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The solar system started to form about 4.56 Gyr ago and despite the long intervening time span, there still exist several clues about its formation. The three major sources for this information are meteorites, the present solar system…

地球与行星天体物理 · 物理学 2015-06-23 S. Pfalzner , M. B. Davies , M. Gounelle , A. Johansen , C. Muenker , P. Lacerda , S. Portegies Zwart , L. Testi , M. Trieloff , D. Veras

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

One in every two atoms in the Earth, Mars, and the Moon is oxygen; it is the third most abundant element in the solar system. The oxygen isotopic compositions of the terrestrial planets are different from those of the Sun and demonstrate…

地球物理 · 物理学 2025-05-07 William F McDonough

Classical Newtonian gravitational theory does not satisfy the causality principle because it is based on instantaneous action-at-a-distance. A causal version of Newtonian theory for a large rotating sphere is derived herein by…

综合物理 · 物理学 2012-02-28 J. C. Hafele

After decades of effort, the solar activity cycle is exceptionally well characterized but it remains poorly understood. Pioneering work at the Mount Wilson Observatory demonstrated that other sun-like stars also show regular activity…

太阳与恒星天体物理 · 物理学 2017-09-01 Travis S. Metcalfe , Jennifer van Saders

The solar system's terrestrial planets are thought to have accreted over millions of years out of a sea of smaller embryos and planetesimals. Because it is impossible to know the surface density profile for solids and size frequency…

地球与行星天体物理 · 物理学 2020-05-11 Matthew S. Clement , Nathan A. Kaib , John E. Chambers

The Moon is believed to have formed in the aftermath of a giant impact between a planetary mass body and the proto-Earth. In a typical giant impact scenario, a disk of vapor, liquid, and solid debris forms around the proto-Earth and--after…

地球与行星天体物理 · 物理学 2020-11-11 P. D. Mullen , C. F. Gammie

Cosmologically motivated theories that explain small acceleration rate of the Universe via modification of gravity at very large, horizon or super-horizon distances, can be tested by precision gravitational measurements at much shorter…

高能物理 - 唯象学 · 物理学 2009-11-07 Gia Dvali , Andrei Gruzinov , Matias Zaldarriaga

In Einstein's general relativity theory the metric component gxx in the direction of motion (x-direction) of the sun deviates from unity due to a tensor potential caused by the black hole existing around the center of the galaxy. Because…

综合物理 · 物理学 2008-10-14 Masataka Mizushima

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 Earth's Moon is thought to have formed from a circumterrestrial disk generated by a giant impact between the proto-Earth and an impactor approximately 4.5 billion years ago. Since the impact was energetic, the disk would have been hot…

地球与行星天体物理 · 物理学 2018-12-31 Miki Nakajima , David J. Stevenson

[abridged] In the typical giant-impact scenario for the Moon formation most of the Moon's material originates from the impactor. Any Earth-impactor composition difference should, therefore, correspond to a comparable Earth-Moon composition…

地球与行星天体物理 · 物理学 2017-06-21 Alessandra Mastrobuono-Battisti , Hagai B. Perets

The Earth--Moon system has been experiencing impacts from asteroids and comets for billions of years. The Moon, as an airless body, has preserved a distinct record of these events in form of impact craters and ejecta deposits, offering…

地球与行星天体物理 · 物理学 2026-02-16 Yifei Jiao , Bin Cheng , Hexi Baoyin

Previous work has demonstrated orbital stability for 100 Myr of initially near-circular and coplanar small bodies in a region termed the 'Earth-Mars belt' from 1.08 au $< a <$ 1.28 au. Via numerical integration of 3000 particles, we studied…

地球与行星天体物理 · 物理学 2020-10-14 Yukun Huang , Brett Gladman

The geometric arrangement of planet and moon orbits into a regularly spaced pattern of distances is the result of a self-organizing system. The positive feedback mechanism that operates a self-organizing system is accomplished by harmonic…

地球与行星天体物理 · 物理学 2017-08-30 Markus J. Aschwanden

This review provides an introduction to the generation and evolution of the Sun's magnetic field, summarising both observational evidence and theoretical models. The eleven year solar cycle, which is well known from a variety of observed…

太阳与恒星天体物理 · 物理学 2011-10-17 Alan W. Hood , David W. Hughes

A new analysis of extended data records collected with the Lunar Laser Ranging (LLR) technique performed with improved tidal models was not able to resolve the issue of the anomalous rate $\dot e$ of the eccentricity $e$ of the orbit of the…

广义相对论与量子宇宙学 · 物理学 2014-05-05 Lorenzo Iorio

The perturbation of the Earth caused by variability of mass of Earth as additional reason with gravity of celestial bodies and shape of the Earth. The Earth eating and collecting matters from space and loss or eject matters to space through…

综合物理 · 物理学 2022-03-29 Ramy Mawad

Embryos of the Moon and the Earth may have formed as a result of contraction of a common parental rarefied condensation. The required angular momentum of this condensation could largely be acquired in a collision of two rarefied…

地球与行星天体物理 · 物理学 2020-03-24 S. I. Ipatov

We show that the assembly of the Solar System terrestrial planets can be successfully modelled with all of the mass initially confined to a narrow annulus between 0.7 and 1.0 AU. With this configuration, analogues of Mercury and Mars often…

地球与行星天体物理 · 物理学 2015-05-13 Brad Hansen