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Red terrestrial planets: Searching for evidence for life beyond the Solar System

2021
Red dwarfs, which are stars that are typically born with masses below 0.6 Msun, are the most numerous stars and comprise about 70% of the stellar population in the Solar neighbourhood. Since we rely on indirect methods for detection of exoplanets, this small stars provide a number of advantages for the detection of the smallest planets.
openaire   +1 more source

Solar System Cratering Chronology and Dating of the Surface Structures of the Terrestrial-Type Planets

1982
The ancient impact record of the terrestrial-type planets Mercury, Mars, earth’s moon, and of the satellites of Jupiter and Saturn is discussed on the basis of data from spacecraft imagery. The mass-velocity distribution of the impactors seems to have been the same or very similar in the inner part of the solar system and probably also at Jupiter and ...
openaire   +1 more source

Early Giant Planet Migration in the Solar System: Geochemical and Cosmochemical Implications for Terrestrial Planet Formation

2010
A new terrestrial planet formation model (Walsh et al., this meeting) explores the effects of a two-stage, inward-then-outward migration of Jupiter and Saturn, as found in numerous hydrodynamical simulations of giant planet formation (Masset & Snellgrove 2001, Morbidelli & Crida 2007, Pierens & Nelson 2008). Walsh et al.
O'Brien, David P.   +5 more
openaire   +1 more source

Combined giant and terrestrial planet formation in the Solar System

Goldschmidt2025 abstracts
Ramon Brasser   +5 more
openaire   +1 more source

Scenarios of giant planet formation and evolution and their impact on the formation of habitable terrestrial planets

Philosophical Transactions Series A, Mathematical, Physical, and Engineering Sciences, 2014
Alessandro Morbidelli
exaly  

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