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                <text>Bran Griffin was born in Medford, Oregon. His father was in the military,  so they moved around a lot. Bran went to the University of Texas his first year of college, and he studied Architecture. Then, he graduated college with a degree in Architecture from Washington State University. He then went to graduate scholl in Southern California, and he received a fine arts degree. After this, Bran wanted to get a degree in something a little more stable, so he went back to school to get his master's degree in Architecture. After this, Bran was on a shuttleship for a couple of years in Rome, and then he came back to start his career in teaching Architecture. Even though he was teaching Architecture, he had an intense passion for space. Because of this passion, he started to become involved with the Johnson Space Center with a faculty fellowship. Bran was in their Spacecraft Design Division. Since he wanted to be closer to be a part of the Space Industry, he decided to move to Washington State. After a while of working in Washington State, he received a job offer from Boeing in Hunstville, AL and began his career there being involved with the space station.</text>
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                  <text>&lt;a href="http://libarchstor.uah.edu:8081/repositories/2/resources/60" target="_blank" rel="noreferrer noopener"&gt;View the Saturn V Collection finding aid in ArchivesSpace&lt;/a&gt;</text>
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                  <text>&lt;p&gt;The Saturn V was a three-stage launch vehicle and the rocket that put man on the moon. (Detailed information about the Saturn V's three stages may be found&lt;span&gt; &lt;/span&gt;&lt;a href="https://www.nasa.gov/centers/johnson/rocketpark/saturn_v_first_stage.html"&gt;here,&lt;span&gt; &lt;/span&gt;&lt;/a&gt;&lt;a href="https://www.nasa.gov/centers/johnson/rocketpark/saturn_v_second_stage.html"&gt;here,&lt;span&gt; &lt;/span&gt;&lt;/a&gt;and&lt;span&gt; &lt;/span&gt;&lt;a href="https://www.nasa.gov/centers/johnson/rocketpark/saturn_v_third_stage.html"&gt;here.&lt;/a&gt;) Wernher von Braun led the Saturn V team, serving as chief architect for the rocket.&lt;/p&gt;
&lt;p&gt;Perhaps the Saturn V’s greatest claim to fame is the Apollo Program, specifically Apollo 11. Several manned and unmanned missions that tested the rocket preceded the Apollo 11 launch. Apollo 11 was the United States’ ultimate victory in the space race with the Soviet Union; the spacecraft successfully landed on the moon, and its crew members were the first men in history to set foot on Earth’s rocky satellite.&lt;/p&gt;
&lt;p&gt;A Saturn V rocket also put Skylab into orbit in 1973. A total of 15 Saturn Vs were built, but only 13 of those were used.&lt;/p&gt;</text>
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                <text>"Philosophy and practices of reliability as applied in the design of the Saturn Instrumentation System."</text>
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                <text>The basic engineering approach used in the Saturn instrumentation system has evolved to provide a highly reliable design for short periods of operation.  The airborne measuring and telemetry systems including preflight tests, inspection, documentation, and feedback between the users and designers are discussed.  The apparent differences between the practice and theory of reliability are rationalized.  Some consideration is given to new problems in designing systems that must operate in hostile environments for long periods.  The potential contribution of redundancy as a design concept is discussed.;  This paper is concerned with the airborne measuring and telemetry systems;  it does not attempt to treat the entire Saturn instrumentation system which consists of tracking devices including optical, radar, and Doppler, plus television, film cameras, and a myriad of instruments connected with factory checkout, ground test, and launch.</text>
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                <text>Griffin, M. A.</text>
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                <text>Rorex, J. E.</text>
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                <text>Saturn launch vehicles</text>
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                <text>Saturn V Collection</text>
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              <elementText elementTextId="210398">
                <text>University of Alabama in Huntsville Archives, Special Collections, and Digital Initiatives, Huntsville, Alabama</text>
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                <text>This material may be protected under U. S. Copyright Law (Title 17, U.S. Code) which governs the making of photocopies or reproductions of copyrighted materials. You may use the digitized material for private study, scholarship, or research. Though the University of Alabama in Huntsville Archives and Special Collections has physical ownership of the material in its collections, in some cases we may not own the copyright to the material. It is the patron's obligation to determine and satisfy copyright restrictions when publishing or otherwise distributing materials found in our collections.</text>
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                <text>spc_stnv_000600_000624</text>
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                <text>http://libarchstor.uah.edu:8081/repositories/2/archival_objects/17574</text>
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                  <text>Goldsmith-Schiffman Collection</text>
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                  <text>&lt;p&gt;"My ancestors were all German Jewish immigrants, members of four families who settled in Huntsville, Alabama before and following the Civil War. The Bernstein, Herstein and Schiffman families arrived during the 1850s, and Oscar Goldsmith arrived in 1879. Subsequent generations united these four families in marriage. Members of the extended family have figured in every phase of the history of Huntsville, both economically and socially; from the agrarian years of the nineteenth century through Huntsville’s growth after World War II, to becoming known as Rocket City USA; and socially, from the time of institutionalized slavery before the Civil War to segregation followed by the civil rights era."&lt;/p&gt;
&lt;p&gt;-&lt;a href="https://www.myjewishlearning.com/southern-and-jewish/highlighting-the-history-of-huntsvilles-jewish-community/"&gt;Margaret Anne Goldsmith in an interview with My Jewish Learning&lt;/a&gt;&lt;/p&gt;</text>
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                <text>Fee report for a claim suit filed by Lawrence Goldsmith against H. Oliver with Parks &amp; Cotton.</text>
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                <text>This document contains a detailed breakdown of the fees associated with the "unlawful detainer suit" filed by Lawrence Goldsmith against H. Oliver.</text>
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                <text>Griffin, Malvern U.</text>
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                <text>I. Schiffman and Company</text>
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                <text>Box 99, Folder Misc. Correspondence</text>
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                <text>University of Alabama in Huntsville Archives, Special Collections, and Digital Initiatives, Huntsville, Alabama</text>
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                <text>This material may be protected under U. S. Copyright Law (Title 17, U.S. Code) which governs the making of photocopies or reproductions of copyrighted materials. You may use the digitized material for private study, scholarship, or research. Though the University of Alabama in Huntsville Archives and Special Collections has physical ownership of the material in its collections, in some cases we may not own the copyright to the material. It is the patron's obligation to determine and satisfy copyright restrictions when publishing or otherwise distributing materials found in our collections.</text>
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                  <text>&lt;p&gt;The Saturn V was a three-stage launch vehicle and the rocket that put man on the moon. (Detailed information about the Saturn V's three stages may be found&lt;span&gt; &lt;/span&gt;&lt;a href="https://www.nasa.gov/centers/johnson/rocketpark/saturn_v_first_stage.html"&gt;here,&lt;span&gt; &lt;/span&gt;&lt;/a&gt;&lt;a href="https://www.nasa.gov/centers/johnson/rocketpark/saturn_v_second_stage.html"&gt;here,&lt;span&gt; &lt;/span&gt;&lt;/a&gt;and&lt;span&gt; &lt;/span&gt;&lt;a href="https://www.nasa.gov/centers/johnson/rocketpark/saturn_v_third_stage.html"&gt;here.&lt;/a&gt;) Wernher von Braun led the Saturn V team, serving as chief architect for the rocket.&lt;/p&gt;
&lt;p&gt;Perhaps the Saturn V’s greatest claim to fame is the Apollo Program, specifically Apollo 11. Several manned and unmanned missions that tested the rocket preceded the Apollo 11 launch. Apollo 11 was the United States’ ultimate victory in the space race with the Soviet Union; the spacecraft successfully landed on the moon, and its crew members were the first men in history to set foot on Earth’s rocky satellite.&lt;/p&gt;
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                  <text>&lt;p&gt;"My ancestors were all German Jewish immigrants, members of four families who settled in Huntsville, Alabama before and following the Civil War. The Bernstein, Herstein and Schiffman families arrived during the 1850s, and Oscar Goldsmith arrived in 1879. Subsequent generations united these four families in marriage. Members of the extended family have figured in every phase of the history of Huntsville, both economically and socially; from the agrarian years of the nineteenth century through Huntsville’s growth after World War II, to becoming known as Rocket City USA; and socially, from the time of institutionalized slavery before the Civil War to segregation followed by the civil rights era."&lt;/p&gt;
&lt;p&gt;-&lt;a href="https://www.myjewishlearning.com/southern-and-jewish/highlighting-the-history-of-huntsvilles-jewish-community/"&gt;Margaret Anne Goldsmith in an interview with My Jewish Learning&lt;/a&gt;&lt;/p&gt;</text>
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                  <text>&lt;p&gt;The Saturn V was a three-stage launch vehicle and the rocket that put man on the moon. (Detailed information about the Saturn V's three stages may be found&lt;span&gt; &lt;/span&gt;&lt;a href="https://www.nasa.gov/centers/johnson/rocketpark/saturn_v_first_stage.html"&gt;here,&lt;span&gt; &lt;/span&gt;&lt;/a&gt;&lt;a href="https://www.nasa.gov/centers/johnson/rocketpark/saturn_v_second_stage.html"&gt;here,&lt;span&gt; &lt;/span&gt;&lt;/a&gt;and&lt;span&gt; &lt;/span&gt;&lt;a href="https://www.nasa.gov/centers/johnson/rocketpark/saturn_v_third_stage.html"&gt;here.&lt;/a&gt;) Wernher von Braun led the Saturn V team, serving as chief architect for the rocket.&lt;/p&gt;
&lt;p&gt;Perhaps the Saturn V’s greatest claim to fame is the Apollo Program, specifically Apollo 11. Several manned and unmanned missions that tested the rocket preceded the Apollo 11 launch. Apollo 11 was the United States’ ultimate victory in the space race with the Soviet Union; the spacecraft successfully landed on the moon, and its crew members were the first men in history to set foot on Earth’s rocky satellite.&lt;/p&gt;
&lt;p&gt;A Saturn V rocket also put Skylab into orbit in 1973. A total of 15 Saturn Vs were built, but only 13 of those were used.&lt;/p&gt;</text>
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                <text>This material may be protected under U. S. Copyright Law (Title 17, U.S. Code) which governs the making of photocopies or reproductions of copyrighted materials. You may use the digitized material for private study, scholarship, or research. Though the University of Alabama in Huntsville Archives and Special Collections has physical ownership of the material in its collections, in some cases we may not own the copyright to the material. It is the patron's obligation to determine and satisfy copyright restrictions when publishing or otherwise distributing materials found in our collections.</text>
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&lt;p&gt;Perhaps the Saturn V’s greatest claim to fame is the Apollo Program, specifically Apollo 11. Several manned and unmanned missions that tested the rocket preceded the Apollo 11 launch. Apollo 11 was the United States’ ultimate victory in the space race with the Soviet Union; the spacecraft successfully landed on the moon, and its crew members were the first men in history to set foot on Earth’s rocky satellite.&lt;/p&gt;
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m

