Results 11 to 20 of about 1,415 (183)
Effects of Outer Giant Planets on In Situ Formation of Inner Super-Earths
Recent studies have found an observational correlation between the presence of outer giant planets and inner super-Earths, which implies that outer giants do not suppress the formation of super-Earths.
Phoebe Sandhaus +4 more
doaj +2 more sources
On the mass of gas giant planets: Is Saturn a failed gas giant?
The formation history of giant planets inside and outside the solar system remains unknown. We suggest that runaway gas accretion is initiated only at a mass of ~100 M_Earth and that this mass corresponds to the transition to a gas giant, a planet that ...
Ravit Helled +2 more
core +1 more source
Giant planet formation in the solar system [PDF]
The formation history of Jupiter has been of interest due to its ability to shape the solar system's history. Yet little attention has been paid to the formation and growth of Saturn and the other giant planets.
Raorane, Anuja +5 more
core +5 more sources
Isotopic ratios D/H and ¹⁵ N/¹⁴N in giant planets [PDF]
The determination of isotopic ratios in planets is important since it allows us to investigate the origins and initial composition of materials. The present work aims to determine the possible range of values for isotopic ratios D/H and ¹⁵N/¹⁴N in giant ...
Amaury Thiabaud +7 more
core +1 more source
Formation of multiple giant planets and their impact on the protoplanetary disc structure [PDF]
The Solar System, together with some exoplanetary systems, is known to host multiple planets. These planets are believed to be born in discs composed of gas and dust in rotation around forming stars. These discs are called protoplanetary discs.
Bergez-Casalou, Camille Arantxa
core +1 more source
THE ANGLO-AUSTRALIAN PLANET SEARCH. XXI. A GAS-GIANT PLANET IN A ONE YEAR ORBIT AND THE HABITABILITY OF GAS-GIANT SATELLITES [PDF]
We have detected the Doppler signature of a gas-giant exoplanet orbiting the star HD 38283, in an eccentric orbit with a period of almost exactly one year (P = 363.2 ± 1.6 d, m sin i = 0.34 ± 0.02 M Jup, e = 0.41 ± 0.16).
C. G. Tinney +15 more
core +1 more source
KOI-3158: The oldest known system of terrestrial-size planets
The first discoveries of exoplanets around Sun-like stars have fueled efforts to find ever smaller worlds evocative of Earth and other terrestrial planets in the Solar System. While gas-giant planets appear to form preferentially around metal-rich stars,
Campante T. L. +40 more
doaj +1 more source
Dependencies of Mantle Shock Heating in Pairwise Accretion
The final assembly of planets involves mutual collisions of large similar-sized protoplanets (“giant impacts”), setting the stage for modern geologic and atmospheric processes.
Travis S. J. Gabriel, Harrison W. Horn
doaj +1 more source
Giant Planets from the Inside-Out
Giant planets acquire gas, ices and rocks during the early formation stages of planetary systems and thus inform us on the formation process itself.
Tristan Guillot (8621181) +5 more
core +3 more sources
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
core +1 more source

