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According to the giant impact theory, the Moon formed by accreting the circum-terrestrial debris disk produced by Theia colliding with the proto-Earth. The giant impact theory can explain most of the properties of the Earth-Moon system,…

地球与行星天体物理 · 物理学 2025-05-15 Wenshuai Liu

(1) Results of analysis of new sets of anthropogenic data are presented. They confirm earlier results of similar analyses. The expected and inevitable massive deceleration of human-induced global change process is demonstrated as an ongoing…

物理与社会 · 物理学 2023-08-15 Ron W Nielsen

We discuss the current state of knowledge of terrestrial planet formation from the aspects of different planet formation models and isotopic data from 182Hf-182W, U-Pb, lithophile-siderophile elements, 48Ca/44Ca isotope samples from…

地球与行星天体物理 · 物理学 2021-02-12 H. Lammer , R. Brasser , A. Johansen , M. Scherf , M. Leitzinger

The Earth itself is not stationary but keeps revolving, and its motion further satisfies the law of equal area according to the heliocentric doctrine. That satisfaction can be used to construct the mathematical relationships between the…

经典物理 · 物理学 2014-11-07 W. Y. Hsiang , H. C. Chang , H. Yao , P. S. Lee

We apply Laplace's tidal theory to the evolution of lunar and solar tides on the geologic timescale of Earth's rotation and focus on the tidal resonance. We study the global tide in the mid-ocean far away from continents. On the short…

地球与行星天体物理 · 物理学 2021-03-31 Xing Wei

From iodine-plutonium-xenon isotope systematics, we re-evaluate time constraints on the early evolution of the Earth-atmosphere system and, by inference, on the Moon-forming event. Two extinct radioactivites (129I, T1/2 = 15.6 Ma, and…

地球与行星天体物理 · 物理学 2015-11-04 Guillaume Avice , Bernard Marty

Using models of the Earth's core evolution and the length of the day observations the change of the dimensionless geodynamo parameters is considered. The evolutionary model includes cooling of the liquid adiabatic core, growing solid core,…

地球物理 · 物理学 2019-05-31 M. Yu. Reshetnyak

In the leading theory of lunar formation, known as the giant impact hypothesis, a collision between two planet-size objects resulted in a young Earth surrounded by a circumplanetary debris disk from which the Moon later accreted. The range…

地球与行星天体物理 · 物理学 2023-07-13 Miles Timpe , Christian Reinhardt , Thomas Meier , Joachim Stadel , Ben Moore

We present integrations of a model Solar System with five terrestrial planets (beginning ~30-50 Myr after the formation of primitive Solar System bodies) in order to determine the preferred regions of parameter space leading to a giant…

地球与行星天体物理 · 物理学 2014-12-03 Billy Quarles , Jack J. Lissauer

We investigate the possibility that the Moon's formation impact was triggered by an early dynamical instability of the giant planets. We consider the well-studied "jumping Jupiter" hypothesis for the solar system's instability, where…

地球与行星天体物理 · 物理学 2021-08-11 Sandro R. DeSouza , Fernando Roig , David Nesvorný

The variation with time from 1956-2002 of the globally averaged rate of ionization produced by cosmic rays in the atmosphere is deduced and shown to have a cyclic component of period roughly twice the 11 year solar cycle period. Long term…

地球物理 · 物理学 2009-11-13 A. D. Erlykin , T. Sloan , A. W. Wolfendale

The role of the moon in triggering earthquakes has been studied since the early 1900s. Theory states that as land tides swept by the moon cross fault lines, stress in the Earth's plates intensifies, increasing the likelihood of small…

地球物理 · 物理学 2012-10-10 Lyndie Chiou

The classical method for measure the Earth-Sun distance is due to Aristarchus and it is based upon the measure of the angle Moon-Earth-Sun when the Moon is exactly in quadrature. Such an angle is only 9 arcminutes smaller than 90 degrees,…

天体物理仪器与方法 · 物理学 2011-07-06 Costantino Sigismondi

Almost all the planets of our solar system have moons. Each planetary system has however unique characteristics. The Martian system has not one single big moon like the Earth, not tens of moons of various sizes like for the giant planets,…

Understanding the origin and long-term evolution of the Solar System is a fundamental goal of planetary science and astrophysics. This chapter describes our current understanding of the key processes that shaped our planetary system,…

地球与行星天体物理 · 物理学 2024-04-24 Sean N. Raymond

One of the unique aspects of Earth is that it has a fractionally large Moon, which is thought to have formed from a Moon-forming disk generated by a giant impact. The Moon stabilizes the Earth's spin axis at least by several degrees and…

地球与行星天体物理 · 物理学 2023-12-27 Miki Nakajima , Hidenori Genda , Erik Asphaug , Shigeru Ida

The attraction of the Moon on objects at the surface of the Earth gives rise to a so-called tidal force which is of the order of 1/10,000,000 times the gravitational force of the Earth. For instance, when the Moon is located between the…

经典物理 · 物理学 2013-06-25 Marcel Betrisey , Bertrand M. Roehner

This is a historian's view of how modern astronomy data can be used to discuss the shifting historical worldview of Late Antiquity. In this article an attemp is made to construct an approximate model of how the cycles of astronomical…

物理学史与哲学 · 物理学 2024-03-07 D. N. Starostin

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

The relationship between the behavior of an ancient geomagnetic field characteristics (paleointensity and frequency of inversions) and cyclic recurrence of endogenic and cosmogeneous processes which are conceivably connected with radial…

地球物理 · 物理学 2008-06-20 A. Yu. Kurazhkovskii , N. A. Kurazhkovskaya , B. I. Klain