LunaIcy: Exploring Europa’s Icy Surface Microstructure through Multiphysics Simulations
A multiphysics simulation model incorporating a sintering model coupled with the MultIHeaTS thermal solver was developed to study the evolution of icy moons’ microstructure.
Cyril Mergny, Frédéric Schmidt
doaj +1 more source
A Multifrequency Global View of Callisto’s Thermal Properties from ALMA
We present thermal observations of Callisto’s leading and trailing hemispheres obtained using the Atacama Large Millimeter/submillimeter Array (ALMA) at 0.87 mm (343 GHz), 1.3 mm (233 GHz), and 3 mm (97 GHz).
Maria Camarca +7 more
doaj +1 more source
Revealing Callisto’s Near-subsurface Thermophysical Properties with ALMA Calibration Data
Thermal images at different wavelengths probe varying subsurface depths of planetary bodies and therefore can inform us about their compositions, thermophysical properties, and impact histories.
Cole Meyer +5 more
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A virtual tour of the Galilean Satellites [PDF]
Galileo's imagination was quick to comprehend the importance of the 4 starry objects he observed near Jupiter in January 1610, not only for himself as a scientist but for our common understanding of the place of the Earth and our species in the cosmos.
openaire +1 more source
China is planning to launch the “Tianwen-4” mission around the year 2030, with its aim being the exploration of Jupiter and its moon, Callisto. Within the realm of deep space exploration, the accuracy of ephemerides is of great importance.
Kai Huang +4 more
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Impact of Jupiter’s Heating and Self-shadowing on the Jovian Circumplanetary Disk Structure
Deciphering the structure of the circumplanetary disk (CPD) that surrounded Jupiter at the end of its formation is key to understanding how the Galilean moons formed.
Antoine Schneeberger, Olivier Mousis
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On the Theory of the Galilean Satellites of Jupiter [PDF]
In this communication the main equations for the variables: radius vector, longitude,PandQ(variables built from Laplace's perihelium first integral) are given in closed form. These equations are used for deriving the equations of a second-order theory.
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Laboratory Investigation of CO2-driven Enhancement of Radiolytic H2O2 on Europa and Other Icy Moons
Observations of Europa’s leading hemisphere reveal elevated H _2 O _2 in the warmer, low-latitude chaos terrains compared to the colder, polar regions.
Bereket D. Mamo +7 more
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Explaining the Galilean Satellites' Density Gradient by Hydrodynamic Escape. [PDF]
Bierson CJ, Nimmo F.
europepmc +1 more source
Slow evolution of Europa's interior: metamorphic ocean origin, delayed metallic core formation, and limited seafloor volcanism. [PDF]
Trinh KT, Bierson CJ, O'Rourke JG.
europepmc +1 more source

