Results 51 to 60 of about 182,451 (170)
Making Extrasolar Planets From Solar Systems Via Dynamical Interactions
Most stars form in some sort of stellar cluster or association. In such environments the number density of stars is much higher than in the solar neighbourhood, which means that close encounters between stars may be relatively common.
D. Malmberg +4 more
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From Earths to Super-Earths: Five New Small Planets Transiting M Dwarf Stars
Earth-sized planets transiting M dwarf stars present one of the best opportunities with current facilities for studying the atmospheric and bulk compositions of terrestrial worlds. Here, we statistically validate five new transiting Earth and super-Earth
Jonathan Gomez Barrientos +41 more
doaj +1 more source
Theoretical frameworks for reflection and emission spectroscopy of exoplanet surfaces are becoming increasingly important for the characterization of rocky exoplanets, especially with the rapid growth of the detected exoplanet population and ...
Leonardos Gkouvelis
doaj +1 more source
The atmospheres of extrasolar planets [PDF]
The discovery of extrasolar planets, or “exoplanets” – i.e., planets orbiting around other stars – may be seen as the major discovery of astronomy over the past two decades.
Thérèse Encrenaz, Encrenaz, Thérèse
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A Formation-stage Bottleneck for Exomoons around Close-in Rocky Planets
Massive moons around rocky exoplanets are expected outcomes of giant impacts, yet no exomoon has been securely confirmed. We address this problem using meshless finite-mass (MFM) simulations of giant impacts between differentiated rocky planets that ...
Rongxi Bi +4 more
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The influence of galactic cosmic rays on ion-neutral hydrocarbon chemistry in the upper atmospheres of free-floating exoplanets [PDF]
The authors highlight financial support of the European Community under the FP7 by an ERC starting grant.Cosmic rays may be linked to the formation of volatiles necessary for prebiotic chemistry.
P. B. Rimmer +5 more
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Small and Close-in Planets are Uncommon Around A-type Stars
The Kepler and K2 missions enabled robust calculations of planet occurrence rates around FGKM-type stars. However, these missions observed too few stars with earlier spectral types to tightly constrain the occurrence rates of planets orbiting hotter ...
Steven Giacalone, Courtney D. Dressing
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In the late stage of terrestrial planet formation, planets are predicted to undergo pairwise collisions known as giant impacts. Here, we present a high-resolution database of giant impacts for differentiated colliding bodies of iron–silicate composition,
Alexandre Emsenhuber +6 more
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Photosynthesis in Hydrogen-Dominated Atmospheres
The diversity of extrasolar planets discovered in the last decade shows that we should not be constrained to look for life in environments similar to early or present-day Earth.
William Bains, Sara Seager, Andras Zsom
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Migration and Extrasolar Terrestrial Planets: Watering the Planets
International audienceSimulations of the compositions of extrasolar terrestrial planets have shown that migration of giant planets assists in producing "Earth-like" terrestrial planets and delivering water and other volatiles to terrestrial planets ...
Carter-Bond, J. C. +2 more
core +3 more sources

