Solving Acceleration Model for Solar Drag Race

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The discussion focuses on developing a mathematical model for a solar-powered drag race over a distance of 250 meters, starting from rest. Key equations are presented for velocity and distance as functions of time, considering power input and losses due to aerodynamic drag, rolling resistance, and wheel rotation. The user seeks assistance in solving a complex cubic equation derived from these factors, which incorporates kinetic energy and various drag coefficients. Suggestions include using numerical methods or online calculators for solving cubic equations, as the problem is challenging to tackle analytically. The goal is to refine the model for accurate predictions of performance in the race.
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I also posted this in one of the engineering forums, but it is essentially a math problem, so I thought I would post it here as well.

I am working on a model of a solar powered drag race.

The race: 250 meters, no incline, initial velocity = 0.

Classical physics gives us the following equations (ignores aero and rolling drag and wheel rotation):

Velocity as a function of time V = (2Pt/M)^.5
P = power, M = mass

Distance as a function of time d = (2/3)((2P/M)^.5)t^(1.5)

Time to travel x distance t = ((1.5d)^(2/3))(M/2P)^1/3


But of course we do lose power to aerodynamic drag forces

Pa = .5rCdAV^3 (r = air density, Cd = aero drag coef., A = frontal area)

and rolling drag at the wheels

Pr = CrMV (Cr = rolling drag coef.)

and wheel rotation

Pw = FwV^3 (Fw = wheel rotational factor)


So if our inertial power equals our power in, Pi (from the solar panel) minus our power lost to friction (aero, rolling, wheel rotation), then our velocity equation becomes:

V = (2((Pi-(.5rCdAV^3)-(CrMV)-(FwV^3))t)/M)^.5

I need help solving this equation. I have approximated the solution by chopping the race up into small pieces and solving iteratively, but I would rather do it right.
 
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Let me sort this out.
Our variable is the velocity function in time: ##v(t)##.
We have a kinetic energy ##E## which you call initial power Pi.
We have air resistance ##P_a = \alpha \cdot v(t)^3## with some constant factor ##\alpha## which you wrote rCdA.
We have a drag of ##P_r= \beta \cdot v(t)## with some constant factor ##\beta## which you wrote CrM.
We have rolling friction ##P_w= \gamma v(t)^3## with some constant factor ##\gamma## which you wrote Fw.

Given your formulas are correct, we end up with ##(\alpha + \gamma) \cdot v(t)^3 + \frac{M}{2}\cdot v(t)^2 + \beta \cdot v(t) - E = 0## which is a bit tricky to solve, cp. https://en.wikipedia.org/wiki/Cubic_function#Cardano's_method
It probably will be easier to use one of these:
https://www.physicsforums.com/threa...h-physics-earth-and-other-curiosities.970262/
 
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