Results 261 to 270 of about 36,303 (299)

Two Novel Cloud-Masking Algorithms Tested in a Tropical Forest Setting Using High-Resolution NICFI-Planet Basemaps. [PDF]

Sensors (Basel)
Islam KMA, Abir S, Kennedy R.
europepmc   +1 more source

The hidden mysteries of our ice giant planets. [PDF]

Nat Commun
de Villa K, Ge H.
europepmc   +1 more source

Improvement of merging processes in N-body simulations in circumstellar disks

Zimmermann M, Pilat-Lohinger E.
europepmc   +1 more source

Planet Formation

, 2006
When this book was published in 2006, it had been just over ten years since the first planet outside our solar system was detected. Since then, much work has focused on understanding how extrasolar planets may form, and discovering the frequency of potentially habitable Earth-like planets.
Klahr, Hubert, Brandner, Wolfgang
core   +3 more sources

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Formation and Evolution of Planets

Astrophysics and Space Science, 1994
The basic stages of the formation of the planets are considered. Decay of turbulence in the solar nebula allows the precipitation of dust particles to the solar nebula’s equatorial plane, their growth occurring by sticking at collisions and transformation into kilometer-sized bodies (planetesimals) partly by direct growth and partly via gravitational ...
V. S. Safronov, E. L. Ruskol
openaire   +1 more source

Formation of Stars and Planets

Astronomische Nachrichten, 2004
A01 Modeling the Resonant Planetary System GJ 876 A02 First Classification of Dusty Protoplanets A03 IDL-Models of Infrared Emission from Dust Objects (Applied to Dust in Comets) A04 Theoretical Predicitions and Observational Tests of the Migration Hypothesis A05 Towards Characterization of Exoplanetary Spectra with the VLT ...
Wuchterl, Günther, Guenther, Eike
openaire   +2 more sources

Sandwiched planet formation: restricting the mass of a middle planet [PDF]

Monthly Notices of the Royal Astronomical Society
We conduct gas and dust hydrodynamical simulations of protoplanetary discs with one and two embedded planets to determine the impact that a second planet located further out in the disc has on the potential for subsequent planet formation in the region ...
D J Armstrong, Sahl Rowther, Farzana Meru   +2 more
exaly   +2 more sources

Extrasolar Planets: Constraints for Planet Formation Models

Science, 2005
Since 1995, more than 150 extrasolar planets have been discovered, most of them in orbits quite different from those of the giant planets in our own solar system. The number of discovered extrasolar planets demonstrates that planetary systems are common but also that they may possess a large variety of properties.
Nuno C, Santos, Willy, Benz, Michel, Mayor   +2 more
openaire   +2 more sources

Formation of the terrestrial planets

Earth, Moon, and Planets, 1994
The early phases of formation in the inner solar system were dominated by collisions and short-range dynamical interactions among planetesimals. But the later phases, which account for most of the differences among planets, are unsure because the dynamics are more subtle. Jupiter’s influence became more important, leading to drastic clearing out of the
openaire   +1 more source