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&lt;p&gt;&lt;/p&gt;
&lt;p&gt;Sources:&lt;br /&gt;Lundquist, Charles. "Transplanted Rocket Pioneers," 2015.&lt;br /&gt;&lt;br /&gt;Wade, Mark. "Sieber, Werner." &lt;em&gt;Encyclopedia Astronautica&lt;/em&gt;, &lt;a href="http://www.astronautix.com/s/sieber.html"&gt;http://www.astronautix.com/s/sieber.html&lt;/a&gt;.&lt;/p&gt;</text>
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're/art

MR-13

NATIONAL B AERONAUTICS AND SPACE ADMINISTRATION

"Man Still Matters"-The Story of The First Skylab Mission
"I guess the way I could summarize this project is that it proves
that man still matters. . . . You have made us all very proud with the
way you handled some difficult problems in this project."
—President Richard M. Nixon in a radio telephone conversation with the
orbiting Skylab astronauts on June 18, 1973.

The first Skylab mission, epitomized above by the
President, dramatized the fact that man working in
combination with automated instruments can far
more fully explore and utilize space for world bene­
fit than either can alone.
Skylab 1—which includes the Orbital Workshop
(OWS) where men live and conduct experiments,
the Apollo Telescope Mount (ATM) which is a solar
observatory, and related docking, airlock, and elec­
tronic components—was launched at 1:31 p.m.
EDT, May 14, 1973. About a minute after launch,
an 800-pound meteoroid shield was torn from the
OWS, ripping away one OWS solar wing and jam­
ming the other so that it could not operate or open
properly. Solar wings have arrays of silicon solar
cells that convert sunlight to electricity for powering
spacecraft and their experiments. Without the OWS
wings, Skylab's available power supply was cut in
half.
The power loss was but one of the major problems
confronting Skylab. Equally serious was the loss of
the shield.
The purpose of the cylindrical shield was two-fold.
Without the .025-inch thin aluminum shield, Skylab
is directly exposed to microscopic dust particles
that could make tiny punctures in its walls. How­
ever, engineers believe Skylab's pressurization sys­
tem can readily compensate for such circumstances.
More important, the shield was painted to ward
off much of the Sun's heat and keep the OWS cool.
Its absence caused temperatures inside the OWS to
rise ominously, threatening to spoil the food, medi­
cines, and photographic film stowed on board at
launch. Skylab's outside skin temperatures reached
nearly 300 degrees Fahrenheit. Short of power and

too hot for prolonged habitation, Skylab had all the
hallmarks of a failure. It was saved by the dedicated
and tireless efforts of the first Skylab crew—Capt.
Charles Conrad, Jr.; Commander Joseph P. Kerwin,
and Commander Paul J. Weitz—and NASA and in­
dustry ground personnel.
The Apollo Telescope Mount (ATM) and its solar
panels had properly extended. With this power,
ground controllers were able to operate Skylab.
After a number of maneuvers to decrease the crit­
ical internal temperatures, Skylab was stabilized to
both illuminate the ATM panels (for power) and to
reduce direct sunlight on the OWS. The results:
• Internal temperatures were stabilized at 125 de­
grees Fahrenheit, which was still too hot for nor­
mal habitation.
• Power levels were about 2800 watts, enough for
unmanned operation.
• Skylab was oriented with a 45-50 degree pitch-up
(nose-up) attitude for which it was not designed.
To maintain this orientation put serious strain on
Skylab's supply of nitrogen gas maneuvering fuel.
• Skylab could not be oriented to point the ATM
at the Sun because of temperature increases nor
to aim Earth resources instruments at the ground
because this would reduce sunlight on the ATM
solar panels and drain the batteries.
• Beta angles—the angles between the Sun and
Skylab's orbit—were moving in a way to drive
OWS temperatures up again.
NASA and industry personnel pitched in offering a

1

�View of damaged Skylab workshop, showing
unshielded area where parasol was later deployed.
Jammed solar wing is at lower right.

2

�wide variety of ideas for a makeshift sun shield.
These were trimmed to three that were fabricated.
The three went along with Conrad, Kerwin, and Weitz
when the astronauts were launched on May 25 In
an attempt to save their mission and the Skylab
program. The astronauts also carried other care­
fully selected tools, including bolt cutters, a bending
tool (boat hook), tin snips and food and drugs to
replace those believed already spoiled by the heat.
Launched at 9 a.m. EDT, the crew rendezvoi/sed with
the space station at 4:30 p.m. EDT. They reconnoitered: maneuvering around the station, inspect­
ing the damage, and telecasting these observations
to Earth.
Then, they soft-docked—partially attached their
modified Apollo Command/Service module (CSM)
spacecraft, called Skylab 2, to Skylab 1—while they
made preparations for standing up in Skylab 2 and
attempting to free the jammed soiar panel. Later,
they undocked Skylab 2, maneuvered it to the
jammed solar panel, and attempted unsuccessfully
to free it.
Two problems were responsible for their failure:
the aluminum strip from the meteoroid shield that
had twisted around the wing was held fast by a bolt
that had deeply penetrated the wing; and the slope
of the solar wing was such that the available tools
could not adequately grip it. Ascertaining the prob­
lem, however, proved to be the first step toward its
eventual solution.
When the astronauts returned to the Skylab 1
docking port, they encountered a balky mechanism
which foiled four docking attempts.
On their fifth try, using a planned back-up tech­
nique, they achieved a hard dock—full attachment—
sealing their CSM to the station. The time was
11:50 p.m. The crew spent the remainder of the
night in their docked CSM. (Later, they repaired the
docking mechanism.)
The next day, they entered and prepared to erect
a sun shield over the OWS. They had three ap­
proaches, of which the prime (preferred) one was
a parasol erected from inside the station through
an airlock originally intended for solar-oriented sci­
entific expermients. The parasol was the least diffi­
cult means to deploy. Using procedures conceived
just two days earlier, the crew made a boom com­
posed of five rods screwed end to end at the top
of which was a folded shade. They poked this boom
through the airlock. When the boom was out far
enough, the sunshade was opened. The shade was
designed to cover an area 22 x 24 feet, but it had
a few wrinkles. Still it covered about 90 percent of
the meteoroid shield area and brought inside tem­
peratures gradually down. In about 11 days, the
Inside temperature was a comfortable 75 degrees.

