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Ten
times the space shuttle has
made history.
April
1981 - Space shuttle Columbia, manned by astronauts John
W. Young and Robert L. Crippen, becomes the world's first
reusable spacecraft. Columbia launches again in November,
initiating use of its robot arm.
June
1983 - The Challenger shuttle's second flight carries
Sally Ride, the first American woman to fly in space.
In August, on Challenger's next mission, Guion S. Bluford
becomes the first African-American to fly in space.
February
1984 - Astronauts Bruce McCandless and Robert Stewart
leave Challenger with "rocket packs" for the world's
first untethered spacewalk.
January
1986 - NASA launches its first teacher-astronaut, Christa
McAuliffe. Tragically, though, the Challenger shuttle
explodes 73 seconds after liftoff, killing the 7-person
crew.
April
1990 - Discovery puts the Hubble Space Telescope into
orbit. Later, in December 1993, Endeavour astronauts
Story Musgrave and Jeffrey Hoffman fix the telescope's
blurred vision in the longest spacewalk on record.
May
1992 - Spacewalking astronauts from Endeavor capture
an errant communications satellite, repair it, and release
it into orbit.
February
1995 - Discovery makes a rendezvous with the Russian
space station Mir. In June, Atlantis docks with Mir to
replace its crew. The flights are practice for the new
International Space Station.
November
1996 - Columbia makes the longest space shuttle flight
yet, spanning almost 18 days with a crew of five.
October
1998 - Mercury astronaut (and U.S. senator) John Glenn
returns to space as payload specialist Glenn. At 77,
Glenn becomes the oldest human to fly in space.
July
1999 - Under commander Eileen Collins, Columbia puts
the Chandra X-Ray Observatory into orbit. Collins earned
her wings in February 1995, as the shuttle's first female
pilot. |
01/02/03
The loss of the space shuttle Columbia on February 1 drives home a simple truth:
space travel is never routine, no matter how many shuttles launch and land.
Success depends
on near-perfection, especially during re-entry. Re-entry takes
less than a half-hour to complete, but it's marked by tremendous changes
in gravity, pressure, and speed. Re-entry vehicles must endure
kinetic and thermodynamic
extremes that rival even the hazards of liftoff. There is almost no room
for error. Here's how it's supposed to work.
A
Speeding Bullet
First, the
shuttle has to slow down. While in orbit, it's traveling at more
than 17,000 miles per hour. That's literally faster than a speeding
bullet. Imagine driving down a highway for five minutes, passing
landmark after landmark as you go. The orbiting shuttle would
speed by all of it in a single second.
To shed some
of this speed, shuttle astronauts fire maneuvering thrusters
located along the shuttle's nose and tail, turning the shuttle
so that its tail faces forward. Then they fire the main thrusters
to slow down. Another thruster burn reorients the shuttle to
its proper re-entry attitude (its orientation relative to its
direction of flight), with the nose facing forward and raised
about 30 degrees. These maneuvers are crucial. Too much speed,
and the shuttle will slingshot back out into space; too little,
and it will burn in an uncontrolled plunge. And only the proper,
nose-up attitude presents the bottom surface of the shuttle forward,
to bear re-entry's brunt.
A
Flying Brick
At an altitude
of 400,000 feet (about 75 miles up), the shuttle begins to catch
a little air. Aerodynamic forces take effect. All thruster maneuvering
ceases, and the shuttle becomes a 120-foot glider. Onboard computers
maintain proper descent attitude and speed by adjusting body
flaps, elevons on the wings, and a rudder. Yet without power,
and traveling at hypersonic speeds through the thin atmosphere,
pilots say flying the shuttle is like flying "a brick with
wings."
Plowing through
air, however thin, causes drag, which slows the shuttle down--and
creates gravitational forces that stress the ship and its crew.
Apollo astronauts regularly endured more than 6 Gs during re-entry,
while Mercury astronauts suffered up to 11 Gs, near the maximum
sustained force humans can stand. Shuttle crews experience only
about 3 Gs, significantly less than during liftoff, because of
the shuttle's longer descent time. But mechanical stresses on
the shuttle are intense. Sensor data from early shuttle missions
indicate that the skin of the shuttle suffers peak shear forces
in excess of 7,000 pounds per square inch, while the interior
aluminum trusses and spars of the shuttle's wings face peak tensions
up to 8,000 pounds per square inch.
A
Blunt Bottom
Still, the
most difficult challenge of re-entry comes from another source:
heat. Any object moving through the atmosphere encounters friction
caused by air molecules hitting its surface. At relatively low
speeds, like those of conventional aircraft, the heat caused
by this friction is negligible. But as speeds increase, so does
friction. For some objects, the extreme speed of re-entry can
produce surface temperatures greater than 5,000° F.
