Composite image comparing the sizes of Saturn and Earth
Saturn is a
gas giant because it is predominantly composed of hydrogen and helium. It lacks a definite surface, though it may have a solid core.
 Saturn's rotation causes it to have the shape of an
oblate spheroid; that is, it is flattened at the poles and bulges at its equator. Its equatorial and polar radii differ by almost 10%: 60,268 km versus 54,364 km.
Uranus, and Neptune, the other giant planets in the Solar System, are also oblate but to a lesser extent. The combination of the bulge and rotation rate means that the effective surface gravity along the equator, 2, is 74% that at the poles and is lower than the surface gravity of the Earth. However, the equatorial
8.96 m/sescape velocity of nearly is much higher than that for the Earth. 36 km/s
Saturn is the only planet of the Solar System that is less dense than water—about 30% less.
 Although Saturn's
core is considerably denser than water, the average
specific density of the planet is 3 due to the atmosphere. Jupiter has 318 times the Earth's mass, 0.69 g/cm
 and Saturn is 95 times the mass of the Earth.
 Together, Jupiter and Saturn hold 92% of the total planetary mass in the Solar System.
Diagram of Saturn, to scale
Despite consisting mostly of hydrogen and helium, most of Saturn's mass is not in the
phase, because hydrogen becomes a
non-ideal liquid when the density is above 3, which is reached at a radius containing 99.9% of Saturn's mass. The temperature, pressure, and density inside Saturn all rise steadily toward the core, which causes hydrogen to be a metal in the deeper layers. 0.01 g/cm
Standard planetary models suggest that the interior of Saturn is similar to that of
Jupiter, having a small rocky core surrounded by
helium with trace amounts of various
 This core is similar in composition to the Earth, but more dense. Examination of Saturn's
gravitational moment, in combination with physical models of the interior, has allowed constraints to be placed on the mass of Saturn's core. In 2004, scientists estimated that the core must be 9–22 times the mass of the Earth,
 which corresponds to a diameter of about 25,000 km.
 This is surrounded by a thicker liquid
metallic hydrogen layer, followed by a liquid layer of helium-saturated
molecular hydrogen that gradually transitions to a gas with increasing altitude. The outermost layer spans 1,000 km and consists of gas.
Saturn has a hot interior, reaching 11,700 °C at its core, and it radiates 2.5 times more energy into space than it receives from the Sun. Jupiter's
thermal energy is generated by the
Kelvin–Helmholtz mechanism of slow
gravitational compression, but such a process alone may not be sufficient to explain heat production for Saturn, because it is less massive. An alternative or additional mechanism may be generation of heat through the "raining out" of droplets of helium deep in Saturn's interior. As the droplets descend through the lower-density hydrogen, the process releases heat by
friction and leaves Saturn's outer layers depleted of helium.
 These descending droplets may have accumulated into a helium shell surrounding the core.
diamonds have been suggested to occur within Saturn, as well as in Jupiter
bands circle Saturn. The moon Dione hangs below the rings to the right.
The outer atmosphere of Saturn contains 96.3% molecular hydrogen and 3.25% helium by volume.
 The proportion of helium is significantly deficient compared to the abundance of this element in the Sun.
 The quantity of elements heavier than helium (
metallicity) is not known precisely, but the proportions are assumed to match the primordial abundances from the formation of the Solar System. The total mass of these heavier elements is estimated to be 19–31 times the mass of the Earth, with a significant fraction located in Saturn's core region.
Trace amounts of ammonia,
methane have been detected in Saturn's atmosphere.
 The upper clouds are composed of ammonia crystals, while the lower level clouds appear to consist of either
ammonium hydrosulfide (NH
4SH) or water.
Ultraviolet radiation from the Sun causes methane
photolysis in the upper atmosphere, leading to a series of
hydrocarbon chemical reactions with the resulting products being carried downward by eddies and diffusion. This
photochemical cycle is modulated by Saturn's annual seasonal cycle.
A global storm girdles the planet in 2011. The head of the storm (bright area) passes the tail circling around the left limb.
Saturn's atmosphere exhibits a banded pattern similar to Jupiter's, but Saturn's bands are much fainter and are much wider near the equator. The nomenclature used to describe these bands is the same as on Jupiter. Saturn's finer cloud patterns were not observed until the flybys of the Voyager spacecraft during the 1980s. Since then, Earth-based
telescopy has improved to the point where regular observations can be made.
