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  2. Eclipse season - Wikipedia

    en.wikipedia.org/wiki/Eclipse_season

    In other words, because the eclipse season (34 days long on average) is longer than the synodic month (one lunation, or the time for the Moon to return to a particular phase and about 29.5 days), the Moon will be new or full at least two, and up to three, times during the season. Eclipse seasons occur slightly shy of six months apart ...

  3. Eclipse cycle - Wikipedia

    en.wikipedia.org/wiki/Eclipse_cycle

    6 eclipse seasons, and a fairly short eclipse cycle. Each eclipse in a hexon series (except the last) is followed by an eclipse whose saros series number is 8 lower, always occurring at the same node. It is equal to 35 synodic months, 1 less than 3 lunar years (36 synodic months). At any given time there are six hexon series active. Hepton

  4. Milankovitch cycles - Wikipedia

    en.wikipedia.org/wiki/Milankovitch_cycles

    Milankovitch emphasized the changes experienced at 65° north due to the great amount of land at that latitude. Land masses change temperature more quickly than oceans, because of the mixing of surface and deep water and the fact that soil has a lower volumetric heat capacity than water. [5]

  5. Did the eclipse path change? New map reveals Hoosiers ... - AOL

    www.aol.com/did-eclipse-path-change-map...

    A rare total solar eclipse will cut a 115-mile-wide path April 8 across North America, but less than a week before it happens, new research suggests fewer Hoosiers could experience the totality ...

  6. It's Eclipse Season (Again) - Here's What You Need to Know - AOL

    www.aol.com/lifestyle/eclipse-season-again-heres...

    Eclipse season starts on March 25 with the lunar eclipse in Libra and ends on April 8, 2024, with the solar eclipse in Aries.

  7. Axial precession - Wikipedia

    en.wikipedia.org/wiki/Axial_precession

    The term "precession" typically refers only to this largest part of the motion; other changes in the alignment of Earth's axis—nutation and polar motion—are much smaller in magnitude. Earth's precession was historically called the precession of the equinoxes , because the equinoxes moved westward along the ecliptic relative to the fixed ...

  8. What is an umbra? A penumbra? Here's some terms to know ... - AOL

    www.aol.com/umbra-penumbra-heres-terms-know...

    The super blood moon lunar eclipse occurred late in the night of Sunday, Jan. 20, 2019, and carried over into early morning Monday. The shadow from Earth, called the penumbra, begins to fall upon ...

  9. Lunar node - Wikipedia

    en.wikipedia.org/wiki/Lunar_node

    So the time from one node crossing to the next (see eclipse season) is approximately a half-year minus half of 19.1 days -- or about 173 days. Because the orbital plane of the Moon precesses in space, the lunar nodes also precess around the ecliptic, completing one revolution (called a draconic period or nodal period ) in 18.612958 years (6,798 ...