Results 211 to 220 of about 16,797 (229)

The Role of Atmospheric Composition in Defining the Habitable Zone Limits and Supporting E. coli Growth. [PDF]

Life (Basel)
Kuzucan A, Bolmont E, Chaverot G, Ferreira JQ, Ibelings BW, Bhatnagar S, McGinnis DF.   +6 more
europepmc   +1 more source

Evo-Inspired Engineering of Radical Phenotypes and Emergent Traits. [PDF]

Integr Comp Biol
Babonis LS, Hahn DA, Liu AP, Widhalm JR.
europepmc   +1 more source

Assembly Theory: What It Does and What It Does Not Do. [PDF]

J Mol Evol
Jaeger J.
europepmc   +1 more source

On the equilibrium limit of liquid stability in pressurized aqueous systems. [PDF]

Nat Commun
Zarriz A, Journaux B, Powell-Palm MJ.
europepmc   +1 more source

Precise Masses Reveal that TOI-700 c is Low Density and TOI-700 d is Rocky

Gilbert E, Burt J, Barragán O, Siegel J, Mascareño AS, Silva A, Luque R, Rogers J, Lee E, Lopez E, Vanderburg A, Clement M, Youngblood A, Mamajek E, Sousa S, Cameron AC, Rodriguez J, Martin D, Arney G, Barclay T, Becker J, Colon K, Eisner N, Halverson S, Hord B, Kane S, Kreidberg L, Morley C, Mortier A, Nielsen L, Quintana E, Schlieder J, Suissa G, Triaud A, Trifonov T, Eylen VV.   +35 more
europepmc   +1 more source

Optimizing photosynthetic light-harvesting under stars: Generalized thermodynamic models

Chitnavis S, Gray C, Rousouli I, Gillen E, Mullineaux CW, Haworth TJ, Duffy CDP.   +6 more
europepmc   +1 more source

Spin-Orbital Evolution of Exoplanets [PDF]

EAS Publications Series, 2003
We investigated the equation describing the evolution of the kinetic momentum vector of planets by the action of gravitational and magnetic interaction. The obtained gallery of portraits of the kinetic momentum evolution illustrates the various regimes of planetary system evolution.
A. Gusev, I. Kitiashvili
openaire   +1 more source

Evolution of Angular Momentum Distribution in Exoplanet Systems [PDF]

Astrophysics, 2015
The distribution of angular momentum is investigated in “star–planet systems, taking due account of stellar evolution effects. Numerical simulation is carried out for 15 systems for which stellar rotation data are available. Consideration of changes in stellar structure is confirmed to be significant for the evolution of momentum distribution.
P. A. Tarakanov, A. S. Artamonov
openaire   +1 more source

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Evolution of the obliquity of an exoplanet: A non-resonant case

Icarus, 2020
Abstract We investigate analytically and numerically the variation of the obliquity (the axial tilt) of a hypothetical exo-Earth. A large number of exoplanets was discovered recently; since not much information is available about the masses and orbits of the stars and planets comprising a planetary exo-system, unlike for the planets of the Solar ...
O.M. Podvigina, P.S. Krasilnikov
openaire   +2 more sources

Formation and Evolution of Exoplanets

2010
Introduction Exoplanet Observations Pinpointing Planets in Circumstellar Disks Planet-Planet Interactions Formation via Disk Instability Core Accretion Model Formation of Terrestrial Planets Brown Dwarfs Exoplanet Chemistry Migration and Multiplicity Effects During Giant Planet formation Planets in mean motion resonance Planet-Planet Gravitational ...
openaire   +2 more sources