Trying to grok the draconic year

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SUMMARY

The draconic year, also known as the eclipse year, is defined as the time taken for the Sun to complete one revolution concerning the same lunar node, averaging 346.620075883 days. Eclipses occur when the Sun and Moon are near these nodes, leading to two eclipse seasons within each draconic year. The relationship between the draconic year and the sidereal year can be expressed through the formula Td = 1/(1/Te + 1/Tm), where Te represents the Earth's sidereal period of 365.256 days and Tm denotes the Moon's sidereal orbital precession. Understanding this relationship is crucial for interpreting lunar and solar eclipse cycles.

PREREQUISITES
  • Understanding of lunar nodes and their significance in eclipse cycles
  • Familiarity with the concepts of sidereal and tropical years
  • Basic knowledge of orbital mechanics and precession
  • Mathematical skills to apply the formula for calculating the draconic year
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  • Research the mathematical derivation of the draconic year formula
  • Study the relationship between lunar nodes and eclipse prediction
  • Explore the differences between sidereal and tropical years in detail
  • Investigate the implications of lunar precession on long-term astronomical events
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Astronomers, astrophysicists, and students of celestial mechanics who are interested in understanding eclipse cycles and the dynamics of the Moon's orbit.

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From Wikipedia:
The draconic year, draconitic year, eclipse year, or ecliptic year is the time taken for the Sun (as seen from the Earth) to complete one revolution with respect to the same lunar node (a point where the Moon's orbit intersects the ecliptic). The year is associated with eclipses: these occur only when both the Sun and the Moon are near these nodes; so eclipses occur within about a month of every half eclipse year. Hence there are two eclipse seasons every eclipse year. The average duration of the eclipse year is

346.620075883 days (346 d 14 h 52 min 54 s) (at the epoch J2000.0).

So should this be interpreted as the axis of the sidereal lunar plane precessing at a rate of 346.62/366.25 of a revolution per sidereal year (i.e., the ratio of the draconic & sidereal years) about the axis of the ecliptic?
 
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It takes ~6798 days for the Moon's orbital plane to complete a 360 day precession.
To get the 346 day draconic year, you need to use the formula:
Td = 1/(1/Te+1/Tm)*
where Te is the period of the Earth's orbit. (to be exact, the sidereal period of 365.256... days vs the Tropical year* of 265.242... days)
And Tm is the period of the Moon sidereal orbital precession.

* It is +1/Tm due to the direction the orbit precesses. If the orbit had precessed in the opposite direction, you would have needed to use -1/Tm instead.
** The Tropical year is what our calendar strives to keep in sync with.
 
365.242
 

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