A Visit to McDonald Observatory
Most of the US observatories I visit
are historic sites that have seen their heyday in terms of professional
discoveries or, like Lowell, have moved their real science offsite somewhere
darker and more remote. McDonald in remote west Texas is different. It is still
a major research hub, with one of the world’s very largest optical
telescopes and new observatories still springing up on site. Somewhere like
Lick in California is all but deserted much of the time, but by contrast
McDonald is a thriving small community with all its own amenities (and even its
own water, sewage and power provision).
Also unlike most observatories in the
continental US, McDonald does still have really dark skies. Apparently, light
pollution has increased a bit in recent years, not from towns but rather from
drilling rigs out in the Permian Basin oilfields (another good reason to ditch
fossil fuels then). To me the skies still looked stunningly dark.
The main reason to go to McDonald as
a tourist though is that they have a really comprehensive and varied outreach
program. In this article I’ll tell you what the major outreach events are
and what they’re like. The only caveat being that you will need to plan
ahead and book onto programs well in advance: even as remote as it is,
McDonald’s viewing nights in particular get quickly sold out.
History
McDonald observatory started as a
collaboration between the University of Chicago, who already had a prestigious
astronomy department but wanted to expand beyond their light-polluted
observatory at Yerkes, and the University of Texas who didn’t have an
astronomy program. A wealthy Texas businessman and amateur astronomer named William
J. McDonald thought Texas ought to have a premier observatory and left the
thick end of a million dollars in his will to achieve it.
The observatory was founded on 23rd
November 1932 and within a year work had begin on the
82” reflector that would be the second largest in the world when it was
completed in 1938 and would (thirty years later) be named after the observatory
first Russian-born director, Otto Struve.
A number of major discoveries were
made with the 82” within a decade of its inauguration (see below for
details), most by the famous astronomer and early planetary scientist Gerard
Kuiper.
Much later, in the 1960s, after the
University of Chicago had pulled out, director Harlan J. Smith instigated a
renaissance at the aging facility by partnering with NASA to be build a huge
new instrument, the 107” which now bears his name.
Road from Fort Davis up to McDonald
Observatory.
Getting There
Texas is a big state. You knew that.
But driving to McDonald is a good way to really get it: wherever you
come from the drive will be a long one. Drive? Probably, because remote as
McDonald is, you’ll struggle with public transport.
McDonald is easily accessible from Highway 118 in west Texas,
either from I-10 in the north or from the small town of Fort Davis in the
south. But unlike many of the older observatories I’ve visited, it is a
long way from anywhere else, like much in west Texas. So you’ll be
needing somewhere to stay – this won’t be a day trip.
Fort Davis is 15 miles and 25 minutes’ drive from the
observatory, but it really is a tiny sleepy place, with no chain motels and not
even a McDonalds (!) If you want a standard small US town, then Marfa is 37
miles.
In the other direction, there is Van Horn – it’s
much further off at 74 miles distant, but half of that is on I-10 and
it’s certainly much easier to get to if you’re flying in (likely to
El Paso, the nearest city).
My pick, though, would be Alpine, just a couple of miles
further away than Marfa. Admittedly, Alpine isn’t very alpine, but it
seems a much more quirky and interesting place. It has the usual facilities
– motels, shops and food - but a walkable downtown with historic
buildings and a lively arts scene too.
If you want to combine a day (or two
– might as well do it properly if you’ve travelled a long way) at
McDonald with other attractions, the obvious ones are Guadalupe Mountains
National Park to the north and Big Bend to the south (though much of
what’s worth seeing at Big Bend is a long way off). More offbeat things
of interest include the Marfa Lights viewing station between Marfa and Alpine
and Blue Origin’s secretive rocket testing facility north of Van Horn.
I you need a walk after your long
drive, there is a state park on the Fort Davis side and a wildlife hike between
the observatory and I-10 on the other.
Be careful driving Highway 118.
It’s scenic and fast (esp. from the north), but packed with wildlife. I
saw deer, raptors, hogs and a Great Grey Owl; all actually on the tarmac.
What to see
The Frank Bash Visitor Centre
The VC is new and large, with restrooms,
a café and terrace, the usual gift shop selling T-shirts and small
scopes and a big movie theatre where they show interpretive films but also
conduct remote solar viewing sessions. The VC is the most accessible part of
the observatory from Highway 118 (from either side) and has plenty of parking.
