Scientists have recently discovered a giant planet named TOI-6894b orbiting a very small red dwarf star, which challenges existing theories. TOI-6894b is a gas giant, around 1.07 times the diameter of Saturn but with just over half its mass. This makes it extremely low in density, like a beach ball. It was found about 241 light-years away in the constellation Leo. The planet orbits very close to its host star and completes one full orbit in less than three Earth days.
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