The hexagonal vortex at Saturn’s north pole changed color significantly between June 2013 (left) and April 2017 (right), as seen in views from the Cassini spacecraft. For the left image, each frame occurs approximately 130 minutes after the previous one, and for the right, each frame follows after an average of 230 minutes. Researchers combined images taken with the spacecraft’s red, green and blue filters for the natural-color views.
Credit: NASA/JPL-Caltech/Space Science Institute/Hampton University
The Cassini spacecraft at Saturn watched over the ringed planet’s solstice yesterday (May 24), accomplishing the main goal of its second extended mission. A solstice occurs on Saturn roughly every 15 Earth years as its seasons change.
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.” [Epic Cassini Mission to Saturn Gets Awesome Video Treatment ]
A giant storm passed by its own tail after circling Saturn in this true-color Cassini photo, taken Feb. 25, 2011, about 12 weeks after the storm started. Lightning deep in the planet’s atmosphere produced significant radio noise during the storm. The storm formed and dispersed over the course of seven months; researchers said this type of Saturn storm happens only about every 30 Earth years.
Credit: NASA/JPL-Caltech/Space Science Institute
During the Solstice Mission, researchers watched a huge storm encircle the planet and disperse over the course of seven months. They watched the hexagonal jet stream surrounding Saturn’s north pole change from blue to yellow (except for the very center) over the course of the northern hemisphere’s spring.
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.
Storms on Saturn’s moon Titan changed as Saturn moved through equinox and toward solstice. In this 2011 image, methane clouds can be seen concentrated near the moon’s equator.
Credit: NASA/JPL-Caltech/Space Science Institute
On Saturn’s largest moon, Titan, methane storm clouds shifted up from the south toward the moon’s equator from 2004 to 2010. Their corresponding shift northward as the solstice approached was surprisingly slow; according to the statement, cloud models had expected the activity to happen years earlier.
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.
Cassini is in the middle of the “Grand Finale” phase of its mission, in which it is diving between Saturn and its rings repeatedly to investigate the planet more closely than ever before. Once it finishes seeing the planet through the change of seasons and charting its moons, rings and surface as deeply as possible, Cassini will plunge into Saturn’s atmosphere on Sept. 15. The mission is a collaboration among NASA, the European Space Agency and the Italian Space Agency.
Email Sarah Lewin at slewin@space.com or follow her @SarahExplains . Follow us @Spacedotcom , Facebook and Google+ . Original article on Space.com .
Comments are closed.