Skylab 2/Saturn IB takes off with
Astronauts Conrad, Kerwin, and Weitz.

The other techniques were to be used if debris
blocked the scientific airlock through which the
parasol was poked. In one, the astronauts would
stand in the open hatch of their command module
and unroll a trapezoidal awning from the bottom,
or far end, of Skylab to the handrail of the ATM. The
narrow end of the awning would be toward the ATM.

3

�Close-up of jammed solar
wing, showing aluminum
strapping that held it.

SATURN WORKSHOP LAUNCH CONFIGURATION

APOLLO
TELESCOPE
MOUNT
SECOND

in*

MULTIPLE
DOCKING
ADAPTER

AIRLOCK
MODULE

OWS

Skylab workshop showing
principal components.
In the other, two astronauts would step from an
airlock in the airlock module, affix a special bracket
to the outside wall, and attach two long poles to the
bracket, pointing them toward the bottom of he Skylab. At the ends of the poles are pulleys with rope
threaded through them. A V-shaped sheet of re­
flecting material would be hoisted like an inverted
sail toward the bottom of Skylab.
Immediately after parasol deployment, the crew
activated the OWS and began their planned scien­
tific experiments. They succeeded in making up
time lost more or less but were plagued by a worsen­

4

ORBITAL
WORKSHOP

(MODIFIED S-IVB STAGE]

ing shortage of electric power. Four batteries in the
ATM that were overheated in the pitch-up attitude
when ground controllers tried to balance OWS tem­
peratures and ATM solar panel illumination (see
above) tripped out prematurely (at 50 percent rather
than 20 percent of full charge). Another battery
dropped off the line completely. Because of the
power shortage, the astronauts had to cut back sub­
stantially on such important experiments as Earth
survey and solar studies.
NASA officials were well aware of the difficulties
and dangers (oart'cu'arly where sharp edges might

�Repaired Skylab with parasol sunshade and extended solar wing.

exist) of a spacewalk (extravehicular activity, or
EVA). Moreover, the section of Skylab where the
jammed solar panel was located was never designed
for spacewalking. It had neither handrails nor foot­
holds to serve as anchors to offset forces imposed
by an astronaut's work. But officials were confident
that a well planned and carefully executed EVA
could be successfully carried out despite these hin­
drances.
Ways and tools to loosen the panel were tested
In the Neutral Buoyancy Simulator, the underwater
replica of Skylab, at the Marshall Space Flight Cen­

ter, Huntsville, Ala. The buoyancy of the water simu­
lates to some extent the weightlessness of space.
Later Conrad, Kerwin, ana Weitz practiced the pro­
cedures inside the OWS.
Then, on June 7, 1973, Conrad and Kerwin spent
nearly four hours in the most difficult and daring of
all orbital repair jobs. First, they assembled a 25foot pole with a bolt cutter at one end. A tether, or
lanyard, was fashioned to work the blades of the bolt
cutter. While Conrad held the po'e out from the
side of the airlock module, Kerwin climbed onto the
struts of the ATM. He took the pole from Conrad

5

�Conrad takes advantage of zero
gravity to facilitate mouth
and throat examination by
Kerwin, who is an M.D.
and fastened one end with a tether to the struts.
This job was done while on Earth's night side
under Skylab floodlights. At orbital sunrise, Conrad
maneuvered the pole to clamp the bolt cutters on
the aluminum strip holding the solar panel. Then
Conrad moved hand over hand along the pole to
the solar wing. Tethers were run along the pole
between the ATM struts and the solar wing.
While Conrad held the bolt cutters on the alum­
inum strip, Kerwin pulled on the other end of the
lanyard to snap the blades shut and sever the strip.
They then attached a tether about half-way down
on the solar panel, tied the rope to the ATM struts,
and stood up under the rope. The tension thus ap­
plied to the solar wing broke loose a s'uck bracket
that still held the wing, permitting the wing to swing
out and finally lock into place.
The panels of the wing were not yet fully deployed
because the hydraulic fluid needed to drive them
into position was frozen. When Conrad and Kerwin
were safely back inside of the space station, Mis­
sion Control in Houston pitched Skylab upward
again to direct sunlight on the fluid mechanism.
Shortly, the panels fully deployed, adding approxi­
mately 3000 watts of desperately needed electricity
to Skylab's power. The surge of power also began
to charge eight batteries that had been useless.
In addition, the Skylab "We fix anything crew,"
as they jokingly called themselves, repaired a num­
ber of other malfunctioning instruments. Among
them: a jammed gear mechanism for driving an ultra­
violet telescope, a balky tape recorder, a battery not
producing power because of a stuck contact in its
regulator (Conrad hit it with a hammer), and a nonoperating valves in the cooling system.
Thus, human intelligence, and ability to meet un­
anticipated situations enabled the first Skylab mis­
sion to carry out nearly all of its planned scientific