Use of the Ben Franklin Submersible
As a Space Station Analog

��USE OF THE BEN FRANKLIN SUBMERSIBLE
AS A SPACE STATION ANALOG

Volume I — Summary Technical Report
OSR-70-4

Prepared for
National Aeronautics and Space Administration
George C. Marshall Space Flight Center
Advanced Systems Office
Contract NAS 8-30172
Prepared by
Space Station Analog Study Team

GRUMMAN ^(1P)(Q)II)P@®[1

��THE BEN FRANKLIN DURING THE GULF STREAM DRIFT MISSION

Access to Rear Hatch
\

Surface Radio Antenna

Scientific Control Center
Scienti

Canister-Roiease Air Lock

Ballast Tank
Switch Panel

Conning Tower

Control Consolo
Head

Motor
Guard

Mess and
Wardroom

Waste Tank
Side Looking Sonar
Battery-Oil Reservoirs

Instrument Package
Cameras
Strobe Lights
Hydrophones

��FOREWORD

During 1969, the Ocean Systems Department of Grumman Aeiospace Corporation con­
ducted the 30-day Gulf Stream Drift Mission, using the BEN FRANKLIN submersible. As a
part of this mission, a NASA study was conducted to investigate man related activities which
are analogous to long-duration space station missions. During the mission, a NASA crew
member was aboard the BEN FRANKLIN for data collection, observation, and task partici­
pation. This work was performed in accordance with the Statement of Work in NASA Con­
tract NAS 8-30172, "Use of BEN FRANKLIN as a Space Station Analog," for the George C.
Marshall Space Flight Center, Advanced Systems Office, under the direction of C. B. May.
The program was coordinated by M. Markey of NASA, Washington Headquarters.
The Final Report consists of the following five volumes:
• OSR-70-4, Volume I, Summary Technical Report
• OSR-70-5, Volume II, Psychology and Physiology
• OSR-70-6, Volume III, Habitability
• OSR-70-7, Volume IV, Microbiology
• OSR-70-8, Volume V, Maintainability

iii

��ABSTRACT

This report presents the NASA effort using the BEN FRANKLIN submersible as a
space station analog during the 30-day Drift Mission in the Gulf Stream, starting July 14 and
ending August 14, 1969. The areas of investigation include:
• Psychological and Physiological measurements during the pre-mission, mission,
and post-mission phases
• Habitability in a closed ecology
• Microbiology evaluation of the water system, human flora, and environmental
samples
• Maintainability considerations for scheduled and unscheduled tasks.

AUTHOR CREDIT

The five volumes were prepared by the Space Station Analog Team as follows:
Author(s)

Subject
• Psychology and Physiology

C. P. Seitz, Ph. D.; A. Goldman, Ph. D. ;
R. J. Del Vecchio, Ph. D.; C. J. Phillips, Ph. D.

• Medical

R.P. Jessup, M.D. ;R. Fagin, M. D.

• Habitability
- Habitability Analysis

M. J. Ferguson

- Environmental

F. Abeles

• Microbiology

R.F. Davis, D. Valentine, K. Feindler

• Maintainability

J. R. Kappler, R. Toussaint

• Oceanographic Experiments

H. Reichel

• Summary

M. J. Ferguson

iv

��VOLUME 1.
SUMMARY REPORT
BEN FRANKLIN/SPACE STATION
ANALOG
Section
1.

2.

3.

INTRODUCTION
1. 1

Background

1. 2

Submersible Advantages

1. 3

Ben Franklin GSDM Inputs to Spacecraft Design

1.4

Recommendations

LIFE SCIENCES
2. 1

Objective

2.2

Approach

2.3

Results

2. 4

Inputs to Space

HABITABILITY
3. 1

Objective

3.2

Approach

3.3

Results

3. 4
4.

3. 3. 1

Area Utilization Studies

3. 3. 2

Questionnaire Results

3. 3. 3

Environmental Measurements

Inputs to Space

MICROBIOLOGY
4. 1

Objective

4.2

Approach

4.3

Results
4. 3. 1

Human Flora

��VOLUME 1. (Cont.)
Section

Page

4.4
5.

4.3.2

Food, Garments, Linen

4-4

4.3.3

Water Management

4- 4

4.3.4

Waste Management

4-7

4.3.5

Environment

4-7

Inputs to Space

4-8

MAINTAINABILITY
5.1

Objective

5-1

5.2

Approach

5-1

5.3

Results

5.4

.

5-2

5.3.1

Maintenance Workload

5-2

5.3.2

Maintenance Prediction Analysis

5-2

Inputs to Space

5-7

Appendices
A

BEN FRANKLIN CHARACTERISTICS

A-l

B

TABULATED SCIENTIFIC DATA

B-l

C

CAPTAIN' SLOG

C-l
LIST OF ILLUSTRATIONS

Figure

Page

1-1

Similarities - Spacecraft/submersible/chamber

1-3

3-1

Actual Versus Planned Crew Member Time Lines, Day 1

3-2

3-2

Major Habitability Complaints

3-4

3-3

Privacy and Free Space Complaints

3-5

4-1

Trend of Total Body Simplification

4-2

4-2

Trend of Total Body Shift

4-3

4-3

Environmental Contamination

4-5

vi

��LIST OF ILLUSTRATIONS (Cont. )
Page

Figure
4-4

Potential Pathogen Incidence

4-6

5-1

Percent Maintenance Man-Hours of Total Working Hours Per Day

5-3

5-2

Maintenance Action Summary

5-4

5-3

Crewmember No. 4 Maintenance Workload by Day

5-5

5-4

Comparison of Prediction Characteristics

5-6

vn

��SECTION 1
INTRODUCTION
1.1

Background
The 30 day Gulf Stream Drift Mission (GSDM) was conceived by Dr. Jacques Piccard

in 1965 to explore the Gulfstream from Florida to Nova Scotia, using visual observations,
bottom photography, biological surveys, and acoustical surveys. Early in 1967 the Grumman
Corporation agreed to undertake the mission and established a program for the design, de­
velopment, and construction of the BEN FRANKLIN. See Appendix A for the characterisitcs
of the vehicle.
During the design and development phase, the similarities between the GSDM and
space missions became apparent. At the same time the NASA Office of Manned Space Flight
awarded Grumman contract NASW-1965 to study the feasibility of using undersea facilities
as space mission analogs. Final Report OSR-68-6 11 March 1968, Feasibility Study - Use
of Submersibles as Space Mission Analogs, presents the results of the effort.
that submersible missions would be reasonable analogs of space missions.

It concluded

Both types of

missions would be manned by scientific and engineering crews motivated by a scientific pur­
pose to work under operational hazards. Therefore, the submersible could provide space
programs with data on crew reactions, the man-machine interface, habitability, and the
effects of complete biological isolation during a long-term mission.

In support of these con­

clusions, NASA awarded Grumman a contract to study these factors during the GSDM. The
study is the subject of this report.
The Naval Oceanographic Office (NAVOCEANO) agreed to support the ocean mission
by providing a surface vessel and two BEN FRANKLIN crew members to perform ocean experi­
ments. The remainder of the crew of six consisted of two pilots (including Dr. Piccard), a
relief pilot and oceanographer, and a NASA crew member responsible for the NASA effort.

