Now, scientists have proposed an almost-apocalyptic reason for this: A “planetary embryo” with 10 times more mass than Earth could have slammed into the largest planet in the solar system and disturbed its core. It’s not object that whacked Jupiter last week and was captured by an amateur astronomer on Earth. This event would have taken place in the distant past, and we’re only just learning how it may have shaped Jupiter.
The research, published Wednesday in the journal Nature, details a number of simulations demonstrating how a planetary embryo could have led to the uneven distribution of heavy metals we see throughout Jupiter’s gaseous envelope today. Jupiter is mostly composed of hydrogen and helium gases that move around a dense core. Scientists believed that heavy metals should be confined close to the dense core, but the Juno mission revealed that the metals are actually strewn far from the core.
How could that occur? The research team’s simulations suggest the young Jupiter suffered a giant impact during its formative years, which gave rise to this weird, unexpected distribution.
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Though the collision sounds violent, it’s almost as if the young Jupiter swallowed up the planetary embryo. The simulations show that the core of the protoplanet would have had to collide with Jupiter’s core to throw up the heavy elements and mix them throughout the entire envelope. The models show that the impact would have resulted in the internal structure discovered by NASA’s Juno and inthe heavy element distribution.
Other simulations demonstrate that if the smaller planet only skipped across Jupiter, the collision wouldn’t have the power to redistribute heavy metals throughout the gaseous envelope (though it would still be bad news for the baby planet).
These models also offer an explanation for some of the phenomena seen in a number of easily-discoverable exoplanets, the planets that lie outside our solar system. A number of these planets, known as “hot Jupiters,” are super dense, stacked with heavy elements and orbit very close to their star. They’re also prone to giant impacts. The researchers suggest their model might explain why there are so many heavy metals in these hot Jupiters, since they get smashed by planetary embryos as they form.
Could a series of small events, rather than one huge impact, give rise to the Jupiter we see today? The researchers say this needs more investigation.
The work provides further evidence of the tumultuous environment of the early solar system. Previous research suggests that massive impacts shaped our moon and Earth itself. The new research even suggests Saturn may have experienced a similar impact event during its formation.