Facilities close at about 5:30 pm,
but you’ll find yourself waiting around outside for the bus up to the
domes if you’ve booked on a Special Viewing Night (see below). In the
evening you might see some wildlife, including a herd of small wild hogs,
whilst you wait.
Hobby Eberly Telescope
Looking up from the VC, the
odd-looking silver dome on the peak to the left is the Hobby Eberly Telescope.
You can visit on a tour from the VC or drive yourself up during the day and
park outside. The dome has a large foyer area with its own interpretive
displays and video feeds explaining the telescope and its work. The displays
are really worth perusing, but you’ll immediately be drawn to the
telescope itself – visible through a big window at the back. To
understand what you’re seeing, though, you’ll probably have to head
back to the displays after all!
The HET is McDonald’s premier
research tool. As I write it’s still tied for second place in the list of
largest optical telescopes worldwide at 10m (shared with the Keck twins on
Hawaii). It is a very different beast from Keck though and interesting for it.
The thing about the HET is that it
was designed to be cheap, radically so at around 20 million (though it’s
current upgrade will cost twice that). In order to achieve that super-low (for
a big research telescope) figure, the HET has a unique design and looks …
well, not much like a telescope at all.
Unique? How? For a start, even the
dome looks unusual, because it is really a radar dome with a slit chopped out.
The telescope itself cannot move in altitude, it’s fixed at an elevation
of 55 degrees, only in azimuth. This radical design makes it much smaller and
spindlier and less telescope-like than other big instruments. This sounds like
a huge limitation, but the HET can cover about 80% of the sky because as the
Earth spins and moves around its orbit, various target objects drift into view
at different times.
The HET has other distinctive design
features too. Its mirror is made of thin segments aligned by
computer-controlled actuators, like the Kecks’. But the HET has many more
segments: 91 in place of the Kecks’ 36 each.
Even the instruments are unusual. The
HET dispenses with a secondary mirror and the usual Cassegrain and Coudé foci by having that main mirror focus its
light onto a giant array of fibre optic cables in a special assembly at the
prime focus. Those cables then feed not one, but numerous spectrographs that
give the telescope a low-resolution but ultra-wide field of view and some
special capabilities.
The HET has an odd way of tracking
objects as the Earth turns, too. Instead of having the mount moving like usual,
those fibre optics feeds and a corrector lens are contained withing an 11 ton
moving ‘tracker’ that moves to counter the Earth’s spin.
As I hinted before, the HET is
undergoing a major upgrade for a new study into Dark Energy, for which its
ability to look at the spectra of numerous objects simultaneously is a big
advantage.
HET Dome and foyer with window onto
the telescope.
Hobby-Eberly Telescope: bottom to top
- mirror support (turquoise), primary mirror, detector arrays, tracker
secondary assembly.
The 82” Otto Struve Telescope
The Struve telescope was built between
1933 and 1938 and made some famous observations and discoveries. In 1944 Gerard
P. Kuiper discovered that Saturn’s moon Titan has methane in its
atmosphere. Continuing his solar system observations, Kuiper went on to
discover moons Miranda (of Uranus) and Nereid (of Neptune), also with the
82”.
The 82” has a distinctive
appearance, with a semi-closed tube with wire-braced trusses and a huge yoke
mount, all in dark grey. The McDonald website calls it a work of art and in a
way it really is.
The 82” dome is unusual too.
Unlike most observatories it is a proper building with lots of windows in the
lower stories. That’s because, as the McDonald themselves puts it, the
dome ‘housed all of McDonald’ – those windows open onto rooms
that now serve as offices and a library, but once housed living quarters for
resident astronomers Is it me or is that really romantic – living below a
giant telescope; when can I move in?
Unlike the 107”, the 82”
is a Classical Cassegrain (not a Ritchey-Chrétien), which means it has a
long focal length and is ideal for visual use (for which it was originally
intended – astronomers still did much work visually in the 1930s). Gerard
Kuiper (one of the first ‘modern’ planetary scientists) observed
Mars with the 82” in 1956 and recorded seeing no sign of canals, perhaps
the final nail in the coffin for Lowell’s Martian fantasies.
