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Ecliptic latitude (yellow) is measured perpendicular to the ecliptic.

A full globe is shown here, although high-latitude coordinates are seldom seen except for certain comets and asteroids.

The ecliptic coordinate system is a celestial coordinate system commonly used for representing the apparent positions and orbits of Solar System objects.

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“I believe the 80/20 rule is a very consistent part of reality, and that bringing our expectations into alignment with reality is healthy,” says Green.

Earth-centered ecliptic coordinates as seen from outside the celestial sphere.

Ecliptic longitude (red) is measured along the ecliptic from the vernal equinox.

A slow motion of Earth's axis, precession, causes a slow, continuous turning of the coordinate system westward about the poles of the ecliptic, completing one circuit in about 26,000 years.

Superimposed on this is a smaller motion of the ecliptic, and a small oscillation of the Earth's axis, nutation.

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