Telescope Triplets
© Norman Sperling, November 25, 2011
For decades, I have been proclaiming that focal ratio is one of the most important characteristics in choosing a telescope. Most authorities tout aperture instead. But none of us has ever conducted a true visual test, isolating the variables of focal ratio, aperture, and eyepieces.
I propose that 3 triplets of Newtonian telescopes be made to demonstrate the effects of focal ratio, aperture, and eyepiece. They can be used for classes and at star parties to teach about the properties of the telescopes themselves. Mount each triplet so that viewers can easily shift among all 3 eyepieces to instantly compare views.
The "focal ratio" triplet should consist of 3 telescopes, all with the same aperture and eyepiece. Make one f/5, another f/10, and another f/20. For this triplet, I think 3-inch (76 mm) apertures are best: even the f/20 would be a manageable 5 feet (1.52 m) long. Users will see that Jupiter looks best at f/20, and the Great Andromeda Galaxy best at f/5. Trying this battery of telescopes on the sky's enormous variety of targets will probably reveal very few objects that look best at f/10.
A second application of this same telescope set will use different eyepieces that all result in the same magnification: a long eyepiece on the long scope, a short eyepieces on the short scope, and a middling eyepiece on the middling scope. How different are the views of different targets?
The "aperture" triplet should consist of 3 telescopes, all with the same focal length (perhaps 4 feet = 1.22 m) and eyepiece. Make one 3 inches (76 mm) aperture, the second 6 inches (152 mm), and the third 12 inches (304 mm). Users may be surprised how much even the 3-inch shows.
The "eyepiece" triplet should consist of 3 identical middling telescopes, perhaps 4-inch (102 mm) f/8. Insert eyepieces of equal focal length but different optical designs (such as Huygens versus orthoscopic versus Nagler). A second application of this same telescope array will use eyepieces of equal design but different focal lengths (perhaps Plossls of 6 mm, 12 mm, and 25 mm ...).
Make each triplet so the scopes, and their eyepieces, can also swivel to allow 2, or even 3, different people to watch through one of the scopes at a time. This is because, perhaps once a decade, some sky event brings out throngs, and the host needs to move a whole lot of eyeballs through the scopes in minimal time.
These triplets could be built by amateur-telescope-making workshops, such as several clubs run, or perhaps by a veteran scope-maker. Most are quite small, only one is large. Try hard to hold all but one factor constant so they really test that single variable.
A whole metropolitan area probably needs only one set. Telescope triplets can be passed around among nearby colleges, astronomy clubs, planetaria, etc., to use at their classes, star parties, and member-events.
Novice Astronomy Over 50 Years
© Norman Sperling, July 5, 2011
A presentation I saw on how to get into amateur astronomy showed how much has changed in the half-century since I began ... and how much hasn't. Amateurs from the Phoenix and San Jose areas explained the ins and outs to science fiction buffs at Westercon.
Stars, planets, and humans are still the same, so the principal advice is still to go somewhere dark (away from light pollution), and learn the constellations and how the sky moves. That advice is absolutely identical to what I was told in 1957, and it's right. They mentioned some recent and classic beginner books, as well as the latest 'pod apps. Light pollution is now a lot worse, so getting to a dark place is much more difficult, but the advice is the same.
The second advice is still to not dive into buying a big, complicated, expensive telescope. After the naked eye, use binoculars. After binoculars, a useful beginner telescope is now available for as little as $50 or $60. That price is relatively lower (considering inflation) than in my youth - an advantage of modern design and production. Then and now, beginners must be warned away from flimsy, incompetent, disappointing telescopes from non-specialist merchants.
They still recommend Sky & Telescope and Astronomy magazines. (OK, the latter was founded in 1973.) They still recommend finding your local astronomy club and star parties, and using red-light flashlights to preserve night vision.
They still recommend studying the richest and most informative telescope catalog – though that used to be Edmund's and now it's Orion's. The lust generated by seeing all the glorious equipment used to be called "aperture fever" and is now "Telescope Porn".
Modern optical and electronic technology has outmoded the old equipment, and enabled whole new categories of activities.
The Dobsonian Revolution made far larger telescopes affordable to serious amateurs, and they can observe deep sky objects spectacularly better than 50 years ago. Today's top Schmidt-Cassegrains, Maksutovs, and refractors deliver markedly better images than you could buy 50 years ago. Some astronomers love automatic object-finding telescopes because it's easier to observe what you want; purists consider it cheating if you don't point the telescope correctly yourself.
Electronic imaging has popularized incredible tools like webcams. Commercial mounts now mate phone-cameras to telescopes. Software now lets photographers stack multiple exposures using more skill and time than money. The best amateur astrophotography of 2011 far surpasses the best that the big professional observatories could do just 30 years ago. These tools enable amateurs to study, and make discoveries about, far fainter objects than before.
One aspect that hasn't changed is the mindset that "amateur astronomy" = observing. That wasn't true 50 years ago and it's less true today, but it's what springs to mind. Lots of non-observational aspects are wide open – history, education, tourism, and telescope making are just a few popular options. Data-mining now combs and analyzes enormous amounts of data, usually gathered by professionals. Anyone competent with a computer and an internet connection can do this. Some such projects are called "Citizen Science".