If you do the daytime tour,
you’ll park just below the dome for the 82”, so you will be able to
go and have a look at it on your way to the 107”. Unfortunately, though,
the 82” telescope isn’t open to the public except on Special
Viewing Nights (see below).
The 82” dome: astronomers once
lived, as well as worked, behind those windows. I always dreamed of living in
an observatory among the pines!
The Otto Struve 82” Classical
Cassegrain, equipped with a focuser for a Special Viewing Night.
The 107” Harlan J. Smith
Telescope
The 107” was built between 1964
and 1968, following a request by NASA to use the 82”. NASA wanted to survey
the Moon and planets before sending space probes to them. But the Director of
McDonald at that time, one Harlan J. Smith, told NASA this wouldn’t work
because the 82” was already heavily booked up by astronomers. Smith
proposed that NASA fund half the budget to build a new telescope instead. It
was a ballsy move, but it paid off and Smith got his big new research
instrument, still doing science long after NASA lost interest, probably just as
he planned.
The 107” is a
Ritchey-Chrétien with an F8.8 focal ratio, but it can also employ Coudé and Cassegrain foci by swapping out the
secondary mirror cage. The mounting is a giant equatorial cross-axis yoke
mount, much like the 82”, but with a really huge counterweight. The tube,
as you can see, is unusual (for such a large instrument) in being enclosed.
Another unusual feature of the
107” is the system of weighs and pendula around the visual back. These
are an ingenious and purely mechanical system for cancelling the distortion
suffered by the mirror at different orientations (where a modern telescope
might have computer-controlled pistons).
A visit to the dome on the tour
includes one lucky member of the group getting to press a button and slew the 190
ton telescope and move the 220 ton dome, also of raising the observing floor. Even
if that person isn’t you, the 107” is an impressive sight and well
worth the trouble.
You might get to ride up to the
observing floor in the lift, which is a proper big one like in an office block.
Oddly, the lift misses a floor, because that floor is where the spectrograph
and other sensitive instrumentation is housed and is off limits.
The Smith telescope continues to do
research work and I was lucky enough to see it fitted out with McDonald’s
VIRUS-W spectrograph, that attaches to the side and gimbles so it always stays
vertical. The spectrograph is able to take up to 267 spectra simultaneously via
fibre optical cables which makes it ideal for studying the stellar velocity
variation within a galaxy (which is exactly what the astronomer working that
night would have been doing if the clouds hadn’t closed in!)
A reminder that the 107” also
has a foot in the past is the presence of an optical guide scope and (really) a
Telrad red-dot finder! Our guide said the Telrad is a joke, but a someone has gone to a lot of effort
to attach it properly if so.
Another interesting piece of trivia
about the 107” (and the 82”) is the unusual way they clean the
mirror. Every few weeks, they lay the scope flat and someone walks down it.
They then spray liquid carbon dioxide from a bottle at the mirror. The CO2
falls on the mirror is snow, sweeping away dirt and dust without leaving traces
(the snow sublimated soon after).
Outreach guide explains the
107” Harlan J. Smith Telescope on the day tour.
Other telescopes
Right by the visitor centre is a
large white radio telescope dish that was brand new when I went. This is a 12m
antenna owned by NASA and is part of their Space Geodesy Project (SGP),
specifically part of the Very Long Baseline Interferometer (VLBI).
SGP has also recently completed a
satellite laser rangefinder in a small dome on Mt Fowlkes near the HET.
What’s SGP? It’s all about measuring the Earth’s precise
shape, gravity and rotation and establishing a Terrestrial Reference Frame
(TRF). This is essential to all sorts of science and technology, including oceanography,
climate change, geohazards research and tracking interplanetary spacecraft.
McDonald hosts lots of other smaller
instruments, including a 0.8m made from the glass trepanned from the 107”
mirror and a 0.9m (36”) that is regularly available for viewing nights
(again, see below).
NASA SGP VLBI Dish at McDonald, with
HET dome above and left.
First off, take binoculars! For the dark skies, but for perusing the many
domes of the observatory and for wildlife viewing too.
Just turning up to the observatory and enjoying its scenic location,
having a coffee on the terrace, nosing about the gift shop and checking out all
the domes and dishes, is a pleasurable way to spend a few hours. But McDonald
has one of the best outreach programs of any major observatory and as I noted
at the start, you’ll need to book well in advance to make the most of it.
