Results 71 to 80 of about 25,199 (146)
A numerical exploration of Miranda's dynamical history
The Uranian satellite Miranda presents a high inclination (4.338{\deg}) and evidences of resurfacing. It is accepted since 20 years (e.g. Tittemore and Wisdom 1989, Malhotra and Dermott 1990) that this inclination is due to the past trapping into the 3:1
Lemaitre, Anne +2 more
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Román García Fernández, first guided by Hera and Athena, and then by the two Aphrodites —the carnal and the spiritual: Aphrodite Pandemos and Aphrodite Uranus— completes his history of ancient philosophy.
Silverio Sánchez Corredera
doaj
Enhanced Precipitation of Energetic Protons Due to Uranus' Asymmetric Magnetic Field
Uranus remains one of the most unexplored planets in our solar system, featuring a distinctive magnetic field structure first observed by NASA's Voyager 2 mission almost 40 years ago.
M. Acevski, A. Masters
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Formation of ammonia–helium compounds at high pressure
Helium is generally considered too inert to be present in giant ice planet mantles. The authors, by first-principles calculations and crystal structure searches, find stable ammonia–helium compounds at the conditions of Uranus and Neptune’s upper mantles,
Jingming Shi +5 more
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Modelling of microstructured waveguides using a finite-element-based vectorial mode solver with transparent boundary conditions [PDF]
Finite element vectorial optical mode solver is used to analyze microstructured waveguides in a relatively small computational domain. The presentation will consider the computational method, as well as the applications of it on a number of waveguides ...
Groesen, E. van +2 more
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Ab initio free energy calculations are employed to derive the entropy of liquid and superionic water over a wide range of conditions in the interiors of Uranus and Neptune.
Burkhard Militzer
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Investigation of the small-scale structure and dynamics of Uranus' atmosphere [PDF]
This document constitutes the final technical report of the Uranus Analysis Program. Papers and/or abstracts resulting from this research are presented.
Eshleman, Von R., Hinson, David P.
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Constructing the secular architecture of the solar system I: The giant planets
Using numerical simulations, we show that smooth migration of the giant planets through a planetesimal disk leads to an orbital architecture that is inconsistent with the current one: the resulting eccentricities and inclinations of their orbits are too ...
Alessandro, Morbidelli +4 more
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The area of stable motion for fictitious Trojan asteroids around Uranus' equilateral equilibrium points is investigated with respect to the inclination of the asteroid's orbit to determine the size of the regions and their shape.
A. Morbidelli +32 more
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Internal Heat Flux and Energy Imbalance of Uranus
With its extreme axial tilt, Uranus' radiant energy budget (REB) and internal heat flux remain among the most intriguing mysteries in our solar system.
Xinyue Wang +15 more
doaj +1 more source

