Cyclostratigraphy — where it appears
Named by 2 essays across one field — each of them below, with the objects they name alongside it.
A rhythm in the rock that measures the Moon
The Earth's axis precesses because the Sun and Moon pull on its equatorial bulge, and two-thirds of the pull is the Moon's. When the Moon was nearer and the day shorter, the axis turned faster, and the climate cycles that precession drives were shorter. Sediments laid down 1.4 billion years ago record those cycles — and with nothing in the rock but layer thicknesses, the ratio of two rhythms gives the Moon's distance at the time.
A Moon measured in banded iron
Layers of iron-rich sediment laid down 2.46 billion years ago in what is now Western Australia keep time with the Earth's precession, and the precession's period says how far away the Moon was: about 321,800 kilometres, with a day of seventeen hours. Together with an older-is-closer point from 1.4 billion years ago, it measures how hard the tides worked between them — about a fifth as hard as today. Held further back, that efficiency brings the Moon out from the Earth a few hundred million years too early, which says the young tides worked harder than the middle-aged ones.
Named alongside it
The objects these essays reach for when they reach for this one.
Angular momentumLength of dayLunar recessionMilankovitch cyclesDynamical ellipticityEarth moon systemObliquityPrecessionPrecession constantPrecession of the equinoxesTidal dissipation