- Earth's stable seasons depend on the Moon preventing axis wobble.
- Mars's tilt has swung between 10 and 40 degrees over time.
- Uranus sits tilted 98 degrees, creating 42-year polar seasons.
Gongjie Li studies how planets wobble, and what she found about Earth surprised her.
The Georgia Tech astrophysicist has spent years asking whether other planets have seasons like Earth does, and tracking how their axial tilts shift over time. Her work suggests that Earth's steady four-season rhythm, the predictable cycle that agriculture and ecosystems depend on, is not the cosmic default.
It may be a fortunate anomaly.
Key figure
98°
Uranus's axial tilt, compared to Earth's 23.5°
Mars Looks Like Earth's Seasonal Twin, But It Isn't
Mars tilts at roughly 25 degrees, strikingly close to Earth's 23.5. Shane Byrne, a planetary science professor at the University of Arizona who studies Martian climate records, sees the resemblance. Both planets have polar regions that alternate between permanent daylight and permanent darkness each half year.
More on Mars
Did Mars Once Have a Tropical Climate With Millions of Years of Rainfall?
Light-colored rocks discovered by NASA's Perseverance rover suggest the Red Planet was far wetter than scientists imagined.
→The winters tell a different story.
Temperatures on Mars drop low enough for the atmosphere itself to freeze, coating the surface in carbon dioxide ice rather than the water ice familiar on Earth. Orbital shape adds another layer of complexity.
Planets with highly elliptical paths, like Mercury and Pluto, experience seasonal heating variations from changing distance to the Sun, independent of any tilt at all.
But the critical difference for Mars is stability. Models published in the journal Earth and Planetary Science Letters in 2018 showed that the planet's tilt has swung between 10 and more than 40 degrees over billions of years.
What looks like a twin of Earth today is a planet whose seasons have been reshuffled repeatedly across geological time.
The current similarity is coincidence.
It's almost just random chance that it happens to be similar to the Earth today.
Shane Byrne, planetary science professor, University of Arizona
Earth's Moon Keeps the Seasons Steady
The reason Earth's tilt holds firm comes down to a single companion.
Our Moon is massive enough to pull on Earth's spin axis and force it to precess, or wobble, faster than it otherwise would. That faster wobble prevents a phenomenon called spin-orbit resonance, where gravitational tugs from neighboring planets push a planet's tilt at exactly the wrong frequency, amplifying it over millions of years.
What is spin-orbit resonance?
When a planet's wobble frequency matches the rhythm of gravitational pulls from neighboring planets, the tilt can grow dramatically over time. Earth's Moon speeds up the wobble enough to break this dangerous synchronization.
Think of pushing a child on a swing at precisely the right interval. Each push builds the arc higher. Without the Moon acting as a damper, Earth's tilt could have drifted just as wildly as its neighbor's.
Mars has no such protector, and its climate has paid the price across billions of years.
Li considers it fortunate: Earth's spin axis has stayed remarkably steady.
Uranus Reveals the Extreme
At the far end of the spectrum sits Uranus, tilted 98 degrees from vertical.
The planet rolls around the Sun on its side, producing seasonal extremes unlike anything else in the solar system. Each pole receives about 42 years of continuous sunlight followed by 42 years of total darkness, spread across an 84-year orbit. During the brief equinoxes, sunlight strikes the equator, producing rapid 17-hour day-night cycles before the slow roll returns to decades of polar exposure.
When Voyager 2 flew past Uranus in 1986, it caught the planet deep in its southern summer. The spacecraft saw a nearly featureless blue world. In the decades since, as Uranus has moved through its orbit, telescopes have watched dramatic cloud patterns emerge and shift with the changing seasons.
Li argues that Earth's stable spin axis has been essential for complex life to develop here. Scientists searching for habitable exoplanets now recognize that the right distance from a star is not enough.
More On Planets
How Did Planets Form? The Gas Giants Arrived First
Gas giants like Jupiter formed first in our solar system, then shaped Earth's position in the habitable zone through gravitational migration.
→They also need worlds with stable seasonal patterns.
The exoplanet Kepler-186f offers some encouragement, orbiting far enough from its sibling planets that gravitational disturbance stays minimal. Even without a large moon, its obliquity appears to hold steady.
For most worlds, though, the pattern looks more like Mars or Uranus: seasons that drift across geological time or stretch across human lifetimes.
Earth's predictable cycle, maintained by a Moon at just the right mass and distance, may be far rarer than any of us assumed.
Sources
- Primary Source: Do other planets have seasons? (Live Science)
- Additional Context:
- Earth isn't the only planet with seasons (The Conversation)
- Seasons on other planets (ESA)
- The strange seasons of Uranus (EarthSky)
Fact Check: Claim-by-Claim Verification Verified
All major claims are supported by peer-reviewed research and credible sources; names, numbers, and scientific explanations are accurate.
Commentary
- The article's characterization of Earth's stable seasons as a "rare" or "fortunate anomaly" is well-supported by scientific literature showing that spin-orbit resonance creates chaotic variations in most planets without massive moons
- The article simplifies Mars's complex climate history into seasons defined by CO2 freezing rather than water ice; this is an acceptable simplification for popular science that accurately reflects Mars's modern atmospheric conditions
- The explanation of spin-orbit resonance using a child on a swing is an effective pedagogical metaphor appropriate for popular science communication
- The article notes that Kepler-186f's stability occurs "even without a large moon," which accurately reflects current understanding from Li's research that some exoplanets can maintain stable obliquity through orbital configuration alone
Sources used for verification
Academic/Peer-reviewed:
- Origins: From the Protosun to the First Steps of Life - cambridge.org
- Mars: change in axial tilt due to climate? - PubMed
- Ancient craters on Mars reveal how the planet's tilt has changed over time - Science.org
- Gongjie Li Research Profile - gatech.edu
- Astrophysicist Gongjie Li Unravels the Mysteries of Planetary Seasons - gatech.edu
Other reliable sources:
- Study: Habitable Zone Exoplanets Kepler-62f and Kepler-186f Have Very Stable Axial Tilts - Sci.news
- Voyager 2 met Uranus 40 years ago - EarthSky
- Changes in Tilt of Mars' Axis - NASA.gov
- Study Shows Exoplanet Has a Stable Axis Just Like Earth - Popular Mechanics
Fact-checked by Perplexity Sonar Pro on 2026-03-10
