Calculate ellipse area from semi-major and semi-minor axes. Also shows circumference (Ramanujan approximation), eccentricity, foci distance, linear eccentricity, directrix, and flattening.
An ellipse is the set of all points whose distances to two fixed points (foci) sum to a constant. It appears everywhere — in planetary orbits, satellite dishes, architectural arches, and optical lenses. The area of an ellipse is elegantly simple: A = πab, where a is the semi-major axis and b is the semi-minor axis. But an ellipse has many other interesting properties that our Ellipse Area Calculator computes automatically. The eccentricity e = √(1 − b²/a²) measures how elongated the ellipse is — 0 for a perfect circle, approaching 1 for a very stretched shape. The linear eccentricity c = √(a² − b²) gives the distance from the center to each focus, and the foci distance is 2c. The flattening f = 1 − b/a is used in geodesy to describe Earth's shape. We also compute the circumference using Ramanujan's remarkably accurate approximation, the semi-latus rectum, and the directrix distance where applicable. The tool includes a unit selector for flexibility, eight presets for instant exploration, a visual bar chart comparing the axes and related distances, and a reference table of common ellipses with their properties. Whether you are a student learning conic sections, an engineer designing elliptical components, or an astronomer characterizing orbits, this calculator provides comprehensive, immediate results.
This calculator is useful when an ellipse has to be described by more than area alone. In geometry classes, it helps connect the basic formula A = πab to deeper ellipse properties such as eccentricity, foci distance, and semi-latus rectum. In design and engineering work, those same quantities matter when laying out arches, ducts, lenses, tracks, or orbit-style paths where the overall footprint and the shape profile both matter.
It is also helpful because circumference, focus placement, and flattening are easy to miscompute by hand. The calculator keeps those values synchronized with the chosen semi-axes, so you can explore how changing one axis affects not just the area, but the ellipse's elongation and focal geometry as well.
Area = πab. Circumference ≈ π(a+b)(1 + 3h/(10+√(4−3h))) where h = ((a−b)/(a+b))². Eccentricity e = √(1 − b²/a²). Linear eccentricity c = √(a² − b²). Foci distance = 2c. Flattening f = 1 − b/a. Semi-latus rectum ℓ = b²/a.
Result: Area ≈ 157.08 cm², circumference ≈ 48.44 cm, eccentricity ≈ 0.8660
For a = 10, b = 5: Area = π·10·5 = 157.08. h = (5/15)² ≈ 0.1111. Circumference ≈ 48.44. e = √(1 − 25/100) ≈ 0.866. c = √75 ≈ 8.66. Foci distance ≈ 17.32.
The ellipse area formula uses semi-axes, not full diameters. That means the semi-major axis is half the longest width of the ellipse and the semi-minor axis is half the shortest width. This detail matters because doubling or halving the wrong measurement changes the area by a large factor. If you are starting from a full major axis and minor axis, divide both by two before entering them.
Area measures footprint, but eccentricity describes shape. A circle has eccentricity 0 because both semi-axes are equal. As the semi-minor axis becomes smaller relative to the semi-major axis, the ellipse stretches and the eccentricity moves closer to 1. The linear eccentricity and foci distance quantify where the focal points sit, which is important in orbital geometry, reflective optics, and conic-section problems.
Unlike area, ellipse circumference does not have a simple exact elementary formula, which is why calculators often use Ramanujan's approximation. That approximation is highly accurate for practical work and is useful in layout, trim length, and perimeter-style estimates. Flattening is another helpful measure because it expresses how far the ellipse departs from a circle, which is relevant in geodesy and any application where a nearly circular shape must be compared against a more elongated one.
The semi-major axis (a) is half the longest diameter of the ellipse. The semi-minor axis (b) is half the shortest diameter. They are always perpendicular.
The Ramanujan approximation used here is accurate to within about 0.01% for most practical ellipses. There is no closed-form formula for an ellipse circumference.
Eccentricity (e) ranges from 0 to just under 1. Zero means a perfect circle; values close to 1 indicate a very elongated, cigar-like shape.
The foci are two special interior points. The sum of distances from any point on the ellipse to both foci is constant and equals 2a (the major axis).
Simply divide your full axis lengths by 2 before entering. Semi-major = major axis / 2, semi-minor = minor axis / 2.
An ellipse has a precise mathematical definition (constant sum of focal distances). "Oval" is a general term for any egg-like shape, which may or may not be a true ellipse.