Science

Days Shrink by Up to 1.38 Milliseconds This Summer

Days Shrink by Up to 1.38 Milliseconds This Summer

Introduction

As summer sunsets linger and beach days stretch on, a subtle yet measurable shift is altering the very fabric of time: Earth’s rotation is accelerating. In July and August 2025, multiple days are projected to be shorter than the standard 24 hours—by as much as 1.38 milliseconds. While imperceptible to humans, this phenomenon reflects complex geophysical processes with tangible impacts on global navigation and long-term climate modeling. According to data from the International Earth Rotation and Reference Systems Service (IERS), Earth continues a trend observed over recent decades: a gradual shortening of the solar day. Though not enough to disrupt daily routines, the changes highlight how deeply interconnected Earth’s systems—from its molten core to atmospheric winds—are in shaping planetary motion.

This acceleration follows a broader pattern initiated in the early 2020s, when scientists first noted a reversal in Earth’s long-term rotational slowdown. The shortest day on record, recorded on July 5, 2024, fell 1.66 milliseconds below 86,400 seconds. The 2025 season, while not breaking that record, continues the trend with near-daily deviations. Experts like Duncan Agnew, a geophysicist at Scripps Institution of Oceanography, emphasize that these fluctuations are natural and pose no risk to life. Yet, they demand careful monitoring due to their implications for precision technologies such as GPS and satellite communications.

Key Details

  • On July 10, 2025, Earth completed its rotation 1.38 milliseconds faster than 86,400 seconds—the shortest day of the year so far.
  • July 22, 2025, is projected to be 1.34 milliseconds shorter than a standard day.
  • The current record for shortest day remains July 5, 2024, at 1.66 milliseconds under 24 hours.
  • Data sourced from IERS and analyzed via atomic clocks and radio telescopes.
  • Contributing factors include slowing of Earth’s core, seasonal atmospheric weakening, and lunar tidal effects.
  • These micro-changes affect GPS accuracy, introducing potential location errors of about 1.5 feet per millisecond.
"It’s not something you’d notice," says Duncan Agnew. "But for systems that rely on nanosecond precision, even a millisecond matters."

Background

Earth’s rotation has never been perfectly uniform. Over geological time, the moon’s gravitational pull has slowed Earth’s spin through tidal friction, lengthening days by about 1.7 milliseconds per century. Fossil records from Cretaceous-era mollusks suggest a day was nearly 30 minutes shorter 70 million years ago. However, this long-term deceleration is now being offset by counteracting forces. Since the 1970s, a noticeable trend toward shorter days has emerged, reversing the expected slowdown.

The primary driver appears to be dynamics within Earth’s liquid outer core. Composed of molten iron and nickel, the core generates the planet’s magnetic field through the geodynamo effect. Recent studies, including a 2024 Nature paper, indicate that the core’s rotation has decelerated. Due to the conservation of angular momentum, this loss of rotational energy must be compensated elsewhere in the system—leading to an acceleration of the planet’s surface. As Agnew explains, “It’s like a figure skater pulling in their arms to spin faster—except the skater’s arms are the planet’s surface, and the spin is driven by internal shifts.”

Impact Analysis

While humans won’t perceive milliseconds lost from a day, high-precision systems certainly will. Global Positioning Systems (GPS), which rely on atomic clocks aboard satellites, require exact knowledge of Earth’s orientation and rotation speed. A discrepancy of just one millisecond translates to a positional error of approximately 1.5 feet (45 centimeters), potentially affecting aviation, maritime navigation, and autonomous vehicles. Military operations and telecommunications networks also depend on synchronized timekeeping, making IERS data critical for global infrastructure.

Organizations like the IERS and the U.S. Naval Observatory continuously monitor Earth’s rotation using Very Long Baseline Interferometry (VLBI), which tracks distant quasars to detect minute changes in orientation. These observations inform the Coordinated Universal Time (UTC) system, which may require adjustments—though instead of adding leap seconds, we may soon face the unprecedented need for a negative leap second to keep clocks aligned with solar time.

Broader Context

Seasonal atmospheric changes also contribute to rotational fluctuations. During summer, the jet stream weakens, reducing angular momentum in the upper atmosphere. This energy transfers to Earth’s surface, slightly accelerating rotation. Climate change further complicates this picture: melting ice caps redistribute mass toward the equator, slowing rotation like a spinning ice skater extending their arms. However, this effect is currently outweighed by core dynamics, resulting in a net speed-up.

Additionally, the moon’s elliptical orbit introduces minor periodic variations. When the moon reaches its maximum declination north or south of the equator, its gravitational pull is less effective at slowing Earth, leading to brief accelerations. These combined forces create a complex, multi-layered system of rotational modulation.

Future Outlook

Scientists expect the trend of shorter days to continue in the near term, though long-term predictions remain uncertain due to limited understanding of core behavior. Future research, including seismic imaging and satellite gravimetry, may shed light on core-mantle interactions. As climate change alters atmospheric and cryospheric patterns, their rotational impacts will need continuous reassessment.

The possibility of a negative leap second—removing one second from UTC—is now under discussion by international timekeeping bodies. Last reviewed in 2022, the decision could reshape digital timekeeping standards, affecting everything from financial markets to internet protocols.

Conclusion

The shortening days of summer 2025 are more than a curiosity—they are a reminder of Earth’s dynamic interior and the delicate balance of forces shaping our planet. While these changes won’t alter vacation plans, they underscore the importance of precise scientific monitoring in an interconnected world. From fossilized shells to atomic clocks, humanity’s understanding of time continues to evolve, revealing that even the length of a day is never truly fixed.