Overall, getting to a dark sky is markedly harder nowadays. Learning the sky and climbing above beginner status are about the same. But optical as well as electronic technology have improved spectacularly. Far greater viewing and computing power are affordable, and projects to use them multiply very fast. Nowadays the limiting factor isn't telescope size, or imaging skill, or computing talent, but the creativity to think up a new project. Go for it!
Astroscan Memories
© Norman Sperling, January 15, 2011
A recommendation by Sky & Telescope magazine last month, following a [.pdf] review last July, rekindled an old glow. The Astroscan telescope - my first big project - was once again named one of the 3 best inexpensive telescopes ... 34 years after it was introduced!
I remember its development clearly.
It was meant to be a superior first telescope, and it is. It has also proven to be a superior second telescope: folks keep it after they graduate to something bigger, and use it for a quick session, and as a convenient portable. Because people keep their Astroscans, remarkably few are offered on the used market.
Robert Edmund was taking over Edmund Scientific Company leadership from his father Norman. Norm has enjoyed retirement in Florida ever since. Robert had studied business management and knew how to run a going concern in changing markets. His telescope line was not doing well. Telescope leadership belonged to Criterion, Unitron, Questar, and Celestron, and Edmund Scientific wanted to earn its way to the top tier. The Astroscan was his opening salvo.
Robert Edmund hired me as a consultant in 1975, when I was 28. I was planetarium director at a private school, an hour's drive north of Edmund's. I was young and unknown and had even rougher edges than now. My ideas were unconventional, and entirely untested in the market. I contributed to a lot of Edmund's smaller astronomy projects, too.
I had observed observers observing in amateur, public, and school settings, and discovered that some of the wisdom of my elders wasn't wisdom. Telescope setup took frustratingly long, mountings were clumsy and shaky with narrow pivot points and long overhangs, eyepieces were tough to squint through, and views were underwhelmingly faint and dull. To improve on those, I preferred quick setup with minimal moving parts, stubby bodies, wide fields of view with wide exit pupils and bright contrast, lightweight and cheap. Those all shouted "Rich-Field".
Dr. Harvey Davis of the Lansing Astronomical Society introduced me to the principles of rich-field telescopes in the late 1960s. He was a friendly young math prof at Michigan State, where I was an undergrad. In the early '70s my friend - everybody's friend - Roger Tuthill made an RFT with an optical window (the success of which spurred us to do the same with the Astroscan). Roger's scope had a conventional cylindrical tube with a simple handle, so the only characteristics in which it was a predecessor of the Astroscan were the window and being an RFT. It didn't sell well at all.
No one in all history had ever gotten Americans to buy a LOW-power telescope, and we knew this was a huge hurdle. I assured Edmund that the telescope would please its users, but I explicitly never promised that anyone would buy it, and I wondered whether the expensive project would ever turn a profit. When Marketing VP Jack Sharff claimed that people would buy it, I thought that was bravado more than business sense. Sharff assured me that making it "popular" was his task, not mine. A good thing, because I understood almost nothing about marketing back then.
I wanted to make the eyepiece's exit-pupil an enormous 6 mm, because that's about the widest a dark-adapted human eye can take in. So, figuring from that, I championed a 4 1/4" f/4 (which the company nudged to f/4.2 for manufacturing convenience). Astroscan's richfield view - 3 degrees wide - means that finding things is easy, and keeping them in view is easy. It also means that hundreds of deep-sky objects are unusually contrasty, making them more obvious to beginners. The tradeoffs are minor: no astrophotography (which we wouldn't wish on novices anyway), planets look too tiny, and only a few double stars would look good. But any novice scope would only show pleasing detail on Jupiter and Saturn, the other planets being too small, featureless, and/or faint. So we swapped decent views of 2 objects (Jupiter and Saturn) to get superior views of hundreds of deep-sky objects.
I expounded on telescope design, exit pupils, and surface brightness in "Of Pupils and Brightness", Griffith Observer, January 1985.
At least as important as the optics, I wrote Astroscan's behavioral specifications. I remember blathering on and on for maybe 2/3 of a page singlespaced that I could have shortened enormously had I known the term "user-friendly". I didn't have the term, but I did have the concept. In beginner telescopes, it meant minimizing adjustments to fiddle with, and shortening the setup time (competitors, then and now, often take 15-20 minutes). Our setup time target was 3 minutes. We got it down to 10 seconds, and NO user's attention-span is too short for that.
While I did the optical and behavioral design, a brilliant young optical engineer, Mike Simmons, created the mechanical design that satisfied our needs. Simmons figured out that pushing the tube into the mounting made sense, and Simmons figured out that the ball-in-socket would work best. He was right. He advocated a very large sphere, with just the focuser-end of the tube sticking out. However, manufacturability, aesthetic appearance, and the awkwardness of a large-diameter sphere pointed the company to a smaller sphere, with more of the cylinder sticking out. This, however, is top-heavy, so to balance it, 2 semicircular slugs of cast iron surround the mirror. The extra weight, and the need for it, offended Simmons, and he left Edmund's soon after. I haven't seen him since the early '80s.
