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Compare the Planets

Comparing the physical characteristics of the worlds in our solar system (and beyond)

The worlds of our solar system come in all shapes, sizes, and colors. Red-eyed Jupiter, ringed Saturn, and frigid Uranus and Neptune are giant gassy globes containing nearly all of the matter in the solar system. These Jovian planets, or gas giants, are huge worlds of air, clouds, and fluid that may have no solid surfaces no matter how deep you go. Everything else in the solar system is just rock, ice, and dust. The largest rockballs are known as the terrestrial planets: Mercury, Venus, Earth, and Mars, with our Moon usually considered part of the club, and now Vesta is applying for membership. Earth is the biggest of all the rocky worlds.

But the planets are not the only worlds of the solar system. All but two of the planets are orbited by moons, each of them a world unto itself. The largest moons are bigger than the smallest planets, and 16 or 17 would qualify as dwarf planets if they orbited the Sun. There are more than 100 Kuiper belt dwarf planets, but only one among the asteroids, Ceres.

Six solid worlds -- Venus, Earth, Mars, Titan, Triton, and Pluto -- have atmospheres dense enough to produce weather. Eris likely does, when it is near its perihelion. We have witnessed active geology on four worlds -- Earth, Io, Enceladus, and Triton -- and we suspect it on Venus, Europa, and Titan. Comparing the same processes across many worlds helps us to understand how each planet's unique composition and history influence its present state, and will help us predict what to expect on Earth in the future.

Pretty Pictures with Many Worlds

Dione and Friends

Dione and Friends

Black-and-white montage of Cassini images of Saturn's rings and moons. From left to right, they are Mimas, Dione, Epimetheus, and Prometheus. From a series of images taken December 12, 2011.

Filed under Dione, pretty pictures, Cassini, amateur image processing, Saturn's small moons, global views, Saturn's moons, many worlds, Mimas

Dances with Moons

Dances with Moons

Cassini captures "mutual event" movies to refine the precision with which we know the orbits of Saturn's moons. On September 17, 2011, Cassini took four such movies in rapid succession: Tethys with Titan at about 0100 UTC; Rhea with Titan at 0130; Enceladus with Titan at about 1030; and, at the end, at 1200, a movie with Titan, Dione, Saturn's rings, Pandora, and Pan.

Filed under Enceladus, Dione, Cassini, Tethys, Titan, Rhea, Saturn's small moons, global views, Saturn's moons, many worlds, animation, Saturn's rings, pretty pictures, amateur image processing

Carbon dioxide snow and water ice snow, compared

Carbon dioxide snow and water ice snow, compared

What does a Martian snowflake look like? As seen by Earth-based experimenters, carbon dioxide crystals have a "cuboctahedral" shape – cubes with the corners cut off. These particles are much smaller (about 100x smaller) than terrestrial water snow, and lack their intricate symmetry and platy structure.

Filed under pretty pictures, scale comparisons, Earth, Mars, weather and climate

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Section Highlights

Planetary Facts

Mass, diameter, density, gravity, orbital characteristics, presented both in metric units and measured relative to Earth.

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Asteroids and Comets Visited by Spacecraft

A comparison of all the asteroids and comets ever visited by spacecraft, up to date as of November 10 (when Deep Impact flew past Hartley 2). Vesta is not included.

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Every Round Object in the Solar System, to Scale

A correctly scaled, reasonably correctly colored view of the largest bodies in the solar system.

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