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Alvan Clark 36” Refractor (Lick Observatory) Review


This is the third of my (slightly cheeky) reviews of world-famous telescopes and the experience of visiting and using them (I have also reviewed the 60” Hale Reflector at Mount Wilson and the 24” Clark refractor at Mars Hill).

The Lick 36” is one of a number of giant achromatic refracting telescopes built for (essentially visual) professional use in the late nineteenth century, many of them by the firm of Alvan Clark in Massachusetts. Most of the big refractors were a size down from this one, though, at 20-25” aperture. In fact, the 36” at Lick is the second largest operational refractor ever made for general astronomy and is the largest still in use. The largest of them all – another Clark product, the 40” at Yerkes in Wisconsin – sadly ceased operations in 2018 and may never see starlight again.

One thing is certain, no astronomical lenses of this size will be made in future: not enough aperture for the pro’s; too big and expensive for amateurs. That makes the 36” ‘Great Refractor’, at Lick Observatory on Mount Hamilton above San Jose in California, a singular experience for an observer today (as well as a unique piece of history).

James Lick stipulated that the Great Refractor should be made available for public viewing sessions and it always has been. These days, the sessions are generally scheduled as an encore to other events, such as ‘Summer Series’ concerts. Such truly public open evenings sell out quickly and I wanted a more astronomy-centred experience, so I booked on an observatory tour and viewing evening for ‘Friends of Lick Observatory’ members. The tour was very in-depth and will get its own article. Here I want to concentrate on the viewing session with the 36” refractor which started in early evening and went on until past Midnight.

Private viewing? Oh yes, that’s possible. But the costs (at Lick effectively via a hefty donation) are even higher than at other similar observatories like Mount Wilson and Lowell (and so beyond my budget, sadly).

The 36” refractor at Lick is second only to this, the 40” at Yerkes (sadly no longer operational, here pictured when I visited Yerkes in 2009).


Unlike other founders and funders of great 19th C. observatories like George Ellery Hale, James Lick had no particular interest in astronomy. Rather he was looking for a grand way to memorialise himself. Lick had bought up big chunks of San Francisco after the Gold Rush, so his first thought was to build himself a giant pyramid there – you know like the ones in Egypt, only bigger obviously – in downtown at Fourth and Market.

Fortunately for the residents of San Francisco, Lick had a cultured friend who owned a 6” Clark refractor and regularly went into the local hills to observe. That friend suggested Lick build an observatory instead of a pyramid, which Lick did.

In the event, James Lick died a decade before the observatory was finished, but his involvement didn’t end there. For James Lick was later exhumed and buried at the observatory (he’d built the place instead of a pyramid mausoleum, remember) and not just somewhere in the grounds as you might expect. No, James Lick was re-interred in the black-brick pier base for the Great Refractor and there he remains. His tomb is marked by a plaque just out of sight beneath the observing floor and accessed by a narrow stairwell at the side of the dome.

The era of great refractors lasted less than a century. In 1824, the newly arrived 9” refractor at Dorpat was the largest in the world and just a couple of inches larger than my own refractor today. Just seventy years later came the 40” at Yerkes, the largest refractor ever mounted for astronomy (a bigger refractor was constructed for the Paris Exhibition, but never used). By the early 20th C., reflectors like the 60” at Mount Wilson had made the big lens telescopes obsolete.

The history of the Lick 36” refractor starts in 1880, when the glass blanks arrived from Paris, France by ship and were ground into the lens elements by the Alvan Clark works in Massachusetts. The finished lenses were transported to the west coast by train (sorry, railroad), then up the mountain by horse and cart, to arrive onsite in 1886. The long delay was because one of the lenses broke on the journey and it took many attempts to grind another.

Lick observatory was the first to be built on a mountain-top (at 4200 ft on Mount Hamilton) and an interesting piece of trivia concerns that twenty mile road up to it. I had never driven anything like it. Gruelling hairpin after hairpin that lurch dizzyingly this way and that but hardly seem to climb at all. The reason is that the road was built with a maximum 6% grade for pack animals and carts to lug components for the 36” up the mountain. For me, getting up it in the late afternoon sunshine was tough; getting back down in the pitch dark after midnight was truly horrible.

