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

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direc<strong>to</strong>r <strong>of</strong> development operations at the Army Ballistic<br />

Missile Agency, and then as deputy <strong>to</strong> von Braun at the<br />

Marshall Space Flight Center. In 1970, he succeeded<br />

von Braun as Marshall SFC’s direc<strong>to</strong>r before retiring in<br />

1973.<br />

regenerative cooling<br />

<strong>The</strong> cooling <strong>of</strong> part <strong>of</strong> an engine by the propellant. A<br />

regeneratively cooled engine is one in which the fuel or<br />

oxidizer, or both, is circulated around the combustion<br />

chamber or nozzle.<br />

regimes <strong>of</strong> flight<br />

Ranges <strong>of</strong> speed defined relative <strong>to</strong> the local speed <strong>of</strong><br />

sound. <strong>The</strong>y are subsonic, transonic, supersonic, and<br />

hypersonic.<br />

regressive burning<br />

In solid-propellant rocket mo<strong>to</strong>rs, the burning <strong>of</strong> the fuel<br />

in such a way that the chamber pressure steadily decreases<br />

throughout the burn time, thus delivering steadily<br />

decreasing thrust.<br />

relativistic effects<br />

Several peculiar effects, predicted by Einstein’s special<br />

theory <strong>of</strong> relativity, that come in<strong>to</strong> play when objects—<br />

such as spacecraft—travel at speeds that are a substantial<br />

fraction <strong>of</strong> the speed <strong>of</strong> light. <strong>The</strong>se effects include time<br />

dilation, mass increase, and length contraction. Time<br />

dilation refers <strong>to</strong> the slowing down <strong>of</strong> the passage <strong>of</strong> time<br />

at very high speeds, effectively making it possible <strong>to</strong><br />

spend energy <strong>to</strong> buy time. A potentially important consequence<br />

follows for interstellar flight: simply by traveling<br />

fast enough, an astronaut can reach any destination<br />

within a specified amount <strong>of</strong> (shipboard) time. <strong>The</strong> table<br />

(“Shipboard Travel Times <strong>to</strong> Arcturus”) shows the travel<br />

times, as measured by onboard clocks, <strong>to</strong> the star Arcturus,<br />

which is located 36 light-years away, for a spacecraft<br />

traveling at various speeds.<br />

Shipboard Travel Times <strong>to</strong> Arcturus<br />

Speed (fraction <strong>of</strong><br />

light-speed) 0.1 0.5 0.9 0.99 0.999<br />

Travel time (years) 35.8 31.2 15.7 5.1 1.6<br />

While time dilation enables, in principle, a spacecraft<br />

<strong>to</strong> reach anywhere in the Galaxy (or the Universe) within<br />

a human lifetime simply by traveling fast enough, there is<br />

a serious downside. In exploiting this effect, astronauts<br />

would age less than everyone else, including their friends<br />

Relay 343<br />

and family, who remained behind. For very long journeys<br />

at high fractions <strong>of</strong> the speed <strong>of</strong> light, the time dislocation<br />

would be so great that many generations, and even<br />

millennia, might pass on the home planet before the<br />

interstellar travelers returned. For example, an excursion<br />

from Earth <strong>to</strong> Rigel—900 light-years away—and back, at a<br />

constant 99.99% <strong>of</strong> light-speed, would take 1,800 years as<br />

measured on Earth but only about 28 years as experienced<br />

by those on the spacecraft.<br />

<strong>The</strong> other major consequence for space travel at relativistic<br />

speed is the increase in mass <strong>of</strong> a spacecraft. This<br />

would make it more and more difficult <strong>to</strong> continue <strong>to</strong><br />

accelerate the vehicle. <strong>The</strong> fac<strong>to</strong>r that determines the<br />

amount <strong>of</strong> mass increase and time dilation is called<br />

gamma (γ). For an object moving with speed v relative <strong>to</strong><br />

an observer considered <strong>to</strong> be at rest (for example, on<br />

Earth), γ is given by<br />

γ=1 / �(1 �− v 2 /c 2 �)<br />

where c is the speed <strong>of</strong> light.<br />

<strong>The</strong> relativistic mass, m, <strong>of</strong> a body moving at velocity v<br />

is then<br />

m =γm0 = m0 / �(1 �− v 2 /c 2 �)<br />

where m0 is the rest mass. Note that when v = 0, this<br />

reduces <strong>to</strong> the non-relativistic result m = m0. <strong>The</strong> impossibility<br />

<strong>of</strong> accelerating an object up <strong>to</strong> the speed <strong>of</strong> light is<br />

shown by the fact that when v = c, m becomes infinite.<br />

Similarly, the relativistic time dilation is given by:<br />

t = t0 / γ=t0 �(1 �− v 2 /c 2 �)<br />

Relay<br />

Two spacecraft, designed and built by RCA, <strong>to</strong> test intercontinental<br />

satellite communications technology. Relay<br />

was a communications satellite <strong>of</strong> the active repeater<br />

type, in which signals from one ground station were<br />

picked up and rebroadcast <strong>to</strong> another station by the satellite’s<br />

internal equipment. Relay 1 remained operational<br />

for more than two years; Relay 2 was used in thousands<br />

<strong>of</strong> tests and experiments and in some 40 public demonstrations<br />

through September 1965. See Telstar. (See<br />

table, “Relay Missions.”)<br />

Launch<br />

Vehicle: Delta B<br />

Site: Cape Canaveral<br />

Mass: 78 kg<br />

Relay Missions<br />

Spacecraft Launch Date Orbit<br />

Relay 1 Dec. 13, 1962 1,319 × 7,440 km × 47.5°<br />

Relay 2 Jan. 21, 1964 1,961 × 7,540 km × 46.4°

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