How Old Is Jupiter? Scientists Have A New Theory – BGR

Jupiter is the largest planet in our solar system (so large, in fact, that some scientists think it might have even consumed other worlds), a gas giant so massive that it shaped the orbits and evolution of the neighboring planets. For decades, scientists thought Jupiter was roughly 4.5 billion years old, forming soon after the birth of our sun. And a new study published in August 2025 in Scientific Reports has helped to pin down that age more precisely, while also arguing that Jupiter’s story is much more complex.

This new study takes a closer look at Jupiter’s formation and offers a revised theory about what was happening when this planet came into being. Instead of assuming a very straightforward early origin, the findings point to a more complicated process surrounding Jupiter’s birth — one that offers more insight into the planet’s age. At the heart of the study are chondrules: tiny, once-molten droplets of rock that resemble raindrops and are found in certain meteorites. Let’s take a look at this new study and see how it challenges existing models, and what it means for our broader understanding of planetary formation.

Researchers from Japan’s Nagoya University and the Italian National Institute for Astrophysics (INAF) collaborated to discover how chondrules in meteorites were created. These millimeter-scale droplets of once-molten silicate cooled rapidly in space, and they make up a large fraction of certain meteorites, even those that hit Earth every year. How the chondrules were formed is a question that puzzled scientists for a long time. What melted solid rock and dust in the early solar nebula, and how did those molten droplets cool so quickly to freeze in the droplet shapes we now observe?

Simulations run by authors Sin-Iti Sirono and Diego Turrini propose that Jupiter’s rapid growth stirred our young solar system so dramatically that high-velocity collisions among volatile planetesimals (clumps of space material that eventually form planets) became inevitable. Those collisions created the conditions for molten silicate droplets to form, cool, and solidify into the chondrules we observe today. The timing of peak chondrule production in their model, triggered by Jupiter’s runaway gas accretion, aligns with meteorite chronometry. That alignment points to Jupiter’s date of birth being about 4.6 million years ago — about 1.8 million years after the first solid condensates in our solar system.

What makes this new research stand out is not only its conclusion about Jupiter’s age, but the method it uses to reach it. Traditionally, the ages of planets were estimated through various methods, such as isotope dating or by modeling how long it would take for a planet to accumulate its mass. These are powerful approaches, but they leave gaps in our understanding of the dynamic processes that shaped our early solar system.

The study done by Sin-iti Sirono and Diego Turrini introduces a different approach. They see chondrules as a timestamp for planetary growth. Because their model links the production of chondrules directly to Jupiter’s growth, the timing of when most chondrules formed effectively reveals when Jupiter reached a critical stage in its development. In other words, the researchers tie these microscopic droplets to the gravitational influence of a giant planet, rather than relying on the information about local conditions in the early solar nebula.

This new approach offers a way to bridge small-scale evidence with large-scale planetary history. If chondrules can reliably be linked to the influence that young planets had on their surroundings, they could become a powerful tool for reconstructing when other major bodies in our solar system reached maturity. Similar methods might help scientists refine timelines for Saturn, or even for the formation of Earth (though how life actually began on Earth is another question entirely). In the broader picture, the study highlights how even the tiniest pieces of rock can make us understand cosmic planetary giants. By connecting the chemistry of meteorites to the dynamics of planetary growth, scientists may be opening a new chapter on how we chart the early evolution of planets both in our solar system, or maybe even in a mysterious solar system completely unlike ours.