Results 31 to 40 of about 313,222 (342)
Clearing residual planetesimals by sweeping secular resonances in transitional disks: a lone-planet scenario for the wide gaps in debris disks around Vega and Fomalhaut [PDF]
, 2017 Extended gaps in the debris disks of both Vega and Fomalhaut have been observed. These structures have been attributed to tidal perturbations by multiple super-Jupiter gas giant planets.
Kouwenhoven, M. B. N. +4 more
core +2 more sources
Journal of Petroleum Exploration and Production Technology, 2018 1986 saw the publication of a prognostic map for discovering giant oil and gas fields in the Andes in South America based on the recent block structure of the Earth’s crust.
Shelia Guberman, Yury Pikovskiy
doaj +1 more source
The Nature of Gas Giant Planets
, 2023 Revealing the true nature of the gas giant planets in our Solar System is challenging. The masses of Jupiter and Saturn are about 318 and 95 Earth masses, respectively. While they mostly consist of hydrogen and helium, the total mass and distribution of the heavier elements, which reveal information on their origin, are still unknown.
Helled, Ravit +2 more
openaire +2 more sources
Petroleum Exploration and Development, 2009 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 +1 more source
How fast do Jupiters grow? Signatures of the snowline and growth rate in the distribution of gas giant planets [PDF]
, 2012 We present here observational evidence that the snowline plays a significant role in the formation and evolution of gas giant planets. When considering the population of observed exoplanets, we find a boundary in mass-semimajor axis space that suggests ...
Horne, Keith +2 more
core +3 more sources
Petroleum Exploration and Development, 2014 The Anyue Sinian–Cambrian giant gas field was discovered in central paleo-uplift in the Sichuan Basin in 2013, which is a structural-lithological gas reservoir, with 779.9 km2 proven gas-bearing area and 4 403.8×108 m3 proven geological reserves in the ...
Caineng ZOU +14 more
doaj +1 more source
The migration of gas giant planets in gravitationally unstable disks [PDF]
, 2015 Planets form in the disks of gas and dust that surround young stars. It is not known whether or not gas giant planets on wide orbits form the same way as Jupiter or form by the fragmentation of gravitationally unstable disks.
Stamatellos, Dimitris
core +2 more sources
The Astrophysical Journal, 2023 In warm (equilibrium temperature
Benjamin Fleury +5 more
doaj +1 more source
Superchemistry: dynamics of coupled atomic and molecular Bose-Einstein condensates [PDF]
, 2000 We analyze the dynamics of a dilute, trapped Bose-condensed atomic gas coupled to a diatomic molecular Bose gas by coherent Raman transitions. This system is shown to result in a new type of `superchemistry', in which giant collective oscillations ...
A. A. Abrikosov +35 more
core +2 more sources
Dense gas in a giant molecular filament [PDF]
Astronomy & Astrophysics, 2020 Context. Recent surveys of the Galactic plane in the dust continuum and CO emission lines reveal that large (≳50 pc) and massive (≳105 M⊙) filaments, know as giant molecular filaments (GMFs), may be linked to Galactic dynamics and trace the mid-plane of the gravitational potential in the Milky Way.
Y. Wang +12 more
openaire +3 more sources