6

and technical experiments.
Although NASA has for years studied the Sun with
automated Orbiting Solar Observatories, its more
than 30,000 solar pictures from the four-week Skylab
mission have been described by physicists as ex­
ceeding their wildest expectations.
One of the discoveries from these pictures is that
the Sun's corona is much more dynamic, or change­
able, than many scientists believed. The corona is
the Sun's outer atmosphere which extends millions
of kilometers into space. Its dynamic behavior is
believed due to interactions of its ionized (electri­
fied) gases with the solar magnetic field.
On June 15, automatic instruments on Skylab re­
ported a moderately strong solar flare—a sudden
outburst of matter from the Sun. Immediately the
astronauts directed the ATM instruments toward and
zeroed them in on the flare, making the best sequen­
tial observations yet of this kind of phenomenon.
The flare released as much energy as mankind uses
in decades. Science still does not understand how
energy is accumulated and released in a flare. Skylab's solar studies will contribute to unravelling this
mystery and perhaps to the solution of potential
energy shortages on Earth.
Conrad, Kerwin, and Weitz also brought back
more than 7000 scientific pictures of Earth. The
pictures are in demand by industry, agriculture,
weather services, city planners, ecologists, fishing
companies, prospectors, mapmakers, dam-builders,
and many others concerned with Earths' resources
and environment. They cover 31 states and six other
countries.
Among the most crucial of Skylab experiments
are those about man himself: how he responds and
adapts to weightlessness in prolonged space flight.
The outcome will not only bear significantly on plan­
ning for future flights but also add to knowledge

�Conrad smiles after washing
in Skylab shower facility.
Before washing, the astronaut
pulls the curtain from the
floor and attaches it to the
ceiling. Water is drawn off by a
vacuum cleaner. (If water
escaped, it would float
around.)
Weitz at control and display,
panel of ATM.

about bodily functions. Such additional knowledge
may aid future doctors in fighting human illness.
During the first Skylab mission, as well as the
earlier Mercury and Gemini manned Earth orbital
flights and the Apollo lunar explorations expeditions,
many changes in astronaut bodily systems occurred.
Among these were losses in muscular tissue, bone
calcium, red blood cell mass, and other fluids and
weakening of the cardiovascular (heart and circula­
tory) system—generally those bodily elements and
systems that on Earth must cope with the pull of
gravity. Scientists want to know whether these ef­
fects level off in prolonged space flight or, if not,

plan to develop measures to counteract them.
They also want more information on how man
adapts to work in space. The first Skylab mission
indicated man can adjust rapidly to zero gravity, or
weightlessness. Conrad, Kerwin, and Weitz became
so proficient that ground personnel had to increase
their planned workload to keep them fully occupied.
None of the three experienced space sickness
(as did some astronauts on previous shorter space
missions and the crew of Skylab 3 early in its 59-day
mission that began July 28, 1973). Even when they
were spun at 30 revolutions per minute in a rotating
chair on Skylab, they did not get motion sickness.

7

�Part of New England from Skylab. Note Cape Cod
peninsula at right; Long Island, lower left.
They could tolerate only half that speed on the
ground.
Another significant finding of Skylab is that ade­
quate well designed body restraints are necessary
for men to perform efficiently in space. In another
area, the men advised that tomatoes should be small
enough to be eaten whole and that salt sprinkled
on food bounces off.
Because the body does not have to work as hard
In the zero gravity of space as on Earth, scientists
were concerned about the deconditioning of the
astronauts as a result of their long mission. Because
of this, they wanted to examine them and their in­
flight specimens of frozen urine, freeze-dried blood,
and other materials as soon as possible after re­
covery. They also wished to avoid possible contami­
nation of the specimens by the warm, moist sea air.
As a result, plans were made to pick up the retuning spacemen and Skylab 2 together rather than
their leaving their spacecraft in the water and climb­
ing aboard a helicopter as in previous space mis­
sions, such as Apollo.
Conrad, Kerwin, and Weitz splashed down in the
Pacific about 1344 kilometers (840 miles) southwest
of San Diego, Calif., at 9:50 a.m. EDT, June 22, 1973,
aftre 28 days and 50 minutes of space flight. At
10:34 a.m., they emerged from their spacecraft,
which had been hoisted to the deck of the recovery
ship, U.S.S. Ticonderoga.
All three astronauts stepped unsurely onto the

Conrad and Weitz receive cheers after stepping
from their Apollo command module onto the
recovery vessel, Ticonderoga. Kerwin, in back­
ground, is emerging from module.
carrier deck. The effects they experienced are
comparable to standing up after a long period in
bed.
They wore pressure pants to counteract, if neces­
sary, orthostatic hypertension, a precipitous drop
in blood pressure that could cause them to faint.
As a further precaution, they also lay back on their
couches after splashdown. Orthostatic hypertension
would result from the inability of the cardiovascular
system to fight gravity and push blood up from the
lower extremities. Pooling of blood in the legs has
been a common reaction in returning spacemen.
Kerwin was the only astronaut who felt sufficiently
faint to inflate his pressure pants.
As most of their predecessors, all three astro­
nauts lost weight during their 4-week flight: Conrad,
nearly 4 pounds; Kerwin, 6V2; and Weitz, about 8.
In other ways too, the first Skylab crew, like all
peoole. showed individual variations in their re­
sponses to the 28-day space flight.
The first Skylab mission, in addition to providing
a wealth of scientific, medical and technical data,
set a new record for the longest manned space flight.
Just as and perhaps more important, it made pos­
sible and laid a foundation for the two longer Skylab
missions scheduled to follow it.

