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The Complete Book of Spaceflight: From Apollo 1 to Zero Gravity

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nozzle <strong>The</strong> Space Shuttle main engine test firing in 1981. NASA<br />

tion at the exit, the higher the speed and the lower the<br />

pressure that the gas can achieve at the exit. For optimum<br />

thrust, the gas pressure at the nozzle exit should be<br />

exactly equal <strong>to</strong> the outside air pressure. In the vacuum <strong>of</strong><br />

space the outside pressure is zero, so it is impossible for<br />

this optimum <strong>to</strong> be achieved. <strong>The</strong> bigger the exit area <strong>of</strong><br />

the nozzle, the closer the thrust will be <strong>to</strong> optimum; however,<br />

there is a point at which gains in thrust are <strong>of</strong>fset by<br />

the extra mass needed <strong>to</strong> make the nozzle wider. Even<br />

during the atmospheric portion <strong>of</strong> a rocket’s flight it is<br />

impossible <strong>to</strong> achieve theoretical optimum performance,<br />

because the outside air pressure changes as the vehicle<br />

climbs. All designers can do is target the performance <strong>of</strong> a<br />

nozzle <strong>to</strong> some average outside pressure.<br />

When a nozzle ends before the gas reaches the pressure<br />

<strong>of</strong> the outside air, it is called an under-expanded nozzle.<br />

In the under-expanded case, the rocket design is not getting<br />

all the thrust that it can from the engine. When a<br />

nozzle is <strong>to</strong>o large and keeps trying <strong>to</strong> expand the gas<br />

flow, at some point the rocket plume will separate from<br />

the wall inside the nozzle. This is called an over-expanded<br />

nozzle. <strong>The</strong> performance from an over-expanded nozzle<br />

is worse than in the under-expanded case, because the<br />

nozzle’s large exit area results in extra drag.<br />

nuclear power for spacecraft 299<br />

Like the combustion chamber, the nozzle throat gets<br />

very hot. Nozzle throats are <strong>of</strong>ten cooled by circulating<br />

fuel directly behind the pressure wall <strong>to</strong> cool it. <strong>The</strong> fuel<br />

passes through while it is still cool on its way <strong>to</strong> the combustion<br />

chamber. This has the added bonus <strong>of</strong> preheating<br />

the fuel before combustion, making more energy available<br />

from the combustion <strong>to</strong> provide thrust. Recently,<br />

new materials have become available, including ceramics<br />

and composites, that can withstand extremely high temperatures.<br />

<strong>The</strong>se materials <strong>of</strong>ten slowly ablate under the<br />

extreme conditions in the nozzle throat <strong>of</strong> a highperformance<br />

rocket; however, the ablation rates may be<br />

<strong>to</strong>lerable in a rocket that is only fired once. In the case <strong>of</strong><br />

a rocket designed for multiple firings, either in the same<br />

mission or in multiple missions, cooling rather than ablation<br />

is likely <strong>to</strong> be the method <strong>of</strong> choice.<br />

nozzle area ratio<br />

<strong>The</strong> ratio <strong>of</strong> a nozzle’s throat area <strong>to</strong> the exit area. <strong>The</strong> ideal<br />

nozzle area ratio allows the gases <strong>of</strong> combustion <strong>to</strong> exit the<br />

nozzle at the same pressure as the ambient pressure.<br />

nozzle efficiency<br />

<strong>The</strong> efficiency with which the nozzle converts the potential<br />

energy <strong>of</strong> a burned fuel in<strong>to</strong> kinetic energy for thrust.<br />

nozzle exit angle<br />

<strong>The</strong> angle <strong>of</strong> divergence <strong>of</strong> a nozzle.<br />

nuclear detection satellites<br />

Spacecraft designed <strong>to</strong> detect nuclear explosions on the<br />

ground or in the atmosphere. Although primarily intended<br />

<strong>to</strong> moni<strong>to</strong>r nuclear treaty compliance, these satellites have<br />

also been used <strong>to</strong> detect and observe galactic events such as<br />

supernovae. See Vela and Advanced Vela.<br />

nuclear fission<br />

See fission, nuclear.<br />

nuclear fuel<br />

Fissionable material <strong>of</strong> reasonably long life, used or<br />

usable in producing energy in a nuclear reac<strong>to</strong>r.<br />

nuclear fusion<br />

See fusion, nuclear.<br />

nuclear power for spacecraft<br />

Nuclear power has essentially three applications <strong>to</strong> spaceflight:<br />

<strong>to</strong> provide a source <strong>of</strong> heat <strong>to</strong> keep equipment<br />

warm (see radioiso<strong>to</strong>pe heater unit [RHU]), <strong>to</strong> provide<br />

a source <strong>of</strong> electricity <strong>to</strong> power equipment (see radioiso<strong>to</strong>pe<br />

thermoelectric genera<strong>to</strong>r [RTG]), or <strong>to</strong> provide<br />

a means <strong>of</strong> propulsion either directly (see nuclear

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