J U P I T E R

628,730,000 KM

Jupiter's mass exceeds that of all other planets in our solar system combined. Its iconic Great Red Spot is a centuries-old storm larger than Earth itself.

  • Day

  • 9.93 hours
  • Year

  • 11.86 Earth Years
  • Radius

  • 142,984 kilometers
  • Planet Type

  • Gas Giant
  • Moons

  • 53 confirmed
    26 provisional
  • Quick Facts

    Sections


    Introduction


    As the fifth planet from the Sun, Jupiter is the solar system's undisputed giant, possessing more than double the mass of all its planetary siblings combined. Its swirling stripes are actually cold, windy clouds of ammonia and water, drifting in an atmosphere dominated by hydrogen and helium. The Great Red Spot, a storm larger than Earth, has raged for centuries.

    Jupiter commands a vast retinue of moons and possesses a faint ring system, composed mainly of dust rather than the icy brilliance of Saturn's rings.



    Interesting Facts About Jupiter

    • The four largest moons (the Galilean Satellites) are Io, Europa, Ganymede, and Callisto.

    • It reigns as the largest planet, nearly 11 times Earth's size and 317 times its mass.

    • Fittingly, it is named after the king of the ancient Roman gods.

    • It spins faster than any other planet, completing a rotation in just under 10 hours.

    • Like the Sun, it is primarily hydrogen and helium. Deep inside, it hosts the solar system's largest ocean—made of liquid hydrogen.

    Features



    Exploration


    Nine spacecraft have ventured to Jupiter. NASA's Juno orbiter currently studies the gas giant. Arriving in July 2016, Juno is peeling back the layers of the planet's cloud-shrouded interior. Observations also continue via the Hubble Space Telescope and ground-based observatories.



    Pioneer 10 became the first to fly past Jupiter, followed by Pioneer 11 and the Voyager missions. The Galileo orbiter was the first to circle the planet, dropping a probe into its stormy atmosphere. The Ulysses mission utilized Jupiter's gravity to swing into a polar solar orbit. More recently, Cassini and New Horizons captured data while en route to Saturn and Pluto, respectively.

    Two new missions are in the works to make close studies of Jupiter's moons NASA's Europa Clipper and ESA's JUpiter ICy Moons Explorer (JUICE).



    Jupiter marks a turning point in astronomy. In 1610, Galileo Galilei used his telescope to discover four moons orbiting the giant planet. This observation shattered the geocentric model, proving that not everything in the universe orbited Earth.





    Size and Distance


    With a radius of 43,440.7 miles (69,911 kilometers), Jupiter is 11 times Earth's width. Imagine Earth as a nickel; Jupiter would be a basketball.

    Orbiting at an average distance of 484 million miles (778 million kilometers), Jupiter resides 5.2 astronomical units (AU) from the Sun. Light takes 43 minutes to traverse this distance.



    Orbit and Rotation


    Jupiter rotates faster than any other planet, completing a day in just 10 hours. A full orbit around the Sun takes about 12 Earth years (4,333 days).

    With an axial tilt of just 3 degrees, Jupiter spins nearly upright, meaning it lacks the extreme seasonal variations found on other planets.



    Formation


    Jupiter formed alongside the rest of the solar system 4.5 billion years ago, growing from swirling gas and dust. It claimed the lion's share of the material left over after the Sun's creation, accumulating twice the mass of all other solar system bodies combined. Despite sharing the Sun's composition, it never gained enough mass to ignite into a star.

    Roughly 4 billion years ago, it settled into its current position as the fifth planet.



    Structure


    Jupiter's composition mirrors the Sun, consisting mainly of hydrogen and helium. Deep within, immense pressure compresses hydrogen into a fluid, creating the largest ocean in the solar system—an ocean of liquid hydrogen. Further down, pressures likely strip electrons from hydrogen atoms, creating a liquid metallic hydrogen that conducts electricity. The rapid rotation within this metallic layer generates Jupiter's massive magnetic field. The core remains a mystery; it may be solid or a dense, super-hot soup of iron and silicates at temperatures reaching 90,000°F (50,000°C).



    Internal Structure of Jupiter.


    Surface


    Lacking a true solid surface, Jupiter is a swirling mass of gases and liquids. Any spacecraft attempting to land would find no purchase; instead, it would be crushed, melted, and vaporized by the crushing pressures and searing temperatures deep within.



    Atmosphere


    Jupiter presents a vibrant tapestry of cloud bands and storms. Its atmosphere likely spans 44 miles (71 kilometers) across three distinct layers: an upper layer of ammonia ice, a middle layer of ammonium hydrosulfide, and an inner layer of water ice and vapor.

    The striking colors arise from sulfur and phosphorus gases rising from the warm interior. The planet's rapid rotation creates high-speed jet streams that separate clouds into dark belts and bright zones.

    Without solid land to break them up, storms persist for decades or centuries. The Great Red Spot, a storm twice the width of Earth, has been observed for over 300 years. Winds on Jupiter can scream at speeds up to 335 mph (539 kph).



    Potential for Life


    Life as we understand it is unlikely to exist in Jupiter's volatile environment. However, its moons tell a different story. Europa, with its subsurface ocean beneath an icy crust, is considered one of the most promising places to search for life elsewhere in the solar system.



    Moons


    Jupiter anchors a mini-solar system of 53 confirmed moons and dozens more awaiting confirmation.

    The four largest—Io, Europa, Ganymede, and Callisto—were discovered by Galileo in 1610. Io is a volcanic hellscape, the most active body in the solar system. Ganymede is the largest moon, surpassing even the planet Mercury in size. Callisto is an ancient, cratered world, while Europa lures scientists with its hidden liquid ocean.




    Jupiter and Moons


    E U R O P A


    Rings


    NASA's Voyager 1 spacecraft unveiled Jupiter's rings in 1979. Unlike Saturn's icy spectacles, these rings are faint and dark, composed of small particles. Data suggests they are formed by dust kicked up when meteoroids strike Jupiter's small inner moons.



    Magnetosphere


    Jupiter's magnetosphere is immense, ballooning 1 to 3 million kilometers toward the Sun and stretching a tail over 1 billion kilometers behind the planet—reaching Saturn's orbit.

    Its magnetic field is 16 to 54 times stronger than Earth's. It traps charged particles, accelerating them to high energies that create intense radiation belts capable of damaging spacecraft. This field also drives spectacular aurorae at Jupiter's poles. ​



    Quick Facts