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相关论文: Is the Solar System Stable ?

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The solar magnetic field, thought to be generated by the motion of plasma within the Sun, alternates on the order of 11-year cycles and is incompletely understood. Industries rely on accurate forecasts of solar activity, but can solar…

太阳与恒星天体物理 · 物理学 2025-02-20 Floe Foxon

The Sun provides the energy required to sustain life on Earth and drive our planet's atmospheric circulation. However, establishing a solid physical connection between solar and tropospheric variability has posed a considerable challenge…

太阳与恒星天体物理 · 物理学 2020-02-06 Robert J Leamon , Scott W. McIntosh , Daniel R. Marsh

Nowadays, many extrasolar planetary systems possessing at least one planet on a highly eccentric orbit have been discovered. In this work, we study the possible long-term stability of such systems. We consider the general three body problem…

地球与行星天体物理 · 物理学 2016-12-09 Kyriaki I. Antoniadou , George Voyatzis

With the growing number of discovered exoplanets, the Gaia concept finds its second wind. The Gaia concept defines that the biosphere of an inhabited planet regulates a planetary climate through feedback loops such that the planet remains…

混沌动力学 · 物理学 2021-02-10 Sergey A. Vakulenko , Ivan Sudakov , Sergei V. Petrovskii , Dmitry V. Lukichev

Stability is one of the most fundamental aspects regarding planetary systems. It plays an important role in our understanding on the formation channel of the planetary systems, as well as their habitability. Many approaches have been…

地球与行星天体物理 · 物理学 2024-07-22 Hareesh Gautham Bhaskar , Nathaniel W. H. Moore , Jiapeng Gao , Gongjie Li , Billy Quarles

Investigations were carried out on the stability of the two gas giant system HD 60532 itself including additional, smaller bodies. The methods used were numerical simulations with the Lie Series integration method, and secular perturbation…

地球与行星天体物理 · 物理学 2013-04-08 S. Rothwangl , S. Eggl , R. Dvorak

A simple phenomenological account for planetary climate instabilities is presented. The description is based on the standard model where the balance of incoming stellar radiation and outward thermal radiation is described by the effective…

地球与行星天体物理 · 物理学 2016-11-08 Kasper W Olsen , Jakob Bohr

The apparent regularity of the motion of the giant planets of our solar system suggested for decades that said planets formed onto orbits similar to the current ones and that nothing dramatic ever happened during their lifetime. The…

地球与行星天体物理 · 物理学 2020-07-17 Alessandro Morbidelli

In the solar neighborhood, where the typical relaxation timescale is larger than the cosmic age, at least 10\% to 15\% of Sun-like stars have planetary systems with Jupiter-mass planets. In contrast, dense star clusters, charactered by…

地球与行星天体物理 · 物理学 2017-08-23 Maxwell Xu Cai , Rainer Spurzem , M. B. N. Kouwenhoven

Reconstructions of the paleoclimate indicate that ancient climatic fluctuations on Earth are often correlated with variations in its orbital elements. However, the chaos inherent in the solar system's orbital evolution prevents numerical…

地球与行星天体物理 · 物理学 2024-02-15 Nathan A. Kaib , Sean N. Raymond

Given the inexorable increase in the Sun's luminosity, Earth will exit the habitable zone in ~1 Gyr. There is a negligible chance that Earth's orbit will change during that time through internal Solar System dynamics. However, there is a…

地球与行星天体物理 · 物理学 2023-11-22 Sean N. Raymond , Nathan A. Kaib , Franck Selsis , Herve Bouy

This paper explores the stability of an Earth-like planet orbiting a solar mass star in the presence of an outer-lying intermediate mass companion. The overall goal is to estimate the fraction of binary systems that allow Earth-like planets…

天体物理学 · 物理学 2009-11-07 Eva-Marie David , Elisa V. Quintana , Marco Fatuzzo , Fred C. Adams

The formation of the solar system's giant planets predated the ultimate epoch of massive impacts that concluded the process of terrestrial planet formation. Following their formation, the giant planets' orbits evolved through an episode of…

地球与行星天体物理 · 物理学 2021-06-23 Matthew S. Clement , Nathan A. Kaib , Sean N. Raymond , John E. Chambers

Due to the chaotic nature of the Solar System, the question of its long-term stability can only be answered in a statistical sense, for instance, based on numerical ensemble integrations of nearby orbits. Destabilization of the inner…

地球与行星天体物理 · 物理学 2015-06-26 Richard E. Zeebe

The majority of stars form in star clusters and many are thought to have planetary companions. We demonstrate that multi-planet systems are prone to instabilities as a result of frequent stellar encounters in these star clusters much more…

地球与行星天体物理 · 物理学 2015-06-15 W. Hao , M. B. N. Kouwenhoven , R. Spurzem

For more than four decades, scientists have been trying to find an answer to one of the most fundamental questions in paleoclimatology, the `faint young Sun problem'. For the early Earth, models of stellar evolution predict a solar energy…

地球与行星天体物理 · 物理学 2012-05-28 Georg Feulner

Although classical economic theory is based on the concept of stable equilibrium, real economic systems appear to be always out of equilibrium. Indeed, they share many of the dynamical features of other complex systems, e.g., ecological…

物理与社会 · 物理学 2010-11-16 Sitabhra Sinha

From the axiom of the unrestricted repeatability of all experiments, Bondi and Gold argued that the universe is in a stable, self-perpetuating equilibrium state. This concept generalizes the usual cosmological principle to the perfect…

天体物理学 · 物理学 2007-05-23 Thomas B. Andrews

Some tests of gravity theories - periastron shift, geodetic precession, change in mean motion and gravitational redshift - are applied in solar and stellar systems to constrain the cosmological constant. We thus consider a length scale…

天体物理学 · 物理学 2009-11-11 M. Sereno , Ph. Jetzer

Models of the Sun's long-term evolution suggest that its luminosity was substantially reduced 2-4 billion years ago, which is inconsistent with substantial evidence for warm and wet conditions in the geological records of both ancient Earth…

地球与行星天体物理 · 物理学 2018-12-19 Christopher Spalding , Woodward W. Fischer , Gregory Laughlin