Results 41 to 50 of about 1,894,855 (142)
A new look at the Oort Cloud to Scattered Disc population ratio [PDF]
Workshop program and abstracts available at: http://lal.univ-lille1.fr/oort_workshop_prog.htmlClassical simulations of the formation and evolution of the Oort cloud generally encounter two problems.
Morbidelli, Alessandro, Brasser, Ramon
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Gravitational Time Potential Energy
We extend the Einstein equivalence principle via a supplementary local energy equivalence postulate and propose the gravitational time potential energy (GTP) framework: a time‐dimensional scalar potential accumulating continuously with the proper duration of gravitational action. This framework may provide a potential classical interpretation for alpha
Ne Allen, Mohammad Rezwan Habib
wiley +1 more source
Notes on the outer-Oort-cloud formation efficiency in the simulation of Oort cloud formation
Aims. The formation efficiency of the outer Oort cloud, obtained in the simulation performed in our previous work, appeared to be very low in a comparison with the corresponding results of other authors.
P. A. Dybczyński +4 more
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No Influence of Passing Stars on Paleoclimate Reconstructions Over the Past 56 Million Years
Passing stars (also called stellar flybys) have notable effects on the solar system’s long-term dynamical evolution, injection of Oort cloud comets into the solar system, properties of trans-Neptunian objects, and more. Based on a simplified solar system
Richard E. Zeebe, David M. Hernandez
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Abstract High‐throughput and noninvasive phenotyping methods are promising technology for improving efficiency in plant research and breeding. In this study, we evaluated the performance of a digital phenotyping system (DPS) based on three‐dimensional (3D) model reconstruction for quantifying key growth traits in rice (Oryza sativa).
Sorawich Pongpiyapaiboon +5 more
wiley +1 more source
The formation of periodic three-body orbits for Newtonian systems
Context. Braids are periodic solutions to the general N-body problem in gravitational dynamics. These solutions seem special and unique but may result from rather usual encounters between four bodies. Aims.
Portegies Zwart Simon +2 more
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A Thermal Origin to the Asymmetry of the Permanent Dust Cloud at the Moon
Abstract The Moon's surface, lacking an atmosphere, is continually bombarded by high‐speed micro‐meteoroids, creating a highly porous regolith composed of very fine grains. This regolith's porosity decreases with depth due to compression. Besides creating vapor and melt, micro‐meteoroid impacts eject lunar dust, redistributing regolith grains, which ...
Sébastien Verkercke +9 more
wiley +1 more source
Sedna and the Oort Cloud around a migrating Sun [PDF]
Recent numerical simulations have demonstrated that the Sun's dynamical history within the Milky Way may be much more complex than that suggested by its current low peculiar velocity (Sellwood, J.A., Binney, J.J. [2002]. Mon. Not. R. Astron. Soc.
Roškar, R +5 more
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Read the free Plain Language Summary for this article on the Journal blog. Abstract The light climate at high latitudes, in particular the extended twilight of winter and the reduced diel variation in light level in midsummer and midwinter, potentially constrains visual function and the synchronisation of temporal organisation in polar species. In this
Nicholas J. C. Tyler +3 more
wiley +1 more source
Analytical Solutions for Planet-scattering Small Bodies
Gravitational scattering of small bodies (planetesimals) by a planet remains a fundamental problem in celestial mechanics. It is traditionally modeled within the circular restricted three-body problem, where individual particle trajectories are obtained ...
Yukun Huang +2 more
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