8

GPO 870-932

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MR-14

NATIONAL m AERONAUTICSAND SPACE ADMINISTRATION

The Second Skylab Mission:

A Scientific Cornucopia

The unprecedented wealth of information gained
from man's longest and most productive space voy­
age— the second Skylab mission — has paved the
way for major advances in knowledge about the
Sun, Earth, and life itself. The second Skylab mis­
sion also demonstrated that man can live and work
efficiently for long periods in space.
In addition, new world records were achieved for
the longest time (59 days, 11 hours, and 9 minutes)
and distance (about 341/2 million kilometers, or
211/2-million miles) man has traveled in space. The
men circled Earth 852 times, also a new record.
Launch from the John F. Kennedy Space Center,
Florida, took place at 7:11 a.m. EDT, July 28, 1973.
Splashdown in the Pacific about 370 kilometers
(230 miles) southwest of San Diego, California,
occurred at 6:20 p.m. EDT, September 25, 1973. The
crew included Alan L. Bean, Commander; Owen K.
Garriott, Science Pilot; and Jack R. Lousma, Pilot.
The second Skylab mission again served as a
reminder that space missions are never routine and
that unexpected hazards can develop. It also reemphasized the importance of man in a space
vehicle to make judgments and interpretations,
respond to unforeseen events, refine and improvise
experiments, and repair or replace faulty equipment.
This publication presents highlights of the second
Skylab mission. It includes both achievements and
preliminary scientific results and mission events.
Increased Understanding of Earth
The astronauts returned with nearly 16,000 pic­
tures of Earth and about 29 kilometers (18 miles)
of magnetic tape recording additional Earth data.
The pictures and data will contribute to man's efforts
to make good use of his planet and its resources.
Astronauts Bean, Garriott, and Lousma made 39
successful Earth passes rather than the 26 planned
before the mission. Each required changing the
spacecraft's usual Sun-oriented position so that its

Skylab 3 roll-out. Saturn IB is the launch vehicle.

1

�View of Mission Control Center, Houston, Tex.

Earth-viewing instruments were pointed straight
down at the surface from which they were acquiring
information. The crew also snapped a large number
of Earth photographs with their handheld cameras.
The Earth survey pictures cover most of the
United States and sections of 33 other countries.
They include broad areas of all continents.
The pictures and data support studies, both in
the United States and abroad, in ecology and envi­
ronmental quality, agriculture, forestry,
mapping,
geology, water resources, fishing, oceanography,
mineral prospecting, and meteorology.
Their scope is suggested by the following exam­
ples from the 116 investigations which are using
data from the second Skylab mission.
• Mapped the saline soils in Weslaco, Texas.
• Conducted inventories of rice and related
crops in California and Louisiana.
• Studied the rangeland ecosystem of SierraLahorton and Colorado Plateau.
• Studied infestation of Hemlock Looper in hem­
lock trees in Essex County, Massachusetts.
• Defined surface morphologic and geologic
features related to mineral deposits in parts
of Colorado, Nevada, Utah, California, Arizona
and Pennsylvania.
• Analyzed the Anadarko Basin oil fields in
Oklahoma.

• Studied drainage basins in northern Califor­
nia, Arizona, Texas, New England and Lalle
Ontario area of New York.
• Mapped surface features related to ground
water explorations and water resources inven­
tory in the Midwest.
• Evaluated the usefulness of microwave data
for determining sea state during calm and
disturbed conditions.
• Examined the growth and termination of hur­
ricanes using information gathered for Ava,
Christine, and Delia.
• Mapped the four million tons of seaweed in
the Sargasso Sea east of Florida as a pos­
sible Earth resource.
• Correlated the chlorophyll content, thermal
patterns, and water mass variations in the
eastern Gulf of Mexico with sportfish catches
to assess the effects of water environment on
the distribution of game fish.
• Analyzed conditions preceding severe storms
in Oklahoma.
• Demonstrated applications to land use studies
in the states of California, Colorado, Texas,
Nebraska, Iowa, Indiana, Maryland and New
York, and the countries of Mexico and Austra­
lia.
• Identified soil moisture distribution para-

�Revealed from the Skylab vantage point in space is this apparent impact structure, in the vicinity of
Manicouagan Reservoir, Quebec, Canada.

Lake Mead area, Colorado River, parts of Nevada and Arizona from Skylab.

