Is Dark Matter Spinning Up the Earth? New Research Says Yes

What if something invisible, untouchable, and nearly impossible to detect was slowly—but surely—changing how fast our planet spins? Sounds like science fiction, right? But a new study from researchers at the Chinese Academy of Sciences suggests that dark matter might be quietly influencing planetary rotation and heating, including that of Earth itself.

How Planets Could Capture Dark Matter

According to this study, planets can gradually “capture” dark matter particles through gravity. Once pulled in, these particles interact in rare but important ways with the matter inside the planet. While dark matter doesn’t collide with regular particles in the usual sense, under certain conditions—such as quantum tunneling or annihilation—it can deposit energy into the planet’s interior.

Over time, this steady trickle of energy can lead to two measurable outcomes: a slight warming of the planet and a tiny acceleration in its rotation speed. It’s like having an invisible engine inside the Earth, quietly spinning the globe a little faster and raising its temperature ever so slightly. The scale may be small, but over decades and centuries, these effects could add up—and even be detected.

A Simulation Across the Solar System and Beyond

To test this theory, the research team ran simulations on 15 confirmed exoplanets, as well as Earth and Jupiter. Their calculations showed that on Earth, the combination of dark matter interactions and solar heating could result in a surface atmospheric temperature increase of 0.015 Kelvin per 100 years, and a change in the length of the day by about 12 seconds every century.

While that may sound insignificant, it’s actually a measurable change. Scientists already use atomic clocks and advanced satellite systems to track Earth’s rotation down to fractions of a second. So, if dark matter really is nudging our spin over time, we could see this through long-term observations.

The study also noted that Earth would be more affected than gas giants like Jupiter, due to differences in planetary structure and density. That’s because the way dark matter deposits energy depends heavily on a planet’s mass, radius, internal temperature, and angular velocity—all variables in their energy distribution model.

Why This Matters for Habitability and Life

This idea has far-reaching consequences beyond just an interesting tweak to planetary physics. If dark matter can influence temperature and rotation, it might affect a planet’s habitability—the potential to support liquid water and, by extension, life.

Planetary rotation affects climate stability, weather patterns, magnetic field generation, and more. A faster or slower rotation could impact atmospheric dynamics, the development of jet streams, or how heat is distributed between a planet’s day and night sides. On planets already on the edge of the habitable zone, even a slight change in temperature or spin could determine whether conditions remain suitable for life.

This opens a new chapter in how we assess exoplanets. Traditionally, scientists have focused on factors like distance from the star, atmospheric composition, and surface conditions. But now, we may need to consider the dark matter environment of a planetary system—a factor once thought irrelevant on small scales.

A New Lens for Understanding the Cosmos

What makes this research so exciting is that it connects two seemingly distant fields: cosmology and planetary science. Until now, dark matter was mostly studied in the context of galaxy formation, black holes, and the cosmic microwave background. This paper proposes that the same mysterious matter might also be shaping the physical behavior of planets, something we can study much more directly.

It’s a fresh way to look at an old puzzle. For decades, scientists have tried to detect dark matter through massive underground detectors or via high-energy collisions in particle accelerators. But maybe the key isn’t buried underground—it’s spinning in the sky. If planets can act as “long-term probes” of dark matter effects, as the authors suggest, then measuring their properties over time could provide a completely new way to test dark matter theories.

A Word of Caution: The Challenges of Detection

Of course, like any bold hypothesis, this one isn’t without challenges. Isolating the effects of dark matter from the many other forces influencing a planet is no small feat. Earth’s rotation, for example, is affected by tidal forces from the Moon, tectonic activity, glacial rebound, and atmospheric winds. Any shift in rotation could have many potential causes.

Similarly, changes in surface temperature might be more easily attributed to solar variation or human-induced climate change than to an invisible cosmic force. That’s why precision measurements over long periods will be essential to confirming or refuting this theory.

But what’s encouraging is that the predictions are specific and testable. And in science, that’s a big deal. A model that can be falsified through observation is much more powerful than one that simply explains what we already see.

Dark Matter in Our Search for New Worlds

One of the more intriguing takeaways from this study is how it could change the way we explore and colonize other planets. In the future, as humanity looks beyond Earth for a new home, planetary habitability won’t just depend on sunlight and atmosphere. We might need to consider how a planet’s dark matter environment contributes to its long-term evolution.

In regions of the galaxy where dark matter density is higher, planets might spin faster, warm slightly more, or experience different geological activity.

Final Thoughts: Rethinking Our Place in the Universe

This research challenges us to think differently about the universe—not just as something “out there,” but as something that interacts with the very ground we stand on. If dark matter is silently reshaping our planet’s spin and temperature, then its role in our lives is far more intimate than we ever imagined.

Reference:

 Haihao Shi et al, Dark Matter (S)pins the Planet, arXiv (2025). DOI: 10.48550/arxiv.2503.17206