Results 1 to 10 of about 312,448 (341)
The California Legacy Survey. IV. Lonely, Poor, and Eccentric: A Comparison between Solitary and Neighborly Gas Giants [PDF]
We compare systems with single giant planets to systems with multiple giant planets using a catalog of planets from a high-precision radial velocity survey of FGKM stars.
Lee J. Rosenthal +3 more
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Separating gas-giant and ice-giant planets by halting pebble accretion [PDF]
In the Solar System giant planets come in two flavours: 'gas giants' (Jupiter and Saturn) with massive gas envelopes and 'ice giants' (Uranus and Neptune) with much thinner envelopes around their cores.
Michiel Lambrechts +2 more
openalex +4 more sources
THE TWO MODES OF GAS GIANT PLANET FORMATION [PDF]
Submitted to ApJL after addressing referee's ...
Aaron C. Boley +35 more
openaire +5 more sources
The comprehensive analysis of geological setting, accumulation condition, trapping mechanism and distribution regularity of oil-gas of the Upper Triassic in Sichuan Basin reveals that the gas accumulation in Xujiahe Formation is a layered lithologic ...
Zou Caineng +11 more
doaj +2 more sources
On the Formation of Gas Giant Planets on Wide Orbits [PDF]
A new suite of three dimensional radiative, gravitational hydrodynamical models is used to show that gas giant planets are unlikely to form by the disk instability mechanism at distances of ~100 AU to ~200 AU from young stars.
Alan P. Boss
openalex +4 more sources
Industrial gas giants seek megamerger [PDF]
Alex Scott
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Tidally Heated Exomoons around Gas Giants [PDF]
Abstract Thousands of exoplanets have been discovered; however, the detection of exomoons remains elusive. Tidally heated exomoons have been proposed as candidate targets for observation; vigorous tidal dissipation can raise the moon’s surface temperature, making direct imaging possible, and cause widespread volcanism that can have a ...
Marc Rovira-Navarro +3 more
openaire +3 more sources
What Can Meteorites Tell Us About the Formation of Jupiter?
Gas giants like Jupiter are a fundamental component of planetary systems, but how they formed has been uncertain. Here we discuss how paleomagnetic records in meteorites of the solar nebula may tell us about Jupiter's final growth stage.
Benjamin P. Weiss, William F. Bottke
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Forming Gas Giants around a Range of Protostellar M-dwarfs by Gas Disk Gravitational Instability
Recent discoveries of gas giant exoplanets around M-dwarfs from transiting and radial velocity surveys are difficult to explain with core-accretion models. We present here a homogeneous suite of 162 models of gravitationally unstable gaseous disks. These
Alan P. Boss, Shubham Kanodia
doaj +1 more source
Connotations of scientific development of giant gas fields in China
A giant gas field refers to a gas field with proved geological reserves of natural gas more than 30 billion cubic meters, peak annual output of natural gas more than 1 billion cubic meters, and a certain plateau period.
Caineng Zou +6 more
doaj +1 more source

