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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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220 Kennedy Space Center (KSC)<br />

Kennedy Space Center (KSC)<br />

America’s primary civilian space launch facility, operated<br />

by NASA and located at Cape Canaveral. All Space<br />

Shuttle launches and many unmanned launches take<br />

place from here. Selection <strong>of</strong> the site was influenced by<br />

the fact that the Missile Firing Labora<strong>to</strong>ry had been<br />

launching missiles from Cape Canaveral since 1953. Originally<br />

called the Launch Operations Center, the facility<br />

was renamed the John F. Kennedy Space Center in 1963.<br />

Kepler<br />

A NASA Discovery mission, scheduled for launch in<br />

2006, <strong>to</strong> detect and characterize Earth-sized planets by<br />

pho<strong>to</strong>metry (light-intensity measurements). Kepler’s<br />

objectives over a four-year lifetime are <strong>to</strong> determine: (1)<br />

the frequency <strong>of</strong> Earth-like and larger planets in and near<br />

the habitable zone <strong>of</strong> a wide variety <strong>of</strong> spectral types <strong>of</strong><br />

stars; (2) the distribution <strong>of</strong> diameter and orbital size <strong>of</strong><br />

Earth-like planets; (3) the distribution <strong>of</strong> diameter, mass,<br />

density, albedo (reflectivity), and orbital size <strong>of</strong> giant<br />

inner planets; (4) the frequency <strong>of</strong> planets orbiting multiple<br />

star systems; and (5) the properties <strong>of</strong> stars that have<br />

planetary systems. Kepler’s main instrument will be a<br />

one-m-aperture pho<strong>to</strong>meter with a 12° field <strong>of</strong> view,<br />

about equal <strong>to</strong> the area covered by a hand at arm’s<br />

length; it will continuously and simultaneously moni<strong>to</strong>r<br />

the light from 90,000 main-sequence stars in a star field<br />

in Cygnus. Planets will be discovered and characterized<br />

by the tiny periodic light dips they cause as they pass in<br />

front <strong>of</strong> (transit) their parent stars as seen from Earth.<br />

Detection <strong>of</strong> two transits will be taken as evidence <strong>of</strong> a<br />

candidate planet, with a third and subsequent transits<br />

providing confirmation.<br />

Kepler, Johannes (1571–1630)<br />

A German mathematician and astronomer who assisted<br />

the great observer Tycho Brahe and later used Brahe’s<br />

observations <strong>to</strong> deduce three key laws <strong>of</strong> planetary motion,<br />

now known as Kepler’s laws. Kepler lived when telescopes<br />

were first being used <strong>to</strong> look at the Moon and planets, and<br />

was one <strong>of</strong> the few vocal supporters <strong>of</strong> Galileo’s claim that<br />

the planets orbited the Sun instead <strong>of</strong> the other way<br />

around. He was also the author <strong>of</strong> a lunar tale called Somnium<br />

(<strong>The</strong> Dream), 167 published posthumously in 1634.<br />

<strong>The</strong> hero, Duracotus, an Icelander and a self-proclaimed<br />

student <strong>of</strong> Brahe, is conveyed <strong>to</strong> the Moon by winged<br />

Selenites who trafficked with his mother, a no<strong>to</strong>rious<br />

witch—an arrangement not unfamiliar <strong>to</strong> Kepler, since his<br />

own mother was tried for witchcraft.<br />

Keplerian trajec<strong>to</strong>ry<br />

An elliptical orbit followed by an object in accordance<br />

with the first <strong>of</strong> Kepler’s laws <strong>of</strong> celestial motion.<br />

Johannes Kepler George Philip & Son<br />

Kepler’s laws<br />

Three laws <strong>of</strong> planetary motion, published by Johannes<br />

Kepler and based on accurate observations by Tycho<br />

Brahe; they were subsequently shown by Isaac New<strong>to</strong>n<br />

<strong>to</strong> be a direct result <strong>of</strong> his theory <strong>of</strong> gravitation and laws<br />

<strong>of</strong> motion. <strong>The</strong>y are: (1) A planet orbits the Sun in an<br />

ellipse with the Sun at one focus; (2) A line drawn from<br />

the Sun <strong>to</strong> a planet (the radius vec<strong>to</strong>r) sweeps out equal<br />

areas in equal amounts <strong>of</strong> time; and (3) <strong>The</strong> square <strong>of</strong><br />

the period <strong>of</strong> a planet’s orbit varies as the cube <strong>of</strong> the<br />

planet’s semimajor axis, the constant <strong>of</strong> proportionality<br />

being the same for all planets. <strong>The</strong> first law corrects<br />

the simpler model <strong>of</strong> Copernicus, which assumed circles.<br />

<strong>The</strong> second law expresses the way a planet speeds<br />

up when approaching the Sun and slows down when<br />

drawing away. <strong>The</strong> third law gives the exact relation by<br />

which planets move faster on orbits that are closer <strong>to</strong><br />

the Sun.<br />

kerosene<br />

A commonly used rocket fuel, especially in a mixture<br />

known as RP-1.<br />

Kerwin, Joseph Peter (1932–)<br />

An American astronaut who, as science pilot aboard the<br />

first Skylab mission in 1973, became not only the first<br />

medical doc<strong>to</strong>r <strong>to</strong> practice in orbit but also the first space<br />

repairman. He received a B.A. in philosophy from the<br />

College <strong>of</strong> the Holy Cross in 1953 and an M.D. from<br />

Northwestern University Medical School in 1957. Kerwin<br />

completed his internship at the District <strong>of</strong> Columbia

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