LASP scientists ready for Cassini’s grand finale

During its “Grand Finale,” the Cassini mission studied a never-before-explored region very close to Saturn. The spacecraft has taken ultra-close images of the planet’s rings and clouds, while revealing new details about its interior and the origins of the rings. After 22 of these week-long orbits, on September 15, 2017, the spacecraft will plunge into the giant planet’s upper atmosphere, where it will burn up like a meteor, ending the epic mission to the Saturn system. (Courtesy NASA/JPL)

LASP planetary scientist Larry Esposito has been eyeing the fabulous rings of Saturn for much of his career, beginning as a team scientist on NASA’s Pioneer 11 mission when he discovered the planet’s faint F ring in 1979.

He followed that up with observations of Jupiter’s and Saturn’s rings from the Voyager and Galileo spacecraft, which carried instruments designed and built at LASP. Now, as the principal investigator for the Ultraviolet Imaging Spectrograph (UVIS) on the Cassini-Huygens mission to Saturn, Esposito and his Cassini colleagues are feeling a bit somber as the mission nears its end. The spacecraft has run out of fuel and will disintegrate in Saturn’s dense atmosphere early on the morning of Sept. 15.

“We are still making discoveries about the Saturn system studying the Cassini data, and we expect to be making them for some time,” said Esposito, a professor of astrophysical and planetary sciences at the University of Colorado Boulder. “But September 15th will be a bittersweet ending to a mission that has fascinated us as scientists and enthralled the public with images and new findings for many years.”

The $12 million UVIS instrument suite, a set of telescopes used to measure ultraviolet light from the Saturn system, has been used to study the structure and evolution of Saturn’s rings; the chemistry, clouds, and energy balance of Saturn and its icy moon Titan; and the surfaces and atmospheres of some of Saturn’s 62 known moons, said Esposito.

Launched in 1997 and pulling up at Saturn in 2004 for the first of hundreds of orbits through the Saturnian system, the mission has fostered scores of dazzling discoveries. These include in-depth studies that date and even weigh the astonishing rings; the discovery of methane lakes on Titan; plumes of water found squirting from the moon Enceladus; and close-up views of the bright auroras at the planet’s poles.

One of Esposito’s favorite discoveries using UVIS was the detection of a huge cloud of neutral oxygen atoms in the Saturn system on approach in 2003, which puzzled scientists for years. Subsequent research by the Cassini team indicated the oxygen atoms were coming from a salty, subterranean ocean on Enceladus, which scientists think may have conditions favorable for primitive life.

Many discoveries by Esposito and his UVIS team involve Saturn’s rings—made up of ice, rocks, and moonlets as large as Mt. Everest—the ages of which have been debated for decades. Esposito, who used observations from the Voyager mission to compare the rings of Saturn, Jupiter, and Neptune, believes Saturn’s rings may be as old as the solar system, which is believed to have formed some 4.6 billion years ago.

“When the two Voyager spacecraft passed by Saturn in 1980 and 1981, we thought the rings were relatively young,” Esposito said. “But data from Cassini are consistent with the picture that Saturn has had rings throughout its history. We see extensive, rapid recycling of ring material in which moons are continually shattered into ring particles, which then gather and reform moons.”

Esposito likened the ever-changing rings at Saturn to construction in Beijing, China, where marble from structures erected during the Ming Dynasty (1368-1644) is being recycled to build new structures today.

“The same sort of thing is happening with Saturn’s rings,” Esposito said. “They are renewed continually, so the rings themselves can be ancient, but the structures we see today are just part of their current manifestation. We have even watched the rings changing over the course of this mission.”

The UVIS instrument will be turned on during Cassini’s final dive into Saturn’s atmosphere, taking data and routing it to Earth until the mission is over, said Esposito, one of many mission scientists who gathered at NASA’s Jet Propulsion Laboratory (JPL) in Pasadena, California for Cassini’s final plunge.

Other UVIS team members at LASP include Ian Stewart, George Lawrence, William McClintock, Alain Jouchoux, Greg Holsclaw, Emilie Royer, Anya Portyankina, Michael Aye, and Nicole Albers. A gallery of images from the UVIS instrument is located here: https://go.nasa.gov/2xZw5xn.

The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency, and the Italian Space Agency. JPL, a division of Caltech, manages the mission for NASA’s Science Mission Directorate, Washington. JPL designed, developed, and assembled the Cassini orbiter.

LASP is the only university-based research institute to have designed and built instruments that have visited every planet in the solar system, plus Pluto. LASP students control four NASA satellites from campus, and there are about 120 undergraduate and graduate students working there on different aspects of flight projects, ranging from engineering and spacecraft operations to data management and science analysis.

This story originally appeared in CU Boulder Today: http://www.colorado.edu/today/2017/09/13/cu-boulder-scientists-ready-cassini-mission-grand-finale.

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