Results 111 to 120 of about 7,946 (214)
Orbital theories of outer planet satellites [PDF]
An analytical theory of Mimas and Tethys was developed, retaining terms which produce perturbations of the order of + or - 10 km. The theory uses a novel set of variables, and was developed with the Hori-Lie algorithm, using the algebraic manipulation ...
Jefferys, W. H.
core +1 more source
Particle-in-cell Simulations of Plasma Oscillations Excited by Dust Impacts
Dust-impact-induced plasma oscillations (dust ringing) detected in Saturn’s Enceladus plume provide a novel method for measuring electron density. However, since S. Ye et al. discovered such events, their underlying mechanisms remain unclear.
Han Wu +7 more
doaj +1 more source
Origin and Evolution of Enceladus's Tidal Dissipation. [PDF]
Nimmo F, Neveu M, Howett C.
europepmc +1 more source
Enceladus’ long-period physical librations
The predicted long-period librational response of Saturn’s moon Enceladus proceeds on the assumption that the spin pole is inertially fixed. Actually, the spin pole is expected to occupy a Cassini state where it tracks the motion of the precessing orbit pole.
Giese, B., Rambaux, N.
openaire +2 more sources
Ammonia as a parameter shaping habitability on icy moons. [PDF]
Hopton CM, Cockell CS.
europepmc +1 more source
As above, not so below: Ion fractionation in planetary analog ices. [PDF]
Buffo JJ +11 more
europepmc +1 more source
Unraveling the complex inventory of biorelevant organics in the plumes of icy moons. [PDF]
Kaiser RI.
europepmc +1 more source
Author Correction: Ammonia sets limit to life and alters physiology independently of pH in Halomonas meridiana. [PDF]
Hopton CM, Nienow P, Cockell CS.
europepmc +1 more source

