Saturn is second only to Jupiter in many respects in terms of size, age and line prominence, but in terms of scientific excitement, it is certainly capable of superiority. Saturn is arousing scientific interest not only as a planet, but as a system. Among its attractive qualities, Saturn has a dense ring and seductive moons that may harbor life. Space scientists from different disciplines, from geologists to atmospheric scientists to those studying the possibility of life on other worlds, can find their place in the study of a corner of the Saturn system.
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The small moon, no larger than Arizona or Colorado, has caused a sensation among scientists. The frozen spot hides a formidable secret: under its ice shell there is an ocean of liquid water. "Snow" comes from liquid water that escapes from Enceladus and falls on the moon in the form of ice particles. Although the surface experiences a cold temperature of minus 330 degrees Fahrenheit, the interior of Enceladus is blessed with a temperature of about 200 degrees Fahrenheit, thanks to the tidal heating from Saturn. The enormous gravity of the mother planet pulls the small moon and constantly pushes it until the interior is warm. As a result, the interior is warm enough to contain liquid water.
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Like Little Enceladus, Titan, Saturn's largest moon, is also a humid world and a candidate for habitation. An ocean of liquid water hides inside the moon, and on the outer surface, rivers, lakes, and seas flow with liquid methane instead of water. Kelly Miller, a planetary scientist at the Southwest Research Institute, says the moon has a methane cycle that in many respects mirrors Earth's water cycle. She and other scientists believe that the same atmospheric phenomena that occur on our planet occur on Titan, except that they are driven by methane. Like Earth, Titan has retained a large atmosphere, and is the only moon in our solar system that holds it. The atmosphere is mostly made up of nitrogen, like Earth, but it also contains complex organic molecules that paint the world with orange fog. These huge hydrocarbons, inhaled by Cassini's Huygens probe on the moon in 2005, eventually settle out of the atmosphere and cover the Earth, like a soot crust. The carbon compounds on Titan's surface are hundreds of times equivalent to Earth's fossil fuel reserves.
Every 30 years or so, a planet-sized storm forms in Saturn's atmosphere. Storms can last for months, but their effects can last for centuries. Research by University of Michigan planetary scientist Cheng Li has discovered the common culprit behind Saturn's storms: water. The molecule, which is heavy between the enormous body of hydrogen and helium that make up most of Saturn's weight, prevents heat from dissipating from the core, until it accumulates enough energy to lift the molecule from the depths in the form of steam. Lee says the mechanism is like a pressure cooker, where heavy water acts as a release valve. Eventually, the collective energy released is enough to feed a hurricane orbiting the globe.
A long-lived jet stream covers Saturn's North Pole, with the edge of the cloud following a latitude of 77 degrees. Scientists believe that the hexagonal edge has characterized the northern tip of Saturn for centuries. A central cyclone rotates directly on the pole, while smaller vortices are scattered across the rest of the hexagonal space, many of which rotate in opposite directions. The six-sided vortex was first photographed by Voyager's flights in the early eighties – almost by chance, capturing fragments and pieces of hexagon in each shot. But the existence of the hexagon only emerged when scientists revisited the images in 1988. Since then, Cassini has taken high-resolution images that unequivocally show the engineering storm in all its glory. It reveals a hurricane that extends 20,000 miles in its vicinity, reaches a height of 180 miles and rises at a speed of 300 miles per hour. The most unusual feature is the amazing symmetry of the storm. The hexagonal shape of the storm puzzled scientists.
Of all the planets in the solar system, Saturn is the only planet whose magnetic pole axis corresponds to the planet's axis of rotation. On other planets with a magnetic field, including Earth, the axis of the magnetic pole and the axis of rotation are tilted away from each other and intersect like an X. On Saturn, what you have is a perfect I. This lack of displacement hinders attempts to calculate the planet's rotational speeds using traditional methods. Researchers usually use the magnetic field to tell the time on gas giants, but they haven't figured out how to do so with Saturn's unique composition. While the length of a day on Jupiter has been determined with an accuracy of up to milliseconds, estimates of Saturn's rotation vary by 20 minutes.
Saturn is famous for its stunning rings, which stretch 175,000 miles from the planet. Scientists believe that Saturn's rings are a torn remnant of a moon that was very close to it. Ice fragments the size of mountains or as small as grains of sand circulate around the planet, constrained by its enormous gravity. This narrow gravitational handlebar makes the icy particles in the ring sensitive to rolling below. Waves in rings can reveal clues about the planet's atmosphere and inside the planet. During her lifetime, Cassini collected notes about the spirals in the episode that revealed two major discoveries. First, Saturn consists of stable gas layers and likely has a diffuse rock core. Second, layers are likely to rotate at different speeds.
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