3

�meters, soil and plant relationships, and pos­
sible underground water in the parched re­
gions of Africa.
• Tested the utility of remote sensing for updat­
ing the 1970 census in thirteen U. S. cities.
• Developed photomaps and updated existing
maps of the U. S.
• Demonstrated the use of space photography
for mapping of a remote area such as the
"Green Hell" of Paraguay.
Revolutionary Advance in Solar Knowledge
The astronauts obtained 77,600 telescopic images
of the Sun's corona, or outer atmosphere, in the
X-ray and ultraviolet and visible-light portions of the
spectrum. They spent more than 300 hours on solar
astronomy as compared to the 200 planned. The
information they obtained may contain the answers
to many puzzling questions about the Sun and per­
haps contribute to development of non-polluting,
unlimited energy sources.
Most solar data were obtained when the Sun was

high over the Earth's horizon to avoid
their
being blocked or obscured by the Earth's atmos­
phere. Some observations were made, however,
through the Earth's atmosphere to measure its
constituents.
Among preliminary observations and discoveries
of the second Skylab mission are:
• Coronal holes—places in the Sun's corona
cooler and more rarified than the rest of the solar
atmosphere—extend downward to the chromosphere
(the region where solar temperature reaches a
minimum). In the coronal holes, solar magnetic fields
stretch outward rather than curve back to the Sun's
surface. Scientists speculate that the holes may be
the source of the solar wind, the hot electrified gas
particles rushing outward from the Sun. The particles
travel along solar magnetic lines of force.
• Solar bright points, discovered by Skylab,
occur all over the Sun rather that just in the equa­
torial zone between 40°N and 40°S where most
violent activities take place.
• Solar flares—massive outbursts of matter

Solar image in X-ray wavelengths, taken from Skylab, reveals extremely hot corona.

�Arabella at work.

from the Sun's surface—sometimes arch back to a
different area of the Sun and trigger new flares at
these areas. Scientists had suspected but never
observed this.
• Giant bubbles—often bigger than the Sun—
were observed rising into the outer corona. They
are believed to be responsible for magnetic storms
on Earth.
• Coronal transients—eruptions that frequently
occur in connection with solar flares—reshape a
big volume of the corona, including its magnetic
fields.
• Prominences—condensed streams of hot gas
—erupt more frequently than astronomers expected.
• The life histories of many sunspots—relatively
cool dark areas on the Sun—were recorded on film.
Although the Sun was supposed to be in the
relatively quiet part of its 11-year cycle, it burst
into extraordinary activity during a good part of the
second Skylab mission. As a result, the astronauts
not only obtained quiet Sun information but also
photographs of an active Sun, including some 100
solar flares. The Earth's magnetic field shielded the
astronauts from cosmic and other deadly particle
radiation generated by this intense solar activity.
Although in orbit, Skylab was not outside of the
geomagnetic field which extends to an altitude of
at least 64,000 kilometers (40,000 miles). The crew
also observed and photographed auroras resulting
from this intense solar activity.
New Knowledge About Life Processes
During all manned space missions, astronauts
have experienced many changes in their bodily sys­
tems and elements that on Earth must cope with the
pull of gravity. Among these are losses in muscular

tissue, bone calcium, red blood cells, total blood
volume, and other fluids and weakening of the
heart and circulatory system.
The samples of blood, urine, feces, and perspira­
tion which the astronauts brought back with them
plus the thorough tests and medical examinations
of the astronauts after their return add to knowledge
about biochemical changes resulting from weight­
lessness and from return to Earth's gravity. The con­
tribution that this knowledge makes to understand­
ing of life processes may lead to new medical
advances. The knowledge is also important in plan­
ning for future long duration manned space flight
missions.
Doctors concerned about the effects of prolonged
weightlessness are encouraged by the fact that the
astronauts' physical reactions to weightlessness
appeared to have stabilized after about the 39th
day in space. And, after return to Earth, the astro­
nauts readapted much more quickly than those on
the first mission. Doctors attribute the leveling off
and improved reconditioning mostly to the astro­
nauts' daily hour of rigorous exercise, chiefly on a
stationary bicycle, during their long space mission.
Certainly one of the stars of the second Skylab
mission was Arabella, a common cross spider. Ara­
bella was part of a spider sister act in space (her
co-worker was named Anita) intended to compare
webs spun in weightless and Earth environments.
After a couple of days of disorientation, Arabella
spun webs resembling those made on Earth.
Garriott commented: "It seems she learned very
rapidly in zero g without the benefit of any previous
experience."
Anita, given her chance sometime later, began
spinning normal webs almost immediately. Scientists
note she had time to adapt to zero g.
The spider experiment was one of 25 selected for
Skylab among those submitted by high school sci­
ence students. It was suggested by Judith S. Miles,
Lexington, Mass.
Another intriguing life science experiment in­
volved Mummichug minnows. Those brought aboard
at first swam tail up in tight loops. Those hatched
from eggs that had been carried into space were
observed to swim normally (as on Earth) in zero g.
Scientists are mystified by this development.
Thus, the second Skylab mission showed that
living things appear to be able to function effec­
tively in space after a period of adaptation.
As in the first Skylab mission, weightlessness
proved stimulating to the astronauts. For example,
12-hour workdays were no problem, and the crew
became so proficient that they asked for and were
given additional assignments. As a result, the crew
completed about 11/2 times the work originally
planned for them despite a severe bout with motion
sickness that hampered them during their first few
days in space. To get well, the astronauts took
scopolomine/d/amphetamine, a drug that blocks
nerve pathways between the inner ear and stomach.
Space Manufacturing
The astronauts

