Results 31 to 40 of about 3,207,512 (305)
Sodium and Potassium Signatures of Volcanic Satellites Orbiting Close-in Gas Giant Exoplanets [PDF]
Extrasolar satellites are generally too small to be detected by nominal searches. By analogy to the most active body in the solar system, Io, we describe how sodium (Na i) and potassium (K i) gas could be a signature of the geological activity venting ...
A. Oza +14 more
semanticscholar +1 more source
New progresses in basic geological theories and future exploration domains of natural gas in China
As natural gas exploration expands to deep, ultra-deep and unconventional areas, more and more complex exploration targets are encountered. In this circumstance, it is necessary to improve the existing basic natural gas geological theories for guiding ...
Jian Li +10 more
doaj +1 more source
Influence of Compositional Gradient Effect on Tight Condensate Gas Reservoir Development
Condensate gas is a transition fluid between oil and gas, which is sensitive to the reservoir temperature and pressure. In condensate gas reservoir, especially in the moderate-giant one, fluid composition often varies with depth.
Jing Chen +5 more
doaj +1 more source
From Planetesimal to Planet in Turbulent Disks. II. Formation of Gas Giant Planets [PDF]
In the core accretion scenario, gas giant planets are formed form solid cores with several Earth masses via gas accretion. We investigate the formation of such cores via collisional growth from kilometer-sized planetesimals in turbulent disks.
H. Kobayashi, Hidekazu Tanaka
semanticscholar +1 more source
A series of seismic exploration technologies, such as “wide line and big combination” mountainous seismic acquisition, high steep structure pre-stack depth migration processing and deep tectonic modeling, were used to explore Kuqa deep structures.
Jinhu DU +4 more
doaj +1 more source
Changes in the metallicity of gas giant planets due to pebble accretion [PDF]
We run numerical simulations to study the accretion of gas and dust grains onto gas giant planets embedded into massive protoplanetary discs. The outcome is found to depend on the disc cooling rate, planet mass, grain size and irradiative feedback from ...
J. Humphries, S. Nayakshin
semanticscholar +1 more source
Restrictions on the Growth of Gas Giant Cores via Pebble Accretion [PDF]
We apply an order-of-magnitude model of gas-assisted growth, known as pebble accretion, in a turbulent medium to suggest a reason why some systems form wide orbital separation gas giants while others do not. In contrast to traditional growth by ballistic
M. Rosenthal, R. Murray-Clay
semanticscholar +1 more source
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
In warm (equilibrium temperature
Benjamin Fleury +5 more
doaj +1 more source
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

