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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 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

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

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

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

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 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

According to the giant impact theory, the Moon formed through accreting the debris disk produced by a collision between Theia and the proto-Earth, and the predicted lunar orbital inclination relative to the Earth's equatorial plane is about…

地球与行星天体物理 · 物理学 2026-04-01 Wenshuai Liu

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

The multiple impact hypothesis proposes that the Moon formed through a series of smaller collisions, rather than a single giant impact. This study advances our understanding of this hypothesis, as well as moon collisions in other contexts,…

地球与行星天体物理 · 物理学 2024-11-14 Uri Malamud , Hagai 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

Three principal concepts regarding lunar formation have been examined: the accretion hypothesis, the mega-impact theory, and the multi-impact model. The multi-impact model amalgamates the salient facets of the mega-impact theory and the…

地球与行星天体物理 · 物理学 2023-10-27 Nick Gorkavyi

Understanding the Moon's formation mechanism is necessary for studying not only the Moon itself, but also the evolution, formation, habitability, and structure of other planets and the moons in the Solar system and in extrasolar planetary…

地球与行星天体物理 · 物理学 2014-02-04 Mukesh Gupta

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

The leading hypothesis for the origin of the Moon, that of a single giant impact, faces significant challenges. These include either the need for an impactor with a near-identical composition to Earth or an extremely high-mass or…

地球与行星天体物理 · 物理学 2025-12-12 Harrison Davies , Philip J. Carter , Louis Eddershaw , Jingyao Dou , Zoë M. Leinhardt

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 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

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 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
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