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Journal ArticleDOI

The Structure of Jupiter's Ring System as Revealed by the Galileo Imaging Experiment

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TLDR
The tenuous jovian ring system (normal optical depths <10−5) has three components: the halo, main ring, and gossamer ring as mentioned in this paper, which are observed during four orbits of Galileo's nominal mission, when 25 clear-filter images of the rings were taken at spatial resolutions of 23 to 134 km/pixel; the ring appeared fortuitously in an additional 11 images.
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This article is published in Icarus.The article was published on 1999-04-01. It has received 106 citations till now. The article focuses on the topics: Jupiter & Ring (chemistry).

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The Exoplanet Handbook

TL;DR: In this paper, the authors present an overview of the solar system and its evolution, including the formation and evolution of stars, asteroids, and free-floating planets, as well as their internal and external structures.
Journal ArticleDOI

Energetic Ion and Electron Irradiation of the Icy Galilean Satellites

TL;DR: Galileo Orbiter measurements of energetic ions (20 keV to 100 MeV) and electrons (20-700 keV) in Jupiter's magnetosphere are used, in conjunction with the JPL electron model (less than 40 MeV), to compute irradiation effects in the surface layers of Europa, Ganymede, and Callisto as mentioned in this paper.

The Exoplanet Handbook: Formation and evolution

TL;DR: An overview of the processes described in this chapter is as follows in this paper, where the authors start with star formation in molecular clouds, and then gravitationally accumulate their mantles of ice and/or gas.
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The formation of Jupiter's faint rings

TL;DR: Observations by the Galileo spacecraft and the Keck telescope showed that Jupiter's outermost (gossamer) ring is actually two rings circumscribed by the orbits of the small satellites Amalthea and Thebe, suggesting that faint rings may accompany all small inner satellites of the other jovian planets.
References
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Journal ArticleDOI

Mechanism for the acceleration and ejection of dust grains from Jupiter's magnetosphere

TL;DR: In this article, the Ulysses mission detected quasi-periodic streams of high-velocity submicron-sized dust particles during its encounter with Jupiter, and it was shown how the dust events could result from the acceleration and subsequent ejection of small grains by Jupiter's magnetosphere.
Journal ArticleDOI

The formation of Jupiter's faint rings

TL;DR: Observations by the Galileo spacecraft and the Keck telescope showed that Jupiter's outermost (gossamer) ring is actually two rings circumscribed by the orbits of the small satellites Amalthea and Thebe, suggesting that faint rings may accompany all small inner satellites of the other jovian planets.
Journal ArticleDOI

The main magnetic field of Jupiter

TL;DR: The main magnetic field of Jupiter has been measured by the Goddard Space Flight Center flux gate magnetometer on Pioneer 11 as discussed by the authors, which yields a more detailed model than that obtained from Pioneer 10 results.
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Towards a theory for the Uranian rings

TL;DR: In this article, the authors proposed that the rings of Uranus are confined in radius by gravitational torques from a series of small satellites that orbit within the ring system, and suggested that apse alignment is maintained by the self-gravity of the ring.
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