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Composition of Saturnian Stream Particles
DOI: 10.1126/science.1106218 Bibcode: 2005Sci...307.1274K

Postberg, Frank; Grün, Eberhard; Kempf, Sascha +9 more

During Cassini's approach to Saturn, the Cosmic Dust Analyser (CDA) discovered streams of tiny (less than 20 nanometers) high-velocity (~100 kilometers per second) dust particles escaping from the saturnian system. A fraction of these impactors originated from the outskirts of Saturn's dense A ring. The CDA time-of-flight mass spectrometer recorde…

2005 Science
Cassini 60
Oxygen Ions Observed Near Saturn's A Ring
DOI: 10.1126/science.1105734 Bibcode: 2005Sci...307.1260W

Luhmann, J. G.; Ip, W. -H.; Mueller-Wodarg, I. +8 more

Ions were detected in the vicinity of Saturn's A ring by the Ion and Neutral Mass Spectrometer (INMS) instrument onboard the Cassini Orbiter during the spacecraft's passage over the rings. The INMS saw signatures of molecular and atomic oxygen ions and of protons, thus demonstrating the existence of an ionosphere associated with the A ring. A like…

2005 Science
Cassini 50
Energetic Neutral Atom Emissions from Titan Interaction with Saturn's Magnetosphere
DOI: 10.1126/science.1109805 Bibcode: 2005Sci...308..989M

Krimigis, S. M.; Mitchell, D. G.; Roelof, E. C. +3 more

The Cassini Magnetospheric Imaging Instrument (MIMI) observed the interaction of Saturn's largest moon, Titan, with Saturn's magnetosphere during two close flybys of Titan on 26 October and 13 December 2004. The MIMI Ion and Neutral Camera (INCA) continuously imaged the energetic neutral atoms (ENAs) generated by charge exchange reactions between …

2005 Science
Cassini 41
Cassini Discovers a Kinematic Spiral Ring Around Saturn
DOI: 10.1126/science.1119387 Bibcode: 2005Sci...310.1300C

Charnoz, S.; Porco, C. C.; Déau, E. +4 more

Since the time of the Voyager flybys of Saturn in 1980-1981, Saturn's eccentric F ring has been known to be accompanied on either side by faint strands of material. New Cassini observations show that these strands, initially interpreted as concentric ring segments, are in fact connected and form a single one-arm trailing spiral winding at least th…

2005 Science
Cassini 39
How Long Is the Day on Saturn?
DOI: 10.1126/science.1104956 Bibcode: 2005Sci...307.1223S

Sánchez-Lavega, Agustín

Determining a planet's rotation period can be difficult if the planet lacks a solid surface. However, for planets with an internal magnetic field, emissions at radio wavelengths are modulated by the planet's rotation rate. The latest results from the Cassini spacecraft seem to indicate that Saturn's rotation rate has slowed down by 6 minutes since…

2005 Science
Cassini 24
Saturn's Variable Magnetosphere
DOI: 10.1126/science.1108226 Bibcode: 2005Sci...307.1224G

Hansen, Kenneth C.; Gombosi, Tamas I.

Since the Cassini spacecraft reached Saturn's orbit in 2004, its instruments have been sending back a wealth of data on the planet's magnetosphere (the region dominated by the magnetic field of the planet). In this Viewpoint, we discuss some of these results, which are reported in a collection of reports in this issue. The magnetosphere is shown t…

2005 Science
Cassini 9