Results 151 to 160 of about 698 (200)

CCD photometry and spectroscopy of the outer Jovian satellites

The Astronomical Journal, 1991
openaire   +1 more source

Exo-Geoscience Perspectives Beyond Habitability. [PDF]

Space Sci Rev
Spohn T, Roberge A, Way MJ, Duarte JC, Miozzi F, Baumeister P, Byrne P, Lineweaver CH.   +7 more
europepmc   +1 more source

Inventory of the inner and irregular satellites in the Jovian system

This study presents a comprehensive inventory of the inner and irregular satellites in the Jovian system. The satellites are categorised according to the orbital parameters such as samimajor axis, orbital inclination and eccentricity, and physical characteristics such as density, visual geometric albedo and the discrete compositional characteristics ...
openaire   +1 more source

SUDA: A SUrface Dust Analyser for Compositional Mapping of the Galilean Moon Europa. [PDF]

Space Sci Rev
Kempf S, Tucker S, Altobelli N, Briois C, Cable ML, Grün E, Gudipati MS, Henderson BL, Hsu HW, Hand K, Horanyi M, Postberg F, Schmidt J, Srama R, Sternovsky Z, Tobie G, Zolotov MY, Belting C, Bortfeldt S, Bouwman J, Brennan N, Bryant K, Cassidy T, Crotser D, Curtin A, DeVito E, Ebuen D, Faber N, Fisher M, Fontanese J, Fowle M, Frank W, Gurst S, Haselschwardt S, Hoxie V, Hubbell K, James D, Kien M, Knappmiller S, Kohnert R, Lampe A, Lankton M, Lev-Tov S, McGinn C, Miller M, Newcomb G, Oberg S, O'Brien L, Pilewskie K, Polson S, Scarffe-Barrett V, Summers D, Wade S, Ware A, Yehle A, Wuerthner C, Garcia Arteaga A, Oaida B, Eberl C, Fitton P, Goode W, Levin Z, Lowry G, Stanley J, Tracy A, Ulibarri Z, Williams E, Yoke C, Southworth BS, Hillier JK, Khawaja N, Klenner F, Napoleoni M, Simolka J, Sioeng J.   +74 more
europepmc   +1 more source

Orbital stability of distant satellites of jovian planets

, 2019
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BepiColombo cruise science: overview of the mission contribution to heliophysics. [PDF]

Earth Planets Space
Sánchez-Cano B, Hadid LZ, Aizawa S, Murakami G, Bamba Y, Chiba S, Hara T, Heyner D, Ho G, Iwai K, Kilpua E, Kinoshita G, Lavraud B, Miyoshi Y, Pinto M, Schmid D, Shiota D, Vainio R, Andre N, Aronica A, Asmar S, Auster HU, Barabash S, Barthe A, Baumjohann W, Benkhoff J, Bentley M, Bunce E, Cappuccio P, Delcourt D, di Stefano I, Doria I, Dresing N, Fedorov A, Fischer D, Fiethe B, Fränz M, Gieseler J, Giner F, Giono G, Harada Y, Hussmann H, Iess L, Imamura T, Jeszenszky H, Jones G, Katra B, Kazakov A, Kozyrev A, Laky G, Lefevre C, Lichtenegger H, Lindsay S, Lucente M, Magnafico C, Magnes W, Martindale A, Matsuoka A, Milillo A, Mitrofanov I, Nishiyama G, Oleynik P, Orsini S, Paik M, Palmroos C, Plainaki C, Penou E, Persson M, Quarati F, Quémerais E, Richter I, Robidel R, Rojo M, Saito Y, Santoli F, Stark A, Stumpo M, Tian R, Varsani A, Verdeil C, Williamson H, Witasse O, Yokota S.   +82 more
europepmc   +1 more source

The Orbits of the Outer Jovian Satellites

Astronomical Journal, 2000
We report on the numerically integrated orbits for the nine outer Uranian satellites. The orbits are calculated based on fits to the astrometric observations for the period from 1984 to 2006. The results include the state vectors, post-fit residuals, and mean orbital elements.
R A Jacobson
exaly   +2 more sources

The Galilean satellites as a source of CO in the Jovian upper atmosphere

Icarus, 1979
Material from the Galilean satellites of Jupiter ejected by energetic particles in the Jovian magnetosphere may provide large sources of oxygen to the parent planet.
Darrell F Strobel, Yuk L Yung
exaly   +1 more source

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Multicolor photometry of outer Jovian satellites

Icarus, 1984
Multicolor photometry was obtained of satellites J6 Himalia, J7 Elara, and J10 Lysithea in the prograde cloud of outer Jovian satellites, and of J8 Pasiphae, J9 Sinope, and J11 Carme in the retrograde cloud. The data for J9 are fragmentary; otherwise, the satellites all look like C-class asteroids, except J11, which shows a remarkable brightness in the
David J Tholen, B Zellner
exaly   +2 more sources

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
openaire   +1 more source