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相关论文: Equilibration in the Aftermath of the Lunar-Formin…

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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

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

Despite its importance to questions of lunar origin, the chemical composition of the Moon is not precisely known. In recent years, however, the isotopic composition of lunar samples has been determined to high precision and found to be…

地球与行星天体物理 · 物理学 2010-12-27 Kaveh Pahlevan , David Stevenson , John Eiler

[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

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

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…

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

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

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 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

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

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

The Earth's Moon is thought to have formed by an impact between the Earth and an impactor around 4.5 billion years ago. This impact could have been so energetic that it could have mixed and homogenized the Earth's mantle. However, this view…

地球与行星天体物理 · 物理学 2015-06-17 Miki Nakajima , David J. Stevenson

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 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

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

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

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 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 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
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