At first light in 1888, the Lick 36” refractor became the most powerful telescope in the world and would remain so for some years. Much of its early success was in the field of planetary science. James Keeler discovered the Encke Gap (named by Keeler in honour of Johann Encke) in Saturn’s rings with the 36” in 1888. Later, Edward Emerson Barnard discovered Amalthea, Jupiter’s fifth Moon and the first discovered since Galileo, with it in September 1892. Early spectroscopic work (by William Huggins) with the 36” established the paucity of the Martian atmosphere and the absence of significant water vapour. At the Mars opposition of 1892, the same E. E. Barnard observed Mars and failed to see the canals that four of his Lick colleagues believed they had seen with the 36” refractor. Barnard’s Mars observations – he was renowned as a peerless observer - were an early source of doubt about Lowell’s Martian canals.

Other seminal work by the 36” refractor included the discovery of some 25 comets, along with numerous double stars and spiral nebulae.

Lick’s tomb – in the pier base for the 36”!

Lots of visitors to Lick come for the sunsets and the stars.

At A Glance


36” Clark Refractor


Air-spaced Fraunhofer doublet achromat


36” (914.4 mm)

Focal Length

57 ft (17373.6 mm)

Focal Ratio



57 ft


c. 11,000 kg (OTA)


Design and Build


The optics for the Lick 36” refractor were (like most large US refractors of the time) ground by the famous optician Alvan Graham Clark, using blanks cast in France. The design is a conventional Fraunhofer achromatic doublet, in which the bi-convex crown element is in front, the concave flint behind. Like other Clark designs, the objective incorporates a large air gap between the elements. This design allows access for cleaning, but can also can give more freedom in correcting aberrations.

The exterior of the Lick dome looks outsized. Inside, the reason is clear – this is one very long telescope, even by the standards of big refractors. The reason is that the Lick 36” has a focal length of 57 ft to give a focal ratio of F19, longer than many big refractors of that era and most large achromats today. In contrast, the 24” Clark at Lowell Observatory on Mars Hill at Flagstaff has a focal ratio of F16.

The reason for this long focal length is to reduce the problematic false colour and spherochromatism (change of focus point with wavelength) that affects all achromatic doublets, but especially big ones. A 19th C. paper on the chromatic aberration of the Lick 36” suggests that this approach was largely successful. The author of the paper measured the deviation of focal point for different colours to be no more than another large refractor that had undergone similar testing, the F15 27” Imperial Refractor in Vienna. Even so, the spherochromatism was on a gigantic scale compared to amateur telescopes – several inches, apparently. This was so pronounced, the paper claims, that Wolf-Rayet stars, which emit mostly in two distinct wavelengths, can be identified purely from having two discrete and widely separated best focal points.

Storage box for the 36” Clark objective.

This historic image (hanging in the Lick Observatory lobby) shows the 36” as it once was, with a giant brass visual back.


The tube of the 36” Clark is in three sections. The short middle section that attaches to the mount is a massive casting. The front and rear tubes are made up of riveted steel bands and give it that ‘ship’s-hull’ Steampunk look so typical of big Victorian refractors If slightly less so than the earlier Lowell refractor which is made of individual plates riveted together).

The steel and brass of the Lowell 24” I visited a couple of years ago have been beautifully ‘restored’ with a glossy enamel finish. The Lick refractor retains a more workmanlike and original flat grey painted finish.


As you can see from the historical photo above, the 36” OTA once terminated in a giant visual back made of brass with a threaded port for mounting various instruments. Nowadays, this has been blanked off and fitted with a very ordinary 2” focuser, just like the ones fitted to many fast-food backyard scopes.

With the 55mm eyepiece and a diagonal fitted, the focuser was almost fully racked in, suggesting that it may not accommodate a wide range of eyepieces and magnifications (55mm being about the longest focal length and so lowest magnification you can get in a 2” eyepiece).


The 36” Clark has a huge German equatorial mount, like other big Clark refractors. The mount sits on a tall pier constructed of four cast iron segments and accessed by a spiral staircase at the back. A plaque on the pier states it was designed and built by Warner & Swasey of Cleveland, Ohio.

Pointing the telescope in the modern era was assisted by eight illuminated Selsyn dials above the eyepiece (four each for Dec and R.A.), but these apparently no longer work accurately. During my session, the telescope was pointed manually by the two operators: one at the finder, the other operating the mount by hand from high atop the pier and equipped with a hard-hat and safety harness (essential in the darkness of an observing session).

