Alentejo Megaliths

9 08 2011
Évora Almendres Cromlech

Évora Almendres Stone Circle. Photo credit: Mick L

I’m moving offices, so I’ve been sorting through the stacks of paper that have failed to find a home in a file folder over the past two years. On top of my stack of archaeoastronomy articles was an analysis of the megalithic enclosures in the historical province of Alentejo in south-central Portugal.* I saved it because I thought it might be relevant to my dissertation (it wasn’t); I re-read it because I had been thinking about the distribution of megaliths across northern Europe while writing about Stonehenge knock-offs yesterday.

The Alentejo stretches south from the Tejo River to north of the Algarve (Faro District). The Évora district occupies the middle section of the Alentejo. Within the Évora district are twelve known stone enclosures built during the Middle Neolithic period (sixth to fifth millennia B.C.).  Most of the enclosures were built in a horseshoe shape, with openings oriented to the east. The smallest complex, Vale d’el Rei, has twelve menhirs in a simple horseshoe shape; the largest, Almendres, has 94, with a more complicated configuration.

Site Plan, Almendres. Image credit: Pedro Alvin

Site Plan, Almendres. Image credit: Pedro Alvin

A new archaeological survey was conducted of the twelve known sites, including both the location of the extant menhirs and their relationship to the larger landscape (distance to horizon profile, horizon marks, maximum slope, axis of symmetry).** The survey demonstrated that eight of the twelve sites had axes with orientations within a range of 35.4° of azimuth, in approximately the eastern direction. The research team concluded that the probability of this common orientation occurring by chance was very low (~7 x 10^-7), and there could only be two explanations for it:

“either an astronomical target (Sun, Moon, or planets, based on the possible declinations for 6000-5000 B .C.) or a construction following the slope, turned to the direction of the far horizon, since we verified a Pearson product-moment correlation coefficient of .7 between the azimuth of the symmetry axis and the azimuth of the steepest slope.” (p.7)

I’m not sure of what I think of this first conclusion. What about the 1/3 of the sites that didn’t exhibit this commonality? And what about Xarez, which was excluded from the study because of controversial excavations (see **, below), but may have had a different configuration that then twelve sites included the study? At any rate, this initial conclusion motivated the research team to further analyze their data to determine which of the two options was most probable.

Évora Almendres Cromlech.

Évora Almendres Stone Circle. Photo credit: Phillip Capper

The data crunching is impressive and I direct you to the published article to read the description of their probability models (I am not qualified to comment on the validity of Bayesian analysis in this case). Ultimately, the team discarded the possibility that the structures had been positioned in regard to slope. That left them with option two—the stones were arranged in response to an astronomical target. But which target?

It’s possible that the stones had a lunar association—the crescent symbol is engraved on several menhirs in Almendres, Pórtela de Mogos, and Vale Maria do Meio. Most of the engraved surfaces face the east, which could indicate a lunar orientation. On the other hand, it could also indicate a solar orientation, much like that exhibited by the dolmens (stone tombs) in the same region. The builders of the monuments were likely hunters-gatherers-farmers and may have needed the stones as a tool for telling time or marking the seasons. Or maybe not. The authors seemed to hedge their bets, which is common when writing about ancient architectures, but didn’t leave me feeling convinced of their conclusions.

That being said, the tables that accompanied the article are quite valuable. They include menhir statistics (size, location, position, decorations), enclosure statistics (latitude, azimuth of steepest slope, slope, symmetry axis aximuth, declination, horizon altitude), elevation profiles and horizon features of the sites in the study, and site plans for the Almendres, Vale Maria do Meio, Portela de Mogos, Tojal, Cuncos, Sideral, Fontainhas, and Val d’el Rei enclosures. You can also see site plans for many of the enclosures, drawn by Pedro Alvin, at http://www.crookscape.org/sitios.html (scroll to the bottom of the page).

Notes:

*Fernando Pimenta, Luís Tirapicos, and Andrew Smith. “A Bayesian Approach to the Orientations of Central Alentejo Megalithic Enclosures.” Archaeoastronomy 22 (2009): 1-20.

