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

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324 Planet Imager (PI)<br />

Planet Imager (PI)<br />

A possible future NASA mission, part <strong>of</strong> the Origins<br />

Program, that would follow on from the Terrestrial Planet<br />

Finder (TPF) and produce images <strong>of</strong> Earth-like planets.<br />

To obtain a 25 × 25 pixel image <strong>of</strong> an extrasolar<br />

planet would call for an array <strong>of</strong> five TPF-class optical<br />

interferometers flying in formation. Each interferometer<br />

would consist <strong>of</strong> four 8-m telescopes <strong>to</strong> collect light and<br />

<strong>to</strong> null it before passing it <strong>to</strong> a single 8-m telescope,<br />

which would relay the light <strong>to</strong> a combining spacecraft.<br />

<strong>The</strong> five interferometers would be arranged in a parabola,<br />

creating a very long baseline <strong>of</strong> 6,000 km with the combining<br />

spacecraft at the focal point <strong>of</strong> the array. <strong>The</strong><br />

Planet Imager is identified in NASA’s Office <strong>of</strong> Space Science<br />

Strategic Plan as a potential mission beyond 2007<br />

but remains in the very early concept definition phase.<br />

planetary protection test<br />

A test performed <strong>to</strong> assess that the potential for contamination<br />

<strong>of</strong> (1) Earth by returned spacecraft hardware, or<br />

(2) spacecraft destinations by spacecraft hardware is<br />

within acceptable limits. It typically consists <strong>of</strong> bacterial<br />

spore counts from swabs taken from hardware surfaces.<br />

Planetary Society, <strong>The</strong><br />

A nonpr<strong>of</strong>it, public organization, founded in 1980 by<br />

Carl Sagan, Bruce Murray, and Louis Friedman, and<br />

based in Pasadena, California, <strong>to</strong> encourage and support,<br />

through education, public information events, and special<br />

events, the exploration <strong>of</strong> the Solar System and the<br />

search for extraterrestrial life. With a membership <strong>of</strong> more<br />

than 100,000, from over 100 countries, the Planetary Society<br />

is the largest space advocacy group in the world. It<br />

publishes the bimonthly Planetary Report and provides<br />

financial support for SETI hardware development. It is<br />

also developing the Cosmos 1 solar sail project.<br />

plasma<br />

A low-density gas in which the individual a<strong>to</strong>ms are ionized<br />

(and therefore charged), even though the <strong>to</strong>tal number<br />

<strong>of</strong> positive and negative charges is equal, thus<br />

maintaining overall electrical neutrality. Plasma is sometimes<br />

referred <strong>to</strong> as the fourth state <strong>of</strong> matter. A partially<br />

ionized plasma, such as Earth’s ionosphere, is one that<br />

also contains neutral a<strong>to</strong>ms.<br />

plasma detec<strong>to</strong>r<br />

A device for measuring the density, composition, temperature,<br />

velocity, and three-dimensional distribution <strong>of</strong><br />

plasmas that exist in interplanetary regions and within<br />

planetary magne<strong>to</strong>spheres.<br />

plasma sheath<br />

An envelope <strong>of</strong> ionized gas that surrounds a body moving<br />

through an atmosphere <strong>of</strong> hypersonic velocity.<br />

plasma sheet<br />

Low energy plasma, largely concentrated within a few<br />

planetary radii <strong>of</strong> the equa<strong>to</strong>rial plane, distributed<br />

throughout the magne<strong>to</strong>sphere, throughout which concentrated<br />

electric currents flow.<br />

plasma wave detec<strong>to</strong>r<br />

A device for measuring the electrostatic and electromagnetic<br />

components <strong>of</strong> local plasma waves in three dimensions.<br />

platform<br />

A spacecraft, usually unmanned, that serves as a base for<br />

scientific experiments.<br />

Plesetsk Cosmodrome<br />

A Russian launch complex and missile test range, located<br />

at 62.8° N, 40.4° E, which has launched the most satellites<br />

since the beginning <strong>of</strong> the Space Age. Built in 1960,<br />

south <strong>of</strong> Archangel in northern Russia, its existence was<br />

not <strong>of</strong>ficially acknowledged by the Soviet Union until<br />

1987, but it became publicly known in the West after the<br />

tracking <strong>of</strong> Cosmos 112 by a team <strong>of</strong> schoolboys at Kettering<br />

Grammar School in England. Prior <strong>to</strong> this, it had<br />

been the source <strong>of</strong> many UFO reports from people living<br />

below the site’s launch trajec<strong>to</strong>ries. Western journalists<br />

allowed on<strong>to</strong> the site in 1989 were <strong>to</strong>ld <strong>of</strong> two fatal accidents<br />

that had happened there: on June 26, 1973, nine<br />

technicians were killed in a launch pad accident, and on<br />

March 18, 1980, 50 technicians were killed by an explosion<br />

while fueling a Soyuz booster.<br />

Plesetsk’s location makes it ideal for launching in<strong>to</strong><br />

polar or high-inclination orbits (63° <strong>to</strong> 83° inclination)—<br />

those typically favored by military reconnaissance and<br />

weather satellites. Between 1969 and 1993, it was the<br />

busiest spaceport in the world, accounting for more than<br />

a third <strong>of</strong> all orbital or planetary missions. It continues <strong>to</strong><br />

be highly active <strong>to</strong>day, especially for military launches<br />

and all Molniya-class communications satellites.<br />

Plesetsk has traditionally supported four launch vehicle<br />

types: Cosmos-3M, Soyuz/Molniya, Tskylon-3, and<br />

Start. <strong>The</strong> Russian government is keen <strong>to</strong> shift more<br />

activity, especially unmanned launches, away from<br />

Baikonur (which first surpassed Plesetsk in number <strong>of</strong><br />

launches in 1993), since its current agreement with Kazakhstan<br />

<strong>to</strong> use that facility expires in 2014. To this end,<br />

a program has been put in place <strong>to</strong> build the launch support<br />

infrastructure for the new Angara vehicle at the<br />

northernmost spaceport. <strong>The</strong> first launch <strong>of</strong> this new gen-

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