The composition of the clouds varies with depth and increasing pressure. In the upper cloud layers, with the temperature in the range 100–160 K and pressures extending between 0.5–2
bar, the clouds consist of ammonia ice. Water
ice clouds begin at a level where the pressure is about 2.5 bar and extend down to 9.5 bar, where temperatures range from 185–270 K. Intermixed in this layer is a band of ammonium hydrosulfide ice, lying in the pressure range 3–6 bar with temperatures of 190–235 K. Finally, the lower layers, where pressures are between 10–20 bar and temperatures are 270–330 K, contains a region of water droplets with ammonia in aqueous solution.
Saturn's usually bland atmosphere occasionally exhibits long-lived ovals and other features common on Jupiter. In 1990, the
Hubble Space Telescope imaged an enormous white cloud near Saturn's equator that was not present during the Voyager encounters, and in 1994 another smaller storm was observed. The 1990 storm was an example of a
Great White Spot, a unique but short-lived phenomenon that occurs once every Saturnian year, roughly every 30 Earth years, around the time of the northern hemisphere's
 Previous Great White Spots were observed in 1876, 1903, 1933 and 1960, with the 1933 storm being the most famous. If the periodicity is maintained, another storm will occur in about 2020.
The winds on Saturn are the second fastest among the Solar System's planets, after Neptune's.
Voyager data indicate peak easterly winds of 500 m/s (1,800 km/h).
 In images from the
Cassini spacecraft during 2007, Saturn's northern hemisphere displayed a bright blue hue, similar to Uranus. The color was most likely caused by
Thermography has shown that Saturn's south pole has a warm
polar vortex, the only known example of such a phenomenon in the Solar System.
 Whereas temperatures on Saturn are normally −185 °C, temperatures on the vortex often reach as high as −122 °C, suspected to be the warmest spot on Saturn.
North pole hexagonal cloud pattern
Saturn's north pole (
hexagonal wave pattern around the north polar vortex in the atmosphere at about 78°N was first noted in the Voyager images.
 The sides of the hexagon are each about 13,800 km (8,600 mi) long, which is longer than the diameter of the Earth.
 The entire structure rotates with a period of 10h 39m 24s (the same period as that of the planet's radio emissions) which is assumed to be equal to the period of rotation of Saturn's interior.
 The hexagonal feature does not shift in longitude like the other clouds in the visible atmosphere.
 The pattern's origin is a matter of much speculation. Most scientists think it is a
standing wave pattern in the atmosphere. Polygonal shapes have been replicated in the laboratory through differential rotation of fluids.
South pole vortex
HST imaging of the south polar region indicates the presence of a
jet stream, but no strong polar vortex nor any hexagonal standing wave.
NASA reported in November 2006 that Cassini had observed a "
hurricane-like" storm locked to the south pole that had a clearly defined
 Eyewall clouds had not previously been seen on any planet other than Earth. For example, images from the
Galileo spacecraft did not show an eyewall in the
Great Red Spot of Jupiter.
The south pole storm may have been present for billions of years.
 This vortex is comparable to the size of Earth, and it has winds of 550 km/h.
Cassini has observed a series of cloud features nicknamed "String of Pearls" found in northern latitudes. These features are cloud clearings that reside in deeper cloud layers.
Auroral lights at Saturn’s north pole
Saturn has an intrinsic
magnetic field that has a simple, symmetric shape – a magnetic
dipole. Its strength at the equator – 0.2
µT) – is approximately one twentieth of that of the field around Jupiter and slightly weaker than Earth's
 As a result, Saturn's
magnetosphere is much smaller than Jupiter's.
 When Voyager 2 entered the magnetosphere, the
solar wind pressure was high and the magnetosphere extended only 19 Saturn radii, or 1.1 million km (712,000 mi),
 although it enlarged within several hours, and remained so for about three days.
 Most probably, the magnetic field is generated similarly to that of Jupiter – by currents in the liquid metallic-hydrogen layer called a metallic-hydrogen dynamo.
 This magnetosphere is efficient at deflecting the
solar wind particles from the Sun. The moon Titan orbits within the outer part of Saturn's magnetosphere and contributes plasma from the
ionized particles in Titan's outer atmosphere.
 Saturn's magnetosphere, like