Dynamical evolution of the early solar system
D Nesvorný - Annual Review of Astronomy and Astrophysics, 2018 - annualreviews.org
Several properties of the Solar System, including the wide radial spacing of the giant
planets, can be explained if planets radially migrated by exchanging orbital energy and …
planets, can be explained if planets radially migrated by exchanging orbital energy and …
The late heavy bombardment
Heavily cratered surfaces on the Moon, Mars, and Mercury show that the terrestrial planets
were battered by an intense bombardment during their first billion years or more, but the …
were battered by an intense bombardment during their first billion years or more, but the …
[HTML][HTML] Stagnant lids and mantle overturns: Implications for Archaean tectonics, magmagenesis, crustal growth, mantle evolution, and the start of plate tectonics
JH Bédard - Geoscience Frontiers, 2018 - Elsevier
The lower plate is the dominant agent in modern convergent margins characterized by
active subduction, as negatively buoyant oceanic lithosphere sinks into the asthenosphere …
active subduction, as negatively buoyant oceanic lithosphere sinks into the asthenosphere …
[图书][B] Atmospheric evolution on inhabited and lifeless worlds
DC Catling, JF Kasting - 2017 - books.google.com
As the search for Earth-like exoplanets gathers pace, in order to understand them, we need
comprehensive theories for how planetary atmospheres form and evolve. Written by two well …
comprehensive theories for how planetary atmospheres form and evolve. Written by two well …
The crust of the Moon as seen by GRAIL
High-resolution gravity data obtained from the dual Gravity Recovery and Interior Laboratory
(GRAIL) spacecraft show that the bulk density of the Moon's highlands crust is 2550 …
(GRAIL) spacecraft show that the bulk density of the Moon's highlands crust is 2550 …
Giant impacts and the origin and evolution of continents
Earth is the only planet known to have continents, although how they formed and evolved is
unclear. Here using the oxygen isotope compositions of dated magmatic zircon, we show …
unclear. Here using the oxygen isotope compositions of dated magmatic zircon, we show …
The effect of Jupiter's formation on the distribution of refractory elements and inclusions in meteorites
We present a comprehensive evolutionary model of the Sun's protoplanetary disk,
constructed to resolve the" CAI storage problem" of meteoritics. We predict the abundances …
constructed to resolve the" CAI storage problem" of meteoritics. We predict the abundances …
The timeline of the lunar bombardment: Revisited
A Morbidelli, D Nesvorny, V Laurenz, S Marchi… - Icarus, 2018 - Elsevier
The timeline of the lunar bombardment in the first Gy of Solar System history remains
unclear. Basin-forming impacts (eg Imbrium, Orientale), occurred 3.9–3.7 Gy ago, ie 600 …
unclear. Basin-forming impacts (eg Imbrium, Orientale), occurred 3.9–3.7 Gy ago, ie 600 …
Statistical study of the early solar system's instability with four, five, and six giant planets
D Nesvorný, A Morbidelli - The Astronomical Journal, 2012 - iopscience.iop.org
Several properties of the solar system, including the wide radial spacing and orbital
eccentricities of giant planets, can be explained if the early solar system evolved through a …
eccentricities of giant planets, can be explained if the early solar system evolved through a …
Origin and evolution of the atmospheres of early Venus, Earth and Mars
We review the origin and evolution of the atmospheres of Earth, Venus and Mars from the
time when their accreting bodies were released from the protoplanetary disk a few million …
time when their accreting bodies were released from the protoplanetary disk a few million …