Moon Apparent Size Perigee/Apogee Arcmin

ExactSPHERICALlimb2asin(R/d)Moonangularsizeactualperigee/apogeedistances,not disk2atanor observedpercentageincrease. Actual independent model/unit/frame/epoch/calibration and applicable measurement established;not precise ephemeris,forecast,geodesy operation,identity or safety approval.

Description

A spherical Moon’s apparent limb diameter grows when its center is closer to the observer.

A spherical Moon’s apparent limb diameter grows when its center is closer to the observer.1

This calculator uses a supplied lunar radius and two center distances in kilometers to compare perigee and apogee angles.

When to use Moon Apparent Size Perigee/Apogee Arcmin

Use this tool to apply the stated moon apparent size perigee/apogee arcmin operation with an explicit input and unit basis.

How to use Moon Apparent Size Perigee/Apogee Arcmin and how it works

  1. Establish the measurement basis and units described above.
  2. Enter actualLunarRadiusKm, callerActualPerigeeDistanceKm, callerActualApogeeDistanceKm and run the tool.
  3. Read result.perigeeAngularDiameterArcminutes, result.apogeeAngularDiameterArcminutes using the output meanings below.
  4. If input is rejected, correct the stated type, range, ordering or alignment issue and rerun; review successful results under the declared convention.
Input fieldMeaningValue typeRequirement
actualLunarRadiusKmLunar Radius Km. Units, ordering and applicable branch are specified in the algorithm.numberrequired; finite; strictly positive; further conditions in the algorithm
callerActualPerigeeDistanceKmPerigee Distance Km. Units, ordering and applicable branch are specified in the algorithm.numberrequired; finite; strictly positive; further conditions in the algorithm
callerActualApogeeDistanceKmApogee Distance Km. Units, ordering and applicable branch are specified in the algorithm.numberrequired; finite; strictly positive; further conditions in the algorithm

Require positive radius, perigee distance greater than the radius and apogee distance at least perigee distance. Apply twice arcsin(radius/distance) at each distance and convert radians to arcminutes; no orbital distances are fetched.

angularDiameterArcmin = 2asin(radius/distance) × 180/π × 60

Apply the declared units, ordering and branch conditions.

Output fieldMeaningValue type
resultObject containing the declared output fields.object
result.perigeeAngularDiameterArcminutesSpherical-limb angular diameter at the supplied closer distance, in arcminutes.number
result.apogeeAngularDiameterArcminutesSpherical-limb angular diameter at the supplied farther distance, in arcminutes.number
json
{
  "input": {
    "actualLunarRadiusKm": 1,
    "callerActualPerigeeDistanceKm": 2,
    "callerActualApogeeDistanceKm": 4
  },
  "output": {
    "result": {
      "perigeeAngularDiameterArcminutes": 3600.0000000000005,
      "apogeeAngularDiameterArcminutes": 1737.3014623115907
    }
  }
}

Limitations and assumptions

The output applies the declared operation to the values you supply. Establish the measurement basis, units, coefficients and any caller-selected rules before interpreting it. The tool does not independently collect or verify observations or decide whether a model or reference applies.

Supply explicit required fields with the documented types and dense aligned arrays. Unknown fields, wrong types and nonfinite numbers are rejected. Branch-specific constraints are explained above. A returned boolean, signed difference or tied result follows the stated convention; an input error instead means the required input contract was not satisfied. Very large inputs or outputs may be rejected by shared resource limits.

Alternative or Complementary methods

For a related operation, use Moon Phase Approximation Calculator. A mean synodic lunar cycle is a simple repeating phase clock.

For a related operation, use Golden Hour Duration By Latitude Lookup. Golden-hour definitions vary by photographic convention.

References

  1. Moon Apparent Size Perigee/Apogee Arcmin — tool.io

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