Study suggests moon may have been captured from space rather than formed from collision particles

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Over six missions to the moon, from 1969 to 1972, Apollo astronauts collected more than 800 pounds of lunar rock and soil. Chemical and isotopic analysis of that material showed that it was similar to the rock and soil on Earth: calcium-rich, basaltic and dating to about 60 million years after the solar system formed.

Using that data, the planetary scientists who gathered at the Kona Conference in Hawaii in 1984 came to the consensus that the moon formed from debris after a collision on the young Earth.

But that might not be the moon's true origin story, according to two Penn State researchers. New research published in The Planetary Science Journal by Darren Williams, professor of astronomy and astrophysics at Penn State Behrend, and Michael Zugger, a senior research engineer at the Applied Research Lab at Penn State, offers another possibility: That the moon was captured during a close encounter between a young Earth and a terrestrial binary—the moon and another rocky object.

"The Kona Conference set the narrative for 40 years," Williams said. But questions still lingered. For example, a moon that forms from a planetary collision, taking shape as debris clumps together in a ring, should orbit above the planet's equator. Earth's moon orbits in a different plane.

"The moon is more in line with the sun than it is with the Earth's equator," Williams said.

In the alternative binary-exchange capture theory, the researchers said, Earth's gravity separated the binary, snagging one of the objects—the moon—and making it a satellite that orbits in its current plane.

There is evidence of this happening elsewhere in the solar system, Williams said, pointing to Triton, the largest of Neptune's moons. The reigning hypothesis in the field is that Triton was pulled into orbit from the Kuiper Belt, where 1 of every 10 objects is thought to be a binary.

Triton orbits Neptune in a retrograde orbit, moving in the opposite direction of the planet's rotation. Its orbit is also significantly tilted, angled 67 degrees from Neptune's equator.

Williams and Zugger determined that Earth could have captured a satellite even larger than the moon—an object the size of Mercury or even Mars—but the resulting orbit might not have been stable.

The problem is that the "capture" orbit—the one the moon follows—began as an elongated ellipse, rather than a circle. Over time, influenced by extreme tides, the shape of the orbit changed.

"Today, the Earth tide is ahead of the moon," Williams said. "High tide accelerates the orbit. It gives it a pulse, a little bit of boost. Over time, the moon drifts a bit farther away."

The effect is reversed if the moon is closer to Earth, as it would have been immediately after capture. By calculating tidal changes and the orbit's size and shape, the researchers determined that the moon's initial elliptical orbit contracted over a timescale of thousands of years.

The orbit also became more circular, rounding its path until the lunar spin locked into its orbit around the Earth, as it is today.

At that point, Williams said, the tidal evolution likely reversed, and the moon began to gradually drift away.

Every year, he said, the moon moves 3 centimeters farther from Earth. At its current distance from Earth—239,000 miles—the moon now feels a significant tug from the sun's gravity.

"The moon is now so far away that both the sun and Earth are competing for its attention," Williams said. "Both are pulling on it."

His calculations show that, mathematically, a binary-exchange captured satellite could behave as Earth's moon does. But he's not certain that's how the moon came to be.

"No one knows how the moon was formed," he said. "For the last four decades, we have had one possibility for how it got there. Now, we have two. This opens a treasure trove of new questions and opportunities for further study."

More information: Darren M. Williams et al, Forming Massive Terrestrial Satellites through Binary-exchange Capture, The Planetary Science Journal (2024). DOI: 10.3847/PSJ/ad5a9a

Journal information: The Planetary Science Journal

Provided by Pennsylvania State University