Search Results - "Tiscareno, M.S"

The shape and dynamics of a heliotropic dusty ringlet in the Cassini Division by Hedman, M.M., Burt, J.A., Burns, J.A., Tiscareno, M.S.

“…The so-called “Charming Ringlet” (R/2006 S3) is a low-optical-depth, dusty ringlet located in the Laplace gap in the Cassini Division, roughly 119,940 km from…”
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Enceladus’s measured physical libration requires a global subsurface ocean by Thomas, P.C., Tajeddine, R., Tiscareno, M.S., Burns, J.A., Joseph, J., Loredo, T.J., Helfenstein, P., Porco, C.

“…•Enceladus’s south polar jets originate from a liquid reservoir.•The extent of a subsurface liquid region is not directly observable.•We precisely measured…”
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The inner small satellites of Saturn: A variety of worlds by Thomas, P.C., Burns, J.A., Hedman, M., Helfenstein, P., Morrison, S., Tiscareno, M.S., Veverka, J.

“…•Small satellites in different dynamical positions have different surface morphologies.•Ring-arc embedded moons are likely equilibrium forms of mean density…”
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Aegaeon (Saturn LIII), a G-ring object by Hedman, M.M., Cooper, N.J., Murray, C.D., Beurle, K., Evans, M.W., Tiscareno, M.S., Burns, J.A.

“…Aegaeon (Saturn LIII, S/2008 S1) is a small satellite of Saturn that orbits within a bright arc of material near the inner edge of Saturn’s G-ring. This object…”
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Three tenuous rings/arcs for three tiny moons by Hedman, M.M., Murray, C.D., Cooper, N.J., Tiscareno, M.S., Beurle, K., Evans, M.W., Burns, J.A.

“…Using Cassini images, we examine the faint material along the orbits of Methone, Anthe and Pallene, three small moons that reside between the orbits of Mimas…”
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Organizing some very tenuous things: Resonant structures in Saturn's faint rings by Hedman, M.M., Burns, J.A., Tiscareno, M.S., Porco, C.C.

“…Images of the dusty rings obtained by the Cassini spacecraft in late 2006 and early 2007 reveal unusual structures composed of alternating canted bright and…”
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Scientific rationale for Saturn׳s in situ exploration by Mousis, O., Fletcher, L.N., Lebreton, J.-P., Wurz, P., Cavalié, T., Coustenis, A., Courtin, R., Gautier, D., Helled, R., Irwin, P.G.J., Morse, A.D., Nettelmann, N., Marty, B., Rousselot, P., Venot, O., Atkinson, D.H., Waite, J.H., Reh, K.R., Simon, A.A., Atreya, S., André, N., Blanc, M., Daglis, I.A., Fischer, G., Geppert, W.D., Guillot, T., Hedman, M.M., Hueso, R., Lellouch, E., Lunine, J.I., Murray, C.D., O׳Donoghue, J., Rengel, M., Sánchez-Lavega, A., Schmider, F.-X., Spiga, A., Spilker, T., Petit, J.-M., Tiscareno, M.S., Ali-Dib, M., Altwegg, K., Bolton, S.J., Bouquet, A., Briois, C., Fouchet, T., Guerlet, S., Kostiuk, T., Lebleu, D., Moreno, R., Orton, G.S., Poncy, J.

“…Remote sensing observations meet some limitations when used to study the bulk atmospheric composition of the giant planets of our solar system. A remarkable…”
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