Cassini arrived at Saturn in 2004, and the spacecraft completed its primary mission to study the planet, its rings and its moons by 2008. Its first extended mission, which lasted until 2010, was to observe the system during the planet's equinox, when the sun strikes the rings edge-on and the days are of equal length on the north and south poles. The goal of its second extended mission — a seven-year plan called the Solstice Mission — was to observe all the way up to the north pole's summer solstice (when the days are longest at Saturn's north pole, and shortest at the planet's south pole) and investigate the system's seasonal changes.
"During Cassini's Solstice Mission, we have witnessed — up close for the first time — an entire season at Saturn," Linda Spilker, Cassini project scientist at NASA's Jet Propulsion Laboratory (JPL) in California, said in a statement. "The Saturn system undergoes dramatic transitions from winter to summer, and thanks to Cassini, we had a ringside seat."
Cassini data suggests that the increased sunlight interacts with compounds in the upper atmosphere to form particles called photochemical aerosols, which accumulate into a yellowish haze. The very center may stay blue for one of two reasons, researchers said in an image caption: it hasn't been exposed to sunlight as long as the areas around it because it's at the very top of the planet, or the circulation in the whirling vortex pulls the compounds downward.
Cassini saw the seasonal changes come over the planet suddenly based on latitude, rather than gradually, the researchers said.
"Eventually, a whole hemisphere undergoes change, but it gets there by these jumps at specific latitude bands at different times in the season," Robert West, a member of Cassini's imaging team at JPL, said in the statement.
The solstice's intense sunlight heated Saturn's rings, letting Cassini's instruments better investigate ring particles' composition and the way they clump together. The planet's orientation compared to the sun and Earth, with its rings tipped maximally toward Earth, also meant that Cassini could easily send a radio signal through the densest part of the rings to investigate, according to the statement.
But some action was sudden: In 2013, haze and trace hydrocarbons formerly found only in the north suddenly built up in the Titan's south, indicating that its atmospheric circulation had changed direction due to the changing sun exposure, the statement said.
"Observations of how the locations of cloud activity change and how long such changes take give us important information about the workings of Titan's atmosphere and also its surface, as rainfall and wind patterns change with the seasons too," Elizabeth Turtle, a researcher on Cassini's imaging team at Johns Hopkins University's Applied Physics Laboratory in Maryland, said in the statement.
And on Saturn's moon Enceladus, which hosts a subsurface ocean and blasts geysers of material out through its plumes, the main seasonal change was its southern hemisphere's transition to winter darkness. This change let Cassini monitor the moon's temperature more easily, to investigate the intriguing moon.
Read more at Discovery News