over 30 million students worldwide already upgrade their learning with Vaia!

Key Concepts

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

Python
Python is an incredibly versatile programming language. It's simple and easy to understand for beginners yet powerful for advanced applications. Python is often used in scientific programming due to its wide array of libraries and readability. When dealing with scientific problems like computing velocity and acceleration from position data, Python makes tasks manageable and efficient.
- Python comes equipped with powerful libraries such as NumPy and SciPy that facilitate mathematical computations. - Its syntax is clean and straightforward, allowing programmers to focus on solving scientific problems without getting bogged down by complex code. - Python's functions, like in the kinematics problem, enable the creation of reusable and efficient code blocks that can compute various scientific phenomena seamlessly.
Overall, understanding Python fundamentals is crucial for engaging in scientific programming and creating functions that simulate real-world problems.
Velocity and Acceleration
Velocity and acceleration are fundamental concepts in physics, representing the rate of change of an object's position and the rate of change of its velocity, respectively.

- **Velocity** refers to how fast something is moving and in what direction. It's expressed mathematically as the first derivative of the position function with respect to time.- **Acceleration** is concerned with how an object's velocity changes over time. Mathematically, it's the second derivative of the position function or the first derivative of the velocity function.
In the context of this exercise, velocity is approximated with a finite difference formula: \[ v(t) \approx \frac{x(t+\Delta t) - x(t-\Delta t)}{2 \Delta t} \] while acceleration's formula is:\[ a(t) \approx \frac{x(t+\Delta t) - 2x(t) + x(t-\Delta t)}{\Delta t^2} \] These approximations are derived from calculus and are particularly useful when only discrete data is available, as is often the case in computational problems.
Finite Difference Approximations
Finite Difference Approximations are essential for numerical differentiation. When analytical differentiation isn't feasible or a function is only available at specific points, finite differences offer a practical alternative.

- **Forward Difference**: Uses the function's values at a point and its immediate successor.- **Backward Difference**: Involves values at a point and its immediate predecessor.- **Central Difference**: Averages the forward and backward differences and is generally more accurate.
In the context of the provided exercise, the finite difference approximation for velocity is a central difference method, while the approximation for acceleration uses points around the target time to simulate a second derivative. These methods effectively handle data's discrete nature by sampling at small intervals (denoted by \(\Delta t\)), making them ideal for computational problems like motion analysis.
Kinematics Function
The kinematics function is a Python function devised to calculate the position, velocity, and acceleration of an object based on known position data.

- This function takes a position function, time point \(t\), and a small time interval (\(dt\)) as inputs.- It calculates the position using the provided function at the specified time.- Using finite difference formulas, it computes velocity and acceleration by approximating the derivatives with small changes in time.
For instance, in the problem's testing phase, the position function is defined as \(x(t) = e^{-(t-4)^2}\), simulating a Gaussian curve. When the function is executed, it returns the calculated position, velocity, and acceleration at the chosen time \(t=5\) with \(dt=10^{-5}\). This function is a practical tool for dynamically analyzing an object's movement in one-dimensional space.

One App. One Place for Learning.

All the tools & learning materials you need for study success - in one app.

Get started for free

Most popular questions from this chapter

Find prime numbers. The Sieve of Eratosthenes is an algorithm for finding all prime numbers less than or equal to a number \(N\). Read about this algorithm on Wikipedia and implement it in a Python program. Name of program file: find_primes.py.

Find the max/min elements in a list. Given a list a, the max function in Python's standard library computes the largest element in a: max(a). Similarly, min(a) returns the smallest element in a. The purpose of this exercise is to write your own max and min function. Use the following technique: Initialize a variable max_elem by the first element in the list, then visit all the remaining elements (a [1:]), compare each element to max_elem, and if greater, make max_elem refer to that element. Use a similar technique to compute the minimum element. Collect the two pieces of code in functions. Name of program file: maxmin_list. py.

Compute velocity and acceleration from position data; two dimensions. An object moves a long a path in the \(x y\) plane such that at time \(t\) the object is located at the point \((x(t), y(t))\). The velocity vector in the plane, at time \(t\), can be approximated as $$ v(t) \approx\left(\frac{x(t+\Delta t)-x(t-\Delta t)}{2 \Delta t}, \frac{y(t+\Delta t)-y(t-\Delta t)}{2 \Delta t}\right) $$ The acceleration vector in the plane, at time \(t\), can be approximated as $$ a(t) \approx\left(\frac{x(t+\Delta t)-2 x(t)+x(t-\Delta t)}{\Delta t^{2}}, \frac{y(t+\Delta t)-2 y(t)+y(t-\Delta t)}{\Delta t^{2}}\right) $$ Here, \(\Delta t\) is a small time interval. As \(\Delta t \rightarrow 0\), we have the limits \(v(t)=\left(x^{\prime}(t), y^{\prime}(t)\right)\) and \(a(t)=\left(x^{\prime \prime}(t), y^{\prime \prime}(t)\right)\) Make a function kinematics \((x, y, t, d t=1 E-4)\) for computing the velocity and acceleration of the object according to the formulas above (t corresponds to \(t\), and dt corresponds to \(\Delta t\) ). The function should return three 2 -tuples holding the position, the velocity, and the acceleration vector, all at time \(t\). Test the function for the motion along a circle with radius \(R\) and absolute velocity \(R \omega: x(t)=R \cos \omega t\) and \(y(t)=R \sin \omega t\). Compute the velocity and acceleration for \(t=1\) using \(R=1, \omega=2 \pi\), and \(\Delta t=10^{-5}\). Name of program: kinematics2.py.

