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org.soulspace.astronomy.nutation


argument-of-latitude-moonclj/s

(argument-of-latitude-moon t)

Calculates the argument of latitude for the moon in degrees at the given instant 't' in julian centuries.

Calculates the argument of latitude for the moon in degrees at the
given instant 't' in julian centuries.
sourceraw docstring

longitude-ascending-node-moonclj/s

(longitude-ascending-node-moon t)

Calculates the longitude of ascending node of the moons mean orbit on the ecliptic in degrees at the given instant 't' in julian centuries, measured from the mean equinox of the date.

Calculates the longitude of ascending node of the moons mean orbit on the
ecliptic in degrees at the given instant 't' in julian centuries, measured
from the mean equinox of the date.
sourceraw docstring

mean-anomaly-moonclj/s

(mean-anomaly-moon t)

Calculates the mean anomaly of the moon in degrees at the given instant 't' in julian centuries.

Calculates the mean anomaly of the moon in degrees at the given
instant 't' in julian centuries.
sourceraw docstring

mean-anomaly-sunclj/s

(mean-anomaly-sun t)

Calculates the mean anomaly of the sun in degrees at the given instant 't' in julian centuries.

Calculates the mean anomaly of the sun in degrees at the given
instant 't' in julian centuries.
sourceraw docstring

mean-elongation-moon-from-sunclj/s

(mean-elongation-moon-from-sun t)

Calculates the mean elongation of the moon from the sun in degrees at the given instant 't' in julian centuries.

Calculates the mean elongation of the moon from the sun in degrees
at the given instant 't' in julian centuries.
sourceraw docstring

mean-longitude-moonclj/s

(mean-longitude-moon t)

Calculates the mean longitude of the moon in degrees at the given 't' instant in julian centuries.

Calculates the mean longitude of the moon in degrees at the given
't' instant in julian centuries.
sourceraw docstring

mean-longitude-sunclj/s

(mean-longitude-sun t)

Calculates the mean longitude of the sun in degrees at the given instant 't' in julian centuries.

Calculates the mean longitude of the sun in degrees at the given
instant 't' in julian centuries.
sourceraw docstring

mean-obliquityclj/s

(mean-obliquity jde)

Calculates the mean obliquity of the ecliptic (the inclination of the earth's axis) for the julian ephemerides day. The error is about 1 arc second over a period of 2000 years and 10 arc seconds over a period of 4000 years.

Calculates the mean obliquity of the ecliptic (the inclination of the
earth's axis) for the julian ephemerides day. The error is about
1 arc second over a period of 2000 years and 10 arc seconds over a
period of 4000 years.
sourceraw docstring

mean-obliquity-high-accuracyclj/s

(mean-obliquity-high-accuracy jde)

Calculates the mean obliquity of the ecliptic (the inclination of the earth's axis) for the julian ephemerides day with high accuracy. The error is about 0.01 arc second over a period of 2000 years and a few arc seconds over a period of 20000 years.

Calculates the mean obliquity of the ecliptic (the inclination of the
earth's axis) for the julian ephemerides day with high accuracy.
The error is about 0.01 arc second over a period of 2000 years and
a few arc seconds over a period of 20000 years.
sourceraw docstring

nutation-in-longitudeclj/s

(nutation-in-longitude jde)

Calculates the nutation in longitude (delta psi) in arc seconds for the julian ephemerides day with an accuracy of 0.5 arc seconds.

Calculates the nutation in longitude (delta psi) in arc seconds for the
julian ephemerides day with an accuracy of 0.5 arc seconds. 
sourceraw docstring

nutation-in-obliquityclj/s

(nutation-in-obliquity jde)

Calculates the nutation in obliquity (delta epsilon) in arc seconds for the julian ephemerides day with an accuracy of 0.1 arc seconds.

Calculates the nutation in obliquity (delta epsilon) in arc seconds for the
julian ephemerides day with an accuracy of 0.1 arc seconds.
sourceraw docstring

obliquity_B1950clj/s

source

obliquity_J2000clj/s

source

true-obliquityclj/s

(true-obliquity jde)

Calculates the true obliquity of the ecliptic (the inclination of the earth's axis) for the julian ephemerides day. The error is about 1 arc second over a period of 2000 years and 10 arc seconds over a period of 4000 years.

Calculates the true obliquity of the ecliptic (the inclination of the
earth's axis) for the julian ephemerides day. The error is about
1 arc second over a period of 2000 years and 10 arc seconds over a
period of 4000 years.
sourceraw docstring

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