Wallpaper Wednesday

8 06 2011
James Webb Telescope Wallpaper

James Webb Space Telescope Wallpaper

Okay, I admit this isn’t the most stunning wallpaper but the James Webb Space Telescope (JWST) is on my mind today since NPR played their story on the cost of the instrument over and over and over this a.m.

As the wallpaper suggests, the JWST is going to be searching for the earliest galaxies, observing the formation of stars from the earliest stages to the development of planetary systems, and looking for signs of life in planetary systems. The telescope is designed to make its observations in the infrared (with limited capability for observations in the visible range of the spectrum) and will carry four separate instruments to do so: the Near InfraRed Camera (NIRCam), the Near InfraRed Spectrograph (NIRSpec), the Mid-InfraRed Instrument (MIRI), and the Fine Guidance Sensor Tunable Filter Camera (FGS-TFI). We already make infrared observations from Earth-based telescopes (at the Keck and Mauna Kea Observatories in Hawaii, for instance), but even at those high altitudes, the earth’s atmosphere can cause blurring. Thus, the need for a telescope outside our atmosphere, 1.5 million km outside our atmosphere, in this case.

To get the wallpaper, click the image and scroll down the downloads page. To get instructions for building a paper model of the telescope, visit the model page. To follow the telescope on twitter, look for @NASAWebbTelescp.





Lick Observatory

6 06 2011

Mail call!

This morning, I received this lovely card in my post office box. Postmarked July 2, 1946, the image shows the view looking west across town. (Click on images for high res.)

Lick Observatory, Mt. Hamilton, California.

Lick Observatory, Mt. Hamilton, California.

The note on the back reads, “Expect to be transferred out this way so we are out to look the place over. Nothing settled as yet. Back to Chi. in a couple of weeks. Climate here doing us lots of good. Gladys.”

Back of postcard, Lick Observatory.

Back of postcard, Lick Observatory.





University of Illinois

4 06 2011
Observatory, Small Observatory, and Auditorium, University of Illinois.

Observatory, Small Observatory, and Auditorium, University of Illinois. Photo credit: University of Illinois Archives.

If you’ve been looking for the online version of the excellent National Historic Landmark Theme Study on Astronomy and Astrophysics by the National Parks Service, you should know that most of the NPS links to the title page are broken. You can find the portal to the e-book at http://www.nps.gov/history/history/online_books/butowsky5/astro.htm (not at /butowsky/index.htm as the failed links would have you believe). The book is rather dated (1989), and the information included in it is most comprehensive for the observatories and instruments that have been nominated for National Historic Landmark status, but even the briefer entries are useful for dates and locations. I was happy to read the nomination entry for the observatory of my alma mater, designed by architect Charles A. Gunn in 1896.

University of Illinois Observatory.

University of Illinois Observatory. Photo credit: University of Illinois Archives.

It took me a bit of effort to track down Mr. Gunn, but according to the 1914 Alumni Record of University of Illinois, he was born in Chicago in 1870. He appears to have been a very well-rounded individual:  at university, he was in Adelphic, Sigma Chi, and Glee Club. He was Captain of his class baseball team, played varsity baseball, held the state and conference record for the ball throw, as well as the Hop, Step, and Jump, and broke the university record for the running broad jump in 1890.

Charles A. Gunn, 1913 Alumni Record, University of Illinois.

Charles A. Gunn, Entry from 1913 Alumni Record, University of Illinois.

It would seem Gunn designed the observatory as one of his last projects in Illinois, as he was recorded as working in New York between 1897 and 1903 (first as Assistant Architect at Columbia University, second as a solo act).

Charles Gunn, Semi-Centennial Alumni Record of University of Illinois, 1918.

Charles Gunn, Entry from Semi-Centennial Alumni Record of University of Illinois, 1918.

I’m not quite sure when Mr. Gunn got religion, but two of his children died young, in 1905 and 1907, so maybe he sought solace in the church after those events. At any rate, The Eighty-Second Annual Report of the Board of Foreign Missionaries of the Presbyterian Church of the USA (1919) notes that Mr. and Mrs. Gunn had returned to the Manila Station on the island of Luzon with the Philippine Mission after furlough.

Eighty-second Annual Report, Foreign Missions, Presbyterian Church USA.

