Jupiter - friend or foe? II: the Centaurs

Jupiter - friend or foe? III: the Oort cloud comets

Jupiter - Friend or Foe? IV: The influence of orbital eccentricity and inclination

Jupiter - Structure and composition of the upper atmosphere

Jupiter and Galilean satellites' positions obtained in April 1978 with the GPO 40 CM /f = 4 m/ of the ESO, La Silla

Jupiter and Saturn Rotation Periods

Jupiter and Super-Earth embedded in a gaseous disc

Jupiter and the boron problem

Jupiter Emission Observed Near 1 MHz

Jupiter Hot Spot Makes Trouble For Theory

Jupiter models with improved ab initio hydrogen EOS (H-REOS.2)

Jupiter radio bursts and particle acceleration

Jupiter's composition: sign of a (relatively) late formation in a chemically evolved protosolar disk

Jupiter's Decametric Rotation Period

Jupiter's Galilean Satellites

Jupiter's hydrocarbons observed with ISO-SWS: vertical profiles of C2H6 and C2H2, detection of CH3C2H

Jupiter's magnetic field as revealed by the synchrotron radiation belts. I. Comparison of a 3-D reconstruction with models of the field

Jupiter's magnetic field as revealed by the synchrotron radiation belts. II. Change of the 2-D brightness distribution with D_E

Jupiter's Magnetosphere: The Nearest Astrophysical Plasma

Jupiter's molecular hydrogen layer and the magnetic field