Shock Events in the Solar System: The Message from Minerals in Terrestrial Planets and Asteroids
Annual Review of Earth and Planetary Sciences, 2013 Impacts are central to the origin and evolution of planets of the Solar System. The shapes of craters, which can reach up to 1,000 km in diameter on the Moon, provide critical information on the large-scale dynamics of the impact and related shock. Minerals formed at high pressure and temperature found in shocked terrestrial rocks and meteorites give ...
Philippe Gillet, A. El Goresy
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The great dichotomy of the Solar System: Small terrestrial embryos and massive giant planet cores [PDF]
Icarus, 2015 In press in ...
Alessandro Morbidelli +3 more
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A Resonant Beginning for the Solar System’s Terrestrial Planets
The Astrophysical JournalIn the past two decades, transit surveys have revealed a class of planets with thick atmospheres—sub-Neptunes—that must have completed their accretion in protoplanet disks.
Shuo Huang +4 more
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Terrestrial Planet Formation: The Solar System and Other Systems [PDF]
Symposium - International Astronomical Union, 2004 Accretion of terrestrial planets and solid cores of jovian planets is discussed, based on the results of our N-body simulations. Protoplanets accrete from planetesimals through runaway and oligarchic growth until they become isolated. The isolation mass of protoplanets in terrestrial planet region is about 0.2 Earth mass, which suggests that in the ...
Shigeru Ida, Eiichiro Kokubo
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Atmospheric Retrieval of Terrestrial Solar System Planets for LIFE [PDF]
, 2022 ISSN:0002 ...
Björn S. Konrad +4 more
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A pebble accretion model for the formation of the terrestrial planets in the Solar System
Science Advances, 2021 A new theory for formation of Earth by accretion of small pebbles explains how our planet acquired its water and carbon.
Anders Johansen +6 more
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Terrestrial planet formation from lost inner solar system material [PDF]
Science Advances, 2021 An integrated assessment of isotopic variations among meteorites reveals the process by which Earth and Mars are formed.
Christoph Burkhardt +6 more
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Chromium isotopic insights into early solar system evolution and origin of terrestrial planets [PDF]
, 2021 Les isotopes du chrome (Cr) jouent un rôle important dans la cosmochimie et les sciences planétaires car ce sont de puissants outils pour dater (chronométrie de courte période 53Mn-53Cr), tracer (anomalies nucléosynthétiques 54Cr) les origines des matériaux, et étudier les processus impliqués dans le fractionnement des éléments volatils et la ...
Ke Zhu
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Late Accretion and the Origin of Water on Terrestrial Planets in the Solar System
, 2021 <p>Terrestrial planets in the Solar system generally lack surface liquid water. Earth is at odd with this observation and with the idea of the giant Moon-forming impact that should have vaporized any pre-existing water, leaving behind a dry Earth.
Cédric Gillmann +6 more
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