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Other Cycles of the Earth and of the Moon

Sideric day | Moon culmination | Sideric moon | Metonic Cycle
Saros period | Moon knot | Apsidis rotation



The Sideric Day of the Earth

Tone     194.71 Hz = G (a1 = 437.1 Hz / 440 Hz - 11.4 cent)

Tempo  91.3 bpm

Color     red-orange

Explanation Duration of the true revolution of earth around its axis.The sideric day is about 4 minutes shorter than the average calender day.

      tone sample MP3


Moon-culmination

Tone     187.61 Hz = F# (a1 = 446.2 Hz / 440 Hz + 24.2 cent)

Tempo  87.9 bpm

Color    red

Explanation  The time span for one passage of the moon from one south to the next one. Every day, the moon rises about 50 minutes later than the preceding day. The delay adds up to one day during a (tropical) month.

    tone sample MP3


The Sideric Moon

Tone     227.43 Hz = A# (a1 = 429.3 Hz / 440 Hz - 42.5 cent)

Tempo  106.6 bpm

Color    yellow (yellow)

Explanation  The time span for one revolution of the moon around the earth, as measured against the celestial sphere. The sideric month is about two and a quarter days shorter than a synodic month.This is caused by the apparent course of the sun along the ecliptic. As the sun passes approximately one sign per month, the moon has to pass through 13 signs to "keep up with it".

    tone sample MP3


Moon: Metonic cycle

Tone     229.22 Hz = A# (a1 = 432.7 Hz / 440 Hz - 28.9 cent)

Tempo  107.45 bpm

Color    yellow (yellow)

Explanation  The time span of about 19 year, after which the sun and the moon have the same aspects on the same day. The metonic cycle is the basis of combined soli-lunar calendars.

    tone sample MP3


Moon: Saros Period

Tone     241.56 Hz = B (a1 = 430.4 Hz / 440 Hz - 38.2 cent)

Tempo  113.2 bpm

Color    yellow-green

Explanation  The time span of approximately 18 years and 10 days, after which eclipses of the same type repeat themselves.

    tone sample MP3


Moon: Apsidis rotation

Tone     246.04 Hz = B (a1 = 438.4 Hz / 440 Hz - 6.3 cent)

Tempo  115.3 bpm

Color    yellow-green

Explanation  The duration of the movement of one axis of the elliptical orbit of the moon around the ecliptic. The two extreme points of the bigger axis are called perigee (the point where the moon is closest to the earth) and apogee (the point where the moon is most distant from the earth). One such revolution takes about 8.85 years.

    tone sample MP3


Moon knot

Tone     234.16 Hz = A# (a1 = 442 Hz / 440 Hz + 8 cent)

Tempo  109.8 bpm

Color    yellow (yellow)

Explanation  The duration of the path of the nodes along the ecliptic, about 18,6 years. The nodes are the intersection of the orbit of the moon with the ecliptic. If the moon moves along the ecliptic from South to North, it crosses the North node, which is also called the "head of the dragon". If it moves from North to South, it crosses the South node, which is also called the "tail of the dragon".

    tone sample MP3



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