Slide rule1 – This piece could be about that indispensable,
essential and interesting scientific device that used to hang on the belt of
every engineering or science university student in the pre-1960 era. But it’s
not. It’s about an encounter with a most interesting man, and it might reveal a
tiny sliver of forgotten history. The man is Arthur Frederick Eckel2
(1893 – 1960). Nearly all of us who are now in our nineties remember only his last
name in connection with the magnesium marvel, the Pickett and Eckel slide rule.
After the war, marriage, and the university I began my
working career in the summer of 1951 at the North American Aviation facility in
Downey, California. We were engaged in a very large research and development
project aimed at producing a long range intercontinental air-breathing unmanned
missile for the cold war. At that time, before satellites, the uncertainty of
where Russia was exceeded 10 miles so these missiles were to be armed with
very large hydrogen bombs to assure the distant target’s destruction. My work
was involved with the star tracking guidance system; optical telescopes, gyros
and very high precision mechanical parts.
The dozens of engineers and scientists at Downey were
assigned desks in a very large hanger -- no cubicles or walls. I was fortunate
to have a desk next to an older gentleman introduced to me as “Dr. Eckel.” Only
after having known him for many weeks did I finally learn that he was one of
the inventors of the famous Pickett and Eckel slide rule. That, I certainly
knew about. I was impressed.
Dr. Eckel had been hired by North American because of his
extensive experience in precision machine work, not for his knowledge of slide
rules. The top managers were making an oral history of some of his early work
through detailed interviews. He was depended on for advice in developing the
methods needed for creating the inertial navigation system and the pointing
mechanisms for the star tracking telescopes. I was lucky to have actual hands
on work on those devices. I was also lucky to be able to have conversations
with Dr. Eckel, my desk neighbor, reminiscing about some of his early efforts
in the field of astronomy.
At North American his advice was especially needed in making
what was called a ‘lead screw.’ This threaded item was only about 6 inches long
and about an inch in diameter. It had a very fine thread machined along its
length. As it turned in the final star tracking assembly it pointed the small
telescope at the selected stars with an accuracy of better than one second of
arc. That is hard to do. Some of Eckel’s advice included placing the screw in a
vertical position for machining because of the effect of gravity; even with
that one inch thick rod an imperceptible sag during the machining would
introduce error. And he advised that the final polishing of the threads had to
be done with ground chicken bones. Sounds crazy but he was serious.
In casual conversations he told me of his early career. As a
young machinist he had been employed in the shop in Pasadena that was
constructing the 100 inch Hooker telescope for Mt. Wilson. This was to be the
instrument that Hubble used to discover the universe. As some may know the
original funding given to George Ellery Hale came from a man named Hooker,
hence the name, but later funding to finish the project was given by Andrew Carnegie.
The work began in 1912 and was completed in 1917. During this period Eckel was
responsible for making the large bull gear that rotated the telescope on its
equatorial mount as well as other precision jobs. Eckel told of the day he met Carnegie. “I was
in the machine shop working at a lathe. Carnegie came in on an inspection tour
of his project and came up to me at the lathe. Rather than questions about the
work he was mostly intrigued by the curls of metal on the floor that came from
the lathe cutting tool.”
He also told the story of his difficulty in making the lead
screw for the device that produced the very large diffraction grating at Mt.
Palomar. It was made in four sections, each 5.5 by 7 inches, to solve the
problem of wear on the engraving tool. The excessive length that might be
needed for the screw that controlled the engraving tool if they tried to make
the full 14 inch surface at one go was an impossibly difficult problem. No
grating engine of this size had ever been made before. This large grating surface
was necessary to take full advantage of the light gathering capability of the Hale
telescope’s 200 inch diameter. Nearly every observation made by large
telescopes involves the use of a diffracting device to examine the spectral characteristics
of the observed object. For those not familiar with the history of large
telescopes the Hale instrument dominated astronomical research from it
inauguration in 1948 until the Keck was put into service in Hawaii in 1993. The
earlier Russian BTA-6 which was larger never achieved successful operation.
I hate to end on a negative note but the story does have a
coda and it’s not so nice. Eckel had three children. I was able to track down
some of his relatives and eventually found a grandson in North Carolina. I
placed a call to the business where he worked and spoke to his boss. The grandson
was busy and couldn’t come to the phone. I explained my mission and left a
message for him to call. I wanted to give him the information that I had which
I presumed he would never have heard. He did not call back and I can’t find my
notes which would allow me to repeat my efforts.
1In about 1620 E. Gunter and W. Oughtred
of Cambridge produced what today we would recognize as a slide rule computing
device based on the work of John Napier. Wikipedia notes that H. Coggeshall
designed a slide rule device for the measurement of timber in 1677; however, Samuel
Pepys notes in his journal that he came into possession of a slide rule device
for computing ship construction materials, including timber, much earlier –
about 1666.
2Born in Illinois,
USA in 1893 to Albert
Edward Eckel and Ida
Lill Wilson. Arthur Frederick Eckel
married Myrtle
Elizabeth Scott and had 3 children. He passed away on 22
Jun 1960 in Burbank, Los Angeles, California,
USA.
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