**The archaeological survey did not include the stone circle of Xarez, citing controversial excavation and reconstruction techniques as described in: Manuel Calado, Menires do Alentejo central. Genese e evoluçâo da paisagem Megalitica regional, Lisboa. 2004. Unpublished Ph.D. dissertation. University of Lisbon.





Stonehenge Revisited

8 08 2011
Stonehenge Aotearoa Stormy Sky

Stonehenge Aotearoa Stormy Sky. Photo credit: Chris Picking

True story: when I first visited the Stonehenge Memorial at the Maryhill Museum of Art in Washington State, I didn’t know it was an imitation. I usually attribute my ignorance to my age at the time and my upbringing in a rural area in the dark ages before the Internet, but even with those allowances, you’d think I would’ve learned at some point in grade school that Stonehenge was at Avebury on Salisbury Plain.* Luckily, I was smart enough to keep my mouth shut on the way to Maryhill, where the signage explained that the monument was a replica.

There are so many Stonehenge replicas in the world, some more accurate than other. Of the less accurate but more entertaining variety, Carhenge is probably the most famous. I’ve managed to drive through the State (uh, Official Commonwealth) of Virginia several times without ever stopping at Foamhenge. And, no, I wasn’t at Glastonbury in 2007 to see the construction of Banksy’s Loohenge.

More interesting to me are the models that attempt to establish some relationship between the architecture and astronomy. Although the sentiment behind the Maryhill Stonehenge was misplaced, as a structure, it is carefully designed and well-built, with the altar stone aligned with the sunrise at the summer solstice. Similarly, although Stonehenge Aotearoa was built at a similar scale to the structure at Salisbury, it was aligned for the southern skies. For example, the heel stones of the henge mark the rise and set points of the sun at the midsummer and midwinter solstices, and the autumn and spring equinoxes. In addition, a well-placed obelisk points to the celestial south pole, acting as an axis mundi for the night-time visitor. Specific to the Aotearoa site are stone representing the Pleiades, or the “Seven Sisters”. Maori refer to this group of stars as “Matariki” and use its position mark the beginning of a new year in late May/early June.  To the south-west of this group of stones stands a single marker stone indicating the location of Matariki’s rise.

So, I find the models that attempt to investigate/explain the links between astronomy and architecture more interesting than things like “Butterhenge” or “Peepshenge”. Most interesting of all, however, are the many “real” henges that I only learned about in heritage management courses in graduate school:  Woodhenge, Seahenge, the Ring o’ Brodgar, Stenness (Orkney); the Thornborough Henges, Yorkshire; the Mayburgh Henge, Cumbria; and many others. They intrigue me for the obvious reasons—what do they mean, who built them, how were they built—but as a historian with a research interest in cultural heritage studies, I also find them interesting test cases for public and state preservation policy. How do you approach the management of a wood henge that has been almost completely eroded by the sea? Who has the right to access the inner circle of Stonehenge? Can you copyright a neolithic stone structure?

*By the way, don’t listen to all those people who complain about Stonehenge being a tourist trap and a disappointment just because you can’t touch the stones or buy a decent cup of coffee at the site. Stonehenge is awesome, case closed.





Lunar Landing

7 08 2011
Apollo 11 Coaster, front

Apollo 11 Coaster, front

Yesterday, when I was poking around in the Habitat for Humanity ReStore, my partner chased me down and handed me a stack of ceramic coasters. At first I thought she had found a necessary item for our house, since I’ve all but ruined our oak coffee table by letting sweat from my cold glass drip on it, but no. She found something much more interesting—a set of souvenir coasters commemorating the Apollo 11 lunar landing. The graphic is awesomely vintage, with heavy strokes characteristic of graphic design aesthetic of the late 1960s-early 1970s. The astronaut’s boot looks as if it should be accompanied by the “Keep on truckin’!” banner.  The text separators depict (roughly) the four phases of the moon, and the text itself—heavily drop-shadowed—notes two significant events: the landing of the Apollo Lunar Module (LM), Eagle, and Neil Armstrong’s first test of the lunar surface with his foot.