1-1

�The GSDM began on 19 July 1969 when the BEN FRANKLIN submerged into the Gulf
Stream off West Palm Beach, Florida. It terminated 30 days, 11 hours later when the BEN
FRANKLIN surfaced 360 miles south of Nova Scotia.

The drift covered 1444 n mi at an average

depth of 650 ft. Ten excursions were made to depths between 1200 and 1800 ft.*. The
mission was supported by two oceanographic ships, two land bases, and a mobile support van.
1.2

Submersible Advantages
The Gulf Stream Drift Mission (GSDM) generated data and information applicable to

space missions which could not be acquired through other forms of ground-based simulators.
The mission tasks, the diversified crew, the sealed environment, and complete physical
separation from the outside world, produced unique problems, for example:
o The diversified crew and their interaction with the support team indicated potential
command (organizational) problems.
o Microflora of the crew and within the vehicle tended to simplify and to move to­
ward a microbial imbalance which might prove harmful over extended periods of
tinie in isolation.
o Limitations of communications provisions caused the crew to feel cut off from the
world. In addition, a lack of private communications prevented personal dis­
cussions.
o Complete isolation and separation forced the initial provisioning of all food. Foods
were pre-mission tested and accepted, but under mission conditions were found
to be unsatisfactory.
The submersible provides a means for evaluating the operational effectiveness of
crew habitability factors (food, clothing, accommodations), crew skill mix, command struc­
ture, and selected spacecraft subsystems checkout and maintenance during a real ocean mission.
To date, manned space operations, habitability provisions, and life support hardware
have been tested in ground based static simulators or chambers. However, as test durations
have increased in manned testing, motivational problems have resulted due to a lack of
*See Appendix B for a summary of scientific ocean data. Oceanographic scientific experi­
ment results are detailed in the Grumman BEN FRANKLIN GSDM Report OSR 69-19. The
captain's log is presented in Appendix C.
1-2

�meaningful work activities.

The GSDM showed that the submersible overcomes this problem

since a variety of meaningful scientific tasks are performed by the crew in support of the
mission. At the same time, the effectiveness of candidate long duration spacecraft hardware
and operational procedures, as well as crew interaction factors, can be evaluated in the closed/
stressed environment.
Submersibles and ground based chambers are complementary facilities.

Chambers

are required for thermal, vibration, radiation, and life tests under simulated environmental
conditions. The submersible offers a means for expanding on such tests, by providing men
and equipment an analogous mission environment. Fig. 1-1 lists the many similarities
between spacecraft and submersibles and compares them with chambers.
Spacecraft

Submersible

Chamber

Confinement

X

X

X

Social Isolation

X

X

X

Deprivation

X

X

X

Close Quarters

X

X

X

Meaningful Mission

X

X

Sustained Motivation

X

X

Hostile Environment

X

X

Operational Stress

X

X

Remote Operations

X

X

Abort Difficulty

X

X

Require Maneuvering

X

X

Scientific Crew

X

X

Data Transmission

X

X

On-Board Maintenance Provisions

X

X

Complete Biological Isolation

X

X

Command Structure

X

X

Figure 1-1. Similarities - Spacecraft/submersible/chamber

1-3

�1. 3

BEN FRANKLIN GSDM Inputs to Manned Spacecraft Systems Design
The objective of the NASA contract on the GSDM was to explore the areas of Life

Sciences, Habitability, Microbiology, and Maintainability for the purpose of obtaining space
station design criteria. The GSDM schedule precluded the acquisition and installation of
space subsystems.

BEN FRANKLIN subsystems and operations were, therefore, the basis for

the space studies, and only incidental space equipment was provided.
Volumes 2, 3, 4, and 5 describe the results of the investigations in detail.

The

following are a few examples of the types of spacecraft design guidelines which resulted from
the NASA contract:
Habitability:
Crew Accommodations
• Where volume is limited, bunks should be designed and located to be convertible
to private lounges for relaxation, reading, and writing.
• Soundproof the crew quarters and locate as far as possible from operating equip­
ment and work areas.
• Work areas and living/recreation areas should be separate.

Where limited volume

prevents this, activities must be scheduled to avoid overlap and interference.
• Provide for private communications with family and friends.
• Provide privacy, recreation, and storage for personal belongings.
Food
• Provide home type food and preparation facilities.
• The crew should not be forced to accept a monotonous diet and disagreeable foods.
• Variety and individual preference should be considered.

1-4

�Clothing
• Daily underwear change is essential
• Provide for internal environment off-design temperature conditions.
• Provide two piece garments rather than jumpsuits.
Biotechnology
• Develop automated on-line contamination monitoring and provide simple means
for decontaminating the vehicle surfaces, internal atmosphere and water manage­
ment subsystem.
• Compartmentize the spacecraft to prevent spread of contamination.
• Provide negative pressure in hygiene areas to prevent issue of contaminants into
living areas.
• Review all materials and designs to eliminate microbial nutrients and breeding
grounds.
• Provide microbiological screening of crew to eliminate pathogen carriers.
• Monitor individual crew microbial makeup to detect potential spread of infection.
• Provide for microbe incineration, in addition to filters, to assist in atmosphere
decontamination.
• Provide safe means for final disposal of microbially contaminated items.
• Provide an on-board microbiological laboratory to facilitate prompt
analysis.
A study of the command structure during the GSDM was not part of NASA contract,
but it is evident that such a study would have provided valuable data for space missions.

The

BEN FRANKLIN crew comprised a "mini" crew of scientists and operational personnel
similar in composition to spacecraft crew mixes. During the GSDM, operations problems
arose related to command structure, scientific/operations personnel skill mix, and the
mission control team decisions made on the support ship, PRIVATEER. These problems

1-5

�are analogous to those anticipated in Space Station operations. An investigation into the
causes and resolution of such problems in submersible missions could help provide insight
into similar situations on future space missions.
1.4

Recommendations
During BEN FRANKLIN ocean missions in the future, the space investigations of the

GSDM should be expanded to further develop general space technology, and to support the
Orbital Workshop (OWS), the Space Station, and the Space Base Programs.
A joint NASA/Grumman effort is required to establish a definitive space operations
and test program.

The OWS and future space program needs should be reviewed jointly to

select candidate tests.

Grumman would establish a program which integrates hardware and

tests into the BEN FRANKLIN and ocean missions schedules.
Recommended BEN FRANKLIN Future Space Tests:
1.

Life Sciences
(a) Crew performance evaluation
(b) Biomedical instrumentation (e. g. IMBLMS) *
(c) Crew Selection Test Verification
(d) Work Task unit

2.

Habitability
(a) Personal Hygiene Provisions
(b) Food Management
(c) Clothing
(d) Recreation Provisions
(e) Noise control
(f)

3.

Personal Accommodations

Biotechnology
(a) 60/90 day mission with crew rotation
(b) H O and atmosphere contaminant measurement and control
(c) Spacecraft and subsystems decontamination

*Integrated Medical Behavioral Laboratory Measuring System

1-6

�4.

Subsystems Operation
(a) Water management
(b) Waste management
(c) Atmosphere storage/supply

5.

Maintainability (of space equipment)
(a) Failure prediction techniques
(b) Scheduled and unscheduled task analysis
(c) Spares and tools requirements
(d) Repair techniques/operations

6.

Mission Operations
(a) Command Structure evaluation

1-7/1-8

��SECTION 2
LIFE SCIENCES

2. 1

Objective
The objective in "observing" the crew during the GSDM was to relate observed crew

performance to variables which designers can use to influence space systems performance,
ie:
• the engineering design (human engineering, environment)
• the choice of crew
• crew training
2. 2

Approach
Pre-mission data were obtained to establish a personality profile of the crewmen, to

establish a physical fitness index, and to develop a baseline on a motor skills test.
Data were obtained during the mission by means of a daily questionnaire or log that
included, in addition to items related to the operation, the mission and the environment,
the Cornell Medical Index, a Mood Scale Check List, a Subjective Stress Scale, a Sleep Recall
Questionnaire, a number of tests to evaluate fitness, and daily tests of proficiency on the
Langley Research Center Complex Coordinator.
These observations were supplemented by time-lapse photographs of most of the
vehicle by judicous location of 3 cameras and by recording approximately 1 hour of conver­
sation each day.
At the end of the mission, most of the pre-mission tests were repeated and the crew­
men were intensively interviewed.

2-1

�2.3

Results
Although selected only for special skills and desire to participate, the crewmen

assigned to work together were reasonably compatible.

Predictions of crew behavior based

on pre-mission psychological tests, clinical interpretation and observation of the crew were
proven reasonably accurate in the mission. However, the number of personality tests might
be considerably reduced and still provide the same degree of insight.
Predicted annoyance and psychological stress were produced by the austere BEN
FRANKLIN characteristics. These included the bunks, their location, food, the small galley,
people noise, odors, lack of privacy, clothing, inaccessability of equipment, limited personal
hygiene facilities, and environmental control.
As time increased, the men showed a general trend toward withdrawal and an in­
creased need for privacy.

This was in part evidenced by a tendency of the crewmen to eat

more and more meals alone as the mission progressed.