formed

crystals and

alloys

to

5

�determine the practicability of manufacturing new
or improved products in space. The metallic spheres
and the crystals formed appeared to be more per­
fect and the alloys stronger than those made on
Earth.
The astronauts also found that they could weld
pieces of metal with electron beams. This demon­
strates that large structures can be built in space.
Red Alert
The workmanlike performance which character­
ized the Skylab astronauts was carried out despite
a problem early in the mission which could have
developed into a serious emergency. While the crew
were maneuvering their modified Apollo ferry craft
(Skylab 3) to rendezvous with the orbiting space
station (Skylab 1), Astronaut Bean reported seeing
"some kind of sparklers." Mission Control, Houston,
Tex., noted a pressure drop in one of four thruster
assemblies, which are small rockets used for steer­
ing the craft, and concluded that propellant was
leaking. To contain the situation, Mission Control
ordered the astronauts to shut the leaking assembly
down. Six days later, another thruster sprang a leak
and had to be shut down. Among other things, the
thrusters are needed to orient the Apollo ferry craft
so that its main rocket can fire in the right direction
for safe reentry and return to Earth.
Round-the-clock preparations were immediately
begun to activate the Skylab rescue vehicle: an
Apollo craft modified to accommodate five rather
than three astronauts and a Saturn IB rocket vehicle
to launch the rescue ship into orbit. At the same
time, ground personnel initiated studies of the fail­
ures on Skylab 3.

Lousma flies experimental Buck Rogers' type back­
pack inside of Skylab.
The two leaks were found to be unrelated and
not, as feared, indicative of a general system break­
down. One was caused by a stuck valve; the other,
by loose fittings. The two remaining thruster assem­
blies checked out perfectly.
The next steps were to determine whether and
how Skylab 3 could be steered with half of its operat­
ing thrusters. Computer studies and ground simula­
tions showed how it could be done. The information
was flashed to the astronauts aboard Skylab 1.
The astronauts were told that they would stay
aloft for 59 days, as planned. Preparation of a res­
cue vehicle was continued, but on a less urgent
basis. Before separating Skylab 3 from Skylab 1, the
astronauts were to check pressures in all their
rocket systems and then fire the two good thrusters
for a second to assure that they worked.
All went as intended. Astronauts Bean, Garriott,
and Lousma were able to complete their mission
and return safely to Earth in their own ship.
Three (Including One Record) EVA's
Three EVA's (extravehicular activities) were car­
ried out to perform operational and repair work. The

r

�first, on August 6, 1973, totaled 6 hours 31 minutes
and set a new world record for spacewalks. Be­
tween 1:32 p.m. and 8:01 p.m. EDT, astronauts Garriott and Lousma loaded film canisters in their
telescopic cameras, installed panels to measure
micrometeoroid (cosmic dust) impacts, inspected
the thrusters of the Skylab 3 ferry craft (they could
find no apparent cause for the leakage), and erected
a new awning over the parasol that had been set up

by the first Skylab astronauts to cool down their
overheated space station, whose heat shield had
been lost. (See "Man Still Matters — the Story of
the First Skylab Mission," MR-13). Solar radiation
and micrometeoroids had caused some deteriora­
tion of the parasol.
in the second EVA, from 12:24 p.m. EDT to 4:55
p.m. EDT, August 24, Garriott and Lousma plugged
in an assembly of six gyroscopes on Skylab 1, the

View of Skylab space station (Skylab 1) as the second Skylab crew approached it in their Apollo ferry craft
(Skylab 3).

7

�space station. The gyroscopes are needed to keep
Skylab 1 from pitching up and down, yawing from
side to side, or rolling. With this replacement, Skylab was held steady by three good gyroscopes in
each of its three axes. One in each axis could do
the job, but redundancy is a form of insurance for
this vital function. The astronauts also reloaded
film in their solar telescopes and retrieved the
micrometeoroid panel they had set up during their
first EVA.
The third and final EVA was conducted as part of
the preparations for completing the mission. Bean
and Garriott were outside their craft from 7:18 a.m.
EDT to 9:59 a.m. EDT, September 21, to unload film
cassettes from their six solar telescopes. In this as
in other EVA's, the astronauts viewed with awe the
Earth below and the sky above and were reluctant
to return to their spacecraft.
The film, tape recordings, and samples acquired
through the second Skylab mission will keep sci­
entists and planners busy for years to come. Out
of these will be derived new knowledge that can
contribute to making this a better world for all
mankind.

"By your scientific endeavor and your
physical endurance you have converted
a space vehicle into a repository of more
scientific knowledge than mankind can
immediately consume. In doing so, you
have provided the basis for a quantum
jump in human knowledge."
—From the message of President
Richard M. Nixon to the Skylab 3
astronauts, September 25, 1973.

Bean is assisted from spacecraft to chair mounted on forkiitt truck which carried the astronauts to the ship's
laboratory. These were part of precautions taken at splashdown because of concern over degradation of
bodily systems due to length of mission. The men are aboard the U.S.S. New Orleans, a helicopter carrier,
which is the main recovery ship.

8
GPO

872-390

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                    <text>JACK R. LOUSMA
Pilot
Also making his first space flight. Jack R. Lousma was
one of 19 astronauts selected by NASA in April, 1966.
He served as a member of astronaut support crews for the
Apollo IX, X, and XIII missions. A major in the U.S.
Marine Corps, he has logged more than 2,600 hours of
flight time.

LAUNCH ESCAPE SYSTEM (LES)
APOLLO COMMAND MODULE (CM)
APOLLO SERVICE MODULE (SM)
Space Div
Rockwell International

ALAN BEAN

OWEN GARRIOTT

JACK LOUSMA

2nd Skylab crewC.