The shell satisfied all my specifications, including being nearly student-proof (it's meant to be checked out by students and carried home on a school bus). An industrial designer did the detail work. It's cast in 2 pieces of ABS plastic (one with the focuser insert, one without) and glued together.
In the fall of 1976, just before the first ads came out, I asked Robert Edmund what amount of sales he'd consider successful. He said 800 units by Christmas. Privately I thought that unlikely. Well, they sold 3,000 Astroscans in those first 3 months, which taught me another business lesson: there are DISeconomies of scale, as well as economies of scale. For example, the company couldn't produce the telescopes fast enough, and had to add shifts. Part of the optical design was meant to use an excellent, but slow-selling eyepiece that Edmund had a thousand of. They ran out, and had to scramble, buying every eyepiece on the world market that could possibly work - some Astroscans were shipped with Clave Plossls worth almost as much as the entire scope! Robert Edmund soon had Penn State's Dr. David Rank design the RKE eyepiece line, stimulated by the need to make a new eyepiece for the Astroscan. I'm happy that the company has sold in the neighborhood of 100,000 of them.
It was Robert Edmund who selected and hired and coordinated all the various people whose work combined to make Astroscan a success. He paid for all the work and assumed all the risk. He paid me quite well. In addition, the Edmund family and company ALWAYS treated me exceptionally well, and very often did me favors far beyond a conventional business relationship. Then and now, I regard my relationship with Edmund as one of the best I have ever had. I consulted for them for 9 years, 1975-84, but I have been a customer of theirs for 50 years, and endorse them as a fine set of people.
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Nobody since then has hired me to design a telescope, and such a project is beyond my personal resources. But I still get ideas.
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Parts of this post appeared on the Old Scope list in February 2002.
FFNs, LBBs, and LBMs
© Norman Sperling 2002. Excerpted from his book What Your Astronomy Textbook Won't Tell You, 0-913399-04-3.
FFNs
When novices start to use their first telescope, they look at the sky's major showpieces, such as the Messier nebulae, clusters and galaxies. They're big and bright enough to show up in binoculars, and a beginner's telescope shows detail in many of them. In the background lurk many more faint objects.
Experienced skywatchers buy bigger and better telescopes, seeing ever-richer detail in more and more nebulae, clusters and galaxies. But always, in the background, there are even more objects, too small and faint to make out. Some irreverent amateur astronomers in San Jose call those background objects "Faint Fuzzy Nothings" – FFNs.
Primary Use of Right Eye versus Left Eye by Members of the Public Observing Through Telescopes at Chabot Observatory
Norman Sperling. Originally published in The Refractor, vol. 73 #1, September 1996, p6.
Do people use their right eyes, or their left eyes, to observe through telescopes? If they predominantly use one, the design of telescope eyepiece areas might be specialized for that side.
On 5 public nights in March through July, 1996, tallies were kept of which eye was first used by members of the public who were observing celestial objects through telescopes at Chabot Observatory. The nights were selected for the following characteristics:
The sky was clear.
At least 30 members of the public were present
No other duties promised to distract from the tally.
In fact, answering questions from patrons did indeed distract from tallying approximately 10 observers. Also, fewer than 10% were noticed to try both eyes while at the telescope. Only the side first used was tallied.
Night Left Eye Right Eye
1 19 22
2 26 23
3 26 34
4 11 22
5 11 36
Total 93 137
Each side is used by large numbers of the public. Therefore, as expected, the design of eyepiece areas of telescopes for public viewing must accommodate both sides.
The Disappearance of Darkness
Norman Sperling
Adapted from an invited paper presented at International Astronomical Union Colloquium 112, Washington, DC, 1988. Originally published in: David L. Crawford, ed, Light Pollution, Radio Interference, and Space Debris. Astronomical Society of the Pacific Conference Series, Vol. 17.
Introduction
Until the 1900s, virtually all humans knew the appearance of the dark night sky. Even unschooled urbanites knew some constellations and planets. By 1909, light pollution made authors admonish readers to do their skywatching from the countryside rather than the city. The warnings have escalated along with the light pollution. Light pollution's effect on professional and volunteer observational astronomy, along with telescopes' changing focal ratios, largely determine which kinds of astronomy are done in which institutions. In times and places where individuals perceive little possibility to change their culture, astronomers cope as best they can. When activism earns results in other cultural matters, astronomers sometimes become activists to fight light pollution. Despite winning some battles, the war against light pollution is still being lost, so a different approach is suggested.
Of Pupils & Brightness
by Norman Sperling
Copyright © 1985, Griffith Observer magazine, January 1985
reprinted by permission
All you pupils in this short-course want to select telescopes. Great! You have an idea that skywatching can be a nice hobby. In fact, it is sensational. And you think that a telescope will show some impressive sights. In fact, the views can be awesome. If you pay moderate attention you can learn enough to buy acceptable telescopes. But it's a much brighter idea to learn the ins and outs and get a telescope tailored to your wants.
Selecting a telescope can bewilder the beginning astronomer. There are so many types -



