Cassini-Huygens, launched in 1997, was a joint mission between NASA, the European Space Agency (ESA), and the Italian Space Agency, ASI (Agenzia Spaziale Italiana). Cassini-Huygens is humanity’s first in-depth study of Saturn and its system of rings and moons. Its seven-year-long journey to Saturn included two gravity-assist fly-bys of Venus. Spacecraft use gravity-assists to increase their velocity.
Having exhausted its fuel supply, and to eliminate any chance of crashing into and contaminating potentially life-containing worlds, Cassini dove into Saturn on the morning of September 15th, to send data back to Earth until it finally disintegrates in Saturn’s atmosphere.
As it ventured into the outer solar system, Cassini-Huygens provided the most high-resolution photos of Jupiter to date. After arriving at the Saturnian system in 2004 and completing its initial survey of Saturn in 2008, Cassini would undergo two mission extensions. Cassini sent back a trove of data on Saturnian weather, and, most notably, two of Saturn’s moons, Enceladus and Titan. Because of Cassini, Enceladus and Titan are now considered to be prime candidates for harboring extraterrestrial life.
Saturn, its famous rings, and 61 known moons orbit the Sun at nearly 900 million miles, approximately ten times the average distance between the Sun and Earth. With a diameter of 72,367 miles, Saturn is made mostly of hydrogen, yet it could float on water (in a tank large enough of course) due to its low density.
Wild Weather on Saturn
Because Saturn is so far from the Sun, most of its heat comes from inside the planet. The core temperature on Saturn is 22,000 degrees Fahrenheit, nearly three times hotter than the surface of the Sun. Like Jupiter, Saturn has a nickel-iron core surrounded by liquid metallic hydrogen, a fluid created when gaseous hydrogen is under enough pressure be in a liquid state. Saturn rotates rapidly; a day on Saturn lasts only ten and a half Earth hours. Cassini observed storms in Saturn’s atmosphere, which contains the second-fastest winds in the solar system. These winds are caused by Saturn’s fast rotation and from heat coming from the planet’s interior, resulting in bands of different colors and wind speeds. In 2004, Cassini photographed two atmospheric storms merging into one. Some storms are as big as or larger than Earth. In fact, 764 earths could fit inside Saturn. Cassini also observed lightning strikes thousands of times more powerful than on Earth.
At Saturn’s north pole churns a unique, hexagon-shaped storm. Though first observed by Voyager, Cassini documented the storm in unprecedented detail. The polar storm resembles a hurricane, though the differences are vast; the eye alone is 1,250 miles in diameter, and wind speeds exceed 220 miles per hour. Amazingly, the eye of the storm descends at least as far into Saturn as Cassini can see.
Cassini helped to unlock the mysteries behind Saturn’s majestic system of rings. Saturn’s rings are composed of ice particles and chunks of rock, ranging in size from grains of sand to mountains. “The rings are believed to be pieces of comets, asteroids, or shattered moons that broke up before they reached the planet,” NASA states. Although they stretch out 175,000 miles from Saturn, the planet’s rings are remarkably thin. Their depth ranges from 33 feet to around 3,200 feet.
Cassini observed small moons embedded within the rings, whose gravity pushes ring particles apart. This causes propeller-shaped gaps to form inside the rings. In general, Saturn’s rings sit closely to one another. Separating rings B and A, however, is a 2,920-mile-wide gap called the Cassini Division. It was discovered by 17th-century astronomer Giovanni Cassini, after whom the spacecraft is named. The Cassini Division’s empty space is maintained by Mimas, a small moon orbiting Saturn within its rings. Cassini also discovered that eruptions from Enceladus are largely responsible for forming Saturn’s E-ring. Images of Saturn’s rings provided by Cassini can be found here.
Enceladus May Harbor Life
Enceladus, a 300-mile-wide ice-covered moon of Saturn, is where Cassini made its most profound discoveries. According to readings from Cassini, Enceladus has a global ocean underneath a solid water-ice crust. Water-ice ejected from Enceladus’ ice geysers analyzed by Cassini contains salt and organic compounds, the presence of which makes Enceladus a potential home for extraterrestrial life. Tidal forces between Enceladus and Saturn generate heat in the moon’s core, which enable the global ocean to remain liquid. Enceladus may even have hydrothermal vents at the bottom of its ocean. If so, they could deliver nutrients and energy for living organisms, just as hydrothermal vents do on Earth. Cassini captured unprecedented images of Enceladus and its geysers during its mission.
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