SPACECRAFT - LUNAR MODULE
ADAPTER (SLA)

ALAN L. BEAN
Commander

•INSTRUMENT UNIT (IU)
International Business Machines, Inc.

Commander for the second manned Skylab mission, Alan
L. Bean is a veteran of the Apollo Program, having served
as lunar module pilot for the flight of Apollo XII in
November, 1969.
During that Apollo mission, he
brought the lunar module to a precision landing within
300 feet of the targeted landing point. He helped install
the first nuclear power generator on the moon. He has
logged a total of 244 hours, 36 minutes of space flight,
which includes seven hours and 45 minutes outside the
spacecraft on the lunar surface.

•S-IVB STAGE
McDonnell Douglas
Astronautics Co.
-1 J-2 ENGINE
Rocketdyne Div
Rockwell International
. INTERSTAGE

A captain in the U.S. Navy, Bean became a NASA astro­
naut in 1963. He was born in Wheeler, Texas, on March
15, 1932. After graduating from Paschal High School in
Fort Worth, Texas, he received a BS degree in aeronauti­
cal engineering from the University of Texas in 1955.

•FIRST STAGE BOOSTER
Chrysler Corp.

Bean holds many awards, including the NASA Distin­
guished Service Medal, Navy Astronaut Wings and the
Navy Distinguished Service Medal. During his career, he
has flown 27 types of military aircraft, logging more than
4,410 hours flying time.

8 H-1 ENGINES
Rocketdyne Div
Rockwell International

OWEN K. GARRIOTT
Science Pilot

Each member of the space team has an im­
portant role in achieving the Manned Flight
Awareness objective of preventing errors
and defects in space flight hardware and
operations. The error prevented helps en­
sure a safe and successful mission - and
eliminates the cost of correction. Error-free
performance truly means more space pro­
gram per dollar.

MANNED FLIGHT AWARENESS
Marshall Space Flight Center, S81A - DIR
Marshall Space Flight Center, Alabama 35812

Making his first space flight, Owen K. Garriott was
selected as a scientist-astronaut by NASA in June, 1965.
He has since completed a course in flight training and has
logged more than 1,600 hours flying time.

SCIENCE &amp; ENGINEERING IN OR

Garriott was born in Enid, Okla., on Nov. 22, 1930. He
graduated from Enid High School and then received a BS
degree in electrical engineering from the University of
Oklahoma in 1953. He also holds a master of science
degree and a doctorate in electrical engineering from
Stanford University in 1957 and 1960, respectively. He
has performed research in ionospheric physics since ob­
taining his doctorate, and he has authored and coauthored more than 25 scientific papers and one book.
He was awarded a National Science Foundation Fellow­
ship at Cambridge University and at the Radio Research
Station at Slough, England, 1960-1961.

He was born in Grand Rapids, Mich., on Feb. 29, 1936.
He attended Ann Arbor High School and received a BS
degree in aeronautical engineering from the University of
Michigan in 1959. He holds the degree of aeronautical
engineer from the U.S. Naval Post-graduate School
in 1965.
Lousma has been a Marine Corps officer since 1959. He
was awarded the MSC Certificate of Commendation in
1970.

BACKUP CREW
Vance D. Brand, Commander
William B. Lenoir, Science Pilot
Don L. Lind, Pilot

SL-3 EXPERIMENT ASSIGNMENTS
Number

M071
M073
M074
M092
M093
Ml 12—
Ml 15
M131
M133
M151
M171
M172
T003
M479
T002
T027
M487
T020
SOI 9
S020
S063
S073
SI 49
S183
S228
S230
S052
S054
S055A
S056
S082A
S082B
S190A
S190B
S191
S192
S193
SI 94
S071/
S072

Title

Cluster
Location

Science
Pilot

Cmdr.

Pilot

•
•

•
•

0

•
•
•

•
•
•

0

Mineral Balance
Bioassay of 8ody Fluids
Specimen Mass Measurement
In-Flight Lower Body Neg Press.
Vectorcardiogram
Blood Studies

OWS
OWS
OWS
OWS
OWS
OWS

Human Vestibular Function
Sleep Monitoring
Time and Motion Study
Metabolic Activity

OWS
OWS
OWS
OWS
OWS
OWS
MDA
OWS
OWS

•

•

0

•

0

0
0

0

0

OWS

•

OWS

•

Body Mass Measurement
In-F light Aerosol Analysis
Zero Gravity Flammabiliiy
Manual Navigation Sightings
ATM Contamination
Measurement
Habitability and Crew
Quarters
Foot Controlled
Maneuvering Unit
UV Stellar Astronomy
UV/X-Ray Solar Photography
UV Airglow Horizon Photo
Gegenschein/Zodiacal Light
Particle Collection
Ultraviolet Panorama
Transuranic Cosmic Rays
Magnetospheric Particle Collection
White Light Coronagraph
X Ray Spectrographs Telescope
UV Scanning Polychromator/
Spectroheliometer
X Ray Telescope
XUV Coronal Spectrohehograph
UV Spectrometer
Multispectral Photo. Facility
Earth Terrain Camera
Infrared Spectrometer
Multispectral Scanner
Microwave Rariiometei/
Scatterometcr Radai and Altimeter
L Band Radiometei
Orcadian Phythm of Pocket Mice
Orcadian Rhythm of Vineqai Gnats

OWS
OWS
OWS
OWS
OWS
OWS
OWS
ATM
ATM
ATM
ATM
ATM
ATM
ATM
MDA
OWS
MDA

•

0
0
0
0

0
0
0

•
0
0

0

©
0
0
0
0
0

TBD
T8D

•

0

0

0

0

0

0
0

•

0
0

0

0

0

•
•

•
•

0

0

0
0

0

MDA
MDA

•
•

0

MDA
CSM
CSM

•
•
•

0

0

�SCHEDULE OF EVENTS
DATE

TIME/EDT

EVENT AND BRIEF DESCRIPTION

JULY

7:08 a.m.

