Calculating Distance Traveled on a Winding Trajectory From North to South Pole

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SUMMARY

The discussion focuses on calculating the total distance traveled by an airplane flying from the North Pole to the South Pole along a winding trajectory. The trajectory is defined within a sphere of radius R, with the z-coordinate described by z(t) = R - vt and the azimuthal angle by ϕ(t) = ωt. The solution requires transforming the parametrization from time t to the spherical coordinate θ, ultimately leading to the integral form ∫A√(1+B²(sin(θ))ⁿ)dθ, where A, B, and n are constants related to R, v, and ω. Participants express difficulty in manipulating the integral into the specified form.

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  • Spherical coordinates and their applications
  • Understanding of parametric equations in three-dimensional space
  • Basic calculus, particularly integration techniques
  • Familiarity with angular velocity and its implications in motion
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  • Learn about integrating functions in spherical coordinates
  • Explore the concept of angular velocity and its mathematical representation
  • Investigate the derivation of integrals involving square roots and trigonometric functions
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kitsh
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Homework Statement


An airplane flies from the North Pole to the South Pole, following a winding trajectory. Place the center of the Earth at the origin of your coordinate system, and align the south-to-north axis of the Earth with your z axis. The pilot’s trajectory can then be described as follows:
1) The plane’s trajectory is confined to a sphere of radius R centered on the origin.
2) The pilot maintains a constant velocity v in the -z direction, thus the z coordinate can be described as z(t)=R-vt
3) The pilot "winds" around the Earth as she travels south, covering a constant ω radians per second in the azimuthal angle ϕ, thus ϕ(t)=ωt

Calculate the total distance traveled by the pilot. What you will find is that time t is not the best IP with which to parametrize this path. You can start with it, certainly … but then get rid of it in terms of a different choice for your IP: θ, from spherical coordinates

Homework Equations


Spherical coordinates are (r, θ, ϕ)
The Answer should be in the form of ∫A√(1+B^2(sin(θ))^n)dθ where A, B and n are either numerical constants or constants in in the terms of R, v and ω

The Attempt at a Solution


I honestly have no idea how I am supposed to approach this question, it is nothing like anything I have seen in this class or any other
 
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I would start with spherical coordinates. With constant radius, R, x= R cos(\theta)sin(\phi), y= R sin(\theta)sin(\phi), z= R cos(phi). Here we have z= R cos(\phi)= R- vt and \phi= \omega t[/te]x] so z= R cos(\omega t)= R- vt
 
So I converted everything to spherical which helps some and I know the bounds of integration are going to be from 0 to pi and that the integration constant is rdθ but I still can't figure out how to get the integral into the form indicated above.
 
kitsh said:
So I converted everything to spherical which helps some and I know the bounds of integration are going to be from 0 to pi and that the integration constant is rdθ but I still can't figure out how to get the integral into the form indicated above.
Please post your working as far as you get.
 

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