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Ellipse Calculator

Compute the 2D area, Ramanujan perimeter approximation, linear eccentricity (focal distance), orbital eccentricity, and semi-latus rectum of an ellipse.

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Interactive Ellipse Calculator Workspace

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Ellipse Calculation: Compute exact 2D area, Ramanujan perimeter approximation, focal distance (foci), orbital eccentricity, semi-latus rectum, and geometric flattening.
Distance from center along longest horizontal radius.
Distance from center along shortest vertical radius.

Ellipse Properties

Area (A)125.6637
Circumference (C)41.3863
Eccentricity (e)0.7806
Focal Distance (c)6.2450
Semi-Latus Rectum3.1250
Flattening (f)37.50%

Analytical Formula Breakdown

1. Area: Area = π × a × b = π × 8 × 5 = 125.6637

2. Ramanujan Circumference: C ≈ 41.3863 (accurate to within 0.0001% without needing elliptic integrals)

3. Focal Points (Foci): Located at distance c = √(a² - b²) = √(64.00 - 25.00) = 6.2450 on either side of center.

4. Eccentricity: Measures elongation e = c / a = 0.7806 (e = 0 is a circle, e → 1 is an elongated ellipse).

Mathematical Formula & Variables

Equation ModelArea = π × a × b, Perimeter ≈ π × (a+b) × [1 + 3h/(10 + √(4 - 3h))]

Determines geometric metrics for planar curves where the sum of distances from any point on the boundary to two fixed foci is constant.

Variable Definitions

SymbolDescription
a (Semi-Major Axis)Half the length of the widest horizontal diameter.
b (Semi-Minor Axis)Half the length of the shortest vertical diameter.
c (Focal Distance)Distance from the center to each focal point: c = √(a² - b²).
e (Eccentricity)Ratio of focal distance to semi-major axis (e = c/a, where 0 ≤ e < 1).

How to Use the Ellipse Calculator

  • Enter the Semi-Major Axis (a) representing the longer radius from the center.
  • Enter the Semi-Minor Axis (b) representing the shorter radius from the center.
  • Check the real-time Area output (exact: π × a × b).
  • Review the high-precision Ramanujan circumference approximation, focal distance, and eccentricity ratio.

Practical Example Calculation

Scenario Context: An astronomer is modeling a planetary elliptical orbit with a semi-major axis of 10 AU and a semi-minor axis of 8 AU.

Step 1: Identify given axes: Semi-major axis a = 10, Semi-minor axis b = 8.
Step 2: Calculate Area: A = π × a × b = π × 10 × 8 = 80 × π ≈ 251.33 square AU.
Step 3: Calculate Focal Distance (c): c = √(a² - b²) = √(100 - 64) = √36 = 6 AU.
Step 4: Calculate Eccentricity (e): e = c / a = 6 / 10 = 0.60.
Step 5: Calculate Ramanujan Circumference: C ≈ π × [3(18) - √(38 × 34)] ≈ π × [54 - 35.944] ≈ 56.72 AU.
Step 6: Calculate Semi-Latus Rectum (l): l = b² / a = 64 / 10 = 6.4 AU.
The orbit encloses an area of 251.33 AU², has a perimeter of 56.72 AU, an eccentricity of 0.60, and foci located 6 AU from center.

Frequently Asked Questions

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