Axial tilt

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In astronomy, Axial Tilt, known to astronomers as obliquity, is the angle between an object's rotational axis and its orbital axis, or, equivalently, the angle between its equatorial plane and orbital plane.[1] It differs from orbital inclination.

Obliquity

The principal component of the precession of the equinoxes, produced by the gravitational attraction of the sun and the moon on the equatorial bulge of the earth

Lunisolar Precession

"...the appreciation of where our Earth feats in..."

Axial tilt

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