Cassini Spacecraft Shows Saturn's Ring System Has Atmosphere

18 August 2005

Oxygen molecules held in place by gravity, ring particle movement

Data from the Cassini spacecraft indicate that Saturn's majestic ring system has its own atmosphere, separate from that of the planet, according to an August 17 press release from the European Space Agency (ESA).

The Cassini-Huygens mission is a cooperative project of NASA, ESA and Agenzia Spaziale Italiana, the Italian space agency.

During its close fly-bys of Saturn’s ring system, Cassini's instruments showed that the environment around the rings is an atmosphere composed mainly of oxygen molecules, similar to the atmospheres of Jupiter's moons Europa and Ganymede.

“As water comes off the rings, it is split by sunlight; the resulting hydrogen and atomic oxygen are then lost, leaving molecular oxygen,” said Andrew Coates, a co-investigator for one of the instruments from University College London.

Saturn's rings are mainly water ice mixed with smaller amounts of dust and rocky matter. They are very thin – no more than 1.5 kilometers, although they are 250,000 kilometers or more in diameter.

The rings’ origin is unknown. Scientists once thought they formed at the same time as the planets, coalescing from swirling clouds of interstellar gas 4,000 million years ago. But the rings now appear to be young, perhaps only hundreds of millions of years old.

Another theory suggests that a comet flew too close to Saturn and was broken up by the planet’s tidal forces. Alternatively, one of Saturn's moons might have been struck by an asteroid, smashing it into the pieces that now form the rings.

The ring system is unstable and must be constantly regenerated, probably by the breakup of larger planetary bodies. The atmosphere is likely kept in place by gravitational forces and a balance between the loss and replacement of ring particles, Coates said.

Last month, mission scientists celebrated Cassini’s first year in orbit around Saturn. The spacecraft began to orbit Saturn in July 2004 after a six-year journey of more than 3 billion kilometers.

Additional information about the mission is available on both the NASA Web site and the European Space Agency Web site.

Text of the ESA press release follows:

(begin text)

European Space Agency
[Paris, France]
Press release, August 17, 2005

Saturn’s rings have own atmosphere

Spectrum from Cassini instruments indicating atmosphere over rings

Data from the NASA/ESA/ASI Cassini spacecraft indicate that Saturn's majestic ring system has its own atmosphere -- separate from that of the planet itself.

During its close fly-bys of the ring system, instruments on Cassini have been able to determine that the environment around the rings is like an atmosphere, composed principally of molecular oxygen.

This atmosphere is very similar to that of Jupiter's moons Europa and Ganymede.

The finding was made by two instruments on Cassini, both of which have European involvement: the Ion and Neutral Mass Spectrometer (INMS) has co-investigators from USA and Germany, and the Cassini Plasma Spectrometer (CAPS) instrument has co-investigators from US, Finland, Hungary, France, Norway and UK.

Saturn's rings consist largely of water ice mixed with smaller amounts of dust and rocky matter. They are extraordinarily thin: though they are 250 000 kilometres or more in diameter they are no more than 1.5 kilometres thick.

Despite their impressive appearance, there is very little material in the rings -- if the rings were compressed into a single body it would be no more than 100 kilometres across.

The origin of the rings is unknown. Scientists once thought that the rings were formed at the same time as the planets, coalescing out of swirling clouds of interstellar gas 4000 million years ago. However, the rings now appear to be young, perhaps only hundreds of millions of years old. Another theory suggests that a comet flew too close to Saturn and was broken up by tidal forces. Possibly one of Saturn's moons was struck by an asteroid smashing it to pieces that now form the rings.

Though Saturn may have had rings since it formed, the ring system is not stable and must be regenerated by ongoing processes, probably the break-up of larger satellites.

Water molecules are first driven off the ring particles by solar ultraviolet light. They are then split into hydrogen, and molecular and atomic oxygen, by photodissocation. The hydrogen gas is lost to space, the atomic oxygen and any remaining water are frozen back into the ring material due to the low temperatures, and this leaves behind a concentration of oxygen molecules.

Dr Andrew Coates, co-investigator for CAPS, from the Mullard Space Science Laboratory (MSSL) at University College London, said: "As water comes off the rings, it is split by sunlight; the resulting hydrogen and atomic oxygen are then lost, leaving molecular oxygen.

"The INMS sees the neutral oxygen gas, CAPS sees molecular oxygen ions and an ‘electron view’ of the rings. These represent the ionised products of that oxygen and some additional electrons driven off the rings by sunlight."

Dr Coates said the ring atmosphere was probably kept in check by gravitational forces and a balance between loss of material from the ring system and a re-supply of material from the ring particles. Last month, Cassini-Huygens mission scientists celebrated the spacecraft's first year in orbit around Saturn. Cassini performed its Saturn Orbit Insertion (SOI) on 1 July 2004 after its six-year journey to the ringed planet, travelling over three thousand million kilometres.

The Cassini-Huygens mission is a co-operative project of NASA, ESA and ASI, the Italian space agency.

These findings were published by Coates, A.J., H.J. McAndrews, A.M. Rymer, D.T.Young, F.J. Crary, S. Maurice, R.E. Johnson, R. Baragiola, R.L. Tokar, E.C. Sittler, G.R.Lewis, as 'Plasma electrons above Saturn’s main rings: CAPS observations', in Geophys Res Letters, 32, L14S09, doi:10.1029/2005GL022694, 2005. Published online 18 June and in Cassini special issue 23 July 2005.

• At Saturn and Titan (http://www.esa.int/SPECIALS/Cassini-Huygens/index.html)

More about...

• Saturn's rings (http://www.esa.int/SPECIALS/Cassini-Huygens/SEMSP6HHZTD_0.html)

• More on Saturn's rings (http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=35135)

• Rippled rings (http://www.esa.int/SPECIALS/Cassini-Huygens/SEMQFCQ3K3E_0.html)

• Discoverer of Titan: Christiaan Huygens (http://www.esa.int/esaSC/SEMJRT57ESD_index_0.html)

• Astrology to astronomy: Jean-Dominique Cassini (http://www.esa.int/esaSC/SEMJ2T57ESD_index_0.html)