Latest in Space · Friday, September 25, 2026

Space2 min read

Mars's spin speeds up and slows down on a mysterious 26-year rhythm

Nearly 50 years of radio signals from Mars spacecraft show the planet doesn't turn at a perfectly steady pace, and nobody knows why yet.

Read the story
Studied
Mars's spin and gravity
Sample
47 million+ radio measurements
Time frame
Nearly 50 years of tracking
Where
NASA JPL (US) and Belgium
How sure are we?Spacecraft tracking data

Three orbiters independently show the same rhythm, but only about one full cycle has been seen so far. This rating is our read of the evidence, not the authors'.

01The question

Mars turns once every 24 hours and 37 minutes or so. Scientists care about that number down to tiny fractions of a second. Knowing exactly how Mars is tilted and how fast it spins is what lets spacecraft land in precise spots, and the spin also carries clues about what's happening inside the planet and in its thin air.

In 2023, the team behind NASA's InSight lander noticed something odd: Mars seemed to be spinning very slightly faster during InSight's mission (2018–2022) than during the Viking landers of the 1970s and '80s. They described it as a slow, steady speed-up. This new study asked whether that picture holds up once far more data is added.

02What they did

Researchers at NASA's Jet Propulsion Laboratory and in Belgium combined radio tracking from six spacecraft spanning nearly 50 years: three landers (Viking, Pathfinder and InSight) and three orbiters (Mars Global Surveyor, Mars Odyssey and Mars Reconnaissance Orbiter).

The trick is the Doppler effect, the same thing that makes a passing siren change pitch. When a spacecraft moves, its radio signal arrives on Earth at a slightly shifted frequency. A lander sitting on the ground moves only because Mars is turning, so its signal tracks the spin directly. Orbiters are tugged by Mars's lumpy gravity field as it rotates beneath them, which also reveals how the planet is turning.

In all, more than 47 million radio measurements went into one giant calculation that solves for Mars's gravity, tilt and spin together.

03What they found

All three orbiters, each analyzed on its own, told the same story: Mars's spin isn't changing at a steady rate. Instead it drifts ahead and then falls back in a cycle about 25.8 years long. The orbiters detected the change at 20 to 30 times their measurement error, so it isn't just noise.

The effect is tiny. At its biggest, a spot on Mars's equator ends up only about 4 meters ahead of or behind where a perfectly steady spin would put it. The most recent tracking data suggests the spin has started slowing down again after the InSight years, which a simple steady speed-up can't explain.

Along the way, the team also produced a sharper map of Mars's gravity and a recommended official model of how Mars is oriented in space. It pins down the direction of Mars's spin axis to within about 1 meter from 1950 to 2050.

04Why it matters

A planet's spin changes when mass moves around on it, just as a figure skater spins faster by pulling in their arms. Mars already shows a yearly version of this: carbon dioxide frost piles onto the poles in winter and turns back into gas in summer. Finding a new, unexplained 26-year rhythm means something on or inside Mars may be moving mass around on a much longer schedule. The authors suggest the atmosphere or the planet's interior as possible causes.

The cycle is also intriguingly close to the Sun's 22-year magnetic cycle, although no link has been shown. Solving the mystery could teach us something new about how Mars works, and the improved maps will help future missions navigate.

See it

The picture

01

The 26-year wobble

Over about 26 years, a spot on the equator drifts up to about 4 m ahead of a perfectly steady spin, then falls about 4 m behind.

Cycle length (25.8 years) and size (245.7 milliarcseconds, about 4 m at the equator) are from the paper. Where the cycle starts is drawn for illustration.
Show the numbers
Point in cycleDrift
Start (0 yr)0 m
Quarter (6.5 yr)+4 m
Half (12.9 yr)0 m
Three-quarters (19.4 yr)−4 m
Full cycle (25.8 yr)0 m

How far a spot on Mars's equator drifts from a perfectly steady spin

−4 m 0 +4 m0510152025.8Years into the cycle ≈ 4 m ahead ≈ 4 m behind

02

Weighing a planet's spin with radio

Tiny changes in a radio signal's pitch reveal how each spacecraft moves, and therefore how Mars turns.

A lander rides along with Mars's spin; an orbiter feels the planet's uneven gravity turning beneath it. Tiny frequency shifts in their radio signals reveal both.

Two ways spacecraft reveal how Mars turns

Diagram: a radio dish on Earth exchanges signals with a lander on Mars's surface and an orbiter circling Mars. The lander is carried along by Mars's rotation; the orbiter is tugged by Mars's uneven gravity. Small shifts in the signals' frequency reveal both motions. Earth one turn every ~24.6 hours Mars radio signals Lander: carried by the planet's spin Orbiter: tugged by uneven gravity

Key terms

Lander
A spacecraft that touches down and stays on a planet's surface.
Orbiter
A spacecraft that circles a planet instead of landing on it.
Doppler effect
The change in a wave's frequency when its source moves toward or away from you, like the drop in pitch of a passing siren.
Gravity field
A map of how strongly a planet pulls at each place. Mountains, basins and dense rock make it slightly uneven.

The fine print

  • Only about one full cycle has been observed so far, so scientists can't yet be sure it will repeat.
  • The cause is unknown. The atmosphere and the planet's interior are suggestions, not tested explanations.
  • The signal is very small, close to the roughly 1-meter precision that orbiters can reach, and the 1970s Viking data is about 10 times noisier than modern tracking.
  • The size in meters (about 4 m) is converted from the paper's angle (245.7 milliarcseconds) using Mars's average radius.

Think about it

Spin slowly on an office chair with your arms stretched out, then pull them in. What happens? What kinds of things on Mars (ice, dust, air) could move around in a way that nudges the whole planet's spin?

Read the original paper

Updated Mars Orientation and Gravity Field and Indication of Decadal Changes in Rotation Rate

The Planetary Science Journal · Published Sep 14, 2026

Konopliv, A. S., Park, R. S., Le Maistre, S., Yseboodt, M., & Baland, R.-M. (2026). Updated Mars Orientation and Gravity Field and Indication of Decadal Changes in Rotation Rate. The Planetary Science Journal, 7(9), 212. https://doi.org/10.3847/PSJ/ae9ba7

On the map

Where this research happened

  1. NASA Jet Propulsion Laboratory, Pasadena
  2. Royal Observatory of Belgium, Brussels
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