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

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40 Artemis Project<br />

ESA devised a four-step recovery strategy that should<br />

allow ARTEMIS eventually <strong>to</strong> reach its correct geostationary<br />

position and function as originally planned for at<br />

least five years. <strong>The</strong> first two steps <strong>of</strong> this strategy involved<br />

several firings <strong>of</strong> the satellite’s solid-propellant apogee<br />

kick mo<strong>to</strong>r <strong>to</strong> raise the apogee (highest point <strong>of</strong> the orbit)<br />

and then circularize the orbit at about 31,000 km, while<br />

the second two involved an unforeseen use <strong>of</strong> the ion<br />

engine for maneuvering in<strong>to</strong> geostationary orbit.<br />

Launch<br />

Vehicle: Ariane 5<br />

Date: July 12, 2001<br />

Site: Kourou<br />

Initial orbit<br />

Intended: 858 × 35,853 km × 2°<br />

Actual: 590 × 17,487 km × 2.9°<br />

Artemis Project, the<br />

A multi-industry program <strong>to</strong> establish a commercial lunar<br />

base, led by the Lunar Resources Company <strong>of</strong> Hous<strong>to</strong>n.<br />

It is supported by the Artemis Society, which publishes<br />

Pleiades, a monthly newsletter, and Artemis, a bimonthly<br />

commercial magazine.<br />

artificial gravity<br />

<strong>The</strong> simulation <strong>of</strong> the pull <strong>of</strong> gravity aboard a space station,<br />

space colony, or manned spacecraft by the steady<br />

rotation, at an appropriate angular speed, <strong>of</strong> all or part <strong>of</strong><br />

the vessel. Such a technique may be essential for longduration<br />

missions <strong>to</strong> avoid adverse physiological (and possibly<br />

psychological) reactions <strong>to</strong> weightlessness.<br />

<strong>The</strong> idea <strong>of</strong> a rotating wheel-like space station goes back<br />

as far as 1928 in the writings <strong>of</strong> Herman Noordung and<br />

was developed further by Werhner von Braun. Its most<br />

famous fictional representation is in the film 2001: A<br />

Space Odyssey, which depicts spin-generated artificial gravity<br />

aboard a spaceship bound for Jupiter. <strong>The</strong> O’Neill-type<br />

space colony provides another classic illustration <strong>of</strong> this<br />

technique.<br />

However, there are several reasons why large-scale rotation<br />

is unlikely <strong>to</strong> be used <strong>to</strong> simulate gravity in the near<br />

ARTV Missions<br />

future. In the case <strong>of</strong> a manned Mars spacecraft, for example,<br />

the structure required would be prohibitively big, massive,<br />

and costly in terms <strong>of</strong> energy <strong>to</strong> run (except possibly<br />

in the case <strong>of</strong> an orbital cycler). A better approach for such<br />

a mission, and one being explored, is <strong>to</strong> provide astronauts<br />

with a small spinning bed on which they can lie for an<br />

hour or so each day, head at the center and feet pointing<br />

out, so that their bodies can be loaded in approximately<br />

the same way they would be under Earth-normal gravity.<br />

In the case <strong>of</strong> space stations, one <strong>of</strong> the objects is <strong>to</strong><br />

carry out experiments in zero-g,or, more precisely, microgravity.<br />

In a rotating structure, the only gravity-free place<br />

is along the axis <strong>of</strong> rotation. At right-angles <strong>to</strong> this axis,<br />

the pull <strong>of</strong> simulated gravity varies as the square <strong>of</strong> the<br />

tangential speed.<br />

Another way <strong>to</strong> achieve Earth-normal gravity is not<br />

by constant rotation, which produces the required force<br />

through angular acceleration, but by steadily increasing<br />

straight-line speed at just the right rate. This is the<br />

method used in the hypothetical 1g spacecraft. 279<br />

ARTV (Advanced Reentry Test Vehicle)<br />

Early American suborbital reentry tests involving mice<br />

named Mia, Mia II, and Wickie. (See table, “ARTV Missions.”)<br />

Launch<br />

Vehicle: Thor-Able<br />

Site: Cape Canaveral<br />

Aryabhata<br />

India’s first satellite, named for the Indian mathematician<br />

(c. A.D. 450). <strong>The</strong> Soviet Union assisted India in developing<br />

Aryabhata, which carried out satellite technology tests<br />

and made observations <strong>of</strong> the upper atmosphere.<br />

Launch<br />

Date: April 19, 1975<br />

Vehicle: Cosmos-3M<br />

Site: Kapustin Yar<br />

Orbit: 398 × 409 km × 50.7°<br />

Mass: 360 kg<br />

Mission Launch Date Notes<br />

ARTV 1 Apr. 24, 1958 Failed due <strong>to</strong> Thor turbopump problem; Mouse Mia not recovered<br />

ARTV 2 Jul. 10, 1958 Mouse Mia II reached 1,600 km altitude, flew 9,600 km range, but reentry vehicle not<br />

recovered<br />

ARTV 3 Jul. 23, 1958 Mouse Wickie not recovered; nosecone lost

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