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Saturn spacecraft begins science swan-song

NASA’s Cassini probe will go where no spacecraft has gone before — between a planet and its rings.

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NASA/JPL-Caltech/Space Science Institute

Planetary scientists still debate the age and provenance of Saturn’s rings.

After 13 years exploring Saturn and its moons, NASA’s Cassini spacecraft has just 5 months left to live. But it will go out with a scientific bang.

On 22 April, Cassini will slingshot past Titan, Saturn’s largest moon, for the last time. Four days later, the probe will hurtle into the unexplored region between the giant planet and its rings. Cassini will thread that 2,400-kilometre-wide gap 22 times before its kamikaze dive into Saturn’s atmosphere on 15 September.

This unprecedented journey promises to yield fresh discoveries for the venerable spacecraft. “It will be like a whole new mission,” says Linda Spilker, Cassini’s project scientist at NASA’s Jet Propulsion Laboratory (JPL) in Pasadena, California. “There are fundamental new scientific measurements to make.”

Those include the first direct tastes of particles in Saturn’s rings, and of its upper atmosphere; the best measurements yet of the planet’s magnetic and gravitational fields, which could answer long-standing questions such as how fast the planet rotates and how old its rings are; and the sharpest look yet at the inner rings.

It all begins with the spacecraft’s final fly-by of Titan, the 127th such close encounter. Cassini will scan the moon’s methane lakes one last time, looking for waves, bubbles or other phenomena roiling the surface. Earlier fly-bys have revealed changes in the lakes over time, and the final pass is the last chance to look for seasonal shifts, says Sarah Hörst, a planetary scientist at Johns Hopkins University in Baltimore, Maryland.

Titan’s gravitational pull will fling Cassini into its ‘grand finale’ orbits, plunging between Saturn’s innermost ring and the planet’s cloud tops (see ‘Cassini: the final frontier’). The spacecraft will turn its main antenna forward, to act as a protective shield against any errant ring particles as it whizzes along at 110,000 kilometres per hour. 

Since November, the probe has been climbing higher relative to Saturn’s equatorial plane, providing a new vantage point on the planet’s outer rings. The upcoming inner dives will also reveal spectacular new details, says Carolyn Porco, a planetary scientist at the University of California, Berkeley, who leads the mission’s imaging team.

Source: NASA/JPL-Caltech/SSI

High-resolution photographs have captured mysterious propeller-shaped gaps that ripple through some of the farther-out rings, probably formed by unseen moonlets. “The rings really are changing before our eyes,” says Jeffrey Cuzzi, a planetary scientist at NASA’s Ames Research Center in Moffett Field, California.

Cassini’s remote-sensing instruments will get their closest look yet at the rings, on sides both lit and unlit by the Sun. Measurements will show how the chemical make-up of the ring particles varies from place to place — information that is crucial for researchers who are trying to tease out which compounds pollute the rings’ otherwise pure ice.

And scientists might finally unravel the rings’ biggest mystery — how old they are and how they formed. Between May and July, Cassini will make its most precise measurements of Saturn’s gravitational field; by tracking the spacecraft’s motion as it flies between the planet and the rings, mission scientists expect to improve their calculations of the mass of the rings by an order of magnitude. A relatively high mass would suggest that the rings were ancient, perhaps formed by a big moon ripped apart billions of years ago. Lighter-weight rings would suggest a more recent formation, perhaps from a visiting comet that disintegrated.

Other fundamental measurements will tackle the giant planet itself. On the grand-finale orbits, Cassini’s magnetometer will measure Saturn’s magnetic field close to the planet. There, it is roughly ten times stronger — and more complex and scientifically interesting — than in areas already probed, says Marcia Burton, a planetary scientist at JPL.

Those data should shed light on long-standing mysteries such as the depth of Saturn’s metallic hydrogen core — which powers its magnetic field — and how quickly the planet rotates. Observations by the Voyager spacecraft in the 1980s suggested that one rotation takes just under 11 hours. But the numbers are different when measured in the northern and southern hemispheres, which hints that something more complicated is going on. “It is hard to imagine how the grand-finale orbits could not lead to a huge improvement in our understanding of Saturn’s magnetic field,” Burton says.

On 15 September, with its tanks almost out of fuel, mission controllers will steer Cassini directly into Saturn. But the craft will still radio back observations of the gases that make up Saturn’s atmosphere. “Even in its final moments, Cassini will be doing groundbreaking science,” says Hörst.

Journal name:
Nature
Volume:
544,
Pages:
149–150
Date published:
()
DOI:
doi:10.1038/544149a

Corrections

Corrected:

An earlier version of this story erred in implying that the inner rings are known to contain propeller-shaped gaps. The gaps are known to exist in outer rings, but no hints have yet been seen of them in the inner ones.

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