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
Cassini captured this Titan, Rhea (lower left) and Mimas mutual event on March 25, 2015 with its narrow-angle camera. A very faint ring (G ring?) that is almost undetectable unless the photo is viewed in darkness runs horizontally between Rhea's upper limb and Mimas' disk. Several faint stars are also visible.
Amateur astronomer Christopher Go captured these views of Ganymede passing in front of Jupiter—visible next to the Red Oval BA (sometimes affectionately referred to as "Red Spot Jr." or "The Little Red Spot")—on March 2, 2014. Visit his website for additional information.
Amateur astronomer Christopher Go captured these views of Europa passing in front of Jupiter along the southern boundary of the south equatorial band on April 18, 2014. Visit his website for additional information.
An asteroid or comet headed for Earth is the only large-scale natural disaster we can prevent. Working together to fund our Shoemaker NEO Grants for astronomers, we can help save the world.