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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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-