Eighty-second Annual Report, Foreign Missions, Presbyterian Church USA.

Eighty-Second Annual Report, Presbyterian Church USA.

Eighty-Second Annual Report, Presbyterian Church USA.

But when did the Gunn family returned to mainland U.S.? Mr. Gunn continued to work in the Philippines, South China and Hainan from 1916 to 1921, after which point he worked in Shanghai until 1939 (see, for instance, the Missions Building, 169 Yuanmingyuan Road). He made the national U.S. press when hostilities between China and Japan came to a head in 1937 (“Daughter Fears for Parents in Peiping Mission,” Chicago Daily Tribune, July 31, 1937; “Charles A. Gunn.” New York Times, Oct. 20, 1945), but I haven’t been able find any trace of him after that year. It would seem, however, that the observatory was a one-off, and his true calling was in the architecture of religion, not science.

University of Illinois Observatory.

University of Illinois Observatory. Photo credit: University of Illinois Archives.

For more information on the observatory, including plans to restore the space, check out the Facebook group, Friends of the University of Illinois Observatory (thanks, Mike!).





Wallpaper Wednesday

1 06 2011

Australia Compact Telescope Array at Night.

Australia Compact Telescope Array at Night. Photo credit: S. Amy, CSIRO


Obviously, I have a thing for the architecture of radio astronomy.  I blame my appreciation for the dish on COMSAT first, NRAO second, and only those who grew up in the Okanogan know why (unless you followed the links in this sentence). The image above shows four of the six 22-m antennae that comprise the Australia Compact Telescope Array at the Paul Wild Observatory near Narrabri, NSW, Australia. My favorite part of the observatory’s website is the ATCA Live! page, which tells me what the array is currently tracking (“As you read this astronomers are observing the source HD135344AB which has an azimuth of 247.3 degrees and an elevation of 60.1 degrees. The telescope is setup to observe at 17000 and 19000 MHz simultaneously.”). There’s also a nice archive of construction and upgrade photos available for public viewing online. I can’t see finding myself in Narrabri Shire anytime soon, but if you’re in the neighborhood (500 km northwest of Sydney), hit the Visitors Center:  always open, admission is free.





Knightridge Observatory

30 05 2011
Knightridge Observatory, Bloomington, Indiana.

Knightridge Observatory, Bloomington, Indiana. Photo credit: JR.

In my earlier post about (then upcoming) events at the New Jersey Astronomical Association, I mentioned that the telescope at the Paul H. Robinson Observatory used a frame and mount acquired from Indiana University in the mid-1960s.  The images of the frame in its previous home on the NJAA website inspired me to make the ten-minute trip over to Knightridge to inspect the abandoned IU observatory.

As you can see from the photo above, the rather squat building is now surrounded by a small, young wood in suburban Bloomington. At the time of its construction in 1936-37, however, this was a relatively remote site. In fact, it’s far enough outside the (then) city limits that I was surprised to see the obvious signs of electrical connections on the outside of the building (below).  My neighborhood, which is closer to town, didn’t get electricity until 1960, so I guess I’m envious that IU managed to run a line out into the fields of Knightridge.

West approach, Knightridge Observatory.

Approach from West, Knightridge Observatory. Photo credit: JR.

The building is in remarkably good condition.  The mortar between the bricks is holding up well, and although the roof is highly oxidized, it’s still keeping the rain water outside where it belongs—for the most part, that is.  The southeast roof of the building, including one of the shutter doors in the dome, was hit by a falling tree, unfortunately. If this hadn’t happened, the interior would still be dry and tight. Now, as you can see, not only are daylight and water making their way inside, so are plant seeds.

Storm Damage, Knightridge Observatory.

Storm Damage, Knightridge Observatory. Photo credit: JR.

From the outside, the dome looks truly round, but the construction details inside tell a different story. Underneath the sheet metal is a dome constructed of jointed wood ribs in-filled with flat lumber that diminished in length as it approached the apex of the dome. It’s not quite a corbeled beehive vault, but it gives a good approximation of the effect, rendered in wood.

Wooden dome, Knightridge Observatory.

Dome Interior, Knightridge Observatory. Photo credit: JR.

The dome was raised on steel tracks that rested on wheels attached directly to the brick walls of the observatory.

Wheel, Knightridge Observatory.

