T
T. Van Hoolst
Researcher at Royal Observatory of Belgium
Publications - 99
Citations - 3080
T. Van Hoolst is an academic researcher from Royal Observatory of Belgium. The author has contributed to research in topics: Mars Exploration Program & Martian. The author has an hindex of 30, co-authored 96 publications receiving 2671 citations. Previous affiliations of T. Van Hoolst include Katholieke Universiteit Leuven.
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JUpiter ICy moons Explorer (JUICE): An ESA mission to orbit Ganymede and to characterise the Jupiter system
Olivier Grasset,M. K. Dougherty,Athena Coustenis,Emma J. Bunce,Christian Erd,Dmitrij V. Titov,Michel Blanc,Andrew J. Coates,Pierre Drossart,Leigh N. Fletcher,H. Hussmann,Ralf Jaumann,Norbert Krupp,Jean-Pierre Lebreton,Olga Prieto-Ballesteros,Paolo Tortora,Federico Tosi,T. Van Hoolst +17 more
TL;DR: The JUpiter ICy moons Explorer (JUICE) mission as mentioned in this paper was selected by ESA in May 2012 to perform detailed investigations of Jupiter and its system in all their interrelations and complexity with particular emphasis on Ganymede as a planetary body and potential habitat.
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Geodesy constraints on the interior structure and composition of Mars
Attilio Rivoldini,Attilio Rivoldini,T. Van Hoolst,O. Verhoeven,Antoine Mocquet,Véronique Dehant +5 more
TL;DR: In this article, the authors used the moment of inertia and tidal Love number k2 to infer the interior structure of the Mars, which is the most prominent interior structure properties of the core, solid or liquid.
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Long-Term Evolution of the Martian Crust-Mantle System
Matthias Grott,David Baratoux,Ernst Hauber,Violaine Sautter,John F. Mustard,Olivier Gasnault,Steven W. Ruff,Shun-ichiro Karato,Vinciane Debaille,Martin Knapmeyer,Frank Sohl,T. Van Hoolst,Doris Breuer,Achim Morschhauser,Michael J. Toplis +14 more
TL;DR: In this article, the authors show that the long-term evolution of the crust-mantle system of Mars is driven by mantle convection, partial melting, and silicate differentiation.
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Water-rich planets: How habitable is a water layer deeper than on Earth?
Lena Noack,Dennis Höning,Attilio Rivoldini,Clemens Heistracher,Nastasia Zimov,Baptiste Journaux,Helmut Lammer,T. Van Hoolst,Jan Hendrik Bredehöft +8 more
TL;DR: In this article, a new ocean model was developed that is coupled with a thermal evolution model of the mantle and core of a water-rich super-Earth-size planet, and a new habitability classification was introduced.
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The interior structure of Mercury and its core sulfur content
TL;DR: In this paper, depth-dependent interior structure models of Mercury are calculated for several plausible chemical compositions of the core and of the mantle, and the expected precision on the moment of inertia is estimated to a precision of about 50 km.