Results 161 to 170 of about 6,474 (200)

Jovian satellite nomenclature

Icarus, 1976
A brief review of the history of Jovian satellite nomenclature is given to indicate the background for the names proposed for the numbered satellites. The new names are consistent with established tradition and should cause minimal confusion with other named objects in the solar system.
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The Orbits of the Retrograde Jovian Satellites

Icarus, 1993
Abstract The orbits of Jupiter's four retrograde satellites are strongly perturbed by the Sun and therefore resist treatment by the perturbative methods of classical celestial mechanics. We have integrated the orbits of these satellites over an interval of 2 Myr. We confirm the finding of A.L. Whipple and P.J.
Prasenjit Saha, Scott Tremaine
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Jovian satellite-satellite eclipses and occultations

Icarus, 1973
Toward the end of 1973 and in the first part of 1974, when the planes of the orbits of the four large Galilean satellites cross the sun and the earth, satellite-satellite eclipses and occultations will occur. Calculations indicate that during this period 350 such events will occur, most of them potentially observable. From observation of a few of these
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Mutual phenomena of Jovian satellites

Journal of Astrophysics and Astronomy, 1991
Results of the observations of mutual eclipses of Galilean satellites observed from the Vainu Bappu Observatory during 1985 are presented. Theoretical models assuming a uniform disc, Lambert’s law and Lommel-Seeliger’s law describing the scattering characteristics of the surface of the eclipsed satellite were used to fit the observations.
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Filamentation of Volcanic Plumes on the Jovian Satellite IO

Astrophysics and Space Science, 1988
Volcanic plumes on the Jovian satellite Io may be a visible manifestation of a plasma-arc discharge phenomenon. The amount of power in the plasma arc (~ 1011 W) is not enough to account for all the energy dissipated by the volcanoes. However, once a volcano is initiated by tidal and geologic processes, the dynamics of the volcanic plumes can be ...
Anthony L. Peratt, A. J. Dessler
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Another 'Ocean' for a Jovian Satellite?

Science, 1999
PLANETARY SCIENCEObservations from the ground and the Galileo spacecraft suggest the existence of an ocean on the fiery Jovian satellite Io. But there are no tantalizing prospects for life in Io's proposed ocean. At something like 2000 Kelvin, the ocean seething beneath Io's volcanoes and lava lakes would vaporize the hardiest creature, for this ocean ...
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Dielectric Measurements of Saline Ices: Implication for Jovian Satellites Radar Exploration

Proceedings, 2011
A spacecraft in orbit around Jupiter's moon Ganimede can use ice penetrating radar to probe for a possible liquid water ocean beneath Ganimede's surface ice. The success of such a mission is constrained to the electromagnetic properties of ice, possible subsurface temperature gradients, and possible impurities in the ice.
De Santis M, Lauro S E, Mattei E, Cosciotti B, Pettinelli E, Vannaroni G   +5 more
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Regions of possible motions for new Jovian satellites

Solar System Research, 2007
We present the results of our simulation and study of the regions of possible motions for 46 newly discovered Jovian satellites. We show that the orbits of some satellites (such as S/2003 J02, S/2003 J03, S/2003 J04, S/2003 J10, S/2003 J12, and S/2003 J23) presently cannot yet be determined with an acceptable accuracy for planning observations, because
V. A. Avdyushev, M. A. Banschikova
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Jovian satellite positions from Hubble Space Telescope images

Icarus, 2004
An accurate technique has been developed for measuring planetocentric positions of Jupiter's satellites from Wide Field/Planetary Camera images. Our method of finding the centers of the satellites and planet is based upon established limb-fitting techniques, but we have adapted those techniques to astrometry.
Anthony Mallama, Halley M Aelion, Celeste A Mallama   +2 more
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1979J2: The Discovery of a Previously Unknown Jovian Satellite

Science, 1980
During a detailed examination of imaging data taken by the Voyager 1 spacecraft within 4.5 hours of its closest approach to Jupiter, a shadow-like image was observed on the bright disk of the planet in two consecutive wide-angle frames. Analysis of the motion of the image on the Jovian disk proved that it was not an atmospheric feature ...
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