. 24/7 Space News .
SATURN DAILY
Saturn's bulging core implies moons younger than thought
by Staff Writers
Ithaca NY (SPX) Dec 09, 2016


While Saturn is mostly a gigantic shroud of liquid hydrogen and liquid helium, it contains a rocky core - about 18 times the size of Earth, which responds to tidal forces from all of Saturn's major moons by bulging. The forces of the bulging core, in turn, push the moons slightly away.

Freshly harvested data from NASA's Cassini mission reveals that the ringed planet's moons may be younger than previously thought. "All of these Cassini mission measurements are changing our view of the Saturnian system, as it turns our old theories upside down," said Radwan Tajeddine, Cornell University research associate in astronomy and a member of the European-based Encelade scientific team that pored over the Cassini data and published a paper in the astronomy journal Icarus (January 2017).

The Encelade team - lead by Valery Lainey of the Paris Observatory - provided two key measurements in the research: the rigidity of the tidal bulge, or the Love number - named for Augustus E.H. Love, a famed British mathematician who studied elasticity - and the dissipation factor, which controls the speed at which moons move away.

While Saturn is mostly a gigantic shroud of liquid hydrogen and liquid helium, it contains a rocky core - about 18 times the size of Earth, which responds to tidal forces from all of Saturn's major moons by bulging. The forces of the bulging core, in turn, push the moons slightly away. "Those two parameters - the Love number and dissipation factor - are difficult to separate," Tajeddine said.

So the team detected and examined the orbits of four tiny moons associated with the larger moons Tethys (Telesto and Calypso) and Dione (Helene and Polydeuces). While these tiny moons do not affect the tidal forces on Saturn, their orbits are disturbed by Saturn's core tidal bulges.

"By monitoring these disturbances, we managed to obtain the first measurement of Saturn's Love number and distinguish it from the planet's dissipation factor," Tajeddine said. "The moons are migrating away much faster than expected."

Tajeddine explains that if Saturn moons actually formed 4.5 billion years ago, their current distances from the home planet should be greater. Thus, this new research suggests, the moons are younger than 4.5 billion years, favoring a theory that the moons formed from Saturn's rings.

The team also found that Saturn moon Rhea is moving away 10 times faster than the other moons, which is the first evidence that a planet's dissipation factor can vary with its distance in relation to the moon. The scientists have no definitive explanation.

"What we believe about Saturn's moons history might still change in the coming years with the finale of the Cassini mission," said Lainey, who suggested, "The more we learn about Saturn, the more we learn about exoplanets."

Research paper


Comment on this article using your Disqus, Facebook, Google or Twitter login.


Thanks for being here;
We need your help. The SpaceDaily news network continues to grow but revenues have never been harder to maintain.

With the rise of Ad Blockers, and Facebook - our traditional revenue sources via quality network advertising continues to decline. And unlike so many other news sites, we don't have a paywall - with those annoying usernames and passwords.

Our news coverage takes time and effort to publish 365 days a year.

If you find our news sites informative and useful then please consider becoming a regular supporter or for now make a one off contribution.
SpaceDaily Contributor
$5 Billed Once


credit card or paypal
SpaceDaily Monthly Supporter
$5 Billed Monthly


paypal only


.


Related Links
Cornell University
Explore The Ring World of Saturn and her moons
Jupiter and its Moons
The million outer planets of a star called Sol
News Flash at Mercury






Share this article via these popular social media networks
del.icio.usdel.icio.us DiggDigg RedditReddit GoogleGoogle

Previous Report
SATURN DAILY
Cassini Beams Back First Images from New Orbit
Pasadena CA (JPL) Dec 07, 2016
NASA's Cassini spacecraft has sent to Earth its first views of Saturn's atmosphere since beginning the latest phase of its mission. The new images show scenes from high above Saturn's northern hemisphere, including the planet's intriguing hexagon-shaped jet stream. Cassini began its new mission phase, called its Ring-Grazing Orbits, on Nov. 30. Each of these weeklong orbits - 20 in all - c ... read more


SATURN DAILY
Early US astronauts faced uncertainty, danger and death

NASA Tech - it's all around us

NASA Communications Network to Double Space Station Data Rates

NASA's Exo-Brake 'Parachute' to Enable Safe Return for Small Spacecraft

SATURN DAILY
Technical glitch postpones NASA satellite launch

After glitch, NASA satellite launch set for Wednesday

NASA Engineers Test Combustion Chamber to Advance 3-D Printed Rocket Engine Design

ULA launches eighth Wideband Global SATCOM satellite

SATURN DAILY
Mars Rock-Ingredient Stew Seen as Plus for Habitability

ExoMars orbiter images Phobos

Mars One puts back planned colonisation of Red Planet

Opportunity team plot path forward to the 'Gully'

SATURN DAILY
Chinese missile giant seeks 20% of a satellite market

China-made satellites in high demand

Space exploration plans unveiled

China launches 4th data relay satellite

SATURN DAILY
Air New Zealand signs contract for Inmarsat's GX Aviation

UAE launches national space policy

European ministers ready ESA for a United Space in Europe in the era of Space 4.0

Nordic entrepreneurial spirit boosted by space

SATURN DAILY
Japan launches 'space junk' collector

Teaching an old satellite new tricks

Orbital ATK to develop critical technology for in-orbit assembly

Decoding cement's shape promises greener concrete

SATURN DAILY
Who needs a body? Not these larvae, which are basically swimming heads

Scientists examine bacterium found 1,000 feet underground

Rings around young star suggest planet formation in progress

ALMA finds compelling evidence for pair of infant planets around young star

SATURN DAILY
Juno Mission Prepares for December 11 Jupiter Flyby

Research Offers Clues About the Timing of Jupiter's Formation

New Perspective on How Pluto's "Icy Heart" Came to Be

New analysis adds to support for a subsurface ocean on Pluto









The content herein, unless otherwise known to be public domain, are Copyright 1995-2024 - Space Media Network. All websites are published in Australia and are solely subject to Australian law and governed by Fair Use principals for news reporting and research purposes. AFP, UPI and IANS news wire stories are copyright Agence France-Presse, United Press International and Indo-Asia News Service. ESA news reports are copyright European Space Agency. All NASA sourced material is public domain. Additional copyrights may apply in whole or part to other bona fide parties. All articles labeled "by Staff Writers" include reports supplied to Space Media Network by industry news wires, PR agencies, corporate press officers and the like. Such articles are individually curated and edited by Space Media Network staff on the basis of the report's information value to our industry and professional readership. Advertising does not imply endorsement, agreement or approval of any opinions, statements or information provided by Space Media Network on any Web page published or hosted by Space Media Network. General Data Protection Regulation (GDPR) Statement Our advertisers use various cookies and the like to deliver the best ad banner available at one time. All network advertising suppliers have GDPR policies (Legitimate Interest) that conform with EU regulations for data collection. By using our websites you consent to cookie based advertising. If you do not agree with this then you must stop using the websites from May 25, 2018. Privacy Statement. Additional information can be found here at About Us.