Results 81 to 90 of about 299,348 (228)
Elemental ratios in stars vs planets
Context. The chemical composition of planets is an important constraint for planet formation and subsequent differentiation. While theoretical studies try to derive the compositions of planets from planet formation models in order to link the composition
Alibert, Yann +4 more
core +1 more source
Correction to the references Nurhasan OY et al (2006) and Tseng KH et al (2020)
Earth, Planets and Space
doaj +1 more source
On the Love Numbers of an Andrade Planet
The Andrade rheological model is often employed to describe the response of solar system or extra‐solar planets to tidal perturbations, especially when their properties are still poorly constrained.
Anastasia Consorzi +3 more
doaj +1 more source
Disruption of Planetary System Architectures by Stellar Flybys
We investigate the survivability of solar system-like planetary systems during close encounters in stellar associations using a suite of 1980 N-body simulations.
Robert Przyłuski +9 more
doaj +1 more source
Long range outward migration of giant planets, with application to Fomalhaut b
Recent observations of exoplanets by direct imaging, reveal that giant planets orbit at a few dozens to more than a hundred of AU from their central star.
Alessandro Morbidelli +16 more
core +3 more sources
Terrestrial planets across space and time
The study of cosmology, galaxy formation and exoplanets has now advanced to a stage where a cosmic inventory of terrestrial planets may be attempted. By coupling semi-analytic models of galaxy formation to a recipe that relates the occurrence of planets ...
Benson, A. +5 more
core +1 more source
Extrasolar planet population synthesis IV. Correlations with disk metallicity, mass and lifetime
Context. This is the fourth paper in a series showing the results of planet population synthesis calculations. Aims. Our goal in this paper is to systematically study the effects of important disk properties, namely disk metallicity, mass and lifetime ...
Alexander +107 more
core +2 more sources
Measurements of the frequency with which short-period planets occur around main sequence stars allows a direct prediction of the number and types of such planets that will be amenable to characterization by high-contrast instruments on future giant ...
Crossfield, Ian J. M.
core +1 more source
During the late stage of planet formation when Mars-size cores appear, interactions among planetary cores can excite their orbital eccentricities, speed their merges and thus sculpture the final architecture of planet systems.
Andrews +38 more
core +1 more source
Organic Molecules in the Icy Bodies of Planetary Systems – Accepted Notions and New Ideas
Cometary bodies are acknowledged to contain some of the most pristine matter in the Solar System, including ices and minerals. Certain number of previously unidentified spectral emission features detected in comets can be explained as emission by ...
Simonia Irakli, Cruikshank Dale P.
doaj +1 more source