None of the crewmen reported

psychosomatic or hypochrondrical symptomatology. Levels of depression and lack of
personal well-being were greatest at the mid-point of the mission (days 13-15) when
there were procedural disagreements with the surface crew.
None of the crew suffered serious deterioration in proficiency.

However, as judged

from measurement of complex coordination, changes in proficiency in one instance could
be related to a mood of depression.

Potentially serious problems resulted from failures

and misunderstandings in communications with the surface crew.
when expected personal news was inexplicably lacking.

This was especially true

None of the crewmen showed signs

of physical deconditioning (there were no significant changes in recovery pulse or in hand
and wrist strength) and all were declared by the Grumman physicians to be medically fit
subsequent to completion of the drift mission.
Events in the GSDM indicate that expected communication of personal news at regu­
lar intervals probably is unwise because, if communications are delayed or interrupted,
crewmen tend to become distressed and concerned.

On the other hand, a lack of private

communications to the surface was a source of annoyance during the mission.

2-2

�Food provided a topic of conversation and possibly allowed for at least limited sub­
limation of psychological stress. Other topics such as daily questionnaires, and the inter­
actions with support personnel, accomplished the same result. These are not, however,
appiopriate avenues for the release of tension. Investigation is recommended to develop more
acceptable techniques to relieve tension.
2.4

Inputs to Space
Detailed consideration must be given early in a design to those aspects which could

cause crew annoyance and frustration, and which could be further aggravated by the long
duration confinement.

Particularly important are:

• the environmental control/life support system
• privacy areas
• illumination
• noise
• food/preparation/clean-up facilities
• recreation
• work areas
• multiple use of spaces
• personal hygiene
Selection of crew pairs for compatibility will help reduce psychological stress in
small closed systems. In addition, the mixed crews of future space missions should have a
voice in the selection of teammates. A better understanding of the importance of this input
is required and further investigations are recommended.
Performance rating both psychological (clinical) and operational can be obtained by
self reporting of the crew if they believe that the information they provide will be held in
confidence.

The development of improved techniques is recommended for obtaining self

evaluations by the crew with the intent of reducing the number of questions, eliciting

2-3

�observations not specifically called for, solicitiations of reports about others and for re­
porting during a mission. An objective measure of skill by a device like the Langley
Research Coordinator appears to be predictive and was accepted by the crew. Further
investigation to develop its utility is recommended.

2-4

�SECTION 3
HABITABILITY

3. 1

Objective
The objective was todetermine the suitability of BEN FRANKLIN habitability data for

providing guidelines for future spacecraft design.

Factors considered in the study were

food, clothing, control of environmental conditions, hygiene provision, crew equipment
items, and crew reactions to these provisions.
3.2

Approach
The procedures and records used in the study included:
• Time-lapse cameras located at three places, set to function every two minutes.
• Environmental measurements (light, noise, temperature, etc.).
• Counters to measure use of toilet facilities, etc.
• Ships logs.
• Crewmembers personal logs and questionnaires.
• Debriefing
• Comparison of actual activities with planned activities in the Mission Plan.

3.3

Results

3.3.1 Area Utilization Studies
Analysis of the camera photos coupled with a study of the logs established a record of
each man's location and activity throughout the mission.

From these studies of area utili­

zation and deviations from planned activities, it was determined that half of the crew
followed their plan and half did not.

Figure 3-1 illustrates this type of activity on day 1

of the mission, crewman #1 deviating from the plan and #6 following the plan. These

3-1

�LOCATION
CREW MEMBER 1

PLANNED ACTUAL

AFT SCIENTIFIC
AREA
PRIVATE AREA
PILOT AREA
GALLEY AREA
WARD RM/
OBSERVATION
AREA

A A A •

4-4

• A A A A i

PLANNED ACTIVITY
ACTUAL ACTIVITY
1 2

3 4

5 6

7

—A—*-

8 9 1 0 11 12 13 1 4 1 5 1 6 1718 19 20 21 2 2 23 24

DAY 1, HOUR

LOCATION

CREW MEMBER 6

AFT SCIENTIFIC
AREA

PLANNED ACTUAL

PRIVATE AREA
PILOT AREA

GALLEY AREA
WARD RM/
OBSERVATION
AREA

PLANNED ACTIVITY
ACTUAL ACTIVITY
1

2 3 4

5 6

7 8 9 10 11 12 13 1415 16 17 18 19 20 21 2223 24

DAY 1, HOUR
Figure 3-1.

Actual Versus Planned Crew Member Time Lines, Day 1

3-2

�deviations are due in part to lack of pre-mission training establishing each man's roll and
to changes in work/rest cycles.

The significant factor from this habitability standpoint is

the overlap of work and recreation activities in a given area.
3. 3. 2 Questionnaire Results
The ten top complaints on questionnaires and volunteered complaints are shown in
Figure 3-2. These indicate items which demand man/machine consideration both in sub­
mersible and spacecraft design.
Food complaints stemmed principally from the difficulties in preparation. Cooking
was ruled out since it would contaminate the atmosphere.

Canned, freeze dried, food

was provided and was satisfactory from a nutritional and storage viewpoint.

However,

complaints about food increased with time.
The crew complaints on privacy and free space are presented in Figure 3-3.
maximum of four complaints were made on Day 15.

A

The complaints decreased to one on

Day 22 and started to increase to Day 29. It is interesting to note that no volunteered
complaints were made throughout the mission. The principal complaint was that there was
a need for a place for each crew member other than his bunk.
Although the bunks were oversized, the crew complained that it was not possible
to sit up or bend knees without hitting the pressure hull.
3. 3. 3 Environmental Measurements
Atmospheric conditions were monitored and recorded throughout the mission.
Variations were readily maintained within reasonable limits.
Atmospheric constituents and trace contaminants were monitored with Drager Tubes
and a gas chromatograph.

The Drager tubes identified a continuing rise in CO throughout

the mission to a maximum of 40 PPM, identifying the need for greater capacity in the CO
removal apparatus.

3-3

���3. 4

Inputs to Spacecraft Design
On the basis of the habitability study during the drift mission the following guide­

lines are recommended for future spacecraft design:
• A separate area with soundproofing, adequate lighting and comfortable chairs,
is needed for reading and writing.
• Sleeping quarters should be noise isolated to minimize work area noise.
• Food preparation devices and techniques should be simple.
• Environmental monitoring should be semi-automatic to free the crew for more
useful activity.
• Clothing and bedding for space stations should be evaluated at off-design con­
ditions, to determine their adequacy.
• Illumination levels should be adequate for the task to be performed.
• The crew's use of the vehicle, crew activity, crew time lines, crew living and
working areas require detailed consideration and integration.

3-6

�SECTION 4
MICROBIOLOGY

4. 1

Objective
The 30-day submergence during the GSDM produced a unique internal environment

which, with regard to biological isolation, closely resembles that of future spacecraft.
The objective of the microbiological investigation was to study the effects of total
biological isolation upon the floras of the crew, environment and life support subsystems.
4.2

Approach
For comparison purposes, pre-mission, mission, and post-mission sampling were

scheduled.
To make the bacterial counts, a variety of sampling media and devices were taken
aboard including:
• Andersen samplers, (atmosphere)
• swabs and agar plates (human and surface environmental sampling)
• field-type water monitoring unit (field monitor kit).
Food was tested for bacterial count pre and post mission. Waste, garments and
linen were stored on board until the completion of the mission and were then returned to
the biotechnology lab for bacterial counts and identification of the types of bacteria present.
Approximately 15, 000 separate culturing steps were required to identify to Genus the 2230
isolates obtained.
4.3

Results

4. 3. 1 Human Flora
There appears to have been a general simplification and shift towards gramnegative organisms, (Figures 4-1 and 4-2), particularly Pseudomonas and Aerobactor.

4-1

���This has been postulated as an effect of long term isolation, but could have been biased
by on-board sample incubation at low temperature, followed by long-term storage, or by
the use of antimicrobial soap.
With the exception of one crew member (who had a history of Staph infections),
there were only transitory occurrences of Staph Aureus in the crew and the environment
(Figure 4-3.) Beta Hemolytic Streptococci were isolated from 5 of the 6 crew members
(Figure 4-4). These 5 also developed upper respiratory infections during the early mission
phase.
4. 3. 2 Food, Garments, Linens
Contamination levels of the foods were well within acceptable limits both pre a!nd
post mission.
Garments and linen had generally low levels of contamination when cultured after
use and onboard storage. It would appear that antimicrobial treatment of garments
and linen were effective in suppressing bacterial proliferation and odor.
4. 3. 3 Water Management
Iodine treatment was planned for control of the cold water system microbial con­
tamination. However, the crew objected to the iodine taste in the water and the recon­
stituted food.

In addition, the iodine treatment was difficult to perform and was not imple­

mented. This contributed to cold water contamination.
Pseudomonas, which had been a problem during much of the pre-mission attempts
at cleaning the system reappeared as a consistent contaminant.

Later in the mission a

variety of human associated organisms were recovered, including the fecal E coli.
Several filters (head, galley, shower-sink) when cultured post-mission were found to be
contaminated with Pseudomonas. Serious discrepancies existed between the on-board
readings and base laboratory analysis of the same sets of samples.

