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The Gas Giants

2016
Saturn and Jupiter have more in common than they have in isolation, thus Chap. 7 compares and contrasts the two giant masters of the Sun’s planetary realm. Despite some issues of scale, the broad brush strokes of each planet are rather similar. Within this broad canvas there are specific differences in the appearance of each world and the behavior of ...
openaire   +2 more sources

DISCOVERY OF INTRA-CRATONIC RIFT IN THE UPPER YANGTZE AND ITS CONTROL EFFECT ON THE FORMATION OF ANYUE GIANT GAS FIELD

Геология и геофизика, 2020
: According to the drilling and seismic data, the Late Sinian-Early Cambrian intra-cratonic rift was found in Deyang-Anyue area of the Upper Yangtze craton.
Du Jinhu   +7 more
semanticscholar   +1 more source

Discovery of Intracratonic Rift in the Upper Yangtze and Its Control Effect on the Formation of the Anyue Giant Gas Field

Russian Geology and Geophysics, 2020
—According to drilling and seismic data, the Late Sinian–Early Cambrian intracratonic rift was found in the Deyang–Anyue area of the Upper Yangtze craton.
Jinhu Du   +7 more
semanticscholar   +1 more source

Giants of Gas and Ice

2013
Immediately beyond the orbit of Mars lies a wide gulf uninhabited by any major planet. It is, however, the abode of a great number of smaller sub-planetary bodies known as “asteroids,” about which more shall be said in the following chapter. Further beyond this region, extending to the very edges of the system of major planets, lies the realm of the ...
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Rapid formation of gas giants, ice giants and super-Earths [PDF]

open access: possiblePhysica Scripta, 2008
Giant planets might have been formed by either of the two basic mechanisms, top-down (disk instability) or bottom-up (core accretion). The latter mechanism is the most generally accepted mechanism and it begins with the collisional accumulation of solid cores that may then accrete sufficient gas to become gas giants.
openaire   +1 more source

On the current limits of simulating gas giant entry flows in an expansion tube

, 2015
Atmospheric entry to the Gas Giants involves entry velocities from 20 - 50 km/s, which is mostly beyond the capabilities of current ground testing facilities.
C. James   +5 more
semanticscholar   +1 more source

Jupiter: The Gas Giant

2016
Jupiter has a system of four thin rings composed of rocks and dust particles surrounding its atmosphere in an equatorial plane.
openaire   +2 more sources

Geology of giant gas fields in China

Marine and Petroleum Geology, 2008
Twenty-five gas fields with recognized ultimate recoveries larger than 25 billion cubic meters have been found in six basins in China. The earliest was found in 1959 and the latest in 2005. Recognition of more recent discoveries as giants will probably further increase the population.
Quanyou Liu   +8 more
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Giant Fluctuations in a Degenerate Fermi Gas

Physical Review Letters, 1960
It was suggested that the ground stute of an interacting gas of fermions has giart density or spin-density fluctuations and that the Hartree and Hartree- Fcck equations of a one-dimensional gas have solutions which give lower enengies than customary plane wave solutions.
Walter Kohn, Stephen J. Nettel
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Deep jets on gas-giant planets

Icarus, 2008
Abstract Three-dimensional numerical simulations of the atmospheric flow on giant planets using the primitive equations show that shallow thermal forcing confined to pressures near the cloud tops can produce deep zonal winds from the tropopause all the way down to the bottom of the atmosphere.
Yuan Lian, Adam P. Showman
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