Four Term Nutation Components
Evaluate a four-term low-precision nutation approximation from supplied mean angles; not an IAU 2000/2006 implementation.
Description
Nutation adds short-period variations to longitude and obliquity.
Nutation adds short-period variations to longitude and obliquity. A four-term approximation gives a low-precision correction from supplied mean angular arguments rather than a full modern standard series.1
Evaluate a four-term low-precision nutation approximation from supplied mean angles; not an IAU 2000/2006 implementation.
When to use Four Term Nutation Components
Use this tool to evaluate a four-term low-precision nutation approximation from supplied mean angles; not an IAU 2000/2006 implementation.
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 Four Term Nutation Components 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 nodeLongitudeDegrees, sunMeanLongitudeDegrees, moonMeanLongitudeDegrees using the field table and calculation rules, then run the tool.
- Read longitudeNutationArcseconds, obliquityNutationArcseconds. 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 |
|---|---|---|---|
| nodeLongitudeDegrees | Node longitude degrees | number | Required |
| sunMeanLongitudeDegrees | Sun mean longitude degrees | number | Required |
| moonMeanLongitudeDegrees | Moon mean longitude degrees | number | Required |
Enter finite node longitude and Sun/Moon mean longitudes in degrees. The tool converts them to radians, evaluates the sine/cosine sums and returns longitude and obliquity nutation in arcseconds.
Δψ=−17.2sinΩ−1.32sin2L−0.23sin2l+0.21sin2Ω; Δε=9.2cosΩ+0.57cos2L+0.1cos2l−0.09cos2Ω Units, indexing, boundary conditions and exceptional cases are defined in the calculation rules above.
| Output field | Meaning | Value type |
|---|---|---|
| longitudeNutationArcseconds | Longitude nutation arcseconds | number |
| obliquityNutationArcseconds | Obliquity nutation arcseconds | number |
{
"input": {
"nodeLongitudeDegrees": 90,
"sunMeanLongitudeDegrees": 0,
"moonMeanLongitudeDegrees": 0
},
"output": {
"longitudeNutationArcseconds": -17.2,
"obliquityNutationArcseconds": 0.7600000000000005
}
} Limitations and assumptions
It does not calculate mean arguments from time or implement IAU 2000/2006 nutation. Frame bias, precession, apparent coordinate corrections and accuracy estimates are not included.
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 Laskar Mean Obliquity: Evaluate the Laskar long-term mean-obliquity polynomial within ±10000 years of J2000; nutation and reference-frame realization are separate. For a complementary task, use Iau1976 Epoch Precession: Precess a mean equatorial direction with the bounded IAU 1976 approximation; proper motion, nutation and modern frame bias are not included.
References
-
Four Term Nutation Components — tool.io
Similar or alternative tools
- Laskar Mean Obliquity
Evaluate the Laskar long-term mean-obliquity polynomial within ±10000 years of J2000; nutation and reference-frame realization are separate.
- Iau1976 Epoch Precession
Precess a mean equatorial direction with the bounded IAU 1976 approximation; proper motion, nutation and modern frame bias are not included.