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相关论文: Tidal Evolution of the Earth-Moon System with a Hi…

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It is known since the seminal study of Laskar (1989) that the inner planetary system is chaotic with respect to its orbits and even escapes are not impossible, although in time scales of billions of years. The aim of this investigation is…

地球与行星天体物理 · 物理学 2015-05-14 Ákos Bazsó , Veresa Eybl , Rudolf Dvorak , Elke Pilat-Lohinger , Christoph Lhotka

Recent experiments conducted in the International Space Station highlight the apparent periodicity of leaf oscillations and other biological phenomena associated with rhythmic variations of lunisolar forces. These events are similar to…

经典物理 · 物理学 2020-11-03 Henri Gouin

The magma ocean concept was first conceived to explain the geology of the Moon, but hemispherical or global oceans of silicate melt could be a widespread "lava world" phase of rocky planet accretion, and could persist on planets on…

地球与行星天体物理 · 物理学 2021-06-30 Keng-Hsien Chao , Rebecca deGraffenried , Mackenzie Lach , William Nelson , Kelly Truax , Eric Gaidos

Venus and Earth are similar in bulk properties yet followed dramatically different climatic trajectories. Reconstructing Venus's climate evolution requires understanding how rotation, obliquity, eccentricity, and solar luminosity shaped…

地球与行星天体物理 · 物理学 2026-05-13 Stephen R. Kane

In order to examine the ``giant impact hypothesis'' for the Moon formation, we run the first grid-based, high-resolution hydrodynamic simulations for an impact between proto-Earth and a proto-planet. The spatial resolution for the…

天体物理学 · 物理学 2009-11-11 Keiichi Wada , Eiichiro Kokubo , Junichiro Makino

We demonstrate that tidal evolution of the inner planet (`e') of the system orbiting the star rho 55 Cancri could have led to passage through two secular resonances with other planets in the system. The consequence of this evolution is…

地球与行星天体物理 · 物理学 2015-06-17 Brad Hansen , Jonathon Zink

It has been posited that lunar eclipse observations may help predict the in-transit signature of Earth-like extrasolar planets. However, a comparative analysis of the two phenomena addressing in detail the transport of stellar light through…

太阳与恒星天体物理 · 物理学 2015-06-05 A. García Muñoz , M. R. Zapatero Osorio , R. Barrena , P. Montañés-Rodríguez , E. L. Martín , E. Pallé

Saturn's largest moon, Titan, has an Earth-like volatile cycle, but with methane playing the role of water and surface liquid reservoirs geographically isolated at high latitudes. We recreate Titan's characteristic dry hydroclimate at the…

地球与行星天体物理 · 物理学 2022-07-14 Matthew McKinney , J. Mitchell , S. I. Thomson

This article investigates long-term orbits within the Earth's magnetosphere, specifically focusing on orbits where the argument of periapsis is synchronized with changes induced by lunar gravity assists and the Earth's argument of latitude…

地球与行星天体物理 · 物理学 2024-10-01 Jinsung Lee , Jaeyoung Kwak , Jaemyung Ahn

Many science missions require an unobstructed view of space and a stable thermal environment but lack the technical or programmatic resources to reach orbits that satisfy these needs. This paper presents a high Earth orbit in 2:1 resonance…

地球与行星天体物理 · 物理学 2013-08-09 Joseph W. Gangestad , Gregory A. Henning , Randy R. Persinger , George R. Ricker

Understanding the concept of habitability is related to an evolutionary knowledge of the particular planet-in-question. Additional indications so-called "systemic aspects" of the planetary system as a whole governs a particular planet's…

We explore the past evolution of Saturn's moons using direct numerical integrations. We find that the past Tethys-Dione 3:2 orbital resonance predicted in standard models likely did not occur, implying that the system is less evolved than…

地球与行星天体物理 · 物理学 2016-04-06 Matija Ćuk , Luke Dones , David Nesvorný

Solid Earth tide represents the response of solid Earth to the lunar (solar) gravitational force. The yielding solid Earth due to the force has been thought to be a prolate ellipsoid since the time of Lord Kelvin, yet the ellipsoid's…

地球物理 · 物理学 2024-11-26 Yongfeng Yang , Yunfei Zhang , Qiang Liu , Xianqing Lv , Pu Huang

Similarities in the non-mass dependent isotopic composition of refractory elements with the bulk silicate Earth suggest that both the Earth and the Moon formed from the same material reservoir. On the other hand, the Moon's volatile…

地球与行星天体物理 · 物理学 2024-12-03 Gustavo Madeira , Leandro Esteves , Sebastien Charnoz , Elena Lega , Frederic Moynier

The current standard theory of the origin of the Moon is that the Earth was hit by a giant impactor the size of Mars causing ejection of iron poor impactor mantle debris that coalesced to form the Moon. But where did this Mars-sized…

天体物理学 · 物理学 2014-10-13 Edward Belbruno , J. Richard Gott

Direct-imaging techniques of exoplanets have made significant progress recently, and will eventually enable to monitor photometric and spectroscopic signals of earth-like habitable planets in the future. The presence of clouds, however,…

The equilibrium rotation of tidally evolved "Earth-like" extra-solar planets is often assumed to be synchronous with their orbital mean motion. The same assumption persisted for Mercury and Venus until radar observations revealed their true…

天体物理学 · 物理学 2008-08-08 Alexandre C. M. Correia , Benjamin Levrard , Jacques Laskar

The paper addresses the possibility of a young Mars having had a massive moon, which synchronised the rotation of Mars, and gave Mars an initial asymmetric triaxiality to be later boosted by geological processes. It turns out that a moon of…

地球与行星天体物理 · 物理学 2024-10-15 Michael Efroimsky

The Milankovitch cycles of Earth result from gravitational interactions with other bodies in the Solar System. These interactions lead to slow changes in the orbit and angular momentum vector of Earth, and correspondingly influence Earth's…

地球与行星天体物理 · 物理学 2025-12-05 Stephen R. Kane , Pam Vervoort , Jonathan Horner

The problem of the formation of the Moon is still not explained satisfactorily. While it is a generally accepted scenario that the last giant impact on Earth between some 50 to 100 million years after the starting of the formation of the…

地球与行星天体物理 · 物理学 2015-07-01 Rudolf Dvorak , Birgit Loibnegger , Thomas I. Maindl