Goldendale Observatory State Park

18 04 2011

There are very few truly public observatories in the U.S.  Most are owned by universities or research institutes (so, quasi-public), or are managed and operated by a complex public/state/private cooperative effort (take Mount Wilson, for instance:  it’s run by the Mount Wilson Institute under an agreement with the Carnegie Institution in Washington, but the observatory sits on USDA Forest Service land, so it has to operate according to federal guidelines).  A lot of these observatories have public programs so visitors can experience basic observational astronomy and learn about historical or current R&D, but for the most part, the observatories are reserved for institutional use.

So, we were excited when we learned that one of the few observatories in Washington state was designed from its outset as a “as public as we can get” space.  The Goldendale Observatory State Park owes its existence to a group of four men, M.W. McConnell, John Marshall, Don Conner and O.W. VanderVelden, who built a  24.5 inch Cassegrain reflector telescope together. They donated the scope to the city of Goldendale, and the city obtained federal funds to build the observatory in 1973.  From 1973 to 1980, the observatory was managed by a non-profit organization, and in 1981, the Washington State Parks Commission took over responsibility.  (Don Hardin has written up a much more extensive history of the observatory.)  So, now it’s a State Park, which is something neat and unusual.

At least, we found the whole thing exciting.  We timed our visit to coincide with the August Perseid meteor shower and joined a group of enthusiastic viewers for some naked-eye skywatching for a large portion of the night.  The evening public viewing program was fun, although someone did take a spill off the stairs leading up to the eyepiece of the 24.5 inch telescope.  We saw all the usual suspects (globular cluster, binary star, etc.) and considered our evening well spent.

The BEST part of the Goldendale experience, however, is the daytime viewing.  Not many public programs run during the day, which is a shame, because the sunspot viewing was fantastic.  Then, too, looking through a telescope at Mercury on a sunny afternoon is its own kind of awesome.

24.5" Cassegrain at Goldendale Observatory. Photo courtesy of Bernt Rostad.





Wallpaper Wednesday

13 04 2011

AUT 30-meter Cassegrain Wheel-and-Track Beam-Waveguide Antenna

I love it when New Zealand and Australia get together to do things, as they always come up with great ANZ+ words. Take for instance, anzSKA, the Australian and New Zealand component of the Square Kilometre Array, a collaborative effort in radio astronomy.

The SKA project is immense in terms of territory and stated goals. Some twenty countries will be participating in the development of antennae, fiber networks, signal processing, and computing. The SKA will use 3,000 dish antennae, each about 15 m in diameter. The antennae will be distributed in five spiral arms extending at least 3,000 km from the center of the array. Last month, SKA announced that the Project Office will be at the Jodrell Bank Observatory near Manchester, UK, beginning January 2012.   The actual SKA array will be built either in Southern Africa or in Australia-New Zealand, knocking China and a joint Argentina-Brazilian proposal off the long list.  The final site choice is scheduled to be named next year.

So, today’s wallpaper is an image of a former Telecom New Zealand dish. Located north of Auckland, it previously was used for telephone, television, and broadband communications. In November 2010, Auckland University of Technology acquired the dish and set to repurposing it as the country’s largest radio telescope antenna. In addition to promoting more opportunities for research in practical radio astronomy, the dish is seen as a tool for enhancing New Zealand’s chances to co-host the SKA with Australia.





Yerkes Observatory

11 04 2011

Albert Einstein and the observatory staff in front of the 40-inch Refractor, 1921. Photo courtesy Yerkes Observatory.

I like to check into Yerkes Observatory in Williams Bay, Wisconsin, every once in awhile, just to make sure it’s still standing.  The observatory, which houses multiple instruments (a 102 cm [40 inch] refracting telescope, a 102 cm reflecting telescope, and a 61 cm [24 inch] reflecting telescope, and several small telescopes), is one of several founded by the incredibly energetic astronomer, George Ellery Hale (dates).  Although conditions at this observatory are not ideal for observing—they perhaps never were, as Hale eventually left Wisconsin for California in search of skies with less atmospheric turbulence—the observatory still functions as a research space for the University of Chicago.