Wheel, Knightridge Observatory. Photo credit: JR.

All of the wires and most of the mechanics that supported the rotating dome have been stripped from the observatory, leaving behind interesting but non-functional bits and pieces on the second story of the building.

Abandoned Knightridge Observatory.

Abandoned Knightridge Observatory. Photo credit: JR.

Because the dome is no longer water tight, this upper floor is starting to rot. The rectangular opening that once held the mount for the telescope frame is dangerous territory, and I can only hope the people who’ve been using the observatory for late night séances are being very, very careful.

Second Floor, Knightridge Observatory.

Second Floor, Knightridge Observatory. Photo credit: JR.

Despite the weather damage, it’s clear that this is one sturdy little building. It’s also clear that Professor Cogshall wasn’t all that concerned about aesthetics.  Reconsider the Lick Observatory: a dome painted to resemble the heavens, walls finished in California redwood, floor finished with a high-polish mahogany. This modest university observatory bears no trace of a finish plaster or floor varnish. Cogshall was here to get the job done, apparently, and saw no need for embellishments that probably wouldn’t look like much under a red light at night, anyway.

You can view a few more photos of the abandoned building on my flickr site.





NRAO Green Bank

27 05 2011
Howard E. Tatel 85-foot Radio Telescope, NRAO, Green Bank, West Virginia

Howard E. Tatel 85-foot Radio Telescope, NRAO, Green Bank, West Virginia

Wednesday’s mail brought me this “vintage” postcard of the Howard E. Tatel Radio Telescope.  Built in 1958, the Tatel was the first major radio telescope at the National Radio Astronomy Observatory (NRAO) in Green Bank, West Virginia.  Also known as “85-1,” the scope has served as a fixed element in the Green Bank Interferometer (GBI) since 1964.

Back of Postcard, NRAO, Green Bank, West Virginia

Back of Postcard, NRAO, Green Bank, West Virginia





Lick Observatory Historic Photos

26 05 2011

A look at a few of the photos I picked up in California last week:

Great Lick 36" Refractor Telescope

Great Lick 36" Refractor Telescope. Copyright: UC Regents.

Anna Nickel 40" Telescope

Anna Nickel 40" Telescope. Copyright: UC Regents.

Shane 120" Telescope

Shane 120" Telescope. Copyright: UC Regents.





Wallpaper Wednesday

25 05 2011
Alpha Magnetic Spectrometer-2

Alpha Magnetic Spectrometer-2. Photo credit: NASA.

Today’s wallpaper shows the Alpha Magnetic Spectrometer-2 (AMS-02) holding steady in its new home on the integrated truss structure of the International Space Station. Delivered to the ISS on May 19th by STS-134 under the command of Mark Kelly, the AMS-02 will be the first magnetic spectrometer used in space.  From its orbital position, the instrument will gather and measure cosmic rays as part of the on-going search for primordial antimatter and dark matter in the universe.  At the heart of the AMS-02 is a large magnet, the field of which will be used to distinguish matter from anti-matter. As particles and anti-particles pass through a uniform magnetic field, they bend in opposite directions.  The specific particle curvature (positive or negative) identifies the particle as electron or positron.  In addition, the radius of the curvature allows scientists to measure the particles momentum at the time of collection. More on the science (dark matter, anti-matter, strangelets, and cosmic rays) and technology (instruments) of the AMS-02 can be found on the instrument’s website. You can also follow the instrument on twitter @AMS-02.





Lick Observatory

22 05 2011
36" Lick Reflector

36" Lick Refractor. Photo Credit: JR.

Life unexpectedly detoured me through central California last week, so I thought I would take advantage of its (relative) proximity to visit Lick Observatory. The observatory is draped across the uppermost peaks of Mt. Hamilton in the Diablo Range east of San Jose. It’s open to the public on most days of the year, but hours and days are restricted during the winter months, so check the opening schedule before making the drive.

The daytime public program is focused on the historic instruments of the observatory, especially the Great Refractor installed under the dome custom-built for it in 1887.  This 36″ telescope, the lenses for which were ground by Alvan Clark & Son (the same workshop that ground the lenses for the refractors at the Yerkes and Cincinnati observatories), lives in the largest of two domes flanking the Main Building of the observatory.  A 12″ reflector that had been purchased second-hand from Alvan Clark originally lived in the smaller dome at the opposite end of the building; it now houses the 40″ Nickel Reflector. One has to wonder what instrumental astronomy would have looked like in the U.S. at the end of the nineteenth century had Alvan Clark not been around to polish the needed lenses and mirrors.

