Falling

\[ \begin{align}\begin{aligned}\newcommand\blank{~\underline{\hspace{1.2cm}}~}\\% Bold symbols (vectors) \newcommand\bs[1]{\mathbf{#1}}\\% Poor man's siunitx \newcommand\unit[1]{\mathrm{#1}} \newcommand\num[1]{#1} \newcommand\qty[2]{#1~\unit{#2}}\\\newcommand\per{/} \newcommand\squared{{}^2} % % Scale \newcommand\milli{\unit{m}} \newcommand\centi{\unit{c}} \newcommand\kilo{\unit{k}} \newcommand\mega{\unit{M}} % % Angle \newcommand\radian{\unit{rad}} \newcommand\degree{\unit{{}^\circ}} % % Time \newcommand\second{\unit{s}} % % Distance \newcommand\meter{\unit{m}} \newcommand\m{\meter} \newcommand\inch{\unit{in}} \newcommand\feet{\unit{ft}} \newcommand\mile{\unit{mi}} \newcommand\mi{\mile} % % Volume \newcommand\gallon{\unit{gal}} % % Mass \newcommand\gram{\unit{g}} \newcommand\g{\gram} % % Frequency \newcommand\hertz{\unit{Hz}} \newcommand\rpm{\unit{rpm}} % % Voltage \newcommand\volt{\unit{V}} \newcommand\V{\volt} \newcommand\millivolt{\milli\volt} \newcommand\mV{\milli\volt} \newcommand\kilovolt{\kilo\volt} \newcommand\kV{\kilo\volt} % % Current \newcommand\ampere{\unit{A}} \newcommand\A{\ampere} \newcommand\milliampereA{\milli\ampere} \newcommand\mA{\milli\ampere} \newcommand\kiloampereA{\kilo\ampere} \newcommand\kA{\kilo\ampere} % % Resistance \newcommand\ohm{\Omega} \newcommand\milliohm{\milli\ohm} \newcommand\kiloohm{\kilo\ohm} % correct SI spelling \newcommand\kilohm{\kilo\ohm} % "American" spelling used in siunitx \newcommand\megaohm{\mega\ohm} % correct SI spelling \newcommand\megohm{\mega\ohm} % "American" spelling used in siunitx % % Inductance \newcommand\henry{\unit{H}} \newcommand\H{\henry} \newcommand\millihenry{\milli\henry} \newcommand\mH{\milli\henry} % % Temperature \newcommand\celsius{\unit{^{\circ}C}} \newcommand\C{\unit{\celsius}} \newcommand\fahrenheit{\unit{^{\circ}F}} \newcommand\F{\unit{\fahrenheit}} \newcommand\kelvin{\unit{\K}} \newcommand\K{\unit{\kelvin}}\\% Power \newcommand\watt{\unit{W}} \newcommand\W{\watt} \newcommand\milliwatt{\milli\watt} \newcommand\mW{\milli\watt} \newcommand\kilowatt{\kilo\watt} \newcommand\kW{\kilo\watt} % % Torque \newcommand\ozin{\unit{oz}\text{-}\unit{in}} \newcommand\newtonmeter{\unit{N\text{-}m}}\end{aligned}\end{align} \]

Apr 16, 2025 | 216 words | 2 min read

4.2.1. Falling#

When an object begins falling due to gravity, the distance the object falls in a given time \(t\) can be found as shown

(4.1)#\[d={1 \over 2}gt^2\]

where \(d\) is the distance in meters (\(\meter\)), \(g\) is the gravitational force, and \(t\) is the time in seconds (\(\second\)).

Write a function named falling_dist that accepts an object’s falling time (in seconds [\(\second\)]) as an argument, and then calculates and returns the distance in meters \((\meter)\) that the object will fall during that time. Assume that the gravitational force is constant at \(8.87 \ {\meter \over \second^2}\) (mean surface gravity of Venus). Make sure to define this function outside your main function.

Then, inside your main function, write a loop to iterate through time values from \(5 (\second)\) to \(50 (\second)\) in \(5 (\second)\) increments. Inside this loop, call your falling_dist function to calculate the falling distance at each time. Finally, format the results as shown in the table below, using the data in the output table.

Sample Output#

Ensure your program’s output matches the provided samples exactly. This includes all characters, white space, and punctuation. In the samples, user input is highlighted like this for clarity, but your program should not highlight user input in this way.

Sample Output

$ python3 falling_login.py Time (s) Distance (m) ---------------------- 5 110.9 10 443.5 15 997.9 20 1774.0 25 2771.9 30 3991.5 35 5432.9 40 7096.0 45 8980.9 50 11087.5

Deliverables#

Save your finished program as falling_login.py, replacing login with your Purdue login. Then submit it along with all the deliverables listed in Table 4.1 below.

Table 4.1 Deliverables#

Deliverable

Description

falling_login.py

Your finished program.

Screenshot(s)

PNG(s) capturing the test case.