Apollo 11 Coaster, back

Apollo 11 Coaster, back

The back of the coaster tells us that the set hasn’t traveled very far in the world. It was apparently a reward for a successful membership drive for the McKinley YMCA (now the Champaign County YMCA), and we picked it up just a few blocks away from the Y at the Champaign Restore. I like to think that the person who won the set thought they were too special to use, so she or he set them away in a safe place. Maybe they’ve been in that safe place for the last 43 years and they were donated to Habitat for Humanity during a massive cleaning-out project by the recipient’s offspring. Whoever let them go obviously didn’t value them too much, since we picked them up for two bucks, but you know what? They’re going back into a safe place because in this household, they’re too special to use.





First Light

3 08 2011

When the world’s greatest telescopes opened their eyes.





Wallpaper Wednesday

3 08 2011
Westerbork Synthesis Radio Telescope

Westerbork Synthesis Radio Telescope

Today’s lovely wallpaper (click on image to download) shows the Westerbork Synthesis Radio Telescope (WSRT), at the Netherlands Institute for Radio Astronomy (ASTRON), not the Onsala Space Observatory, as the linked page would have you believe. The Westerbork telescope works on the same interferometry principles that determine the design and use of other mobile arrays, such as the Very Large Array (VLA) at the National Radio Astronomy Observatory, the One-Mile Telescope at the Mullard Radio Astronomy Observatory (MRAO), and the Australia Telescope Compact Array at the Paul Wild Observatory. Although you can’t really tell from this photo, one thing that sets this array apart from most is that the telescopes have equatorial, rather than alt-azimuth, mounts.





Herschel Space Observatory

1 08 2011
Oxygen in Orion

Oxygen in Orion. Image credit: ESA/NASA/JPL-Caltech

Very cool:  the large telescope of the Herschel Space Observatory (formerly called Far Infrared and Sub-millimetre Telescope or FIRST) has detected oxygen molecules in the Orion nebula. The existence of oxygen in space makes sense, since it’s the third most common element in the universe. It’s taken something like 230 years for anyone to detect it, though.

The Herschel Space Observatory is one of those projects that demonstrates the benefits of international collaborative efforts. Herschel is a major mission for the European Space Agency, with several nations contributing to the design and build of the instruments and the spacecraft.* However, Herschel is also supported by NASA resources. NASA’s Herschel Project Office is based at JPL, a major contributor for two of the observatory’s three science instruments. JPL itself is a joint project of sorts, since Caltech manages it for NASA. International, multi-national cooperation at its most productive—they found oxygen, after all.

*By my reckoning, Austria, Belgium, Denmark, Finland, France, Germany, Ireland, Italy, Norway, Netherlands, Portugal, Spain, Sweden, Switzerland, the United Kingdom, and the United States all contributed during the industrial phase of the project.





Ed-U-Cards

31 07 2011

Let me take a minute or two to tell you why I was looking at Meteor Crater a few weeks ago. My motivation wasn’t linked specifically to observatories or instruments, but more to the historical ephemera of science and astronomy. But I’m a historian, so that’s okay.

Front of Card

Card No. 6, A Close-Up of the Craters

Back of Card

Card No. 6, reverse

This is Card No. 6 from the Ed-U-Cards of Astronomy published by Random House in the 1960s. Random House pretty much had the science and entertainment industries covered with these card collections. I’ve seen Ed-U-Cards of Science (Biology, Chemistry, Astronomy), Ed-U-Cards Baseball Card Game, Ed-U-Cards Book of Knowledge and Ed-U-Cards Quick Draw McGraw Card Game (which I totally want!). I happen to own the Astronomy set.

Cover

Box Cover

Considering they were written in the 1960s, they’re amazingly relevant. Okay, the card on the expanding universe doesn’t include new thinking about the moment of inflation or the competing theories on the expand/collapse of the universe. It did, however, include a description of the balloon experiment, which I found super useful as a youngster trying to understand the expansion of space.

Most of the cards have  useful activities for children: how to find Arcturus by using handle of the Big Dipper as a guide; how to recreate the phases of the moon with a ball in motion; how to draw a model of our solar system.

