Photographic History of Table Mountain
Observatory
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Part 3: Smithsonian Expands - Planetary
Astronomy Early Solar Panel Development
By James W. Young
retired astronomer from Table Mountain Observatory
Smithsonian continued site
development by adding more necessary buildings, additions, and storage sheds
for equipment. The site was proving extremely valuable for the
solarconstant
measurements, with weather and sky conditions better than Mount
Wilson, as well as other sites currently in use in Egypt and Chile.In the end, Table
Mountain had the longest run of any of the Smithsonian field stations.
Adding to the
1925 map, this represents many new out buildings, and several additions
as
Smithsonian's Table Mountain Field Station became their prime
'solar constant' measuring
facility. Note Edson's two telescope sites that were temporarily
established in 1940-41.
Following are images of the new
buildings, additions, and the areas used by Edson's
Caltech 'Planetary Group' to study both Venus and Mars in 1940-41.
The Residence for the Table Mountain Field Station's Director
This is the residence in 1938
late 1930s
Winter of 1940 - Delilah Butler
(Preston Butler's wife)
Winter of 1949
This is the Office and Shop
mid 1930s
Shop 1949
1950s
Inside Views of the Shop
late 1930s
Preston Butler - 1941
The Original Garage, Now the
Bunk House
1940s
late 1950s
The Assistant Director's
Residence
early 1930s
late 1930s
early 1940s
Original Bunker/Tunnel
1930s
mid 1940s
Water Tanks and Tennis Court Fence
early 1940s
Original Smithsonian Water Tanks and the Tennis Court - 1962
The two original Smithsonian water tanks, and tennis court (behind the
closer-lying fence)
in 1964
Optical astronomy was not a part
of the Table Mountain effort to study the solar constant, however, there
were several small telescopes on the site for personnel use. No
information was found as to the exact nature of their use. These telescopes images were
found in the archives dating from the 1930s.
3-inch Refractor - early 1930s
4 and 6-inch Refractor Telescopes
from the 1930s
This was a 12-inch reflector of
unknown design - late 1930s
A Caltech professor, James B. Edson, knew of the Smithsonian solar
research conducted at
Table Mountain, and contacted the field director, Preston
Butler. Butler gave permission to
Edson to make observations of Venus and
Mars in 1940-41, and offered the site's 6-inch
telescope to help with the Venus
observations.
Edson then offered to a number of Caltech students the opportunity to
photograph the Venus
inferior conjunction of June, 1940, as well as the Mars opposition
during the late 1940s into
October, 1941. Four students answered Edson's suggestion; John
Spencer, James Winget,
Richard Canright, and Aden Meinel. These students, under Edson's
direction, formed the
Caltech 'Planetary Group'. Edson found a spare 6-inch reflector
telescope that he modified
to hold a glass plate camera for the Venus imagery. Still later,
Edson acquired access to the
still working scale model of Mount Wilson's 100-inch Hooker
Telescope...a 20-inch Nasmyth-
Cassegrain telescope to use for the Mars opposition into 1941.
VENUS INFERIOR CONJUNCTION
SETUP & OPERATIONS
Edson's rough map of their
observing site
Students cutting large stump for
telescope placement
Edson checking setup, then
checking 6-inch finder alignment
Students learning the system,
practicing telescope placement
Aligning telescope and plate
camera testing
The final configuration arrangement of the 6-inch reflecting telescope
(upper left), with
attached plate camera (upper right). This was attached and
aligned to the Smithsonian
6-inch refractor (for guiding and centering) in the bottom center,
with eyepiece in place.
Telescopes, and their configuration
Final testing of telescopes, alignment, and camera operations
Making observations and taking
imagery
Using the 28-foot sun screen
(shield) to block the sun's glare
Students resting in one of the
site's storage buildings
The good and best imagery examples
Venus inferior conjunction collage
imagery results of two weeks centered on the inferior
conjunction of June 26, 1940.
MARS OPPOSITION SETUP &
OPERATIONS
Title page of the group's notebook
Setting up the 20-inch telescope
in 1940
20-inch telescope ready for
operations - late 1940
20-inch telescope with Edson
(left) and two students - late 1940
Aden Meinel using the telescope in
the late winter of 1940-41
Closing up the 20-inch telescope
building - early 1941
Telescope building in the spring
of 1941
John Spencer using the telescope
in the summer of 1941
Four of the 'group's Mars image
plates from late August and early September 1941. Unfortunately, there was a lengthy
and long enduring dust storm on Mars during this opposition, and the imagery was
never as good as was expected.
Well after Edson's group left
Table Mountain, Smithsonian added a second inderground bunker west of the first
one. These bunkers, and the various instrumentation continued to provide Smithsonian with
additional solar constant data.
Look carefully...the original bunker is just to the right center,
almost hidden behind this
newer one built in 1950.
As Smithsonian's Table Mountain
solar constant studies came to a hault, the artificial satellite effort by the USA and
USSR created an almost instant need for solar cell development (to power
spacecraft once in orbit). So housing these solar cells in the form of a 'solar panel'
was an almost instant need. Table Mountain became a testing site for this developing
need, with JPL first obtaining permission for their 'Mobile
Solar Measurements Laboratory' to be brought to Table Mountain
to test their own
solar panel
development.
JPL installed their 'Mobile Solar
Measurements Laboratory' in the late 1950s to test their developing solar panels for JPL
unmanned spacecraft.
Early 1960s testing the Ranger
spacecraft solar panels
The Ranger Spacecraft solar panel
testing
An aerial view of Table Mountain,
showing JPL's solar panel testing area in 1962 (lower
left center). Looking
carefully, one can see the two Smithsonian underground bunkers in
the lower center of this
image. But, under even more careful inspection, one can see the
two dark spots just above
the lower right bunker...the exact spot where Edson's 20-inch
telescope building was used for
the 1941 Mars observations by Caltech's 'Planet Group'.
Following JPL's initial use of
Table Mountain for solar panel development and testing, four
other companies
also acquired permission to conduct their own solar cell developing
tests as
news spread of this
perfect testing site became well-known; Spectrolab, Hughes
Aircraft,
Electro-Optical Systems (EOS), and Hoffamn Electronics
Corporation.