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  2. Lunar precession - Wikipedia

    en.wikipedia.org/wiki/Lunar_precession

    As a result of this nodal precession, the time for the Sun to return to the same lunar node, the eclipse year, is about 18.6377 days shorter than a sidereal year. The number of solar orbits (years) during one lunar nodal precession period equals the period of orbit (one year [ specify ] ) divided by this difference, minus one: ⁠ 365.2422 / 18 ...

  3. Lunar standstill - Wikipedia

    en.wikipedia.org/wiki/Lunar_standstill

    The lunar standstill phenomenon was probably known from Megalithic times. In high latitudes, there was a period within the 18.6 years cycle, when the Moon became circumpolar. [4] It would have drawn the attention of locals. In other latitudes, the major lunar standstill featured constant scene illumination during the full Moon.

  4. Lunar node - Wikipedia

    en.wikipedia.org/wiki/Lunar_node

    The 19-year recording period is the nearest full-year count to the 18.6-year cycle of the lunar nodes. [9] In conjunction with sea level rise caused by global warming, lunar nodal precession is predicted to contribute to a rapid rise in the frequency of coastal flooding throughout the 2030s. [10]

  5. List of lunar eclipses in the 21st century - Wikipedia

    en.wikipedia.org/wiki/List_of_lunar_eclipses_in...

    There will be 230 lunar eclipses in the 21st century (2001–2100): 87 penumbral, 58 partial and 85 total. [1] Eclipses are listed in sets by lunar years, repeating every 12 months for each node. Ascending node eclipses are given a red background highlight.

  6. Louise McWhirter - Wikipedia

    en.wikipedia.org/wiki/Louise_McWhirter

    It is timetable with alternating 18- and 19-year cycle, which mimics the Nodal cycle very closely. Like McWhirter's theory, Gann also found that the stock market follows a rhythm of 18–19 years. [27] Here is a modernised example of the table:

  7. List of 19th-century lunar eclipses - Wikipedia

    en.wikipedia.org/wiki/List_of_19th-century_lunar...

    Date Time UT (hr:mn) Type Node Saros Gamma Magnitude Duration (min) Moon position Contacts UT (hr:mn) Greatest Pen. Umb. Par Tot RA Decl. U1 U2 U3 U4 (Three eclipses are added before 1801 to complete the first cycle.)

  8. Lunar month - Wikipedia

    en.wikipedia.org/wiki/Lunar_month

    In lunar calendars, a lunar month is the time between two successive syzygies of the same type: new moons or full moons. The precise definition varies, especially for the beginning of the month. Animation of the Moon as it cycles through its phases, as seen from the Northern Hemisphere. The apparent wobbling of the Moon is known as libration.

  9. Chart datum - Wikipedia

    en.wikipedia.org/wiki/Chart_datum

    The 19-year recording period is the nearest full year count to the 18.6-year cycle of the lunar node regression, which has an effect on tides. [ 10 ] Lower low water large tide