Mutual Event Inclination Band

Screen circular mutual-event geometry against the sum-of-radii projected inclination band; orbital phase is not inferred.

Description

A circular mutual event requires projected inclination close enough to edge-on for the bodies' apparent disks to overlap.

A circular mutual event requires projected inclination close enough to edge-on for the bodies' apparent disks to overlap. This geometric band depends on their summed radii relative to separation.1

Screen circular mutual-event geometry against the sum-of-radii projected inclination band; orbital phase is not inferred.

When to use Mutual Event Inclination Band

Use this tool to screen circular mutual-event geometry against the sum-of-radii projected inclination band; orbital phase is not inferred.

Prepare the orbital state or model parameters in one reference frame. Confirm compatible distance/time units and the stated angular and gravitational-parameter conventions.

How to use Mutual Event Inclination Band and understand its results

  1. Prepare the orbital state or model parameters in one reference frame. Confirm compatible distance/time units and the stated angular and gravitational-parameter conventions.
  2. Enter firstRadius, secondRadius, separation, viewingOffsetDegrees using the field table and calculation rules, then run the tool.
  3. Read maximumOffsetDegrees, eventGeometryPossible. The explanation below defines the units, signs, ordering and any flags or placeholder values.
  4. If the tool reports an input issue, correct the values and run it again. Apply the stated assumptions when interpreting a successfully returned result.
Input fieldMeaningValue type; see rules belowRequirement
firstRadiusFirst radiusnumberRequired
secondRadiusSecond radiusnumberRequired
separationSeparationnumberRequired
viewingOffsetDegreesViewing offset degreesnumberRequired

Enter nonnegative radii, positive separation at least their sum, and a signed viewing offset within ±90 degrees. The tool returns the maximum offset and tests absolute viewing offset inclusively against it. Zero total radius gives a zero-width band.

maximumOffset = asin[(radius1+radius2)/separation] in degrees

Units, indexing, boundary conditions and exceptional cases are defined in the calculation rules above.

Output fieldMeaningValue type
maximumOffsetDegreesMaximum offset degreesnumber
eventGeometryPossibleEvent geometry possibleboolean
json
{
  "input": {
    "firstRadius": 1,
    "secondRadius": 1,
    "separation": 10,
    "viewingOffsetDegrees": 10
  },
  "output": {
    "maximumOffsetDegrees": 11.536959032815489,
    "eventGeometryPossible": true
  }
}

Limitations and assumptions

This does not determine orbital phase, event timing, brightness or actual visibility. Spherical bodies and the supplied circular geometry are assumptions, and all lengths must share a unit.

Numeric inputs must be finite. Follow the calculation-specific rules for overflow, underflow and exceptional cases. Missing required fields, extra fields, wrong value types and violations of the calculation rules are input errors. A successfully returned false flag is an evaluated outcome; its meaning is explained above.

Alternative or Complementary methods

Use Planetary Phase Triangle Angle: Solve the Sun–planet–observer phase angle from simultaneous triangle side lengths in any common distance unit. For a complementary task, use Ellipse From Apsis Radii: Recover ellipse shape parameters from ordered center-referenced periapsis and apoapsis radii, not surface altitudes.

References

  1. Mutual Event Inclination Band — tool.io

Similar or alternative tools

  • Planetary Phase Triangle Angle

    Solve the Sun–planet–observer phase angle from simultaneous triangle side lengths in any common distance unit.

  • Ellipse From Apsis Radii

    Recover ellipse shape parameters from ordered center-referenced periapsis and apoapsis radii, not surface altitudes.

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