Description
Calculate second eccentricity squared from explicit oblate or spherical semiaxes.
Geodesy distinguishes a mathematical reference ellipsoid, a realized coordinate datum and the physical gravity field. Geodetic latitude follows the ellipsoid normal; geocentric latitude follows a radius from the center. Ellipsoidal height, orthometric height and geoid undulation are separate signed quantities. Keep the declared ellipsoid, coordinate axes, angular units and time scale with a result.
Calculate second eccentricity squared from explicit oblate or spherical semiaxes.
When to use this tool
Use this tool when you need to calculate second eccentricity squared from explicit oblate or spherical semiaxes.
How to use the tool and how it works
- Enter semiMajorMeters, semiMinorMeters using the definitions below.
- Run the operation. Resolve input-format errors before interpreting an output.
- Read result.secondEccentricitySquared, using the stated boundary, ordering, sign and absence conventions.
Calculate (a²−b²)/b² from explicit semiaxes, using e²/(1−e²) internally.1
| Input field | Meaning and units | Accepted input |
|---|---|---|
| semiMajorMeters | Equatorial semiaxis a in meters, 1–10⁸. It is a radius, not a diameter. | Finite numeric value satisfying the stated comparisons. |
| semiMinorMeters | Polar semiaxis b in meters, with 0.9a≤b≤a under the explicit-axis model. | Finite numeric value satisfying the stated comparisons. |
| Output field | Interpretation |
|---|---|
| result | Object containing the fields below. |
| result.secondEccentricitySquared | Dimensionless (a²−b²)/b². |
{
"input": {
"semiMajorMeters": 10,
"semiMinorMeters": 9
},
"output": {
"result": {
"secondEccentricitySquared": 0.2345679012345679
}
}
}Limitations and assumptions
- The result is second eccentricity squared, not first eccentricity squared or linear eccentricity. Axes follow the oblate/spherical bounds and use matching meter units.
- All quantities are finite and retain the units stated for this operation. Ellipsoid-parameter tools use semi-major axis 1–10⁸ m and dimensionless flattening 0–0.02; explicit-axis tools use 0.9a≤b≤a unless a tighter bound is stated. These tools do not fetch datums, geoid grids, satellite observations or Earth-orientation updates.
- Every declared outer field is required and unknown outer fields are rejected. Strings and JSON text have size limits, lists are bounded to 128 entries, and JSON nesting/node counts are bounded. Tighter operation-specific bounds stated above take precedence.
- Numeric results must be finite. Large physical magnitudes are allowed by the output evidence checks, while integer fields and source schemas retain their exactness rules. Source indexes are zero-based. Floating-point residues can remain even where an ideal formula gives an exact zero.
Alternative or Complementary methods
Use a coordinate transform for a change of representation and explicit datum parameters for a change of reference frame. Preserve model and convergence metadata, and use observation and datum information appropriate to a real survey before interpreting a computed tolerance as accuracy.
References
Similar or alternative tools
- Third Flattening n Computation Calculator
Calculate dimensionless third flattening from explicit oblate or spherical semiaxes.
- Linear Eccentricity c from a and e Calculator
Calculate linear eccentricity in meters from a semimajor axis and dimensionless first eccentricity.