Earth's rotation is not a perfect metronome

Earth's spin feels like the most dependable rhythm in nature, but it is not perfectly steady. Scientists have been logging small shifts in the length of a day for decades, and those changes can be as slight as a few milliseconds. Most people would never notice them, yet researchers care deeply because the measurements point to something much larger than a flickering clock: the speed of the planet's rotation is changing.

Several overlapping causes are already known. Shifts in the atmosphere and oceans can nudge rotation faster or slower. Large earthquakes can move mass around the planet. Melting continental ice adds enormous volumes of water to the oceans, another process that can redistribute weight. Those factors help explain some of the more abrupt and recent changes, but they do not account for all of the variation seen over multi-decade spans.

Looking deeper than the mantle

Some of that unexplained variation appears to come from far below the surface. Under Earth's rocky mantle sits the outer core, a layer roughly 1,400 miles thick made of extremely hot liquid metal that is always moving. When those flows change, they can subtly alter how fast the rest of the planet turns.

The difficulty has been explaining how that influence travels from one layer to another. Friction between the core and the mantle is too weak to do the job alone, so geologists have been looking for other mechanisms inside the planet. A new study published this week in Nature suggests they may have found one of those hidden connections.

A contest between gravity and resistance

The researchers propose that gravity from the inner core pulls rotation in one direction while other interactions between the core and mantle push back. Over decades, that competition could produce small accelerations and decelerations in Earth's spin. The idea depends on the fact that the inner core does not rotate at the same rate as the rest of the planet, leaving it slightly out of alignment with certain mass irregularities in the mantle.

Gravity, however, works to restore balance. Mathieu Dumberry, a geophysicist at the University of Alberta who was involved in the study, said in a press release that the core essentially wants to be aligned. In other words, gravity tries to pull the layers of Earth's interior back toward a more harmonious arrangement. That tug, however slight, can affect the rotation of the planet's surface.

Reconstructing the spin from 1964 to 2019

To evaluate the hypothesis, the authors reconstructed how this interaction might have influenced Earth's spin between 1964 and 2019. They relied on seismic estimates of the inner core's rotation and models of liquid metal flows in the outer core. That combination allowed them to examine whether gravitational coupling between deep layers could account for some of the observed changes in rotation.

What emerges is not a single dramatic event but a slow accumulation. Small pushes and pulls, repeated over many years, can add up to detectable shifts in the length of a day. The study does not claim that this mechanism explains every variation. Instead, it adds a candidate process to a growing list of influences that operate across different parts of the Earth system.

Why milliseconds matter

A difference of a few milliseconds in the length of a day may sound trivial. But precise measurements of rotation give scientists a window into the planet's interior. The fact that the rotation speed is shifting is itself important, and the quest to explain it has revealed how many layers of the Earth are connected.

The atmosphere, oceans, earthquakes, melting ice, outer core flows, and inner core gravity all belong to the same coupled system. Each acts on its own timescale, and each can leave a faint signature in the planet's spin. Untangling those signatures helps researchers understand which forces dominate at which moments and how energy and mass move through the Earth.

The many forces shaping a day

The new proposal fits into a broader picture of Earth as a dynamic, layered world rather than a solid, static ball. The known and suspected contributors include:

  • Atmospheric and oceanic fluctuations: Changes in air and water circulation can slightly speed up or slow down the planet's rotation.
  • Major earthquakes: These events can redistribute mass within the Earth, altering rotation in small but measurable ways.
  • Melting continental ice: Water added to the oceans changes the distribution of mass and can influence spin.
  • Outer core flows: Movement in the liquid metal layer can change the rotation speed of the rest of the planet.
  • Inner core gravity: The gravitational pull between the inner core and mantle irregularities may create a long-term push-and-pull that affects day length.

These mechanisms do not operate in isolation. A change in one region can propagate through another, and the resulting rotation changes are the sum of many subtle effects.

What the study does and does not settle

The researchers believe they have identified one hidden gear in Earth's rotation, not the entire clockwork. How forces are transmitted from the deep interior to the surface has remained a mystery, and the weak friction between core and mantle could not explain it alone. The new work proposes gravity as a possible transmission belt, with the inner core's attraction to mantle irregularities providing the necessary coupling.

The finding is important because it connects processes that operate thousands of miles apart. It also gives scientists a new way to think about decade-scale changes in day length. At the same time, the study does not eliminate the roles of the atmosphere, oceans, earthquakes, or ice melt. Those forces remain part of the explanation, especially for more rapid shifts.

For now, Earth's days will continue to vary by tiny fractions that no one can feel. But those milliseconds carry information about a gravitational struggle deep inside the planet, a slow contest that helps shape the length of every day.

This article is based on reporting by Wired. Read the original article.

Originally published on wired.com