The colossal length of the 36” Lick refractor means that the eyepiece height changes a lot between target objects at different altitudes. This was originally accommodated by a movable observing floor, with a range of some 5 metres, supported on a massive radial fan of cast girders, operated by hydraulic presses and a system of ratchets to keep the huge circular parquet floor level. Sadly, the system has fallen into disrepair and many of the ratchets have teeth missing. This means an extremely tall step ladder is used for viewing, one of several available. Even so, objects at low altitude (which in 2019 means all the planets) end up with the eyepiece high above the steps and unreachable.


On the evening I was there, they only used a 55mm Tele Vue Plössl in the 36” Clark, an eyepiece that seems a favourite at observatories with classic, long-focal-length instruments. In this case, that 55mm Plössl gives a magnification of 316x and the widest possible field given the 2” focuser (no huge bespoke eyepieces like the ones I used at Mount Wilson here). That maximum-possible field is just 0.15 degrees!

The 36” Clark has a single 6” finder/guide scope, also by Alvan Clark. The finder retains its original brass focuser.

The Clark was at various times fitted with professional instrumentation, including an early spectrograph; but it is now (almost) solely used for visual outreach.


The dome is a brick base, lined with wood and supporting a lattice of girders clad in plates. It’s a more sophisticated thing than Lowell Observatories ‘upturned wooden pale’, but without the neoclassical grandeur of Yerkes. The dome has a narrow balcony running around it (with a rather flimsy and low railing). Steps at one side lead into the basement which houses the mechanism for the movable floor, various bits of equipment (including a storage/transport box for the 36” lens); and, of course, James Lick himself!

Underneath the observing floor; Lick’s tomb is just out of sight to the right.

The 36” at Lick is a giant among refractors.

Operating the telescope these days requires a hard hat and harness.

In Use – Astrophotography

The 36” Clark has been used extensively for astrophotography in the past. I had no opportunity to try photography through the Clark.

In Use – The Night Sky

General Observing Notes

My visit to Lick was straight after returning from Hawaii and the seeing at Lick, whilst good, was not as good Mauna Kea’s. For that matter, it didn’t seem to me as good as the outstanding seeing on Mount Wilson a few years back, but obviously individual nights vary.

Whilst some violet blur was evident on the double star we viewed, we didn’t view anything really bright like a planet or the Moon (see below). The professional astronomer helping on the tour said that on a night some years before, when he had viewed the planets, false colour had been a problem and the Great Refractor had been stopped down in the way the 24” is at Lowell Observatory.

The observing session was long and you might wonder at so few targets. Part of the explanation is that this was a group session, with short queues for the eyepiece, but mainly it was because the scope took a long time to point by hand, with one operator at the eyepiece of the 6” Clark finder and the other high up on the pier in his safety harness in the dark, working the mount clamps and controls with the giant setting circles. Even so, all the targets we viewed were in the same small region of sky.

All of our viewing was with a TeleVue 55mm Plossl giving 316x.

What’s it like?

The sheer experience of using it isn’t something I generally discuss with telescopes, but this is different.

First there is the dome. The interior is cavernous, echoey and dimly lit, even with the white lights on. The circular walls are lined with dark planks and the dome rafters – a network of steel beams supporting the external plates – arch high overhead. The floor is of concentric rings of polished parquet, picked out in light and dark woods. The 57-foot-long telescope virtually fills the space, the objective extending almost to the dome slit, which is open and showing stars.

Getting to the eyepiece involves climbing fifteen rungs up a step ladder. It feels secure enough and is edged with lights to help see the steps, but ends up at a surprising height. Some folks need a bit of help and encouragement to get up there. Looking into the eyepiece then involves stooping below a big wooden capstan wheel and the ring of switches that surrounds the visual back.

For the first target, a double star, they kept the white lights on. Thereafter, it was just dim red lights and the dome became very dark indeed, so that climbing those tall steps seemed a bit more daunting for some.

The Lick’s modest altitude and the balmy California summer meant it never got really cold in the 36” dome, but I did have to don a jacket towards midnight.

Deep Sky

Gamma Virginis (Porrima) was our first target.