Liftoff of Second Skylab Crew

7:10a.m.

First/Second Stage Separation

7:18 a.m.

Spacecraft in Orbit

9:26 a.m.

First Spacecraft Maneuver to
Accomplish Rendezvous

2:21 p.m.

Final Maneuver Toward Rendezvous
With Skylab

3:38 p.m.

Docking With Workshop Cluster

3:21 p.m.

Undocking From Cluster

8:38 p.m.

Landing

28

of persons in NASA and industry worked around the
clock to conceive, design, produce, and test the methods
needed t o save the mission.
The effort was successful.
A sun shield was deployed over the station's habitable
area reducing temperatures to acceptable levels. Later,
the astronauts made a space walk that resulted in a suc­
cessful deployment of the jammed solar array wing.
PARASOL (Sun Shade)

SEPT.

22
NOTE:

At printing time of this brochure, the above timeline
was tentative and subject to change

MISSION PROFILE
The second Skylab crew will be launched to a rendezvous
with the orbiting cluster atop a Saturn IB and aboard a
modified Apollo Command and Service Module.
They are first launched into a preliminary orbit. Several
sequence maneuvers are required to reach the orbit of the
Skylab cluster. After docking, the crew rests before en­
tering the station.
Present plans call for the crew, early in the mission, to re­
place a sun shade which was deployed above the cluster
by the first Skylab crew. Tests have shown that the sun
shade deteriorates in strength due t o exposure t o direct
rays of the Sun. The shade will be replaced by the astro­
nauts working outside the orbiting station. They will
deploy two long poles. The new sun shade will be sent
out along the poles in a manner similar to raising a flag.
While the first crew completed a 28-day mission, the
second crew plans to remain aloft for 56 days.
The
mission will be similar t o the first one, but places more
emphasis on solar astronomy and earth resources experi­
ments.
SKYLAB REPAIRS
Two problems developed during the launch of the
unmanned Skylab cluster on May 14, 1973. The meteoroid shield, a thin, .025-inch aluminum cover on the out­
side of the station, was torn loose during launch. This
caused extreme overheating of the station.
The second problem involved the loss of one of two large
solar array wings attached t o the sides of the station. The
second wing deployed only partially. This caused the loss
of more than half the electrical power needed to operate
the station.
Because of these problems, the launch of the first crew
was delayed eleven days. During this interim, thousands

TYPICAL WORK DAY IN SPACE
The mission will be run on Central Daylight Time and the
sleep periods will run fairly constantly from 1 0 p.m. to
6 a.m.
After entering the workshop, the first two big
jobs will be shutting down the command module and
activating the Workshop.
During a regular mission day, the crew will spend the
morning hours from 6 t o 8 preparing for work. Check­
lists and plans for the day's work will be sent t o Skylab
from the ground, and received on a teleprinter aboard
Skylab.
The major experiments are solar astronomy, using the
Apollo Telescope Mount; earth resources, using the
camera and sensor package; biomedical, involving the
crew and several items of equipment; and another large
group called the corollary experiments.

SATURN WORKSHOP

Each of these major areas, with their various experiments,
must be fitted into the crew's work day. Conducting
earth resources experiments will depend upon the orbital
position of Skylab and the condition of the cloud cover
on earth. When the solar astronomy experiments are
being conducted, the ATM consoles must be manned dur­
ing every daylight pass. However, solar flares or other
sun conditions might call for manning the console at odd
hours.
Two out of every three days, each crewman will be a sub­
ject in the various medical experiments. At other times
he will monitor equipment while another crewman is the
subject.

Element

Command
and Service
Module

Function

Crew Ascent
&amp; Descent

The one period in which the astronauts will attempt to
stop work and get together will be the dinner hour. At
this time they can take a look at the flight plan and
tighten up loose ends.

Docking
Interface

Apollo
Telescope
Mount

Airlock
Module/Fixed
Airlock Shroud

Instrument
Unit

Orbital
Workshop

Solar
Observation

Power Control
&amp; Distribution

Launch
Vehicle
Control

Primary Living
&amp; Working Area

Environmental
Control

ATM/EREP
Controls
&amp; Displays

Experiment
Laboratory

Utility Center
Stowage

Data System

SKYLAB OBJECTIVES
President Nixon: "...the Skylab... will be aimed not at
advancing the exploration of deep space, but at gaining in
space new knowledge for the improvement of life here on
Earth.
It will help develop new methods of learning
about the Earth's environment and the Earth's resources,
and new methods of evaluating programs aimed at pre­
serving and enhancing the resources of all the world. It
will seek new knowledge about our star, the Sun, and
about its tremendous influence on" our environment."

Extravehicular
Activity Port
Length (ft)

34.3

17.3

13.3

17.6

3.0

48.1

Diameter (ft)

13.0

10.0

-

10.0

21.5

21.6

366

1,140

~

613

~

9,550

Working
Volume
(cu ft)

�</text>
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