Why does the wobble in Earth's tilt called orbital precession happen?

Orbital precession happens because the Sun and Moon pull on Earth's equatorial bulge, and since Earth is spinning, that pull doesn't straighten it out but instead makes the whole axis sweep slowly in a circle, the way a tilted spinning top wobbles rather than falls over.

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The spinning top you already know

Picture a toy top. When it's perfectly upright it spins fine, but when it leans, gravity pulls on that lean and the top wobbles in a slow circle instead of tipping straight over. Earth does the same thing: as it rotates, it wobbles slightly on its rotational axis, and the cause is tidal forces from the gravitational pull of the Sun and Moon acting on Earth's equatorial bulge.

Here is why the bulge matters. As Earth spins, centrifugal force makes the equator bulge outward, so the planet isn't a perfect sphere but a flattened one, and Earth's axis isn't vertical relative to its orbit but tilted by about 23.5 degrees. The gravitational pull of the Sun and Moon is the "tap" that causes the axis to precess, but gravity alone won't do it: it's specifically the equatorial bulge that gets the gravitational tug, and if Earth were a perfect sphere, there would be no precession at all.

The Sun's gravity pulls on that misaligned bulge, creating a torque by trying to drag it into alignment with the orbital plane; the Moon, orbiting in a plane tipped toward the bulge, yanks on it too; and the combined result is that Earth's axis slowly traces a complete circle once every 26,000 years or so.

The three Milankovitch cycles

Precession is one of three slow orbital rhythms that together are called Milankovitch cycles, named for the Serbian astronomer Milutin Milanković who worked out the mathematics in the early 20th century. The full set includes a 100,000-year cycle in the shape of Earth's orbit (eccentricity), a 41,000-year cycle in the tilt of Earth's axis (obliquity), and a 20,000-year cycle in the wobble of Earth's axis (precession).

  • Eccentricity is how oval versus circular Earth's orbit around the Sun gets, driven mostly by Jupiter and Saturn's gravity.
  • Obliquity is how much the axis itself tilts, varying between about 22 and 24.5 degrees over 41,000 years.
  • Precession is the direction the tilt points, completing its circle in roughly 26,000 years.
Eccentricity: Earth's orbit changes from nearly circular to more oval
Eccentricity: the shape of Earth’s orbit stretches from nearly circular to more oval and back about every 100,000 years, with a longer 405,000-year rhythm. Today it is close to circular. The drawing is exaggerated so you can see the change.
Obliquity: Earth's tilt moves between 22.1 and 24.5 degrees
Obliquity: the tilt of Earth’s axis moves between 22.1° and 24.5° and back over about 41,000 years. Today it is 23.44°. More tilt means hotter summers and colder winters.
Precession: Earth's axis traces a circle every 26,000 years
Precession: like a spinning top, Earth’s axis slowly traces a circle, once about every 26,000 years. Today it points at Polaris. In about 12,000 years it will point near Vega. This shifts which season falls when Earth is closest to the Sun.

Why precession turned the Sahara green

This is the direct connection to the Green Sahara you've been reading about. The precession of the equinoxes is regarded as the most important orbital parameter in the formation of the "green Sahara" and "desert Sahara" cycle.

Here's the chain of cause and effect. Precession controls which season Earth is closest to the Sun. When precession moved the Northern Hemisphere closer to the Sun during the summer months, it caused warmer Northern Hemisphere summers, warmer air capable of holding more moisture, intensifying the West African Monsoon and shifting the African rainbelt northward into what is now the Sahara.

Since precession controls summer insolation over North Africa, it effectively controls the amount and northward penetration of the monsoonal rains. Roughly 11,000 years ago, Earth's axis was pointed such that the Northern Hemisphere summer coincided with perihelion, the closest point to the Sun. The precession cycle varies on a 21,000-year timescale, and the similarity between this cycle and the timing of the African Humid Periods indicates that precession is their dominant driver, because precession influences seasonal contrasts, increasing them in one hemisphere while reducing them in the other.

Today the axis has wobbled far enough that Northern Hemisphere summer happens when Earth is farther from the Sun, the monsoon is weaker, and the Sahara is dry. Give it another 10,000 years and the axis will have swung back around. The Sahara has greened and dried hundreds of times before this last one, all paced by the same slow wobble.

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This follows on from
When was the African Humid period?

The African Humid Period ran from roughly 14,800 to 5,500 years ago, turning the Sahara green for nearly 9,000 years before it dried back out.

Read that one first

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