Enjoying McDonald’s dark skies with binoculars, outside the
36” observatory.
Daytime (obvs) Solar Viewing
The visitor centre has several small observatories clustered around it
and one of these houses a pair of solar telescopes, one with a Herschel wedge
for white light viewing of sunspots and granulation, the other with a special
filter that reveals the chromosphere for filaments and prominences. But
don’t expect to look through an eyepiece, because all the solar viewing
is done remotely via video cameras.
You’ll watch the show in the movie theatre, with the sun projected
live onto a big screen via a computer. The live feed from the telescopes is
accompanied by an interpretive talk that covers a lot of interesting stuff
about the Sun and its cycles, as well as explaining the views you’re
getting through the telescopes.
It was an interesting show and projecting the solar images enables a much
larger audience to view in comfort. Personally, I missed looking through an
eyepiece though.
Tour
You can book onto an afternoon tour which lasts several hours and takes
you up onto Mount Locke for a visit to the 107” Harlan J. Smith telescope
and then Mount Fowlkes for the Hobby Eberly Telescope. People with walking
difficulties or disabilities can take a small bus; the rest drive themselves
up.
The tour isn’t strictly necessary for the HET, which has an
interpretive area you can access independently. However, it is the only way
you’ll get into the 107” observatory apart from on a viewing night,
to see the telescope from the observing floor and watch it and the dome being
moved around.
The tour I took was excellent, the guide friendly helpful and
knowledgeable. I’m not a big fan of tours in general, but this one is
well worth it. However, note that if you were hoping to see the historically-important
82” Struve telescope you will be disappointed. You do get to see its
unusual dome close up because it’s right by the 107” dome, but the
telescope isn’t accessible, perhaps because of the long and narrow stairs
to get up to the observing floor.
Star Parties
The visitor centre hosts regular star parties, which look fun and should
be good given the dark skies, but I didn’t attend one during my visit as
my evenings at McDonald were taken up doing Special Viewing Nights (worth
noting that you can’t do both on the same night).
Special Viewing Nights
These events
– where you actually get to observe through a big professional telescope
- are currently available on three of McDonald’s instruments: the
36”, the 82” Otto Struve telescope and the 107” Harlan J.
Smith. These are some of the best such experiences available and at
ridiculously low prices (the most expensive, the 82”, was $125 at the
time of writing). However, be prepared for weather
problems. Two of my nights were clouded out and other visitors spoke of
blizzards and thick fog on previous attempts!
By far the
most desirable Special Viewing Night is the 82”. Not only is it the most
famous telescope of the three, but it was designed and configured specifically
for visual use (unlike the 107”) and is likely of much higher optical
quality than the 36”. I’m told it gives the best viewing experience
of any telescope, anywhere. Unfortunately, the 82” is still used for
research and only rarely available for viewing nights. My night on the
82” was frustratingly curtailed by the weather, but was enough to
convince me to make the trip again some day if I can.
Even so, I got to tour the dome, see and photograph the telescope and hear
about its history.
The
107” experience is very different, with more of the evening spent on
interpretation with a professional astronomer and just one or two objects
viewed at (I’m told) extreme high power, via an eyepiece in the control
room (you don’t get the experience of climbing a step ladder up to the
telescope itself to view). I ended up doing the interpretive part of the
107” Special Viewing Night – and very interesting it was, seeing
the scope and control room in operation and talking to the astronomer - but not
the actual viewing, again due to the weather.
The
36” Special Viewing Night is the cheapest, the most frequently available (because
it’s no longer much used for research, unlike the 82” and
107”) and probably covers the most objects due its swift goto slewing and pointing. I did it on a night of clear
dark skies and I can highly recommend it.
But
again, please do note that demand exceeds supply on these Special Viewing
Nights, so you will have to book early: don’t expect to just turn up and
view the way you can at Lowell, for example.
Summary
McDonald observatory is a must-do if
you have an interest in astronomy. I liked all the activities I took part in,
but a Special Viewing Night (especially, but not only, if it’s actually
clear) is the highlight. If you are a keen observer then a night on the
82” in particular should be on your bucket list, but the 36” was a
really excellent few hours of deep sky viewing and the 107” very
interesting in its own way too.
Dome of the 107” looms into a
starry sky at McDonald Observatory (spot the Pleiades, Andromeda Galaxy and
Double Cluster).