Gerald P. Dyck
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| Walter Dyck and Paul Kuhlmann at 1931 telescope |
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I got my start in astronomy eight years before I was
born. In 1931 my father, Walter (on the left), and his
cousin Paul Kuhlmann made a 7" reflector from scratch.
This was before kits were commercially available. An
article in Scientific American got them started. They
ordered two blanks and an eyepiece, but made
everything else from
what they could find on their Kansas farm. The base was a stove; the RA and Dec shafts were two halves of a
Model-T axle; the gears and drive motor came from a Victrola player; and the tube was a silage pipe. It was all very non-portable. By the time I was born only the tube assembly survived. Through this scope I got my first
enhanced looks at the heavens. These views were the start
of six decades of astronomical joy and adventure. I am
grateful for the resourcefulness of my Dad and Uncle Paul.
Today our observing facility consists of two observatories
and a variety of portable instruments. The main building
is a merry-go-round observatory built in 1983 which houses
a home-made 17.5" reflector, built a year earlier. This
telescope won an award for mechanical design at Stellafane
in 1983. The observatory is described in detail on page
297 in the September 1988 issue of Sky and Telescope. This
is the instrument with which I make the bulk of my variable
star observations for the AAVSO. The second building
nearby is a roll-roof observatory which houses a home-made
10" reflector and a commercial 4" refractor, both of which
are used for group observing sessions.
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| Wide view of two observatories |
I am frequently accompanied by Sophie and Smudge. The
replica of the Stellafane logo on the sliding door was
painted by my wife Helga who is a keen astronomical observer, a frequent
companion at the telescope and a strong supporter of my
astronomical activities.
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| Gerry, Sophie and Smudge in doorway | Helga at the 10" telescope |
The most notable guest to visit our observatories was Clyde W. Tombaugh, discoverer
of Pluto, who came to New England in 1986. Before giving a lecture at the Skyscrapers Club he was escorted around to visit members' observatories. He is seen here inscribing some gracious words into my logbook.
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| Clyde W. Tombaugh visits |
Sophie is a keen observer of all things around her, but
rarely allows herself to be photographed in a pose not of
her own choosing.
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| Sophie at the 4" refractor | Laura at the dual solar scopes |
I used a variety of solar scopes before deciding upon the
very practical and portable set-up of side-by-side 80mm
refractors on an altaz mount. A spring serves as a
counter-balance. With these twin scopes I make regular
sunspot counts for the AAVSO and share the solar wonders
with my students, friends and family. Pictured above is my
daughter Laura.
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| Dual solar telescopes |
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The two refractors are mounted on a flat board with a steering paddle.
Vertical collimation is done with shims. Horizontal collimation is done with a turn buckle. The left scope has a 40mm Coronado H-Alpha filter; the right scope has a white light filter. They are not binoculars, but provide excellent comparison views of active regions. The little wooden block with two plastic triangles is a simple reflection finder.
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| Twin solar prominences | Transit of Venus |
Astrophotography is not an area in which I concentrate, but I have taken several solar photographs which please me. Two of these are of the twin solar prominences in January of 1999 and the much-awaited transit of Venus in May of 2004. I have contributed sunspot counts to the AAVSO Solar Division since 1998.
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| Left: Reaching a personal milestone of 100,000 CV observations. Right: Helga and I are seen reflected in the coelostat of the Snow Solar Telescope at Mt. Wilson |
I joined the AAVSO in 1978 and began observing Mira variables. I caught the spark
four years later when I saw my first outburst of U Geminorum. This coincided with the construction of the merry-go-round observatory. At that point I determined that such
a facility should not be used for casual observing alone. In 1982 I began a sustained effort to observe all the dwarf novae I could manage. In 1996, while at Mt. Wilson as
an instructor in the CUREA hands-on astronomy program of Joe Snider of Oberlin, I taught variable-star astronomy and reached my personal milestone of 100,000 CV observations. Beside me is a 1/12 model of the merry-go-round observatory. I reached the milestone of 150,000 observations in 2005.
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| Solar spectroscope with lid on |
Another home-made instrument is my solar spectroscope. It
was shown at the 1999 fall meeting of the AAVSO in
Hyannis. It is made with two razor blades for a slit, a
pair of surplus binocular objectives, a $6 grating, an
elastic band for a tuner, and one commercial eyepiece. A
filter wheel in front of the slit allows for greater
definition in various portions of the spectrum. This
simple instrument shows several hundred absorption lines
and has been a very useful teaching tool. It won a special
exhibit award at Stellafane in 1982.
A look under the lid shows the workings. Light enters the
slit at upper right, then passes through a baffle, to a
collimating lens focused on the tilt-mounted grating at far
left. The reflected spectrum travels through a second
collimating lens and a second baffle to the eyepiece.
Tuning is achieved by turning the black wheel below the
eyepiece, thus controling the tilt of the grating. All
elements of the spectroscope were first mounted
individually like chess pieces. I moved them to and fro
until everything worked, then traced the pattern onto a
"floor plan" and built a box around everything. Anyone
interested in receiving a free drawing may do so by sending
me a self-addressed stamped envelope.
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| Travelscope in trunk of car | Travelscope assembled |
My 17.5" Dobsonian was built as one solid unit. This works
well in a permanent observatory. In 1995 I built a second
tube assembly for the same optics, this time with "some
assembly required." The rocker box is collapsible, the
octagonal head piece fits into the tail piece, and struts
remain as four triangular units for quick assembly. Assembly takes about twenty minutes and collimation another
ten. Smudge's assistance makes the work more enjoyable,
but not significantly shorter in duration.
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| The travel scope in New Mexico |
In the summer of 2003 Helga and I took the travel scope to New Mexico Skies guest observatories for five nights of superb viewing of variable stars and deep-sky objects.
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| Sun Dial |
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Rounding out my astronomical equipment is a partially viable sun dial. The gnomon and dial face work as they should; the remaining features are for the benefit of my fun-loving or gullible friends. Below the face is the wake alarm. Below that, the crank for winding it on cloudy days. Furthest down is the energy saver switch which I turn off during vacations. The rear-view mirror is for night use only.
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| In the classroom | Sidewalk astronomy
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Since my retirement from daily music teaching in the Dartmouth Public Schools
I have developed a program of astronomy instruction for elementary schools called
"Have Scope — Will Travel." PowerPoint slide shows on solar, lunar, planetary and stellar astronomy are geared for the classroom and precede observing parties
for students and their parents. I also take my 5-inch refractor to where the public are in the good tradition of sidewalk astronomy.
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| Gerry Dyck receives the 150,000 Visual Observer Award presented by AAVSO council member David Hurdis at the Amateur Astronomical Society of Rhode Island meeting | Anti-Evil Eye, "Nazar Boncugu" |
Among my most prized astro-possessions is a 5-inch diameter carving which adorns
and protects our observatories. It is the Turkish Anti-Evil Eye given to us by Janet
Mattei when she and Mike visited us in 1990. I trust it and the spirit of the giver to
bless our astronomical endeavors far into the future.
Respectfully submitted,