The 40-inch refractor at Yerkes is still the largest of its kind in the world (the 49-inch refractor exhibited at the Great Paris Exhibition of 1900 was dismantled afterward).  The mirror for the scope was ground by Alvan Clark & Sons from a 42-inch blank that Hale heard about “by chance.”  Some chance!  The scope’s tube, mounting, dome, and rising floor were designed by the firm of Warner & Swasey, out of Cleveland, Ohio.  Hale had been working in his private observatory (Kenwood Observatory), but after some back-and-forth with the president of University of Chicago, secured an associate professorship and the promise of new observatory in which he could install the great refractor.  The money to build the observatory came from the pockets of Chicagoan Charles Yerkes, who allegedly was enamored with the project simply because he wanted to build “the biggest” of some interesting thing.  The scope was in place by 1897, and astronomers instantly put the refractor to good use.  For instance, Burnham’s Catalogue of Double Stars was finished at Yerkes, as was Barnard’s Photographic Atlas of Selected Regions of the Milky Way.  A great many of astrophotographic  techniques were pioneered at Yerkes, as well.

One of the strengths of the Yerkes Observatory is the condition of its telescopes, despite their age.  Because of the good state of preservation of the observatory and its continuing relationship with academic institutions, visitors not only have an opportunity to learn about the history of observational astronomy, they can see how observatory and its instruments  contributed to the professionalization of astronomy.  Yerkes runs programs for students of all ages (including the visually impaired!), putting young people in contact with both historical and contemporary approaches to research and development at the observatory.

The R&D program occasionally makes use of the historic instruments at the observatory.  For instance, a project to measure stellar motion takes advantage of photographs taken in the early 1900s and the 1980s with the 40-inch refractor.  Yerkes has over 170,000 photographic plates for use by researchers.

In truth, however, the observatory is mostly important because of its history, not because R&D relies on the original telescopes (University of Chicago does most of its observational astronomy at the Apache Point Observatory in New Mexico).  Because of this, the observatory is frequently under threat by plans to sell or develop the surrounding property.  Most recently, the property was slated for development for a luxury residential complex, but in the end, an appointed study group felt the observatory had too much potential as an educational center to surrender the property to a private developer (the final report was made available to the public).

As a historian of observatories, I can only be pleased that University of Chicago has re-dedicated itself to the preservation of the property, not just because it played a large role in the development of astronomy in the United States, but because the architecture of and the landscape surrounding the building are unique in their aesthetic. Those of you who have done work at the Newberry Library in Chicago might recognize the design hand of Henry Ivy Cobb in the Yerkes Observatory buildings.

Yerkes Observatory, Williams Bay, Wisconsin

Detail of Pillar, Yerkes Observatory. Photo courtesy of Yerkes Observatory.





Reflecting Telescopes

2 04 2011

Reflecting telescopes use mirrors to gather light.  A large concave mirror (the “objective” mirror) collects the light as it enters the tube of the telescope.  It then reflects the collected light onto a smaller mirror, which in turn reflects it into the eyepiece for magnification.





Refracting Telescopes

2 04 2011

re·fract  (r-frkt)

tr.v. re·fract·edre·fract·ingre·fracts 

1. To deflect (light, for example) from a straight path by refraction.

Refracting telescopes use convex lenses to gather light.  The lenses refract (bend) the light to bring it into focus.  The lens is thicker in the center than it is at its edges.  This means that the light bends more at the edges, sending to toward a central focus point.  The point of focus is where the image is created.

The Yerkes 40-inch refractor is the largest refracting telescope in the world.





Cassegrain Telescope

2 04 2011

Cassegrains are reflectors.  The classic Cassegrain has a parabolic (concave) primary mirror and a hyperbolic (convex) secondary mirror.  As you can see from the diagram below, the mirrors are aligned with the focal point behind the primary mirror (outside the telescope tube, at the end of the tube).  The light is gathered through the open end of the tube on the left and bounced off the primary mirror onto the secondary mirror. The secondary mirror then bounces the light to the central focal point, through a hole in the primary mirror at the right.

Cassegrain Telescope

After some searching, I found the original description of the Cassegrain telescope in the 29 February 1672 issue of the Journal des Sçavans.* Here’s the .pdf, Cassegrain Telescope, 1672 Journal of Sçavans, courtesy of Gallica Bibliothèque Numérique.








Observatories and Instruments