This layer, extending thousands of kilometers, behaves in strange ways, conducting electricity like a metal due to the dissociation of molecules under immense pressure. The Glorious Cloud Tops The visible face of Jupiter is its atmosphere, a dynamic tapestry of ammonia crystals that form the white clouds we see.
Jupiter's Matter: The Rules Behind the Planet's Strange Metallic Hydrogen and Extreme Cores
This core is so hot—tens of thousands of degrees—that it may be partially dissolved in the surrounding metallic hydrogen, creating a unique state of matter that challenges our current understanding of physics. Every new observation from missions like Juno peels back another layer of this giant, revealing that the boundaries between the layers are more complex and turbulent than previously imagined.
Current models suggest a dense aggregation of rock and metal, possibly weighing up to 10 times the mass of Earth, crushed into a state of extreme density. By studying this massive world, we are not only learning about a single planet, but also probing the fundamental forces that shape all gas giants.
Jupiter's Matter Defies Physics in Its Metallic Hydrogen Depths
Beneath the banded clouds of Jupiter lies the most extreme environment in the inner solar system. These cloud decks act like a veil, hiding the violent churning that occurs deeper within the planet, making remote observation and data interpretation a challenging puzzle for scientists.
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