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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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CERISE (Characterisation de l’Environment Radio-electrique par un Instrument Spatial Embarque) 71<br />

exclusively in tandem with Atlas but was then adapted<br />

for mating <strong>to</strong> the Titan III <strong>to</strong> boost heavier payloads in<strong>to</strong><br />

Earth orbit and interplanetary trajec<strong>to</strong>ries. Today, when<br />

combined with the Titan IV, it makes up the most powerful<br />

expendable launch vehicle in the world. <strong>The</strong> Centaur<br />

is manufactured by Lockheed Martin and powered<br />

by two Pratt & Whitney restartable RL10 engines. It interfaces<br />

with the payload via a forward adapter, where the<br />

avionics, electrical, flight termination, telemetry, and<br />

tracking systems are mounted. 200 See Ehricke, Krafft.<br />

(See also table, “Centaur Rocket Stage.”)<br />

center <strong>of</strong> mass<br />

<strong>The</strong> point in a body at which its entire mass can be considered<br />

<strong>to</strong> be concentrated.<br />

center <strong>of</strong> pressure<br />

<strong>The</strong> point at which the aerodynamic lift on a rocket is<br />

centered. Half the surface area <strong>of</strong> a rocket lies on one side<br />

<strong>of</strong> the center <strong>of</strong> pressure and half on the other side.<br />

centrifugal force<br />

A force that must be included in the calculation <strong>of</strong> equilibria<br />

between forces in a spinning frame <strong>of</strong> reference,<br />

such as that <strong>of</strong> a rotating space station. In the rotating<br />

frame, the forces on a body <strong>of</strong> mass m are in equilibrium<br />

(as evidenced by the body staying at the same place) only<br />

if all forces acting on it, plus a “centrifugal force” mv 2 /R<br />

directed away from the center <strong>of</strong> rotation at a distance R,<br />

add up <strong>to</strong> zero.<br />

centrifuge<br />

A large mo<strong>to</strong>r-driven apparatus with a long arm at the<br />

end <strong>of</strong> which human and animal subjects or equipment<br />

can be rotated at various speeds <strong>to</strong> simulate the prolonged<br />

accelerations encountered in high-performance<br />

aircraft, rockets, and spacecraft. <strong>The</strong> earliest centrifuges<br />

were set up in the World War II era, at a time when aircraft<br />

were coming in<strong>to</strong> use that were capable <strong>of</strong> such<br />

Centaur Rocket Stage<br />

high-g maneuvers that pilots could easily black out. It was<br />

also realized that pilots who were less susceptible <strong>to</strong> the<br />

effects <strong>of</strong> g-forces would be able <strong>to</strong> twist and turn their<br />

planes more sharply and thereby outperform an enemy.<br />

Centrifuges thus served a dual role: <strong>to</strong> study the medical<br />

effects <strong>of</strong> high acceleration and <strong>to</strong> select individuals best<br />

able <strong>to</strong> cope with such acceleration. A pioneer in this<br />

field was Heinz von Diringsh<strong>of</strong>en <strong>of</strong> Germany, who, in<br />

1931, began research in<strong>to</strong> the physiology <strong>of</strong> radial acceleration<br />

forces and established the limits <strong>of</strong> <strong>to</strong>lerance <strong>to</strong><br />

g-forces that could be sustained for any length <strong>of</strong> time<br />

without loss <strong>of</strong> vision or consciousness. Early centrifuges<br />

were set up at two labora<strong>to</strong>ries in Germany, at the Mayo<br />

Clinic, at the University <strong>of</strong> Southern California, and at<br />

Farnborough in England. Others were built after the war,<br />

including the immense Johnsville Centrifuge, used <strong>to</strong><br />

test and train the first American astronauts.<br />

centripetal acceleration<br />

<strong>The</strong> acceleration associated with motion in a circle and<br />

directed <strong>to</strong> the center <strong>of</strong> the circle.<br />

centripetal force<br />

<strong>The</strong> force that acts <strong>to</strong>ward the center <strong>of</strong> a circle and makes<br />

circular motion possible. To enable an object <strong>of</strong> mass m <strong>to</strong><br />

move with velocity v around a circle <strong>of</strong> radius R, a centripetal<br />

force <strong>of</strong> magnitude mv 2 /R must be applied.<br />

CERISE (Characterisation de l’Environment Radioelectrique<br />

par un Instrument Spatial Embarque)<br />

An experimental ELINT (electronic intelligence) microsatellite<br />

built for the French arms procurement agency<br />

DGA (Delegation Generale pour l’Armement). It is<br />

notable for having suffered the first known accidental<br />

collision between two independent orbiting objects. On<br />

July 21, 1995, a piece <strong>of</strong> debris from the Ariane 1 third<br />

stage that launched SPOT 1 in 1986 collided with<br />

CERISE. During the impact, the upper portion <strong>of</strong><br />

CERISE’s gravity-gradient boom was snapped <strong>of</strong>f. <strong>The</strong><br />

Version Diameter (m) Length (m) Engine Type Propellant Mass (kg) Thrust (N)<br />

Centaur I 3.1 9.2 RL-10A-3A (x2) 13,900 147,000<br />

Centaur II 3.1 10.1 RL-10A-3A (x2) 16,800 147,000<br />

Centaur IIA 3.1 10.1 RL-10A-4 (x2) 16,800 185,000<br />

Centaur IIIA (Atlas IIIA) 3.1 10.0 RL-10-4-1 (x1) 16,800 99,000<br />

Centaur IIIB (Atlas IIIB) 3.1 11.7 RL-10-4-1 (x2) 20,800 198,000<br />

Centaur G (Titan IV) 4.3 9.0 RL-10-3A (x2) 20,900 147,000

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