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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88 Copernicus Observa<strong>to</strong>ry<br />
longest Mercury orbital mission and spent eight days in<br />
space aboard Gemini 5. He earned a B.S. in aeronautical<br />
engineering from the Air Force Institute <strong>of</strong> Technology in<br />
1956. Having received an Army commission, he transferred<br />
<strong>to</strong> the Air Force and flew F-84 and F-86 jets in Germany<br />
for four years. Back in the United States he<br />
received his degree and then attended the Air Force<br />
Experimental Flight Test School at Edwards Air Force<br />
Base before being assigned as an aeronautical engineer<br />
and test pilot in the Performance Engineering Branch <strong>of</strong><br />
the Flight Test Division at Edwards. In 1959, he was<br />
selected by NASA and on May 15–16, 1963, piloted his<br />
Faith 7 capsule on the sixth and final Mercury Project<br />
mission. Electrical problems near the end <strong>of</strong> the mission<br />
meant he had <strong>to</strong> manually fire his retrorockets and steer<br />
the capsule through reentry. Problems also beset Cooper<br />
on his next flight, a then-record eight-day trip aboard<br />
Gemini 5 in August 1965. Trouble with fuel supplies,<br />
power systems, and a computer-generated command led<br />
Gemini 5 <strong>to</strong> land 166 km short <strong>of</strong> its designated target.<br />
Cooper retired from NASA and the Air Force in 1970,<br />
and has since been involved in technical research with<br />
several companies. 60<br />
Copernicus Observa<strong>to</strong>ry<br />
See OAO-3 (Orbiting Astronomical Observa<strong>to</strong>ry 3).<br />
Coriolis<br />
A test mission for the U.S. Air Force that carries two scientific<br />
payloads: Wind, and the Solar Mass Ejection<br />
Imager (SMEI). Wind is a Navy experiment built by the<br />
Naval Research Labora<strong>to</strong>ry <strong>to</strong> passively measure ocean<br />
surface wind directions, while SMEI is an Air Force<br />
Research Labora<strong>to</strong>ry experiment <strong>to</strong> observe coronal mass<br />
ejections in visible light. <strong>The</strong> spacecraft’s two payloads<br />
will collect data continuously during a three-year mission.<br />
Launch was scheduled for January 2003 from Vandenberg<br />
Air Force Base by a Titan II rocket in<strong>to</strong> a circular<br />
830 km × 98.7° orbit.<br />
Coriolis effect<br />
<strong>The</strong> deflection <strong>of</strong> the flight path <strong>of</strong> a spacecraft caused by<br />
Earth’s rotation. Over the northern hemisphere, the deviation<br />
is <strong>to</strong> the right; over the southern hemisphere, it is<br />
<strong>to</strong> the left.<br />
corona<br />
<strong>The</strong> outermost layer <strong>of</strong> the Sun’s (or some other star’s)<br />
atmosphere, visible <strong>to</strong> the eye during a <strong>to</strong>tal solar eclipse;<br />
it can also be observed through special filters and, best <strong>of</strong><br />
all, by X-ray cameras aboard satellites. <strong>The</strong> corona is very<br />
hot—up <strong>to</strong> 1.5 million degrees Celsius—and is the source<br />
<strong>of</strong> the solar wind.<br />
Corona<br />
America’s first series <strong>of</strong> pho<strong>to</strong>-reconnaissance or IMINT<br />
(imagery intelligence) satellites, involving more than one<br />
hundred launches between 1959 and 1972. <strong>The</strong> program<br />
had the cover name Discoverer and was only declassified<br />
in 1995. A Discoverer satellite would be placed in a polar<br />
orbit by a Thor-Agena rocket in order <strong>to</strong> take pho<strong>to</strong>graphic<br />
swaths as it passed over the Soviet Union. It then<br />
collected its exposed film in a heat-resistant “bucket” at<br />
the nose, and the bucket would reenter over the Pacific<br />
Ocean, deploy two small parachutes, and be recovered in<br />
midair by an aircraft <strong>to</strong>wing a trapeze-like snare. Bizarre as<br />
this sounds, the program proved successful after a shaky<br />
start—the first 12 launches failed, and the thirteenth,<br />
though achieving orbit, did not carry a camera. Discoverer<br />
14 marked the program’s first triumph. Its returning<br />
bucket was caught by a C-119 cargo plane on August 18,<br />
1960, and provided the earliest pho<strong>to</strong>s <strong>of</strong> the Soviet<br />
Union’s Plesetsk rocket base. In that single day, Corona<br />
yielded more valuable images <strong>of</strong> the Soviet Union than<br />
did the entire U-2 spy plane program. It proved conclusively<br />
that the Soviets’ intercontinental ballistic missile<br />
(ICBM) arsenal did not number in the hundreds, as was<br />
widely feared, but rather amounted <strong>to</strong> somewhere<br />
between 25 and 50. This knowledge, however, was hidden<br />
from the American public for years. Corona showed that<br />
the supposed missile gap that Kennedy played upon in his<br />
presidential campaign was a myth—a fact he would have<br />
learned at the time had he taken up Eisenhower’s <strong>of</strong>fer <strong>of</strong><br />
intelligence briefings. Corona allowed the U.S. intelligence<br />
community <strong>to</strong> catalog Soviet air defense and<br />
antiballistic missile sites, nuclear weapons–related facilities,<br />
and submarine bases, along with military installations<br />
in China and Eastern Europe. It also provided pictures <strong>of</strong><br />
the 1967 Arab-Israeli war and Soviet arms control compliance.<br />
Its retrieval system helped NASA develop a safe<br />
means <strong>of</strong> recovering manned spacecraft, and its imaging<br />
systems provided the basis for the cameras carried by the<br />
Lunar Orbiters in 1966 and 1967. 74<br />
Coronas<br />
An international project <strong>to</strong> study the Sun and its interaction<br />
with Earth using spacecraft launched by Russia and<br />
carrying experiments developed by Russia and Ukraine<br />
with involvement from scientists in other European<br />
countries and the United States. Coronas satellites are<br />
equipped <strong>to</strong> study solar activity including flares, active<br />
regions, and mass ejections, in various regions <strong>of</strong> the<br />
spectrum from radio waves <strong>to</strong> gamma rays. Coronas-I<br />
reentered the atmosphere on March 4, 2001, two days<br />
before Mir was de-orbited, leaving Russia temporarily<br />
without a single working science payload in orbit.<br />
Coronas-F carries three main groups <strong>of</strong> instruments <strong>to</strong>