13.12.2012 Views

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

SHOW MORE
SHOW LESS

You also want an ePaper? Increase the reach of your titles

YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.

238 LiPS (Living Plume Shield)<br />

LiPS (Living Plume Shield)<br />

Plume shields ejected from the upper stage <strong>of</strong> NOSS<br />

(Naval Ocean Surveillance Satellite) primary payloads;<br />

they were used as subsatellites for conducting technology<br />

demonstrations. <strong>The</strong> plume shield, which deflects the<br />

exhaust <strong>of</strong> the upper-stage mo<strong>to</strong>r away from the primary<br />

payload, is cus<strong>to</strong>marily jettisoned after use <strong>to</strong> become<br />

space debris. However, on the LiPS experiments, the<br />

anterior surfaces <strong>of</strong> the shield, which are unaffected by<br />

the plume, were fitted with a variety <strong>of</strong> small experiments.<br />

(See table, “LiPS Missions.”)<br />

liquid hydrogen (H 2)<br />

Hydrogen in its liquid state, used as a cryogenic rocket<br />

fuel; hydrogen gas turns <strong>to</strong> liquid under standard atmospheric<br />

pressure at −263°C. When oxidized by liquid oxygen,<br />

liquid hydrogen delivers about 40% more thrust per<br />

unit mass than other liquid fuels, such as kerosene.<br />

Commonly referred <strong>to</strong> in rocketry as LH2. 273<br />

liquid oxygen (O 2)<br />

Oxygen in its liquid state, used as the oxidizer in many<br />

liquid fuel engines. Oxygen gas turns <strong>to</strong> liquid under<br />

standard atmospheric pressure at −183°C. Commonly<br />

referred <strong>to</strong> in rocketry as LOX.<br />

liquid propellant<br />

A liquid ingredient used in the combustion chamber <strong>of</strong><br />

a rocket engine. Liquid propellants may be either bipropellants,<br />

which consist <strong>of</strong> a liquid fuel (such as kerosene<br />

or liquid hydrogen) and a liquid oxidizer (such as liquid<br />

oxygen or nitrogen tetroxide), or monopropellants (such<br />

as hydrazine). Liquid propellants, such as liquid oxygen<br />

and liquid hydrogen, that must be kept at a low temperature<br />

in order <strong>to</strong> remain liquid are known as cryogenic<br />

propellants. See liquid-propellant rocket engine.<br />

liquid-air cycle engine<br />

An advanced engine cycle that uses liquid hydrogen fuel<br />

<strong>to</strong> condense air entering an inlet. Liquid oxygen is separated<br />

from the condensed air and pumped in<strong>to</strong> the com-<br />

LiPS Missions<br />

Launch site: Vandenberg Air Force Base<br />

Launch<br />

Mission Date Vehicle Notes<br />

LiPS 1 Dec. 9, 1980 Atlas F Launch vehicle failed on take<strong>of</strong>f.<br />

LiPS 2 Feb. 8, 1983 Atlas H Carried UHF single-channel transponder.<br />

LiPS 3 May 15, 1987 Atlas H Data returned from over 140 solar-cell experiments.<br />

bustion chamber, where it is burned with the hydrogen<br />

<strong>to</strong> produce thrust.<br />

liquid-fueled rocket<br />

A rocket that derives its thrust from one or more liquidpropellant<br />

rocket engines.<br />

liquid-propellant rocket engine<br />

A rocket propulsion system in which a liquid fuel (such<br />

as kerosene or liquid hydrogen) is combined in a thrust<br />

chamber with a liquid oxidizer (such as liquid oxygen or<br />

fuming nitric acid). Very efficient and controllable, such<br />

engines are used extensively in spaceflight. Unlike solidpropellant<br />

rocket mo<strong>to</strong>rs, they can be shut <strong>of</strong>f by<br />

remote command, simply by closing <strong>of</strong>f their fuel line. In<br />

some cases, the thrust can also be varied over a certain<br />

range.<br />

LISA (Laser Interferometer Space Antenna)<br />

An array <strong>of</strong> three NASA spacecraft flying 5 million km<br />

apart in the shape <strong>of</strong> an equilateral triangle. <strong>The</strong> center<br />

<strong>of</strong> the triangle will be in the ecliptic plane one astronomical<br />

unit from the Sun and 20° behind Earth. <strong>The</strong><br />

LISA mission, which is being designed at JPL ( Jet<br />

Propulsion Labora<strong>to</strong>ry), is intended <strong>to</strong> observe gravitational<br />

waves from galactic and extragalactic sources,<br />

including the supermassive black holes found in the centers<br />

<strong>of</strong> many galaxies. Gravitational waves are one <strong>of</strong> the<br />

fundamental building blocks <strong>of</strong> our theoretical picture<br />

<strong>of</strong> the universe, but although there is strong indirect evidence<br />

for their existence, they have not yet been directly<br />

detected. <strong>The</strong> LISA spacecraft, flying in formation, will<br />

be sensitive <strong>to</strong> the dis<strong>to</strong>rtion <strong>of</strong> space caused by passing<br />

gravitational waves. Each spacecraft will contain two<br />

free-floating “pro<strong>of</strong> masses.” <strong>The</strong> pro<strong>of</strong> masses will<br />

define optical paths 5 million km long, with a 60° angle<br />

between them. Lasers in each spacecraft will be used <strong>to</strong><br />

measure changes in the optical path lengths with a precision<br />

<strong>of</strong> 20 pm (trillionths <strong>of</strong> a meter). If approved, the<br />

project will begin development in 2005 with a planned<br />

launch in 2008.

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!