Interior, Dome at Lick Observatory

Interior of Great Refractor Dome, Lick Observatory. Photo credit: JR.

As you can see from the photo above, the Great Refractor was protected by a dome that was designed with a concern for aesthetics as much as functionality. The underside of the dome was tinted with a color meant to evoke the heavens and the walls were finished with California redwood paneling. James Lick might’ve been an odd guy, but he knew his woodworking.

Observatory floor and gears, Lick Observatory

Observing floor and vertical gear, Lick Observatory. Photo credit: JR.

The floor of the observatory, which was finished with mahogany and ringed with brass railings, was designed to move up and down along a vertical system of spur gears. This cleverness allowed observers to stand on a solid surface while looking through the eyepiece of the telescope, rather than on top of a ladder as was customary with large instruments.

Looking East to Shane 3-meter Reflector, Lick Observatory.

Looking East to Shane 3-meter Reflector, Lick Observatory. Photo credit: JR.

In addition to the guide-led program in the Main Building, there is also a small viewing gallery open to the public in the dome of the Shane 3-meter Reflector. I thought the gallery was under-used, in that the interpretive materials were limited, and public view of the instrument was partially blocked by unidentified objects. The most interesting part of the display was the absolutely ancient black-and-white publicity movie that talked about the early history of the instrument. The corners on Mt. Hamilton Road are so tight that they had to use a relay system to get the 120″ glass for the mirror to its destination, using a crane to transfer the glass from the bed of the truck approaching the corner to the truck waiting on the other side of the corner. You can see below that many of the corners are more than just simple switchbacks, they actually start to double-back on themselves.

Approach to Lick Observatory.

Approach to Lick Observatory, Mt. Hamilton Road. Photo credit: JR.

As an architectural historian, I thought the public program was fascinating; I stood through it twice, in fact. As I was wandering around the larger complex, however, I couldn’t help but wish that public programs spent more time explicating current research and observing practices. I suppose it’s not very practical to demonstrate the Automated Planet Finder or the Katzman Automatic Imaging Telescope; most observational data is crunched with computers manned by tired postdocs. (Take a look at a panoramic view of the control room for the Shane 3-meter during an observing run, for instance. Not enough drama for tourists, I’m pretty sure.) But sometimes I wonder if programs focused on the historical leave the public with the feeling that little has changed in instrumental astronomy in the last century, or if it has, that those changes aren’t important or comprehensible. There are at least ten domes at Lick Observatory and new instruments are being added or adapted on a regular basis. I think if the University of California is depending on public dollars to fund the research at the observatory, it might be good to put more information about current research in visitors’ hands. I enjoyed the slide displays of recent discoveries and accomplishments that lined the halls of the Main Building, but I think it would be more effective to have some of those research goals articulated by the guide during public presentations.

Just a side note: if you’re driving up to Lick Observatory from San Jose, be careful. This is a very popular training route for cyclists (in fact, the Amgen Tour of California passed through the day before I went up), so don’t whip around those blind curves—it’s not nice to run over cyclists with your car.





Wallpaper Wednesday

18 05 2011

Atacama Large Millimeter/submillimeter Array (ALMA) antennae

Atacama Large Millimeter/submillimeter Array (ALMA) antennae. Photo credit: ESO/José Francisco Salgado.


Today’s wallpaper comes to us courtesy of the European Southern Observatory (ESO) in Chile.  What you see are four antennae completed as part of the Atacama Large Millimeter/submillimeter Array (ALMA). ESO and its international partners are in the process of constructing sixty-six of these antennae, all tuned to observe cold-body radiation with wavelengths of a millimeter or less. Radiation with such short wavelengths comes mostly from cold gas and dust clouds, in which stars are being born, or from early, cooling galaxies. Astronomers hope that the information gathered from these cold objects will bring us one step closer to understanding the origins of the universe.

ESO has provided a four-minute “trailer” about the project, available in multiple formats (HD always recommended if your system can handle it) in the video archive. Look for the brief glimpses of the construction equipment.








Observatories and Instruments