Jupiter

Overview

Jupiter is the fifth-closest planet to the sun and the largest and oldest planet in the solar system. Named after the king of Roman gods, this gas giant is most easily recognized by its Great Red Spot—a hurricane-like storm larger than Earth that has existed for about 200 years. With more than twice the mass of all other planets combined, thousands of objects—including over 90 moons—orbit Jupiter.

As with all planets in our solar system, Jupiter formed from what remained of the cloud of gas that collapsed into the sun and protoplanetary disk. Large pieces of matter—called planetesimals—likely collided to form Jupiter within a few million years, fast enough to accumulate gas from the disk before solar winds blew it away.

Heat from Jupiter's core moves fluid in convection cells—hot gases rise, and cooler ones sink. The planet's rotation—the fastest in the solar system—spreads these rising and sinking fluids into east-west flows that wrap around it like global jet streams. The color of the flows results from differences in the convection cell temperature and composition, which vary across three distinct cloud layers.

Modeling Jupiter's interior using observational data suggests that gas gradually liquefies with depth until about 20,000 km, at which point immense pressure turns hydrogen into liquid metal.

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