What are the correct ways to use polar form in solving integrals?

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The discussion focuses on the correct application of polar coordinates in solving integrals, specifically addressing the transformation of Cartesian equations into polar form. The participants clarify that polar form requires the use of independent variables, represented as x = r cos(θ) and y = r sin(θ), rather than the dependent variables x = a cos(α) and y = a sin(α). They provide detailed examples, including the parametric equations for the astroid curve x²/3 + y²/3 = a²/3 and the equation y² = x²(a² - x²), demonstrating the proper conversion to polar coordinates.

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For the first problem, find the length of the "astroid", x2/3+ y2/3[/sup]= a2/3, you say you wanted to put it in "polar form" and then give x= a cos((\alpha), y= a sin(\alpha). That is NOT "polar form. Polar form would be x= r cos(\alpha), y= r sin(\alpha), where both r and \alpha are independent variables. There is no reason to thing that x= a cos((\alpha), y= a sin(\alpha) satisfy the equation of the curve.

As for the "method" your text uses, you say they let x= a sin3(t), y= a cos3(t). Okay, then x2/3+ y2/3= a2/3sin2(t)+ a2/3cos2(t)= a2/3 so those are parametric equations for the curve. Also, then dx= 3a cos(t)sin(2(t)dt and dy= -3a sin(t)cos2(t) dt so that ds= \sqrt{(dx/dt)^2+ (dy/dt)^2}= \sqrt{9a^2 cos^2(t)sin^3(t)+ 9a^2 sin^2(t) cos^4(t)}dt.

As for the second one, y2= x2(a2- x2, i don't see why you again have "x= a cos\alpha, y= a sin\alpha". Polar coordinates are x= r cos\theta, y= r sin[\theta]. (of course, it doesn't matter whether you use \alpha or \theta. \theta is the standard notation.)

Then y^2= r^2 sin^2(\theta) and x^2= r^2 cos^2(\theta) so your equation becomes r^2 sin^2(\theta)= r^2(a^2- r^2 cos^2(\theta). We can cancel the two r^2 terms and then we have sin^2(\theta)= a^2- r^2 cos^2(\theta) so r^2 cos^2(\theta)= a^2- sin^2(\theta), r^2= a^2 sec^2(\theta)- tan^2(\theta).
 

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