Stretch a circle, get an ellipse
An ellipse is just a circle viewed through an affine stretch. Any circle formula survives the trip if you scale one axis—no rotation needed.
Tip: Give any sensible combo. The solver prefers to deduce a and b first, then computes area and three perimeter values. If inputs conflict, it warns but still shows a best-fit result.
Ellipse perimeter has no simple closed form. We show three values:
An ellipse is defined by its semi-major axis \(a\) and semi-minor axis \(b\). Area is simple: \(A=\pi ab\). Perimeter (circumference) has no elementary formula, so we compute trusted approximations (Ramanujan I & II) and a high-precision series for the complete elliptic integral \(E(k)\) with \(k=e\).
All computation is 100% client-side for privacy.
An ellipse is just a circle viewed through an affine stretch. Any circle formula survives the trip if you scale one axis—no rotation needed.
Sound or light launched from one focus reflects to the other. That’s why whispering galleries and elliptical billiards feel spooky-precise.
Earth’s orbit is an ellipse, but its eccentricity is only ~0.0167. If you drew it to scale, you’d squint to see it isn’t a circle.
Ramanujan’s 1914 approximations nail ellipse perimeter to many decimals without elliptic integrals—handy when you need speed plus surprising accuracy.
Every point on an ellipse keeps PF₁ + PF₂ constant (equal to 2a). It’s the string-and-pins trick behind the classic boardroom-table demo.
Any of: \(a,b\); \(A=2a,B=2b\); area; eccentricity plus one semi-axis. Multiple inputs are OK; we check consistency.
Ellipse perimeter lacks a simple exact formula. Ramanujan II is typically accurate to many decimals; the elliptic-integral series provides high precision.
Axes and perimeter share your length unit; area uses squared units (e.g., cm²).