Results 21 to 30 of about 3,019 (208)

Geology of the Selk crater region on Titan from Cassini VIMS observations [PDF]

open access: yes, 2010
International audienceObservations of Titan obtained by the Cassini Visual and Infrared Mapping Spectrometer (VIMS) have revealed Selk crater, a geologically young, bright-rimmed, impact crater located similar to 800 km north-northwest of the Huygens ...
Brown, R.H.   +19 more
core   +1 more source

Structural geology of Ganymede regional groove systems (60°N–60°S)

open access: yesJournal of Maps, 2020
Brittle deformation on Ganymede surface is represented by grooves tectonic linear landforms. These are regional scale structures that show well-defined morphology from straight to curvilinear. High density of grooves occupies most of the light terrain of
Costanza Rossi   +2 more
doaj   +1 more source

The NIR transmission spectrum of Jupiter from the observation of a Ganymede’s eclipse

open access: yesEPJ Web of Conferences, 2015
Here, we report the NIR transmission spectrum of Jupiter, with high signal-to-noise ratio, as if it were a transiting planet. Our technique was to observe Ganymede, when crossing Jupiter’s shadow.
Montañés-Rodríguez P.   +4 more
doaj   +1 more source

Early Stages of Galilean Moon Formation in a Water-depleted Environment

open access: yesThe Astrophysical Journal Letters, 2023
A key feature of the Galilean satellite system is its monotonic decrease in bulk density with growing distance from Jupiter, indicating an ice mass fraction that is zero in the innermost moon Io and about half in the outer moons Ganymede and Callisto ...
Olivier Mousis   +5 more
doaj   +1 more source

The generation of Ganymede's diffuse aurora through pitch angle scattering [PDF]

open access: yesAnnales Geophysicae, 2017
Diffuse auroral intensities of neutral atomic oxygen OI λ1356 Å emission on Ganymede due to whistler mode waves are estimated. Pitch angle diffusion of magnetospheric electrons into the loss cone due to resonant wave–particle interaction of whistler ...
A. K. Tripathi   +2 more
doaj   +1 more source

Evidence for Magnetic Reconnection at Ganymede's Upstream Magnetopause During the PJ34 Juno Flyby

open access: yesGeophysical Research Letters, 2022
Juno made a close flyby of Ganymede and flew through its magnetosphere on 7 June 2021, including an outbound crossing of Ganymede's upstream magnetopause. We present plasma and magnetic field observations near the upstream magnetopause from Juno's Jovian
R. W. Ebert   +16 more
doaj   +1 more source

Juno Magnetometer Observations at Ganymede: Comparisons With a Global Hybrid Simulation and Indications of Magnetopause Reconnection

open access: yesGeophysical Research Letters, 2022
Juno's flyby of Ganymede on 7 June 2021, provides a unique opportunity to explore the moon's magnetosphere. By means of Magnetometer (MAG) observations and a hybrid numerical simulation, we provide a global description of this environment and analyze the
N. Romanelli   +11 more
doaj   +1 more source

Mapping and analysis of bulged impact craters on Ganymede

open access: yes, 2022
reservedABSTRACT - L’obiettivo di questa tesi è quello di studiare la morfologia e la distribuzione dei crateri d’impatto sulla superficie di Ganimede, focalizzandoci principalmente su quelli definiti di tipo “bulged”.
PAOLI, CRISTIANO
core  

Thermal Convection in the Core of Ganymede Inferred from Liquid Eutectic Fe-FeS Electrical Resistivity at High Pressures

open access: yesCrystals, 2021
The core of Ganymede is suggested to be mainly Fe but with a significant proportion of S. Effects of S as a core constituent are freezing-point depression, allowing for a molten core at relatively low core temperatures, and modification of transport ...
Joshua A. H. Littleton   +2 more
doaj   +1 more source

Measuring Ganymede’s Librations with Laser Altimetry

open access: yesGeosciences, 2019
Jupiter’s moon Ganymede might be in possession of a subsurface ocean located between two ice layers. However, from Galileo data it is not possible to unambiguously infer the thickness and densities of the individual layers.
Gregor Steinbrügge   +4 more
doaj   +1 more source

Home - About - Disclaimer - Privacy