How Much Bigger Is Jupiter Than Earth?

Jupiter, the largest planet in our solar system, highlights the vast difference between gas giants and smaller, rocky worlds like Earth. Although both planets orbit the same star, their physical properties represent fundamentally different outcomes of planetary formation. The immense disparity in size, mass, and internal structure between Earth and Jupiter shapes the dynamics of the entire solar system. Understanding Jupiter’s scale requires grasping the true volumetric and gravitational gap separating the two planets.

Direct Size and Volume Comparison

Jupiter dwarfs Earth in physical dimensions. Jupiter’s equatorial diameter is about 11.2 times greater than Earth’s diameter, meaning over eleven Earths could line up across Jupiter’s equator. Jupiter’s mean radius is approximately 69,911 kilometers, compared to Earth’s 6,371 kilometers.

This linear difference translates into a volumetric disparity because volume scales with the cube of the radius. Jupiter’s volume is so immense that it could contain over 1,300 planets the size of Earth. Its surface area is also vastly larger, measuring about 120 times that of Earth.

Jupiter’s rapid rotation, completing a full spin in under ten hours, causes a noticeable flattening at its poles, known as oblateness. This fast spin forces a slight bulge around the equator, resulting in the equatorial radius being approximately 4,600 kilometers larger than the polar radius, a proportional difference of about 6.5%.

The Difference in Mass and Density

The mass difference is more dramatic than the size difference. Jupiter is approximately 318 times more massive than Earth, containing nearly 1.9 x \(10^{27}\) kilograms of material. This single planet accounts for about two and a half times the mass of all the other planets in the solar system combined.

Despite its size and mass, Jupiter is far less dense than Earth. Earth is a rocky planet with a mean density of 5.514 grams per cubic centimeter, while Jupiter’s mean density is only 1.326 grams per cubic centimeter. This low density, only slightly more than that of water, results from its composition being primarily hydrogen and helium.

Due to its lower density relative to its mass, Jupiter’s gravity at the cloud tops is only about 2.5 times stronger than Earth’s surface gravity. The immense volume spreads the planet’s mass over a much larger space, lessening the gravitational force felt at the outermost boundary.

Implications of Jupiter’s Scale

Jupiter’s scale generates consequences that affect its environment and the wider solar system. Its powerful gravitational field profoundly influences nearby objects, acting as a major deflector of comets and asteroids.

The rapid, sub-ten-hour rotation creates intense atmospheric dynamics. This quick spin drives powerful jet streams and zonal winds, leading to the colorful, alternating bands of clouds seen in its upper atmosphere. These high-speed winds can reach velocities up to 900 kilometers per hour.

The most prominent result of this atmospheric turbulence is the Great Red Spot, a persistent anticyclonic storm larger than Earth. This high-pressure system generates winds that can exceed 400 miles per hour, illustrating the energy contained within Jupiter’s atmosphere.

Structural Differences: Why the Scale Varies So Much

The vast difference in scale lies in the fundamental classification of the two planets. Earth is a terrestrial planet, composed mainly of silicate rock and metals. Jupiter, in contrast, is a gas giant, meaning its composition is similar to that of the sun.

Jupiter is overwhelmingly composed of hydrogen (about 76%) and helium (24%). As pressure and temperature increase dramatically deeper inside, the gaseous atmosphere transitions into a supercritical fluid state without a clear boundary.

At extreme depths, the immense pressure compresses the hydrogen into a liquid metallic hydrogen layer, which conducts electricity like a metal. This metallic layer generates Jupiter’s incredibly strong magnetic field. Models suggest the presence of a central core composed of heavier elements like ice, rock, and metal, though its exact nature is still being studied.