Earth's Stabilizing Moon May Be Unique Within Universe

Global Swoon Over the Moon Set For Saturday
This recent photo of the moon was taken by astronauts on the International Space Station during the Expedition 24 mission mid-2010. It was posted by cosmonaut Fyodor Yurchikhin of Russia's Federal Space Agency. (Image credit: Roscosmos.)

New simulations show that Earth's moon is not only unique in the solar system, but may also be rare throughout the universe.

Research reveals that less than 10 percent of terrestrial planets may have a satellite large enough to provide the stability life needs to develop.

Earth spins around its orbital axis, changing its angle toward the sun — its obliquity — by a little more than a degree over the course of thousands of years. These small differences are significant enough to cause the ebb and flow of ice ages. [10 Coolest Moon Discoveries]

The moon has long been recognized as a significant stabilizer of Earth's orbital axis. Without it, astronomers have predicted that Earth's tilt could vary as much as 85 degrees. In such a scenario, the sun would swing from being directly over the equator to directly over the poles over the course of a few million years, a change which could result in dramatic climatic shifts.

As it is, Earth's moon is unique in the solar system. The ratio of planet-to-moon mass is around a hundred times larger for Earth than similar comparisons to the moons of Mars. [Our Solar System: A Photo Tour of the Planets]

The vast difference stems from how the moons formed. The other planets in the solar system used gravity to capture free floating bodies. But, Earth's moon was created when a Mars-sized body slammed into the young planet. Gravity captured the debris as it splayed into space and over time, the material eventually congealed into a satellite.

The creation of a moon by impact depends significantly on the characteristics of the object crashing into the planet. For one thing, it must be relatively large – only about ten percent of its mass will stick around to form a moon after the collision. It also depends on the object's speed –  if it gently bumps the planet, it is less likely to have the energy the system would need.

Small moons would easily form, with an immediate effect on the planet's spin. But some could spiral into the planet, while others could quickly leave the orbit. Still others could find themselves kicked out entirely.

"Multiple impacts might…destroy existing satellites," Elser told SPACE.com in an email interview.

Once the violent formation period ended, the researchers' simulation showed 180 planets, almost half of which wound up with a moon. But, most of these satellites were too small to be comparable to our Earth-Moon system. Only fifteen pairs — about eight percent — resemble our unique planetary system.

Nola Taylor Tillman
Contributing Writer

Nola Taylor Tillman is a contributing writer for Space.com. She loves all things space and astronomy-related, and always wants to learn more. She has a Bachelor's degree in English and Astrophysics from Agnes Scott College and served as an intern at Sky & Telescope magazine. She loves to speak to groups on astronomy-related subjects. She lives with her husband in Atlanta, Georgia. Follow her on Bluesky at @astrowriter.social.bluesky