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This is an archive of AGU's GeoSpace blog through 1 July 2020. New content about AGU research can be found on Eos and the AGU newsroom.

You are browsing the archive for Cassini Archives - GeoSpace.

14 January 2020

Final images from Cassini spacecraft

For the last leg of its journey, Cassini was put on a particularly daring orbit passing between Saturn and its rings which brought it closer to Saturn than ever before. This allowed scientists to obtain images of Saturn’s ultraviolet auroras in unprecedented resolution. The new observations are detailed in two new studies published in the AGU journals.

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27 December 2018

Rings make Saturn shadier, bluer and less hazy in winter

Saturn’s rings act like Venetian blinds that block sunlight for the hemisphere that’s tilted farther away from the Sun, limiting winter sunlight. This cuts down on the planet’s haze and golden glow.

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24 October 2018

Researchers describe likely origin of perfect lines on Saturn’s moon

Strange features on Saturn’s moon Dione resembling lines of latitude on a map could be the result of space dust crashing onto Dione’s surface, according to a new study. The streaks have puzzled scientists because of their orientation and straightness, but a new study finds these features, deemed linear virgae, likely originated from low-velocity impacts of space debris from within the Saturn system or beyond.

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9 July 2018

Listen: The sound of electromagnetic energy moving between Saturn, Enceladus

New research from Cassini’s up-close Grand Finale orbits shows a surprisingly powerful and dynamic interaction of plasma waves moving from Saturn to its moon Enceladus and its rings.

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21 June 2016

Saturn moon Enceladus’ ice shell likely thinner than expected

A vast ocean of water beneath the icy crust of Saturn’s moon Enceladus may be more accessible than previously thought, according to new research. A new study has revealed that near the moon’s poles, the ice covering Enceladus could be just two kilometers (one mile) thick—the thinnest known ice shell of any ocean-covered moon. The discovery not only changes scientists’ understanding of Enceladus’ structure, but also makes the moon a more appealing target for future exploration, according to the study’s authors.

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17 December 2015

Scientists Map Titan’s Lakes, Revealing Clues to their Origins

As Saturn’s largest moon, Titan earns its name. It’s also the only known body other than Earth with seas, numerous surface lakes, and even rainy weather. Now scientists have mapped out Titan’s polar lakes for the first time, revealing information about the moon’s climate and surface evolution. They found that the lakes formed differently than had been previously thought—and differently than any lakes on Earth.

A collaboration of scientists led by Alexander Hayes of Cornell University presented their findings at the 2015 American Geophysical Union Fall Meeting. They used NASA’s Cassini spacecraft to penetrate Titan’s smoggy atmosphere and probe the complex lake systems below.

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16 December 2010

Saturn’s moonlets play hide-and-seek

Everyone knows Saturn has rings. Lots of them. They’re big, easily visible, and have achieved iconic status.

But did you know that hiding within those rings are tiny, tiny moons, some less than a kilometer across?

The moons–or moonlets–are so small they’re invisible even to the Cassini spacecraft buzzing around Saturn. But we know they’re there: we can see the distinctive, propeller-shaped patterns they make in Saturn’s rings as they orbit the plane

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29 November 2010

What can geysers tell us about volcanoes on Earth and on distant moons?

Susan Kieffer’s research focuses on geological fluid dynamics with an emphasis on geysers, rivers, meteorite impacts, and volcanoes. An interview provided a good opportunity to catch up with her on planetary science, her career, and current research.

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