Write a sort function for a list of 4 -tuples. Below is a list of the nearest stars and some of their properties. The list elements are 4 -tuples containing the name of the star, the distance from the sun in light years, the apparent brightness, and the luminosity. The apparent brightness is how bright the stars look in our sky compared to the brightness of Sirius A. The luminosity, or the true brightness, is how bright the stars would look if all were at the same distance compared to the Sun. The list data are found in the file stars. list, which looks as follows: The purpose of this exercise is to sort this list with respect to distance, apparent brightness, and luminosity. To sort a list data, one can call sorted(data), which returns the sorted list (cf. Table 2.1). However, in the present case each element is a 4 -tuple, and the default sorting of such 4 -tuples result in a list with the stars appearing in alphabethic order. We need to sort with respect to the 2nd, 3rd, or 4th element of each 4 -tuple. If a tailored sort mechanism is necessary, we can provide our own sort function as a second argument to sorted, as in sorted(data, mysort). Such a tailored sort function mysort must take two arguments, say a and b, and returns \(-1\) if a should become before \(\mathrm{b}\) in the sorted sequence, 1 if \(\mathrm{b}\) should become before a, and 0 if they are equal. In the present case, a and \(b\) are 4-tuples, so we need to make the comparison between the right elements in a and b. For example, to sort with respect to luminosity we write def mysort \((a, b):\) if \(a[3]b[3]:\) return 1 else: return 0 Write the complete program which initializes the data and writes out three sorted tables: star name versus distance, star name versus apparent brightness, and star name versus luminosity. Name of program file: sorted_stars_data.py.

Make a table for approximations of \(\cos x\). The function \(\cos (x)\) can be approximated by the sum $$ C(x ; n)=\sum_{j=0}^{n} c_{j} $$ where $$ c_{j}=-c_{j-1} \frac{x^{2}}{2 j(2 j-1)}, \quad j=1,2, \ldots, n $$ and \(c_{0}=1\). Make a Python function for computing \(C(x ; n)\). (Hint: Represent \(c_{j}\) by a variable term, make updates term = -term*... inside a for loop, and accumulate the term variable in a variable for the sum.) Also make a function for writing out a table of the errors in the approximation \(C(x ; n)\) of \(\cos (x)\) for some \(x\) and \(n\) values given as arguments to the function. Let the \(x\) values run downward in the rowsand the \(n\) values to the right in the columns. For example, a table for \(x=4 \pi, 6 \pi, 8 \pi, 10 \pi\) and \(n=5,25,50,100,200\) can look like \(\begin{array}{rccccc}\mathrm{x} & 5 & 25 & 50 & 100 & 200 \\ 12.5664 & 1.61 \mathrm{e}+04 & 1.87 \mathrm{e}-11 & 1.74 \mathrm{e}-12 & 1.74 \mathrm{e}-12 & 1.74 \mathrm{e}-12 \\ 18.8496 & 1.22 \mathrm{e}+06 & 2.28 \mathrm{e}-02 & 7.12 \mathrm{e}-11 & 7.12 \mathrm{e}-11 & 7.12 \mathrm{e}-11 \\ 25.1327 & 2.41 \mathrm{e}+07 & 6.58 \mathrm{e}+04 & -4.87 \mathrm{e}-07 & -4.87 \mathrm{e}-07 & -4.87 \mathrm{e}-07 \\ 31.4159 & 2.36 \mathrm{e}+08 & 6.52 \mathrm{e}+09 & 1.65 \mathrm{e}-04 & 1.65 \mathrm{e}-04 & 1.65 \mathrm{e}-04\end{array}\) Observe how the error increases with \(x\) and decreases with \(n .\) Name of program file: cossum.py.

See all solutions

Recommended explanations on Computer Science Textbooks

View all explanations

What do you think about this solution?

We value your feedback to improve our textbook solutions.

Study anywhere. Anytime. Across all devices.

Sign-up for free