From
THIS Wiki, I find this:
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Uranus and Neptune may be considered a separate subclass of giant planets, 'ice giants', or 'Uranian planets', as they are mostly composed of ice, rock, as well as gases of water, ammonia and methane, unlike the "traditional" gas giants Jupiter or Saturn. However, they share the same qualities of the lack of the solid surface; their differences stem from the fact that their proportion of hydrogen and helium is lower, due to their greater distance from the Sun.
Gas giants may have a rocky or metallic core—in fact, such a core is thought to be required for a gas giant to form—but the majority of its mass is in the form of the gaseous hydrogen and helium, with traces of water, methane, ammonia, and other hydrogen compounds.
Unlike rocky planets, which have a clearly defined difference between atmosphere and surface, gas giants do not have a well-defined surface; their atmospheres simply become gradually denser toward the core, perhaps with liquid or liquid-like states in between. One cannot "land on" such planets in the traditional sense. Thus, terms such as diameter, surface area, volume, surface temperature and surface density may refer only to the outermost layer visible from space.
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And, I thought this was interesting trivia...
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The term gas giant was coined in 1952 by the science fiction writer James Blish. Arguably it is somewhat of a misnomer, since throughout most of the volume of these planets, there is no distinction between liquids and gases, since all the components (other than solid materials in the core) are above the critical point, so that the transition between gas and liquid is smooth. Jupiter is an exceptional case, having metallic hydrogen near the center, as explained above, but much of its volume is hydrogen, helium and traces of other gases above their critical points.
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As far as a gas giant's "atmosphere" goes, here's what the Wiki says....
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The observable atmospheres of any of these planets (at less than unit optical depth) are quite thin compared to the planetary radii, only extending perhaps one percent of the way to the center.
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That last bit is what we were looking for, folks.
So, in order to skim from a gas giant, the ship has to dive
past the planetary diameter of the gas giant in order to skim fuel.
The STANDARD WORLDS table in Book 2 gives us the G rating of a world at its surface. Looking at the "Gs" column of the table, its easy to see that Jupiter's G rating at its diameter is 2.621 Gs. Saturn's is 1.157 Gs. Uranus is 0.887 Gs. And Neptune's is 1.16 Gs.
Note that the gas giant's G rating will
increase the closer you get to the planet's core.
But, also note Boomslang's correction of my earilier post: Even a ship rated at 1G can defeat the gravitational pull of Jupiter at its diameter if the ship's velocity is great enough.
It's another one of those factors that makes gas giant skimming dangerous.
Funny, isn't it, how this all makes sense when viewing the rules in the LBBs. Under the LESSER KNOWN ASPECTS OF SPACE TRAVEL, the LBBs state that skimming from a GG takes about 8 hours and the ship must
dive deep into the GGs atmosphere with open fuel scoops.
With the atmo of a GG being so thin, we can easily use the rule of thumb of the GG's diameter as the point at which the ship must cross and "dive deep" to obtain fuel.