Results 151 to 160 of about 237 (185)

Modeling and monitoring injectivity evolution during cold CO2 injection with field evidence from aquistore carbon capture and storage operations

Deep Underground Science and Engineering, EarlyView.
This work integrates 5 years of field data from the Aquistore CCS project with a non‐isothermal THM modeling framework to explain how cold CO2 injection alters injectivity over time. The study shows that sustained cooling near the wellbore reduces effective stresses, promotes tensile micro‑cracking, and leads to semi‑reversible permeability enhancement
Alireza Rangriz Shokri, Stephen Talman, Erik Nickel, Rick Chalaturnyk   +3 more
wiley   +1 more source

Geodetic Investigations of the Europa Clipper Mission. [PDF]

Space Sci Rev
Steinbrügge G, Park RS, Roberts JH, Bland M, Brooks S, Castillo-Rogez J, Cascioli G, Genova A, Greathouse T, Hussmann H, Kirk R, Magnanini A, Mazarico E, Nimmo F, Park MS, Petricca F, Retherford K, Schroeder DM, Soderlund KM, Tortora P, Zannoni M.   +20 more
europepmc   +1 more source

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Interiors of Earth-Like Planets and Satellites of the Solar System

Surveys in Geophysics, 2022
The Earth-like planets and moons in our solar system have iron-rich cores, silicate mantles, and a basaltic crust. Differentiated icy moons can have a core and a mantle and an outer water–ice layer. Indirect evidence for several icy moons suggests that this ice is underlain by or includes a water-rich ocean.
Breuer, Doris, Spohn, Tilman, Van Hoolst, Tim, van Westrenen, Wim, Stanley, Sabine, Rambaux, Nicolas   +5 more
openaire   +1 more source

Subsurface oceans and deep interiors of medium-sized outer planet satellites and large trans-neptunian objects

Icarus, 2006
Abstract The detection of induced magnetic fields in the vicinity of the jovian satellites Europa, Ganymede, and Callisto is one of the most surprising findings of the Galileo mission to Jupiter. The observed magnetic signature cannot be generated in solid ice or in silicate rock. It rather suggests the existence of electrically conducting reservoirs
Hussmann, H., Sohl, F., Spohn, T.
openaire   +1 more source

Orbital Dynamics of Kuiper Belt Object Satellites, a Kuiper Belt Family, and Extra-Solar Planet Interiors

2009
This thesis discusses research into four different orbital dynamics problems, where the main goal of each chapter is to characterize the strongest non-Keplerian effect. These problems are introduced and discussed in Chapter 1, to help provide context for the subsequent chapters.
openaire   +1 more source

Interior and Evolution of the Giant Planets

Remote Sensing, 2023
Allona Vazan, Yamila Miguel
exaly  

Session 13. The Deep Cold Biosphere? Interior Processes of Icy Satellites and Dwarf Planets

Astrobiology, 2008
Julie Castillo, Steve Vance
openaire   +1 more source

Redox State and Interior Structure Control on the Long-Term Habitability of Stagnant-Lid Planets

Astronomy and Astrophysics, 2023
Lena Noack, Philipp Baumeister, Nicola Tosi   +2 more
exaly  

COUPLED EVOLUTION OF THE ATMOSPHERES AND INTERIORS OF PLANETS AND SATELLITES

1989
G. SCHUBERT, D. L. TURCOTTE, S. C. SOLOMON, N. H. SLEEP   +3 more
openaire   +1 more source