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The giant impact hypothesis is the dominant theory of how the Earth-Moon system was formed. Models have been created that can produce a disk of debris with the proper mass and composition to create our Moon. Models have also been created…

地球与行星天体物理 · 物理学 2013-07-29 Justin C. Eiland , Travis C. Salzillo , Brett H. Hokr , Justin L. Highland , Bryant M. Wyatt

The hypothesis of lunar origin by a single giant impact can explain some aspects of the Earth-Moon system. However, it is difficult to reconcile giant impact models with the compositional similarity of the Earth and Moon without violating…

地球与行星天体物理 · 物理学 2019-03-07 Raluca Rufu , Oded Aharonson , Hagai B. Perets

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

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

Most of the properties of the Earth-Moon system can be explained by a collision between a planetary embryo and the growing Earth late in the accretion process. Simulations show that most of the material that eventually aggregates to form…

地球与行星天体物理 · 物理学 2015-06-24 Alessandra Mastrobuono-Battisti , Hagai B. Perets , Sean N. Raymond

In the giant impact hypothesis for lunar origin, the Moon accreted from an equatorial circum-terrestrial disk; however the current lunar orbital inclination of 5 degrees requires a subsequent dynamical process that is still debated. In…

地球与行星天体物理 · 物理学 2018-02-12 Matija Ćuk , Douglas P. Hamilton , Simon J. Lock , Sarah T. Stewart

The giant impact hypothesis remains the leading theory for lunar origin. However, current models struggle to explain the Moon's composition and isotopic similarity with Earth. Here we present a new lunar origin model. High-energy,…

地球与行星天体物理 · 物理学 2018-03-01 Simon J. Lock , Sarah T. Stewart , Michail I. Petaev , Zoe M. Leinhardt , Mia T. Mace , Stein B. Jacobsen , Matija Ćuk

[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

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 2024-11-20 Thomas Meier , Christian Reinhardt , Miles Timpe , Joachim Stadel , Ben Moore

A giant impact origin for the Moon is generally accepted, but many aspects of lunar formation remain poorly understood and debated. \'Cuk et al. (2016) proposed that an impact that left the Earth-Moon system with high obliquity and angular…

地球与行星天体物理 · 物理学 2021-07-08 Matija Ćuk , Simon J. Lock , Sarah T. Stewart , Douglas P. Hamilton

The Moon is traditionally thought to have coalesced from the debris ejected by a giant impact onto the early Earth. However, such models struggle to explain the similar isotopic compositions of Earth and lunar rocks at the same time as the…

The Giant Impact is currently accepted as the leading theory for the formation of Earth's Moon. Successful scenarios for lunar origin should be able to explain the chemical composition of the Moon (volatile content and stable isotope…

地球与行星天体物理 · 物理学 2017-11-15 Amy C. Barr

Recent high-precision measurements of the isotopic composition of lunar rocks demonstrate that the bulk silicate Earth and the Moon show an unexpectedly high degree of similarity. This is inconsistent with one of the primary results of…

地球与行星天体物理 · 物理学 2013-01-14 R. J. de Meijer , V. F. Anisichkin , W. van Westrenen

According to the giant impact theory, the Moon formed through accreting the debris disk produced by a collision between Theia and the proto-Earth. The giant impact theory can explain most of the properties of the Earth-Moon system, however,…

地球与行星天体物理 · 物理学 2025-09-09 Wenshuai Liu

The Moon is generally thought to have formed from the debris ejected by the impact of a planet-sized object with the proto-Earth towards the end of planetary accretion. Modeling of the impact process predicts that the lunar material was…

地球与行星天体物理 · 物理学 2016-04-19 Kaveh Pahlevan , Alessandro Morbidelli

Planets are expected to conclude their growth through a series of giant impacts: energetic, global events that significantly alter planetary composition and evolution. Computer models and theory have elucidated the diverse outcomes of giant…

地球与行星天体物理 · 物理学 2023-12-27 Travis S. J. Gabriel , Saverio Cambioni

The Earth-Moon system is suggested to have formed through a single giant collision, in which the Moon accreted from the impact-generated debris disk. However, such giant impacts are rare, and during its evolution the Earth experienced many…

地球与行星天体物理 · 物理学 2018-08-01 Robert I. Citron , Hagai B. Perets , Oded Aharonson

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 leading theory for the origin of the Moon is the giant impact hypothesis, in which the Moon was formed out of the debris left over from the collision of a Mars-sized body with the Earth. Soon after its formation, the orbit of the Moon…

科普物理 · 物理学 2015-03-11 Emil Noordeh , Patrick Hall , Matija Cuk

Earth and Moon are shown here to be composed of oxygen isotope reservoirs that are indistinguishable, with a difference in {\Delta}"17O of -1 +/- 5ppm (2se). Based on these data and our new planet formation simulations that include a…

地球与行星天体物理 · 物理学 2016-03-16 Edward D. Young , Issaku E. Kohl , Paul H. Warren , David C. Rubie , Seth A. Jacobson , Alessandro Morbidelli
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