Moving Cluster Distance
Solve a moving-cluster distance from radial velocity and proper motion toward the convergent point; coherent bulk motion and negligible expansion are assumed.
Description
The moving-cluster method uses coherent bulk motion toward a convergent point to relate radial velocity and aligned proper motion to distance.
The moving-cluster method uses coherent bulk motion toward a convergent point to relate radial velocity and aligned proper motion to distance. Expansion or unrelated motion can violate that geometry.1
Solve a moving-cluster distance from radial velocity and proper motion toward the convergent point; coherent bulk motion and negligible expansion are assumed.
When to use Moving Cluster Distance
Use this tool to solve a moving-cluster distance from radial velocity and proper motion toward the convergent point; coherent bulk motion and negligible expansion are assumed.
Prepare the source, detector or coordinate measurements. Confirm frame, epoch, angular units, axis directions and the stated RA proper-motion convention before entering values.
How to use Moving Cluster Distance and understand its results
- Prepare the source, detector or coordinate measurements. Confirm frame, epoch, angular units, axis directions and the stated RA proper-motion convention before entering values.
- Enter radialKmPerSecond, convergentAngleDegrees, alignedProperMotionArcsecPerYear using the field table and calculation rules, then run the tool.
- Read clusterDistanceParsecs. 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 |
|---|---|---|---|
| radialKmPerSecond | Radial km per second | number | Required |
| convergentAngleDegrees | Convergent angle degrees | number | Required |
| alignedProperMotionArcsecPerYear | Aligned proper motion arcsec per year | number | Required |
Enter positive aligned proper motion, signed radial velocity and convergent angle within (0,180) degrees, excluding angles within 10⁻⁸ degree of 90. The formula must yield a positive finite distance; inconsistent signs are errors. Return parsecs.
distancePc=radialKmPerSecond tan(convergentAngle)/(4.74047 alignedMotionArcsecPerYear) Units, indexing, boundary conditions and exceptional cases are defined in the calculation rules above.
| Output field | Meaning | Value type |
|---|---|---|
| clusterDistanceParsecs | Cluster distance parsecs | number |
{
"input": {
"radialKmPerSecond": 1,
"convergentAngleDegrees": 45,
"alignedProperMotionArcsecPerYear": 1
},
"output": {
"clusterDistanceParsecs": 0.2109495471967969
}
} Limitations and assumptions
It does not establish cluster membership or derive the apex. Internal velocity dispersion, expansion, projection errors and uncertainty are omitted; only the motion component toward the apex belongs in the denominator.
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.
Alternative or Complementary methods
Use Convergent Point Motion Alignment: Compare a measured tangent-plane proper-motion direction with the great-circle direction to a supplied cluster apex; alignment does not establish membership. For a complementary task, use Homologous Cluster Expansion Age: Estimate a homologous ballistic expansion age from radius and outward speed; gravity, acceleration, projection and initial size are excluded.
References
-
Moving Cluster Distance — tool.io
Similar or alternative tools
- Convergent Point Motion Alignment
Compare a measured tangent-plane proper-motion direction with the great-circle direction to a supplied cluster apex; alignment does not establish membership.
- Homologous Cluster Expansion Age
Estimate a homologous ballistic expansion age from radius and outward speed; gravity, acceleration, projection and initial size are excluded.