A spiral that gives the solution to the central orbit
problem under a radial force law
 |
(1)
|
where
is a positive constant. There are three solution regimes,
 |
(2)
|
where
and
are constants,
and
is the specific angular momentum (Whittaker
1944, p. 83). The case
gives an epispiral,
while
leads to a hyperbolic spiral.
See also
Epispiral,
Hyperbolic
Spiral,
Spiral
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References
Cotes, R. Harmonia Mensurarum. p. 31 and 98, 1722.Danby, J. M. "The Case
--Cotes' Spiral." §4.7 in Fundamentals
of Celestial Mechanics, 2nd ed., rev. ed. Richmond, VA: Willmann-Bell, pp. 69-71,
1988.Symon, K. R. Mechanics,
3rd ed. Reading, MA: Addison-Wesley, p. 154, 1971.Whittaker,
E. T. A
Treatise on the Analytical Dynamics of Particles and Rigid Bodies: With an Introduction
to the Problem of Three Bodies. New York: Dover, p. 83, 1944.Referenced
on Wolfram|Alpha
Cotes' Spiral
Cite this as:
Weisstein, Eric W. "Cotes' Spiral." From
MathWorld--A Wolfram Web Resource. https://mathworld.wolfram.com/CotesSpiral.html
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