(Many samples read

as "sterile" on-board were discovered by base lab analysis to be contaminated.) This
was attributed to the limited facilities on board the BEN FRANKLIN:

4-4

�TABLE TOP

300

NOTE: DAILY WASHINGS

200
100

0

.zzzza

X7777&amp;

8

14

11

V///A
17

W/A
21

24

27

Y///A
+8

WALLS

200
a

W 100

•3
CC
LU

to

0

2

CO

A

z
&lt;
a

FLOORS

CC

° 800
CC

UJ 700

SYMBOL OPERATION

CO

A

600
500
400
300
200
100

A

AAAAAAA

MISSION DAYS

Figure 4-3.

Environmental Contamination

4-5

CLEANING

�POTENTIAL PATHOGENS INCIDENCE
MISSION DAYS
CREW

Pre-Mission

MEMBER

1

•6

-4

NS

2

3

NS

4

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4-6

E = EAR

�• low temperature incubation
• poor lighting
• lack of experience
4. 3. 4 Waste Management
Provisions were made for dispensing germicides, replacing odor control canis­
ters, and adding antimicrobial agents to the waste storage tanks.

During the mission,

macerator electrical problems prevented proper mixing of germicide with waste.

This

resulted in noticeable odor levels.
The effectiveness of odor control in the waste management contamination control
system was not evaluated during the mission.
were found to be contaminated with between 10

At post-mission sampling, all waste tanks
6

7

to 10 micro organisms/ml, most of which

were of enteric * origin.
4. 3. 5 Environment
The environmental floi-a, as the mission progressed, reflected more and more of
those organisms found on the men. The pattern of a shift towards gram negative orga­
nisms with respect to number of genera isolated was also similar to that of the human
flora.

Cleaning appeared generally effective in attaining a transitory reduction of total

microbial level, although a general rise in contamination persisted as the mission
progressed. The initial clean-up appeared to lower the microbial load considerably,
because on Day 2, all counts were low.
The dips in contamination levels can be related to cleaning procedures with tran­
sient drops in microbial counts on the walls and floors noted at the general cleanups.
However, after cleaning, there was a rapid rise of the contamination level on the floors
and walls.

The contamination of the table tops increased with time at a slower rate be­

cause of the daily washings.

*Enteric microbs are those found in the intestinal track.

4-7

�4. 4

Input to Space
Even with the limitations imposed by schedules and funding, the microbiology study

was productive in providing guidelines for spacecraft design. Many unknowns exist in
the area of space microbial technology, and this test should be considered only as a
basis for much additional work, i.e.:
•

The continuing shift and simplification of microbial flora on the 30-day mission
indicates a need for investigation of the problem in association with longer space
missions.

•

The personal hygiene areas, and humid areas in general, will prove to be fertile
microbe breeding grounds and require microbial control.

•

The water and waste management systems will be particularly fertile areas and
require suitable contamination monitoring and simple decontamination provisions.

•

The use of anti-microbials offers temporary advantages but the overall effect
may be undesirable. Additional work is required in this area.

•

The stored hot water system was effective in controlling contamination and
should be a candidate for spacecraft. It could eliminate the need for biocides
such as iodine or chlorine which are disagreeable in food and drink.

•

Further testing is required on the effects of crew rotation, i.e., putting a new
crew member into an altered environment.

4-8

�SECTION 5
MAINTAINABILITY

5. 1

Objective
The objective of the Maintainability Experiment was to obtain detailed information

on the frequency, duration, type and complications of the onboard maintenance performed
during the Gulf Stream Drift Mission.

This would permit evaluation of existing main­

tainability techniques for application to space vehicle missions.
5.2

Approach
The maintainability study covered:
• Analysis of the systems and equipment in the BEN FRANKLIN to establish
spares, tools, test equipment, and estimated work loads.
• Preparation of maintenance procedure and data sheets, crew training, and
dock side maintenance time trails, etc.
• Maintenance recording during the mission
• Reducing and evaluating data
This maintainability experiment did not encompass all of the equipment aboard the

vessel. Systems and equipment were selected on the basis of criticality and available
information on which analysis could be performed.

This became the "controlled" portion

of the study. Actual mission data was collected for all maintenance performed.
Logistics preparation consisted of crew training and of maintenance procedures,
trouble shooting information, checklists, computation charts, spares, tools, and test
equipment for the equipment in the controlled maintenance portion of the experiment.
This was successful in satisfying the maintainability objectives. Crew comments indicated
that this preparation was precisely what they needed for approaching the mission with confi­
dence.

5-1

�5.3

Results

5. 3. 1 Maintenance Workload
The crew performed 1354 individual maintenance tasks, an average of 45 per day.
Figure 5. 1 shows the percent of total available manpower expended on maintenance during
the mission.

The maintenance workload actually required from 12 to 31% of the crew's

total available duty time each day.

On the average maintenance occupied the equivalent

of one man full time throughout the mission.
Scheduled maintenance accounted for 1312 of the 1354 maintenance tasks
(See Fig. 5.2.). Successful completion of the remaining 42 unscheduled repair actions,
however, assured mission success.
Two crew members performed 58% of all the maintenance work, but more signifi­
cantly they accomplished 96% of the unscheduled repair actions primarily because of their
highly skilled and maintenance-oriented background.

Fig. 5-3 illustrates the maintenance

workload assumed by the one crew member who was the prime mover in all of the un­
scheduled repairs.

His skill contributed to the mission's success and attest to the need

for this type of crew member on all such missions.
5. 3. 2 Maintenance Prediction Analysis
A.

Task Times
The statistical analysis of mission data indicated that maintenance tasks time

predictions by Method II of MIL Handbook 472 were reasonably effective in de­
termining task times.

Figure 5-4 shows a comparison of the results when regression

analysis was applied to these predictions in mission action dock-side time trials, and
an aircraft program as a control case. In view of the results, we concluded that
Method n was considerably better than Method HI since it is more closely
associated with actual hardware configuration and limitations.
B. Effect Of An Isolated Environment
Mission data analysis indicated that there was no discernable time differential
for the performance of maintenance in the stress of this mission environment versus the

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���relatively unstressed environment of the dock-side time trials. All crew members how­
ever, did admit to feeling the effects of stress at various points during the mission. This
indicates that a better baseline should be prepared to detect these effects on future
missions.
5. 4

Inputs to Space
Since the GSDM maintainability studies had to be performed on submersible sys­

tems, no specific recommendations can be made concerning space systems.

However,

the study showed that the submersible could be used productively for testing maintain­
ability techniques on space hardware.
It was revealing to find that the equivalent of one man out of the six was required
to perform maintenance tasks. Space stations will require many more highly complex
subsystems, and mission duration will be measured in months and years rather than days.
Hence, it appears that sophisticated analysis, training, and automatic failure detection
methods will be required.
Since sophisticated training of many crewmen is expensive, it is apparent that
means must be developed to reduce future space crew training.

The submersible offers

a facility to develop and evaluate alternative crew training procedures, with the aim of
reducing crew training requirements and associated special skill needs.

5-7/5-8

��APPENDIX A
BEN FRANKLIN CHARACTERISTICS

i

4s'9"

General Specification
Displacement

130 Tons

Length

48 feet, 9 inches

Beam (over motor guards)

21 feet, 6 inches

Height

20 feet

Opei'ational Depth

2000 feet

Collapse Depth

4000 feet

Submerged Speed (maximum)

4 knots

Life Support

6 men for 6 weeks

Payload

5 Tons

Total Power

756 Kwh

Viewports

29

A-l/A-2

��APPENDIX B
TABULATED SCIENTIFIC DATA
The following is a tabulation of the scientific data collected during the 30-day drift
mission:
1)

Approximately 900, 000 temperature, sound velocity, and salinity measurements
were recorded with time and depth. The water sensor recorded on magnetic tape each
parameter every 2 seconds. The data have been "dumped" and 80% looks "good".
The 20% "bad" data have not been looked at very closely. The problem on these
data were not in the sensors, but appears to be due to uneven tape take-up on the
magnetic tape recorder.

2)

These data may still be salvaged.

Stereo-photographs (848) of the bottom were taken at five different locations in
conjunction with 3 miles of bottom mapping performed by the side scan sonar.
All the film has been processed, but only a few samplings have been printed.

3)

The Gulf Stream current was measured continuously by tracking the BEN
FRANKLIN over the entire 30-day mission. In addition, a total of 6 hours of
insitu current measurements were made while the BEN FRANKLIN was bottomed.

4)

The side scan sonar operation was stalled in the beginning due to its overvoltage protection circuit (more than 30 volts).

Although this was anticipated,

the dropping resistor added to the input was too low a wattage rating and oper­
ation could not begin until 28-volt BUS dropped below 30 volts.

The data that

were collected (approximately 3 miles) are available.
5)

Over 371 hours of ambient light measurements were recorded on BEN FRANKLIN
and on the M/V PRIVATEER. These data were recorded on the WASP's
magnetic tape. The transmissometer flooded due to improper seating of seals
just before GSDM and light transmission experiments were voided.

