Jupiter, the solar system’s largest planet, used to be even bigger, according to a new study.
The cloud of gas and dust from which the sun and planets formed dissipated around 4.5 billion years ago. At that time, Jupiter was at least twice its current size, and its magnetic field was about 50 times stronger, researchers found. The findings, which the team described in a study published May 20 in the journal Nature Astronomy, could help scientists develop a clearer picture of the early solar system.
“Our ultimate goal is to understand where we come from, and pinning down the early phases of planet formation is essential to solving the puzzle,” study co-author Konstantin Batygin, a planetary scientist at Caltech, said in a statement. “This brings us closer to understanding how not only Jupiter but the entire solar system took shape.”
Jupiter’s immense gravity — along with the sun’s — helped fashion the solar system, shaping the orbits of other planets and rocky bodies. But how the giant planet itself formed remains opaque.
To gain a better picture of Jupiter’s early days, the researchers studied the present-day, slightly tilted orbits of two of Jupiter’s moons, Amalthea and Thebe. The paths these moons chart are similar to what they were when they first formed, but the moons have been pulled slightly over time by their larger, volcanically active neighbor Io. By analyzing the discrepancies between the actual changes and those expected from Io’s nudges, the researchers could work out Jupiter’s original size.
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When the solar nebula dissipated, marking the end of planet formation, Jupiter’s radius would have been between two and 2.5 times its current size to give Amalthea and Thebe their current orbits, the scientists calculated. Over time, the planet has shrunk to its current size as its surface cools. Then, the team used the radius to calculate the strength of the planet’s magnetic field, which would have been around 21 milliteslas — about 50 times stronger than its current value and 400 times stronger than Earth’s.
“It’s astonishing that even after 4.5 billion years, enough clues remain to let us reconstruct Jupiter’s physical state at the dawn of its existence,” study co-author Fred Adams, an astrophysicist at the University of Michigan, said in the statement.
The findings sharpen researchers’ view of the solar system at a critical transition point in its history. The calculations also don’t depend on how Jupiter formed — a process that’s still not understood in detail — relying instead on directly observable quantities.
“What we’ve established here is a valuable benchmark,” Batygin said in the statement. “A point from which we can more confidently reconstruct the evolution of our solar system.”
Jupiter is currently shrinking by about 2 centimeters per year, according to Caltech. This is due to the Kelvin-Helmholtz mechanism — a process by which planets grow smaller as they cool. As Jupiter slowly cools, its internal pressure drops, causing the planet to steadily shrink. It’s unclear when this process began.
