about
Resolved debris disc emission around η Telescopii: a young solar system or ongoing planet formation?Evidence of denser MgSiO3 glass above 133 gigapascal (GPa) and implications for remnants of ultradense silicate melt from a deep magma ocean.Excitation of lunar eccentricity by planetary resonances.Isotopes as clues to the origin and earliest differentiation history of the Earth.Nominally hydrous magmatism on the Moon.Detection of adsorbed water and hydroxyl on the Moon.Lunar-forming impacts: processes and alternatives.Geochemical arguments for an Earth-like Moon-forming impactorLunar formation. Dating the Moon-forming impact event with asteroidal meteorites.Widespread mixing and burial of Earth's Hadean crust by asteroid impacts.Terrestrial planet formationAccretion of the Earth.Collisionless encounters and the origin of the lunar inclination.Large impacts around a solar-analog star in the era of terrestrial planet formation.Stochastic late accretion to Earth, the Moon, and MarsHigh pre-eruptive water contents preserved in lunar melt inclusions.Hit-and-run planetary collisions.Neodymium isotope evidence for a chondritic composition of the Moon.The fate of water within Earth and super-Earths and implications for plate tectonics.Mercury and other iron-rich planetary bodies as relics of inefficient accretionThe faint young Sun problemRecords of the Moon-forming impact and the 470 Ma disruption of the L chondrite parent body in the asteroid belt from U-Pb apatite ages of Novato (L6)
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P2860
description
article
@en
im September 2004 veröffentlichter wissenschaftlicher Artikel
@de
wetenschappelijk artikel
@nl
наукова стаття, опублікована у вересні 2004
@uk
ലേഖനം
@ml
name
Dynamics of Lunar Formation
@en
Dynamics of Lunar Formation
@nl
type
label
Dynamics of Lunar Formation
@en
Dynamics of Lunar Formation
@nl
prefLabel
Dynamics of Lunar Formation
@en
Dynamics of Lunar Formation
@nl
P1476
Dynamics of Lunar Formation
@en
P2093
Robin M. Canup
P304
P356
10.1146/ANNUREV.ASTRO.41.082201.113457
P407
P577
2004-09-22T00:00:00Z