B-l

�Two hours (4 miles) of magnetic anomalies were recorded on paper strip charts
before magnetometer sensor flooded during early stages of GSDM. A rubber
pressure equalizing diaphragm ruptured - cause unknown.
Over 1100 bottom reflectivity and volume reverberation measurements were
made by setting off explosive charges from both the M/V PRIVATEER (blasting
caps) and the USNS LYNCH (SUS charges). The direct and bottom reflected
pulses were recorded on magnetic tape aboard the BEN FRANKLIN.

Prelimin­

ary analysis of the tape is presently underway and the data looks very good.
Typical views of the scientists in the BEN FRANKLIN performing the volume
reverberation experiment are illustrated in Figure C-l.
Approximately 24 hours (50 miles) of gravitational anomalies were recorded on
strip chart recorder aboard the BEN FRANKLIN; data are still to be analyzed.
Forty-one temperature-depth transists across the Gulf Stream were conducted
from the USNS LYNCH, resulting in a total of 500 profiles made by expendable
bathythermographs (X-BT). Three surface temperature transists were made by
airborne radiation thermometer (ART) to assist in positioning BEN FRANKLIN
in the Gulf Stream.
A minimum of 360 hours were spent directly viewing and selectively photo­
graphing the organisms within the water column from the BEN FRANKLIN. This
work was assigned by 24 plankton sampling tows from the USNS LYNCH.
Twenty-four deep Nansen casts were also conducted to further assist in posi­
tioning BEN FRANKLIN.
The 70-mm camera system did not function properly; a bad external wire-splice
is suspected.

Films are being processed, but no images expected since strobes

seemed to be out of synch.

B-2

�Some general comments in conjunction with experiments and the GSDM that come
from NAVOCEANO's F. Busby:
1)

The deep scattering layer along the path followed by BEN FRANKLIN was non­
existent.

2)

There was a notable scarcity of any form of sea life.

3)

When the submersible was trimmed for a selected depth, vertical displacements
up to 100 meters were experienced as the vessel followed undulating isotherms.

4)

One swordfish was observed to attack the vessel, reluctantly accepted defeat,
and retreated (similar to an occurrence experienced by ALVIN).

In addition to the data taken by the NAVOCEANO, a log was kept by Dr. Piccard in
which he recorded a time history of depth, salinity, inside temperature, outside tempera­
ture, humidity, and control actions pertaining to the variable ballast system.

B-3/B-4

��APPENDIX C
CAPTAIN'S LOG
The following is a condensed version of the Captain's Log, describing how the mission
progressed day-by-day and highlighting the significant events.
14 July 1969
At 1025 hours the "Ready for Sea" checkout was completed. It was hoped the BEN
FRANKLIN could leave port quietly with little fanfare; however, quite a crowd was on hand.
The BEN FRANKLIN got underway at 1043 hours and passed the sea buoy at 1123 hours with
only H. Dorr andD. Kazimir aboard to prepare the boat for diving. The remainder of the
crew was aboard the M/V PRIVATEER. At 1635 hours, the LiOH was deployed.

We were

on station at 1844 hours, waiting for the boat DRAGON LADY with additional LiOH panels
that arrived after FRANKLIN was underway. At 2030 hours, the hatch was secured with the
crew aboard. "Rig for Dive" was completed, and bothVBT's were empty. At 2056 hours the
main ballast tank vents were opened - diving (Dive number 41). The boat descended smoothly dribbled shot occasionally to slow descent. Trim good, no propulsion needed. At 2150 hours,
we bottomed in 510 meters of water. Commenced checking boat and NAVOCEANO equipment.
NAVOCEANO gear working well except transmissometer, sub bottom profiler, and magneto­
meter. Side scan sonar will not operate due to high voltage provided by ships batteries. It
was estimated that it would take a few days before the voltage was less than 30 volts.
15 July 1969
The checks were completed at 0100 hours; all hands settled down. Commenced drib­
bling the shot to achieve neutral buoyancy at 20-ft altitude. The BEN FRANKLIN was under­
way drifting north in the Gulf Stream at 0119 hours; visibility good but the current was quite
slow. Sonar in standby when not in use. One landing light used for forward visibility. At
0150 hours noticed a slight air leak in the air reducer and tightened the plug but it still
leaked (very slightly) so it was decided to secure all air flasks. During this period, a few
output fuses blew in the auxiliary 60-cps inverters due to operator error (too much load on
the inverter).

Also discovered a slight hydraulic leak around the valve stem of the depth

gage. The bonnet was tightened and the leak stopped.

At 0500 hours, we were drifting very

slowly; the boat was getting colder and colder. We dribbled shot occasionally to account for

C-l

�hull shrinkage as the boat cooled down.

At 0900 hours, our position was about 19°, 19

miles from Palm Beach Inlet. Decided to terminate bottom cruise due to slow drift speed.
Began ascent to 600 ft by dribbling shot.
NAVOCEANO's penetrator in H-6*.

At 1135 hours, noticed a small drip at

Penetrator tightened. During the 1200 hour routine

checkoff, Drager C02 gage failed; shifted to the Fyrite gage which worked well throughout
the 30 days. Lost communications with PRIVATEER at 1420 hours; had to use new 504 unit
(underwater telephone) at full power to regain communications. Evidently, the PRIVATEER
trackers lost us. Range checks were used to regain position. The Straza 504 paid for it­
self already. At 1500 hours, we achieved neutral buoyancy at 300 meters with both VBT's
(variable ballast tanks) empty. The cabin temperature was still about 55° F, but gradually
rising. During this depth change, the current occasionally came from the north. For
these first 2 days, everyone was quite busy with very little sleep; however, spirits were
quite high.
16 July 1969
We were drifting nicely at 200 meters. The ampere-hour system was in operation;
however, the B-2 counter occasionally counted rapidly for no apparent reason. F. Busby,
D. Kazimir, C. May, and J. Piccard have slight colds.
comfortable 66°F.

The cabin temperature got up to a

C. May checked iodine concentration in the number 1 and 2 fresh water

tanks and found no iodine - cannot understand why, the concentration should be 6 ppm. The
same for tanks 3 and 4. C. May was having difficulty with the bunk counters and some
sleep monitoring caps. The number 1 hot water tank was cooling down fast since the
vacuum was lost - will shift tanks soon. Good luck message was sent to Apollo 11 astro­
nauts.
17 July 1969
We were drifting at approximately 200 meters. Took the first set of battery ground
readings at 0810 hours; .they looked fine. The macerator needed repairs; it wouldn't stop
running, so we had to defuse it.

C. May and K. Haigh found a ground on the case and

*This penetrator dripped occasionally during the 30 days. It was very slight and usually dry.

C-2

�corrected it. At 1030 hours we deployed the LiOH panels. The motors were meggered at
1530 hours; they looked fine. The boat seems to drift with the stern pointing north. She
oscillates a little to either side and occasionally turns around. Began the descent to the
bottom at 1705 hours by flooding the port VBT in increments. At 1800 hours, the compass
was found to be unreliable; shifted to the portable compass**. At 1855 hours, we bottomed
in 458 meters after sitting on the guide rope and gradually reached the bottom as the hull
cooled. Measured the current speed, which was quite slow, less than 0.2 knots. At 2036,
we blew the port VBT slightly to ascend to cruise depth - about 20 ft off the bottom. Sat
on the guide rope waiting for the current to push us, but to no avail - the current was too
slow. The Privateer dropped 50 blasting caps for acoustic studies. The drift rehearsal
now over - we will go for 30 days.
18 July 1969
At 0112 hours, a slow ascent was begun by blowing the port VBT in increments. The
stern 250-watt light was used mainly for observations at shallow depth - it attracts quite a
bit of plankton. At 0609 hours, two swordfish were observed at the aft hemisphere
swimming around rapidly. Once actually attacked the viewport that F. Busby was using.
At 0900 hours, (at 200 meters) the humidity went up to 82%, and more silica gel was de­
ployed. This reduced the level to a satisfactory 75%. Coricidin pills helped in reducing
our cold symptoms. Each day we computed power usage based on the equipment logs and
compared with the actual usage; however, wide variations existed. We will secure the
ampere-hour system when the computed method becomes accurate.
19 July 1969
We were drifting routinely at approximately 230 meters; our position was 60 miles NE
of New Smyrna Beach, Florida. At 1450 hours, at 187 meters, we secured all lights to
check light level.

Large print can be read easily. At 2014 hours, we changed the LiOH

panels (we were averaging about 3 days per set of 12). The Egan Experiment was working
well except for bioluminescence. The boat continues to be very stable at depth.

**This compass worked well throughout the mission.

C-3

�20 July 1969
We were drifting along nicely at 170 meters. We discovered some carbon monoxide
(10 ppm) and a small amount of hydrazine and acetone during our routine checks with the
Drager tubes. The four main and four positioning motors meggered out OK. We had to
flood some water in the starboard VBT as the depth decreased to 142 meters. The
communications with PRIVATEER have been excellent. K. Haigh completed the seismic
studies with LYNCH supplying the SUS charges. The highlight of the day was the moon
landing as reported by the PRIVATEER.
21 July 1969
We continued drifting at approximately 190 meters. Our position was 90 miles east
of Brunswick, Georgia. We commenced another set of SUS charges at 1340 hours for acous­
tic tests.