Sundial

Card No. 3: How to Make A Sundial

The front side of Card No. 3, Telling Time, provides a graphic for U.S. time zones (drawn before the State of Indiana really messed things up for its citizens) and a picture of a rough sundial.* On the reverse is a basic explanation of keeping solar time and instructions for making a sundial out of cardboard or wood.

Back of card

Card No. 3, reverse

The sundial won’t be accurate to the second, or even the minute, but as I found out while constructing a model astrolabe, while you can buy a sundial off the internet, you’ll learn more if you build the instrument yourself.

These cards are still available here and there. My word of caution: don’t buy them from the folks who are charging multiple dollars for a single card on E-bay. They are completely ripping you off.

*You can tell the photos are from the distant past because the kid’s wearing a wristwatch, not checking his smart phone for the time of day.

——————————–

ETA: the photos referred to in the comments section for this post, 29 Jan 2012:

Bottom edge of Astronomy ED-U-CARD box

First page of Astronomy ED-U-CARD pamphlet

Last page of Astronomy ED-U-CARD pamphlet





VLBA NRAO

29 07 2011
Radio Telescope

Radio Telescope. Very Large Baseline Array, Brewster, WA. Photo credit: JR

My flickr set for the Brewster terminus of the Very Large Baseline Array (VLBA) continues to grow. Follow the link for more photos of the radio telescope and its close neighbor, the U. S. Electrodynamics communications satellite station.





Wallpaper Wednesday

28 07 2011
VLBA

VLBA. Photo credit: Troy Mason

In honor of my recent visit to one end of the VLBA, I’m linking you to a beautiful photo of the VLBA telescope on Mauna Kea. Click on the image to access it in various sizes and to thank Troy Mason for making the image available through Creative Commons licensing.





VLBA NRAO

24 07 2011
Approach to VLBA

Approach to VLBA. Photo credit: JR

We started our summer vacation with a trip to the Very Large Baseline Array (VLBA), or I should say, one of the ten radio telescopes that comprise the VLBA. The powers that be at the National Radio Astronomy Observatory (NRAO) saw fit to place one of the dishes near Brewster, Washington, an act which positioned it directly on the path between the Spokane airport and my parents’ house.

Dish with reciever

Dish with receiver, VLBA, Brewster, WA. Photo credit: JR.

At the moment, the VLBA is the world’s largest dedicated telescope array with the sharpest resolution. The telescope spans 5,351 miles (8,611 km), with dishes located near Brewster; Owens Valley, CA; Pie Town, NM; Fort Davis, TX; Los Alamos, NM; North Liberty, IA; Hancock, NH; Mauna Kea, HI; Kitt Peak, AZ; and St. Croix, Virgin Islands. The ten telescopes—each with a reflecting dish, feed/antenna & receiver—are connected via transmission line and combine to form a massive interferometer with a spectacularly high resolution. All the dishes gather a radio signal from the same object at the same time. When the received signal from one telescope is superposed with the next, and so on, the ten single telescopes function as if they were one massive instrument with a baseline as large as the greatest distance between dishes.

Trusswork

Support trusses, Brewster VLBA. Photo credit: JR

Some telescope arrays, like the Very Large Array (VLA), can change the baseline length, and therefore the resolution of an image, by relocating individual telescopes along tracks. The ten telescopes of the VLBA are at fixed points; they rotate, but don’t move horizontally. However, they can be asked to work together with other radio telescopes (Arecibo, Effelsberg, NRAO’s Green Bank Telescope or the VLA) to perform as the High Sensitivity Array.

Antenna

Antenna, Very Large Baseline Array, Brewster. Photo credit: JR

If you’d like to watch the Brewster telescope “in action,” NRAO provides a real-time feed of the instrument (refreshes every five minutes).  They’ve also provided a fairly lucid explanation of radio astronomy and some kind of cool movies of black holes as observed by the VLBA. And, if you’re like me, and prefer to follow inanimate objects on twitter, you can follow the lives of the telescopes @TheNRAO. There are thirty-two more photos of the instrument on my flickr site, including several that can be strung together in a slide show to depict the slewing of the telescope .








Observatories and Instruments