The Complete Book of Spaceflight: From Apollo 1 to Zero Gravity
The Complete Book of Spaceflight: From Apollo 1 to Zero Gravity
The Complete Book of Spaceflight: From Apollo 1 to Zero Gravity
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98 Dawn<br />
preceded, in 2006, by SMART-2—a two-spacecraft array<br />
<strong>to</strong> demonstrate the type <strong>of</strong> formation flying that is essential<br />
<strong>to</strong> Darwin’s success. NASA is developing a similar<br />
mission, the Terrestrial Planet Finder, and it is possible<br />
that NASA and ESA will collaborate on a single mission<br />
that they will launch and operate <strong>to</strong>gether.<br />
Dawn<br />
A future NASA mission <strong>to</strong> two <strong>of</strong> the largest asteroids in<br />
the Solar System, Ceres and Vesta. Dawn, a Discovery<br />
Program mission, is scheduled <strong>to</strong> launch in May 2006,<br />
arrive at Vesta in 2010, orbit it for nine months, then<br />
move on <strong>to</strong> Ceres in 2014 for a further nine-month<br />
orbital stint. Dawn will be NASA’s first purely scientific<br />
mission <strong>to</strong> use ion propulsion <strong>of</strong> the type known as XIPS<br />
(xenon-ion propulsion system) that was flight-validated<br />
by Deep Space 1. <strong>The</strong> probe’s suite <strong>of</strong> science instruments<br />
will measure the exact mass, shape, and spin <strong>of</strong><br />
Vesta and Ceres from orbits 100 <strong>to</strong> 800 km high; record<br />
their magnetization and composition; pho<strong>to</strong>graph their<br />
surfaces; use gravity and magnetic data <strong>to</strong> determine the<br />
size <strong>of</strong> any metallic core; and use infrared and gamma-ray<br />
spectrometry <strong>to</strong> search for water-bearing minerals. Flybys<br />
<strong>of</strong> more than a dozen other asteroids are planned along<br />
the way. <strong>The</strong> overall goal <strong>of</strong> the mission is <strong>to</strong> learn more<br />
about the early his<strong>to</strong>ry <strong>of</strong> the Solar System and the mechanisms<br />
by which the planets formed.<br />
dawn rocket<br />
A rocket launched in<strong>to</strong> orbit in an easterly direction so<br />
that Earth’s rotation augments the rocket’s velocity. Most<br />
launches are <strong>of</strong> this type.<br />
DE (Dynamics Explorer)<br />
A NASA mission launched on August 3, 1981, involving<br />
two spacecraft <strong>to</strong> study the interaction between the hot,<br />
thin, convecting plasma <strong>of</strong> Earth’s magne<strong>to</strong>sphere and<br />
the cooler, denser plasmas and gases in the ionosphere<br />
and upper atmosphere. DE 1 and DE 2 were launched<br />
<strong>to</strong>gether and placed in polar coplanar orbits <strong>to</strong> allow<br />
simultaneous measurements at high and low altitudes in<br />
the same field-line region. <strong>The</strong> spacecraft approximated a<br />
short polygon 137 cm in diameter and 115 cm high. <strong>The</strong><br />
antennas in the x-y plane measured 200 m tip-<strong>to</strong>-tip, and<br />
on the z-axis 9 m tip-<strong>to</strong>-tip. Two 6-m booms were provided<br />
for remote measurements. Science operations continued<br />
successfully over a nine-year period until they<br />
were terminated on Oc<strong>to</strong>ber 22, 1990. <strong>The</strong> spacecraft<br />
were also known as Explorer 62 and 63.<br />
De Laval, Gustav (1845–1913)<br />
A Swedish engineer <strong>of</strong> French descent who, in trying <strong>to</strong><br />
develop a more efficient steam engine, designed a turbine<br />
that was turned by jets <strong>of</strong> steam. <strong>The</strong> critical component—the<br />
one in which heat energy <strong>of</strong> the hot highpressure<br />
steam from the boiler was converted in<strong>to</strong> kinetic<br />
energy—was the nozzle from which the jet blew on<strong>to</strong> the<br />
wheel. De Laval found that the most efficient conversion<br />
occurred when the nozzle first narrowed, increasing the<br />
speed <strong>of</strong> the jet <strong>to</strong> the speed <strong>of</strong> sound, and then<br />
expanded again. Above the speed <strong>of</strong> sound (but not<br />
below it), this expansion caused a further increase in the<br />
speed <strong>of</strong> the jet and led <strong>to</strong> a very efficient conversion <strong>of</strong><br />
heat energy <strong>to</strong> motion. Nowadays, steam turbines are the<br />
preferred power source <strong>of</strong> electric power stations and<br />
large ships, although they usually have a different<br />
design—<strong>to</strong> make best use <strong>of</strong> the fast steam jet, De Laval’s<br />
turbine had <strong>to</strong> run at an impractically high speed. But for<br />
rockets the De Laval nozzle was just what was needed.<br />
De Laval nozzle<br />
A device for efficiently converting the energy <strong>of</strong> a hot gas<br />
<strong>to</strong> kinetic energy <strong>of</strong> motion, originally used in some<br />
steam turbines and now used in practically all rockets. By<br />
constricting the outflow <strong>of</strong> the gas until it reaches the<br />
velocity <strong>of</strong> sound and then letting it expand again, an<br />
extremely fast jet is produced.<br />
Debus, Kurt H. (1908–1983)<br />
An important member <strong>of</strong> Wernher von Braun’s V-2 (see<br />
“V” weapons) development team who subsequently<br />
supervised rocket launchings in the United States. Debus<br />
earned a B.S. in mechanical engineering (1933), and an<br />
M.S. (1935) and a Ph.D. (1939) in electrical engineering,<br />
all from the Technical University <strong>of</strong> Darmstadt, before<br />
being appointed an assistant pr<strong>of</strong>essor there. During<br />
World War II he became an experimental engineer at the<br />
V-2 test stand at Peenemünde, rising <strong>to</strong> become superintendent<br />
<strong>of</strong> the test stand and the test firing stand for the<br />
rocket. In 1945, he came <strong>to</strong> the United States with a<br />
group <strong>of</strong> engineers and scientists headed by von Braun.<br />
<strong>From</strong> 1945 <strong>to</strong> 1950, the group worked at Fort Bliss, Texas,<br />
and then moved <strong>to</strong> the Reds<strong>to</strong>ne Arsenal in Huntsville,<br />
Alabama. <strong>From</strong> 1952 <strong>to</strong> 1960, Debus was chief <strong>of</strong> the<br />
missile firing labora<strong>to</strong>ry <strong>of</strong> the Army Ballistic Missile<br />
Agency (ABMA). In this position, he was located at<br />
Cape Canaveral, where he supervised the launching <strong>of</strong><br />
the first ballistic missile fired from there—an Army Reds<strong>to</strong>ne.<br />
When ABMA became part <strong>of</strong> NASA, Debus continued<br />
<strong>to</strong> supervise missile and space vehicle launchings,<br />
first as direc<strong>to</strong>r <strong>of</strong> the Launch Operations Center and<br />
then <strong>of</strong> the Kennedy Space Center, as it was renamed in<br />
December 1963. He retired from that position in 1974.<br />
decay<br />
See orbit decay.