At 1414 hours, we began the descent to the bottom by flooding the starboard VBT

in increments. By 1555 we were cruising at the 20-ft altitude in a depth of 372 meters.
The current was quite strong. At 1830 hours, we bottomed briefly to measure the current
using our motors to hold position. At 1850, we were cruising at the 30-ft altitude. We
spotted multiple sonar targets and ascended to 100-ft altitude. Decided to remain well
above the bottom and then take another look at 0200 hours. We detected the first bacterial
contamination, using endo and total media in Petri dishes at the head sink. The Grumman
movie camera malfunctioned while attempting to photograph the bottom.
22 July 1969
Drifting at 260 meters; commenced descent at 0150 hours. At 0415, at 70-ft altitude,
conducted acoustic test using blasting caps which were released from the surface vessel.
At 0500 hours we were cruising close to the bottom at a good speed, operating the sonar
continuously. The bottom was hard and bumpy with some small escarpments seen. At 0600,
we commenced ascent to a shallower depth. It would be better to study this area in three
separate excursions during a 24-hr period due to the physical strain, cold, and highpower usage. At 1400 hours, we conducted another 1-hour bottom cruise in conjunction with

C-4

�the seismic studies.

Discovered the B-2 counter* was malfunctioning; decided to rely on

the computed power figures for the 110-vdc load. The ocean bottom in this area was fairly
interesting. The effects of internal waves caused large, slow depth changes.
23 July 1969
Today we were drifting at 200 meters, about 100 miles east of Charleston, South
Carolina. For a short period, internal waves were noted at 1000 hours. The boat some­
times changes depth of 40 meters in wave periods of 15 minutes.

At the end of the day,

decided to secure ampere-hour system and rely on equipment logs to compute the power
usage (saves power).
24 July 1969
At approximately 200 meters today. We were having fits again due to internal waves.
The boat oscillated between 180 and 220 meters. Changed the bacteria filters and replaced
the purafil in the head blower. Had to drain some fresh water into the mini-waste tank for
flushing. The sinks were clear of contaminants - possibly due to changing of the bacteria
filters. The mission has gone well - the crew and boat in good shape.
25 July 1969
Drifting at 270 meters approximately 90 miles south of Cape Fear, North Carolina.
Motors meggered OK at 1112 hours. At 1123 hours, PRIVATEER reported that we broke
through the north wall of the Gulf Stream; we then commenced running on two motors at
60 amps to power back into the Stream, on a course of 100°. At 1705 hours, we completed
the transit. Today we observed endo and total contamination of water at the head sink.
26 July 1969
At 233 meters at 0400 hours, it was quite clear that we did not make our way back into
the Stream. At 0928 hours, we commenced the ascent to the surface. The decision was
made to have PRIVATEER tow FRANKLIN. We ascended slowly in order to prevent battery
gas from escaping too fast. We saw many sharks and a barracuda enroute to the surface.

*This counter in the ampere-hour system monitored the power used from the B-2 battery
string.

�We also heard gas escaping from the batteries. Sometimes it would escape more rapidly
from one side and actually cause a very small roll. At 1205 hours, we surfaced. We then
blew the MFT's only slightly. Divers used scuba air to blow the MBT's and then added shot
to ensure negative buoyancy on the next dive. While under tow, we listened to "News
Radio 88" - the CBS radio station from New York City. The boat got quite warm while on
the surface and the sea was calm. The boat was left sealed during the surfacing and towing
in order not to disturb the "closed environment" which was important to the NASA study.
27 July 1969
At 0313 hours, FRANKLIN arrived at the dive site in the Gulf Stream core. Divers
re-rigged the noise boom, removed the magnetometer and disconnected the tow line. Dive
number 42 commenced at 0401 hours. FRANKLIN submerged rapidly while shot was
dribbled to slow the descent. Several battery vent valve salt water sensors came "ON".
It took several hours for the boat to stabilize in the temperature and she finally settled out
at approximately 200 meters at about noon. Megger readings taken in the evening showed
quite a drop for the number 2 main motor but the reading is still OK. At this point in the
mission, two crew members picked up a rash, probably due to perspiration and the fact
that underwear was changed every 3 days (not often enough). The carbon monoxide level
was now up to 15 ppm. The acetone and hydrazine levels had not increased.
28 July 19G9
We drifted today quite nicely at 200 meters. High bacteria counts throughout the boat
necessitated a thorough wash down with microguard. Also, a routine setup to wash down the
galley, shower, and head areas daily was instituted.

At 1222 hours, we began the descent

to 565 meters to measure the ambient light and to conduct acoustic tests for mid-water
scatterers and bottom reflectivity. Commenced the ascent at 1944 hours. The boat was
very stable, no internal waves. F. Busby and E. Aebersold repaired the wobbly wardroom
table with two C-clamps, one "Vise Grip" and two butter knives for shims.
29 July 1969
Drifting at shallow depths approximately 85 miles SSE of Cape Lookout, North
Carolina. We passed the halfway point in the mission at 2030 hours.

C-6

�MM

30 July 1969
Drifting at 165 meters. The boat was rising slowly. The carbon monoxide level was
up to 20 ppm. We ran the contaminant removal system for 1 hour. The mission was getting
to be quite routine now with plenty of sleep for everyone.
31 July 1969
Today we drifted at shallow depths. We went past Cape Hatteras and headed out to
the open sea. The hot water was heated for 2. 5 hours in tank number 3.
1 August 1969
Again we drifted at shallow depths approximately 35 miles east of Cape Hatteras. At
2055 hours, we released a SAS ball with urine and feces samples in it. The ball was re­
trieved immediately by PRIVATEER. Surprise for someone if it wasn't retrieved. The
galley, shower, and head faucets all show contamination.

This is no problem since cold

water was used only for washing.
2 August 1969
Drifting again at shallow depths today. Motor number 2 meggered - holding steady
at 5 megohms. Had to heat the hot water for 2. 5 hours.

The carbon monoxide level was at

20 ppm. Swiss National Day was celebrated by lighting a match in front of the United States
and Swiss flags.
3 August 1969
Approximately 120 miles east of Cape Hatteras, we drifted at shallow depths. Our
drift speed has increased to close to 3 knots. J. Piccard caught a salp in the plankton
sampler.
4 August 1969
At approximately the 200-meter depth, we drifted 300 miles south of Block Island.
Internal waves made life interesting. The drift speed was up to 3 knots. Plenty of power
available as the batteries continue to hold up well.

C-7

�5 August 1969
Drifting at shallow depths (200 meters) again at a good speed approximately 270 miles
south of Martha's Vineyard.

During the day, many tuna were sighted. The USS LAPON

(SSN661) transited the area on the surface. FRANKLIN and PRIVATEER had underwater
phone contact with her as she passed through the area.

The carbon monoxide level was up

to 30 ppm; ran the contaminant removal system for 4 hours. Drager readings before and
after running the system indicated no change in the level.
6 August 1969
Again drifted at shallow depths approximately 165 miles south of NANTUCKET SHOALS
LIGHTSHIP. Had difficulty blowing the starboard VBT for depth-keeping - the lines seemed
to be plugged. Cleared the system by building air pressure up to 10 atmospheres over sea
pressure. Many whales and porpoises have been heard on sonar for past few days. Internal
waves continue to plague us; however, the experience level in trimming the boat has in­
creased to a point where it is no problem. Ran the contaminant removal system for 4 hours .
The carbon monoxide level was at 30 ppm.
7 August 1969
Drifted at 298 meters, moving up and down with no need for accurate depth keeping.
Our position is now about 195°, 320 miles from Cape Sable, Nova Scotia. Heated hot water
tank number 3 for 8 hours. Ran the contaminant removal system again for 4 hours.
8 August 1969
Proceeded nicely at shallow depths at a good speed. Meggered the motors - all OK.
The batteries are in good shape also.
9 August 1969
Drifted at 265 meters. At 1811 hours, commenced the descent to 500 meters. At
this level, conducted acoustic work using SUS charges. Vibrations could be felt through the
hull even though the charges were set to explode at 60 ft.

C-8

�10 August 1969
Drifted at 500 meters. Completed the deep excursion at 0030 hours. The carbon
monoxide level was up to 40 ppm. The crew is getting restless. We still have not seen
the deep scattering layer.
11 August 1969
Again drifted at shallow depths. Our speed slowed to less than 2 knots.

At 2007

hours, commenced the descent to 500 meters for acoustic work.
12 August 1969
Conducted acoustic experiments at 500 meters. Commenced return to shallow depths
at 0028 hours. The mascerator switch burned out; the system can be used without the
mascerator. Heated the hot water tank number 3. The crew has channel fever - quite
anxious to surface.

Conducted another descent to 500 meters, commencing at 2017 hours.