Two factors
are crucial in foiling this heat: the shape of the re-entry vehicle
and the materials used to make its surface. Strangely enough,
the optimal shape for an object during re-entry is not slender
and streamlined, but blunt-faced. A blunt shape creates more
drag, which allows the re-entry vehicle to decelerate more in
the thin upper atmosphere, so that speeds in the thicker lower
atmosphere remain as low as possible. The blunt shape also produces
shockwaves away from the object's surface, which deflect more
heat away. The capsules used in NASA's Mercury, Gemini, and Apollo
programs had wide, bluntly rounded bottoms that were oriented
downward during re-entry. The flat bottom of the space shuttle
provides a similarly blunt surface.
Covered
in Tile
Although shape
has remained constant throughout the history of space travel,
heat-resistance materials have not. At first, NASA programs relied
on a process called ablation to transfer heat during re-entry.
The protective heat shield on early capsules was made of synthetic
resins that were designed to burn and fall away, taking large
amounts of heat with them.
The space
shuttle, however, requires reusable, lighter weight materials.
So it has more than 20,000 heat-resistant tiles covering its
surface. The nose cone and leading edges of the shuttle's wings,
which reach the highest temperatures during re-entry, are covered
with reinforced carbon capable of withstanding temperatures up
to 3,000° F. The rest of the underside of the shuttle, as
well as the forward fuselage, is covered with silica fiber tiles
capable of withstanding 2,300° F. Lighter "blankets" of
silica fibers cover those parts of the shuttle that face the
lowest re-entry temperatures, below 1,200° F. Underneath
the brittle tiles is a layer of material that cushions them from
the vibration, expansion, and contraction of the shuttle's aluminum
frame and that insulates the frame from the radiating heat.
Briefly
Alone
The tiles
protect the shuttle from the heat, but they can't protect the
radio. The intense heat of re-entry strips electrons right off
oxygen and nitrogen molecules in the air around the shuttle,
forming a highly conductive layer of ionized particles (called
plasma) around the vehicle. Because radio waves cannot penetrate
this layer, the shuttle can temporarily lose communication with
ground control. This "ionization blackout" can occur
from 25 minutes to about 12 minutes before landing. During this
time, shuttle pilots must often operate without benefit of assistance
from ground control, increasing the difficulty of an already
challenging process.
At an altitude
of roughly 83,000 feet, re-entry is over. On a good day, all
that remains are five minutes of relatively cool, gentle, controlled
gliding to the landing site. Yet the tremendous aerodynamic and
thermal forces of re-entry always contain the potential for catastrophe.
It is a tribute to the scientists, engineers, builders, and astronauts
of the space shuttle program that until February 1, 2003, no
re-entry accident had ever occurred.
Troposphere
(up to 9 miles--about 47,500 feet)
The lowest layer of the atmosphere, and the one in which terrestrial life on
Earth lives. Although thin compared to other layers, it's high enough to cover
the tallest mountains. The air is warm and thick and has a lot of horizontal
and vertical movement (wind and convection). It's here, too, that rain, clouds,
and most of our weather occurs. Pressure at the top of the troposphere is roughly
10 percent of that at the surface. The vast majority of airplanes, including
all commercial traffic, fly in this layer.
Stratosphere
(9 to 31 miles up--47,500 to 163,500 feet)
The stratosphere is fairly stable, with little airflow and even less moisture.
Yet it contains the all-important ozone layer, a thin band of unstable oxygen
molecules that absorbs most of the sun's ultraviolet radiation. Pressure at
the stratosphere's farthest reaches is just 0.15 percent of surface pressure.
Only a few specially built planes can fly at this level. The altitude record
for a non-rocket-powered plane is 96,500 feet. The altitude record for a balloon
is 113,740 feet.
Mesosphere
(31 to 53 miles up--163,500 to 280,000 feet)
The mesosphere is extremely cold, with temperatures dropping below -150° F.
The air is extremely thin, too, and pressure at the top is essentially zero.
Only rocket-powered craft can reach these altitudes. In fact, the altitude
record for a rocket-powered plane is 354,200 feet, above the mesosphere and
into the thermosphere.
Thermosphere
(53 to 372 miles up--280,000 to 1,964,000 feet)
There are so few molecules here, the place is almost a vacuum. Those few that
do exist are bombarded with solar radiation, so temperatures are high, climbing
to more than 1,800° F. Air concentrations thin with altitude, as Earth's
atmosphere slowly transitions into space. The lowest part of the thermosphere
is called the ionosphere, a layer of molecules ionized by the sun's energy.
It is here that auroras (the northern and southern lights) form. |
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