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

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eccentricity<br />

A measure <strong>of</strong> the elongation <strong>of</strong> an orbit; specifically, the<br />

distance between the foci <strong>of</strong> an ellipse divided by the<br />

major axis. <strong>The</strong> eccentricity <strong>of</strong> closed orbits varies from 0,<br />

for a perfect circle, <strong>to</strong> almost 1, for an extremely flattened<br />

ellipse. Open orbits have eccentricites <strong>of</strong> 1 (parabolic) or<br />

greater (hyperbolic).<br />

Echo<br />

<strong>The</strong> world’s first passive communications satellites.<br />

Each Echo spacecraft was a large aluminized Mylar balloon<br />

inflated in orbit, which provided a reflective surface<br />

so that two-way voice signals could be bounced from<br />

ground stations on the west and east coasts <strong>of</strong> the United<br />

States. Following the failure <strong>of</strong> the launch vehicle carrying<br />

Echo 1, Echo 1A (commonly referred <strong>to</strong> as Echo 1)<br />

was placed in orbit and used <strong>to</strong> redirect transcontinental<br />

and intercontinental telephone, radio, and television signals.<br />

Its success proved that microwave transmission <strong>to</strong><br />

and from satellites in space was possible and demonstrated<br />

the promise <strong>of</strong> communications satellites. Also,<br />

because <strong>of</strong> its large area-<strong>to</strong>-mass ratio, it provided data for<br />

the calculation <strong>of</strong> atmospheric density and solar pressure.<br />

With a diameter <strong>of</strong> 30.5 m, Echo 1A was visible <strong>to</strong> the<br />

unaided eye over most <strong>of</strong> the Earth and brighter than<br />

most stars. <strong>The</strong> 41.1-m-diameter Echo 2—the first joint<br />

American/Soviet collaboration in space—continued the<br />

passive communications experiments, enabled an investigation<br />

<strong>of</strong> the dynamics <strong>of</strong> large spacecraft, and was used<br />

for global geometric geodesy. Although NASA abandoned<br />

passive communications systems in favor <strong>of</strong> active<br />

satellites following Echo 2, the Echo program demonstrated<br />

several ground station and tracking technologies<br />

that would be used by active systems. (See table, “Echo<br />

Satellites.”)<br />

EchoStar<br />

A constellation <strong>of</strong> direct broadcasting satellites in geosynchronous<br />

orbit operated by EchoStar Orbital Corporation.<br />

<strong>The</strong> seventh EchoStar was launched on February<br />

21, 2002; EchoStar 8 was scheduled for lift<strong>of</strong>f in mid-<br />

2002.<br />

Echo Satellites<br />

Edding<strong>to</strong>n 115<br />

ecliptic<br />

<strong>The</strong> plane in which Earth moves around the Sun.<br />

ecological system<br />

A habitable environment either created artificially, such<br />

as in a space colony, or occurring naturally, such as the<br />

environment on Earth, in which man, animals, and other<br />

organisms live in mutual relationship with one another.<br />

ECS (European Space Agency<br />

Communications Satellites)<br />

A series <strong>of</strong> satellites launched in the 1980s <strong>to</strong> support<br />

European telecommunication services, including telephone,<br />

telex, data, and television.<br />

ECS (Experimental Communications Satellite)<br />

Two Japanese satellites, also known by the national name<br />

<strong>of</strong> Ayama (“expansion”), launched by NASDA (National<br />

Space Development Agency) <strong>to</strong> carry out millimeterwave<br />

communications experiments. Both failed—ECS<br />

because the third stage <strong>of</strong> the N-1 launch vehicle came in<br />

contact with the satellite after separation, and ECS-B<br />

because <strong>of</strong> a fault with the apogee kick mo<strong>to</strong>r.<br />

ECS and ECS-B<br />

Launch<br />

Date: February 6, 1979 (ECS); February 22, 1980<br />

(ECS-B)<br />

Vehicle: N-1<br />

Site: Tanegashima<br />

Size: 1.4-m diameter cylinder<br />

Mass: 130 kg<br />

Edding<strong>to</strong>n<br />

An ESA (European Space Agency) mission <strong>to</strong> detect seismic<br />

vibrations in the surfaces <strong>of</strong> stars and <strong>to</strong> search for<br />

Earth-like extrasolar planets using precise pho<strong>to</strong>metry<br />

(light-intensity measurements). Named in honor <strong>of</strong> the<br />

English astrophysicist Arthur Stanley Edding<strong>to</strong>n (1882–<br />

1944), it is expected <strong>to</strong> be launched after 2008, probably<br />

by a Soyuz-Fregat rocket from Baikonur. Edding<strong>to</strong>n will<br />

Spacecraft Date<br />

Launch<br />

Vehicle Site Orbit Mass (kg)<br />

Echo 1 May 13, 1960 Delta Cape Canaveral Failed <strong>to</strong> reach orbit 56<br />

Echo 1A Aug. 12, 1960 Delta Cape Canaveral 966 × 2,157 km × 47.3° 76<br />

Echo 2 Jan. 25, 1964 Thor-Agena B Vandenberg 1,030 × 1,315 km × 81.5° 256

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