Ran the contaminant removal system for 4 hours.
13 August 1969
Today we drifted routinely at 408 meters ascending to shallow depths. We checked
the number 2 motor and it meggers OK. The carbon monoxide level was at 40 ppm.
Commenced preparations for surfacing. The Coast Guard Cutter COOK INLET, arrived
and will standby in order to transport personnel to Portland, Maine. Since no deep scatter­
ing layer was found during the drift, BEN FRANKLIN will surface with excess power
available.
14 August 1969
Drifted at 288 meters while preparations continued for surfacing. The boat was rigged
for heavy weather, all data packaged for transfer to COOK INLET. Commenced slow ascent
at 0432 hours and surfaced at 0757 hours. LYNCH, COOK INLET, PRIVATEER, two ves­
sels from WHOI, and two rubber boats stood by. The crew and data was transferred to the
COOK INLET. FRANKLIN was taken in tow by the PRIVATEER after the PRIVATEER re­
ceived fuel and provisions from LYNCH.

C-9

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&lt;p&gt;Perhaps the Saturn V’s greatest claim to fame is the Apollo Program, specifically Apollo 11. Several manned and unmanned missions that tested the rocket preceded the Apollo 11 launch. Apollo 11 was the United States’ ultimate victory in the space race with the Soviet Union; the spacecraft successfully landed on the moon, and its crew members were the first men in history to set foot on Earth’s rocky satellite.&lt;/p&gt;
&lt;p&gt;A Saturn V rocket also put Skylab into orbit in 1973. A total of 15 Saturn Vs were built, but only 13 of those were used.&lt;/p&gt;</text>
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&lt;p&gt;-&lt;a href="https://www.myjewishlearning.com/southern-and-jewish/highlighting-the-history-of-huntsvilles-jewish-community/"&gt;Margaret Anne Goldsmith in an interview with My Jewish Learning&lt;/a&gt;&lt;/p&gt;</text>
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                  <text>&lt;p&gt;The Saturn V was a three-stage launch vehicle and the rocket that put man on the moon. (Detailed information about the Saturn V's three stages may be found&lt;span&gt; &lt;/span&gt;&lt;a href="https://www.nasa.gov/centers/johnson/rocketpark/saturn_v_first_stage.html"&gt;here,&lt;span&gt; &lt;/span&gt;&lt;/a&gt;&lt;a href="https://www.nasa.gov/centers/johnson/rocketpark/saturn_v_second_stage.html"&gt;here,&lt;span&gt; &lt;/span&gt;&lt;/a&gt;and&lt;span&gt; &lt;/span&gt;&lt;a href="https://www.nasa.gov/centers/johnson/rocketpark/saturn_v_third_stage.html"&gt;here.&lt;/a&gt;) Wernher von Braun led the Saturn V team, serving as chief architect for the rocket.&lt;/p&gt;
&lt;p&gt;Perhaps the Saturn V’s greatest claim to fame is the Apollo Program, specifically Apollo 11. Several manned and unmanned missions that tested the rocket preceded the Apollo 11 launch. Apollo 11 was the United States’ ultimate victory in the space race with the Soviet Union; the spacecraft successfully landed on the moon, and its crew members were the first men in history to set foot on Earth’s rocky satellite.&lt;/p&gt;
&lt;p&gt;A Saturn V rocket also put Skylab into orbit in 1973. A total of 15 Saturn Vs were built, but only 13 of those were used.&lt;/p&gt;</text>
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                  <text>&lt;p&gt;The Saturn V was a three-stage launch vehicle and the rocket that put man on the moon. (Detailed information about the Saturn V's three stages may be found&lt;span&gt; &lt;/span&gt;&lt;a href="https://www.nasa.gov/centers/johnson/rocketpark/saturn_v_first_stage.html"&gt;here,&lt;span&gt; &lt;/span&gt;&lt;/a&gt;&lt;a href="https://www.nasa.gov/centers/johnson/rocketpark/saturn_v_second_stage.html"&gt;here,&lt;span&gt; &lt;/span&gt;&lt;/a&gt;and&lt;span&gt; &lt;/span&gt;&lt;a href="https://www.nasa.gov/centers/johnson/rocketpark/saturn_v_third_stage.html"&gt;here.&lt;/a&gt;) Wernher von Braun led the Saturn V team, serving as chief architect for the rocket.&lt;/p&gt;
&lt;p&gt;Perhaps the Saturn V’s greatest claim to fame is the Apollo Program, specifically Apollo 11. Several manned and unmanned missions that tested the rocket preceded the Apollo 11 launch. Apollo 11 was the United States’ ultimate victory in the space race with the Soviet Union; the spacecraft successfully landed on the moon, and its crew members were the first men in history to set foot on Earth’s rocky satellite.&lt;/p&gt;
&lt;p&gt;A Saturn V rocket also put Skylab into orbit in 1973. A total of 15 Saturn Vs were built, but only 13 of those were used.&lt;/p&gt;</text>
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                <text>This material may be protected under U. S. Copyright Law (Title 17, U.S. Code) which governs the making of photocopies or reproductions of copyrighted materials. You may use the digitized material for private study, scholarship, or research. Though the University of Alabama in Huntsville Archives and Special Collections has physical ownership of the material in its collections, in some cases we may not own the copyright to the material. It is the patron's obligation to determine and satisfy copyright restrictions when publishing or otherwise distributing materials found in our collections.</text>
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                  <text>&lt;p&gt;The Saturn V was a three-stage launch vehicle and the rocket that put man on the moon. (Detailed information about the Saturn V's three stages may be found&lt;span&gt; &lt;/span&gt;&lt;a href="https://www.nasa.gov/centers/johnson/rocketpark/saturn_v_first_stage.html"&gt;here,&lt;span&gt; &lt;/span&gt;&lt;/a&gt;&lt;a href="https://www.nasa.gov/centers/johnson/rocketpark/saturn_v_second_stage.html"&gt;here,&lt;span&gt; &lt;/span&gt;&lt;/a&gt;and&lt;span&gt; &lt;/span&gt;&lt;a href="https://www.nasa.gov/centers/johnson/rocketpark/saturn_v_third_stage.html"&gt;here.&lt;/a&gt;) Wernher von Braun led the Saturn V team, serving as chief architect for the rocket.&lt;/p&gt;
&lt;p&gt;Perhaps the Saturn V’s greatest claim to fame is the Apollo Program, specifically Apollo 11. Several manned and unmanned missions that tested the rocket preceded the Apollo 11 launch. Apollo 11 was the United States’ ultimate victory in the space race with the Soviet Union; the spacecraft successfully landed on the moon, and its crew members were the first men in history to set foot on Earth’s rocky satellite.&lt;/p&gt;
&lt;p&gt;A Saturn V rocket also put Skylab into orbit in 1973. A total of 15 Saturn Vs were built, but only 13 of those were used.&lt;/p&gt;</text>
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          <element elementId="43">
            <name>Identifier</name>
            <description>An unambiguous reference to the resource within a given context</description>
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                <text>NondesTest_021508092714.pdf</text>
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                <text>spc_stnv_000555</text>
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          <element elementId="50">
            <name>Title</name>
            <description>A name given to the resource</description>
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                <text>"Nondestructive testing of space vehicle liquid propellant rocket engines."</text>
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            <name>Description</name>
            <description>An account of the resource</description>
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                <text>Presented at the Western Metals Congress, Los Angeles, California, 15 March 1967.;  Archive copy is a photocopy.;  ABSTRACT: This report describes the various nondestructive test methods employed to evaluate materials and processes used in the manufacture of large liquid propellant rocket engines at the Rocketdyne Division of North American Aviation, Inc. The contents of the paper were purposely oriented for an audience of aerospace, design and materials engineers.  A brief description of liquid propellant rocket engine reliability is presented. The relationship of standards and specifications to nondestructive testing is discussed and various test methods are described along with a discussion of their applications and limitations. The sequence of events leading up to the use of nondestructive testing in production inspection is presented. Finally, the organization of labor directly related to nondestructive testing is given.</text>
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            <name>Creator</name>
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                <text>Hagemaier, D.</text>
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                <text>North American Rockwell Corporation. Rocketdyne Division</text>
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            <name>Date</name>
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                <text>1967-03-15</text>
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                <text>1960-1969</text>
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            <name>Subject</name>
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                <text>Saturn project</text>
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                <text>Nondestructive testing</text>
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                <text>Liquid propellant rocket engines</text>
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                <text>Saturn V Collection</text>
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              <elementText elementTextId="162575">
                <text>Box 21, Folder 12</text>
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                <text>University of Alabama in Huntsville Archives, Special Collections, and Digital Initiatives, Huntsville, Alabama</text>
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            <name>Language</name>
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                <text>en</text>
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            <name>Rights</name>
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              <elementText elementTextId="162578">
                <text>This material may be protected under U. S. Copyright Law (Title 17, U.S. Code) which governs the making of photocopies or reproductions of copyrighted materials. You may use the digitized material for private study, scholarship, or research. Though the University of Alabama in Huntsville Archives and Special Collections has physical ownership of the material in its collections, in some cases we may not own the copyright to the material. It is the patron's obligation to determine and satisfy copyright restrictions when publishing or otherwise distributing materials found in our collections.</text>
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            <name>Relation</name>
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              <elementText elementTextId="162579">
                <text>spc_stnv_000550_000574</text>
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            <name>Is Referenced By</name>
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                <text>http://libarchstor.uah.edu:8081/repositories/2/archival_objects/17639</text>
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