JUpiter ICy moons Explorer (JUICE): An ESA mission to orbit Ganymede and to characterise the Jupiter system

O Grasset, MK Dougherty, A Coustenis… - Planetary and Space …, 2013 - Elsevier
Past exploration of Jupiter's diverse satellite system has forever changed our understanding
of the unique environments to be found around gas giants, both in our solar system and …

The galilean satellites

AP Showman, R Malhotra - Science, 1999 - science.org
NASA's Galileo mission to Jupiter and improved Earth-based observing capabilities have
allowed major advances in our understanding of Jupiter's moons Io, Europa, Ganymede …

Coherent manipulation of semiconductor quantum bits with terahertz radiation

BE Cole, JB Williams, BT King, MS Sherwin… - Nature, 2001 - nature.com
Abstract Quantum bits,,,,(qubits) are the fundamental building blocks of quantum information
processors, such as quantum computers. A qubit comprises a pair of well characterized …

Formation of giant planet satellites

K Batygin, A Morbidelli - The Astrophysical Journal, 2020 - iopscience.iop.org
Recent analyses have shown that the concluding stages of giant planet formation are
accompanied by the development of a large-scale meridional flow of gas inside the …

Rheological properties of water ice—Applications to satellites of the outer planets

WB Durham, LA Stern - Annual Review of Earth and Planetary …, 2001 - annualreviews.org
▪ Abstract The icy moons of the outer solar system have not been quiescent bodies, in part
because many have a substantial water component and have experienced significant …

Band formation and ocean‐surface interaction on Europa and Ganymede

SM Howell, RT Pappalardo - Geophysical Research Letters, 2018 - Wiley Online Library
Geologic activity in the outer H2O ice shells of Europa and Ganymede, Galilean moons of
Jupiter, may facilitate material exchange between global water oceans and the icy surface …

Mountains on Titan observed by Cassini RADAR

J Radebaugh, RD Lorenz, RL Kirk, JI Lunine… - Icarus, 2007 - Elsevier
The Cassini Titan Radar mapper has observed elevated blocks and ridge-forming block
chains on Saturn's moon Titan demonstrating high topography we term “mountains.” Summit …

Geology of ganymede

RT Pappalardo, GC Collins, JW Head… - Jupiter: The planet …, 2004 - books.google.com
Overview Ganymede is a planet-sized world, the solar system's largest satellite with a radius
of 2631 km. Its physiography, geology, geophysics, surface composition, and evolution are …

Surface composition and properties of Ganymede: Updates from ground-based observations with the near-infrared imaging spectrometer SINFONI/VLT/ESO

N Ligier, C Paranicas, J Carter, F Poulet, WM Calvin… - Icarus, 2019 - Elsevier
Ganymede's surface exhibits great geological diversity, with old dark terrains, expressed
through the surface composition, which is known to be dominated by two constituents: H 2 O …

Mass movement and landform degradation on the icy Galilean satellites: Results of the Galileo nominal mission

JM Moore, E Asphaug, D Morrison, JR Spencer… - Icarus, 1999 - Elsevier
The Galileo mission has revealed remarkable evidence of mass movement and landform
degradation on the icy Galilean satellites of Jupiter. Weakening of surface materials coupled …