The two stars of Porrima – one blue, the other orange – look a bit like Albireo through your scope (or mine). Except that Albireo has a separation of 35”, whereas Porrima just 2.9” – challenging if you don’t happen to have a 36” of aperture and the seeing from a California mountaintop.

The split was excellent and effortless, a yawning black chasm between the two stars. The blue star did show some violet blur due to chromatic aberration through the giant achromatic lens and some atmospheric disturbance (contrast the almost unnaturally still seeing at Mauna Kea a few nights before).


This spectacular, tight globular cluster, is also in Coma Berenices. A condensed mass of stars, surprisingly bright and resolved to the very core and with the outer ones approaching the field stop (in a 55mm eyepiece!), plus a stunning burst of brighter stars scattered across it like a firework– wow!


This famous double galaxy has pin-wheel spiral arms and a smaller companion galaxy. The spiral arms and possibly some individual stars were clearly visible through the 36”, plus the companion galaxy.

Note: one of the operators recounted that following his training they had left him alone with the 36” for a whole night. What did he do? Just moved from galaxy to stunning galaxy, he said, looking for supernovae and revelling in the view. It had been an unforgettable observing experience, but a spooky one. Apparently, the scope and mount creak and groan and unknown creatures scurry about in the darkness outside. Then, of course, there is the eternal presence of James Lick himself.

Simulation of M53 in the <0.2° field of the 36” refractor with a 55mm Plossl eyepiece.

Simulation of M51 in the <0.2° field of the 36” refractor with a 55mm Plossl eyepiece.


Jupiter was the only planet up, at an altitude of about twenty degrees. Given the 36” refractor’s discovery of Amalthea, I hoped some fine Jovian views might be in order. It wasn’t to be. Because the moveable observing floor is out of service, none of the planets will be high enough to view from the 36” for at least the next four years (i.e. until at least 2023). Hopefully I will go back thereafter and report.

A professional astronomer who was there to help out told me that he had viewed the planets some years before. They were an impressive sight through the 36”, he said, with lots of detail and high magnifications possible, but also lots of chromatic aberration.

We can get a more specific idea of how the 36” might perform on the planets from the following passage, taken from the book ‘Is Mars Habitable?’ by the distinguished evolutionary biologist (and the first astrobiologist) Alfred Russel Wallace when discussing the nature of the Martian ‘seas’:

Professor Barnard, with the Lick thirty-six inch telescope, discerned an astonishing wealth of detail on the surface of Mars, so intricate, minute, and abundant, that it baffled all attempts to delineate it; and these peculiarities were seen upon the supposed seas as well as on the land-surfaces.

Viewing with the Great Refractor involves quite a climb!


As a physical presence and a historic instrument (the largest operational refractor in the world and seriously huge), the 36” is a unique and wonderful thing to visit and experience. No other operational refractor and dome come close to this scale. It is a physically much more impressive instrument than even the 24” at Lowell (although it can’t match its restored lacquer-and-brass elegance).

The Lick operators were spot-on too: highly professional and knowledgeable, as well as super-friendly and helpful (compare the rather rude interns at Lowell a few years ago).

However, if you want the best possible experience of viewing through a big Clark refractor, the 24” at Lowell may ultimately be more satisfying. Why? Not only is it newly-restored to a very high standard, but it is also much faster to set onto new targets, so in a typical observing session you’ll see more. Also, the Lowell refractor can easily be set onto the planets, which for now the Lick Great Refractor cannot.

Then again, if stunning views through the telescope are your only priority, the Mount Wilson 60” Cassegrain reflector is incomparably superior to either. It perhaps doesn’t have quite the wow factor and romance of a great Victorian-era refractor, like the Lick 36”, though.

With its slow-to-use manual mount and out of alignment Selsyns (and perhaps a lens needing a good clean), the Lick 36” could benefit from some restoration work, which I really hope it one day gets. I would love to view a bigger range of objects with a wider range of magnifications, but that will need to wait for those repairs and maybe a better focuser too.

Despite some limitations, a night of viewing with the 36” Great Refractor at Lick is a wonderful experience and a bit of a ‘must do’ for anyone with an interest in visual astronomy and/or history of science. But for an expensive private viewing session, I’d choose Mount Wilson, or even Lowell Observatory, instead.