Triangular Lagrange Linear Stability
Evaluate the Routh criterion μ(1−μ)<1/27 for linear L4/L5 stability in the planar circular restricted model.
Description
The triangular L4 and L5 points of the planar circular restricted three-body model have a linear stability condition depending on the smaller primary's share of the total mass.
The triangular L4 and L5 points of the planar circular restricted three-body model have a linear stability condition depending on the smaller primary's share of the total mass. The condition describes perturbations within that idealized model.1
Evaluate the Routh criterion μ(1−μ)<1/27 for linear L4/L5 stability in the planar circular restricted model.
When to use Triangular Lagrange Linear Stability
Use this tool to evaluate the Routh criterion μ(1−μ)<1/27 for linear L4/L5 stability in the planar circular restricted model.
Prepare the orbital state or model parameters in one reference frame. Use compatible distance/time units and the stated angular and gravitational-parameter conventions.
How to use Triangular Lagrange Linear Stability and understand its results
- Prepare the orbital state or model parameters in one reference frame. Use compatible distance/time units and the stated angular and gravitational-parameter conventions.
- Enter smallerMassFraction using the field table and calculation rules, then run the tool.
- Read routhProduct, criticalSmallerMassFraction, linearlyStable. The explanation below defines the units, signs, ordering and any flags or placeholder values.
- 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 field | Meaning | Value type; see rules below | Requirement |
|---|---|---|---|
| smallerMassFraction | Smaller mass fraction | number | Required |
Enter smallerMassFraction as the smaller primary's mass divided by both primary masses combined, strictly above 0 and at most 0.5. The tool calculates the product, the critical fraction and the strict comparison. Equality at the product threshold is not flagged linearlyStable; the output is dimensionless.
routhProduct = μ(1−μ); linearlyStable = routhProduct < 1/27; critical μ = (1−√(23/27))/2 Units, indexing, boundary conditions and exceptional cases are defined in the calculation rules above.
| Output field | Meaning | Value type |
|---|---|---|
| routhProduct | Routh product | number |
| criticalSmallerMassFraction | Critical smaller mass fraction | number |
| linearlyStable | Linearly stable | boolean |
{
"input": {
"smallerMassFraction": 0.01
},
"output": {
"routhProduct": 0.0099,
"criticalSmallerMassFraction": 0.03852089650455137,
"linearlyStable": true
}
} Limitations and assumptions
This does not solve a trajectory, assess nonlinear stability or include eccentric primary orbits and other perturbations. A stable flag is conditional on the planar circular restricted assumptions, not a guarantee of a real object's long-term retention.
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 Tisserand Orbital Parameter: Compute a circular restricted-three-body Tisserand parameter in the supplied planet frame; no universal comet taxonomy cutoff is embedded. For a complementary task, use Soi Handoff Hysteresis: Apply caller-defined sphere-of-influence handoff hysteresis to a sampled trajectory; boundaries are not universal force-dominance limits.
References
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Triangular Lagrange Linear Stability — tool.io
Similar or alternative tools
- Tisserand Orbital Parameter
Compute a circular restricted-three-body Tisserand parameter in the supplied planet frame; no universal comet taxonomy cutoff is embedded.
- Soi Handoff Hysteresis
Apply caller-defined sphere-of-influence handoff hysteresis to a sampled trajectory; boundaries are not universal force-dominance limits.