The Art Of Using A Telescope
Once you’ve obtained an astronomical telescope, what can you expect of it? Both less and more than many new owners realize. You’re using a ‘time machine’ to peer back into the past.
One of the most fun parts of being an amateur astronomer is showing off the heavens to others. The “oohs” and “aahs” at a public star party as people get their first good look at the Moon or Saturn are a pleasant reward for the proud telescope owner. Naturally, you will have aimed the scope at the most spectacular object above the horizon.
Sometimes there’s a temptation to show people more typical objects — ghostly, barely visible apparitions with obscure catalogue numbers — “to give them an idea of real astronomy.” The reactions then are not so encouraging, even when viewers are told they’re looking at a recently recovered comet or a galaxy 40 million light-years away.
The truth is, most of the thousands of objects visible in amateur instruments are not the least bit spectacular. Anyone who gets a telescope expecting dramatic visual thrills is in the wrong hobby.
The riches that astronomy offers are of a different sort. Visual observing outdoors in the dark usually means working to detect something that’s extremely faint, tiny, hard to find, or all three. The more difficult the task, however, the greater the rewards of success. The excitement lies in finding and seeing first-hand remote marvels far beyond our planet — and in gaining skills and knowledge as an amateur scientist.
Too many people buy a telescope as if it were a TV, expecting it to show pictures all by itself. It’s more like a piano, which gives back only as much value as the work you put into it. Learning to use a telescope well is a lot easier than learning a musical instrument, however. If you’re reasonably persistent and careful and are willing to practice the techniques described here, you’ll soon master the skies.
Know Your Equipment
Naturally, everyone first tries out a new telescope in the daytime. This is when to become familiar with its motions, pointing, focusing, different eyepieces, and magnifying powers, so you can then do everything in the dark.
The Finder. Most telescopes have a finderscope attached to the side to help aim it. You need a finder because the main telescope has such a tiny field of view — that is, it shows such a tiny piece of sky — that you can’t tell exactly where it’s pointed just by looking.
The higher the power, the smaller the field of view. For example, at 50 power you’re looking at a magnified piece of sky about as small as your little fingernail covers when held at arm’s length. An 8× finderscope, on the other hand, displays about as much sky as a golf ball covers at arm’s length.
This is big enough to aim at something you see with the naked eye and get it in the finderscope’s view. Once it’s there, you centre it in the finder’s crosshairs. That should be a precise enough aim for the object to appear in the view of the main telescope.
First things first: you’ll need to adjust the finder’s mounting screws so it’s aimed parallel to the main telescope. In daylight, point the main scope at something at least several hundred feet away using the lowest-power eyepiece. (But not the Sun! Never look through a telescope that might get aimed at the Sun or you could blind yourself.) A distant treetop is ideal. Centre it in your view.
Never mind if it appears upside down.
Now look in the finder. See the treetop? Is it centred in the crosshairs? Adjust the screws holding the finder until the crosshairs line up on the target. Now check back in the main telescope to make sure it hasn’t moved. Then switch to a high-power eyepiece in the main telescope, and repeat the operation until the finder is locked in position with perfect aim.
And why, you ask, is the treetop upside down or oriented at some other weird angle? The answer is that this is an astronomical telescope, and after all, there’s no up or down in space. So it doesn’t matter how the field is oriented.
Turning the image right-side up would require extra optical parts, adding to the expense and complication of the instrument and probably degrading its performance slightly. Therefore, “image erecting” lenses are used only in terrestrial telescopes, those intended for looking at things on Earth.
Next let’s turn to the mounting.
Telescope mounts come in two basic types: equatorial and altazimuth.
An equatorial mount allows the telescope to swing only in the directions of celestial north-south and east-west. The altazimuth goes up-down (moving in altitude) and side to side (azimuth). An altazimuth mount at least has the virtue of simplicity. An equatorial mount is ultimately more helpful, but it takes some getting used to.
The Equatorial Mount. If this is what you have, find its polar axis (the rotating part that’s more toward the base and maybe has a setting circle showing right ascension). Outdoors, place the telescope so the polar axis points roughly to where you know Polaris, the North Star, will be located after dark. The telescope’s motion around this axis now traces the paths taken by celestial bodies across the sky as the Earth turns.
Sweep the telescope around its polar axis from the eastern horizon across the sky to the west to visualize nightly star paths. At first the mount’s motions will seem awkward and unpredictable. But remember that no matter where the telescope is pointed, it will move only toward or away from Polaris (celestial north-south) and at right angles to this direction (celestial east-west). The orientation of these varies in different parts of the sky, but with some practice swinging the telescope around in daytime you’ll get used to them.
The Fine Art Of Observing
The challenge of astronomy is that we must view most of the universe from extremely far away. When you’re trying to see something well on Earth your instinct is to move closer for a better look. But when it comes to distant stars and galaxies, we’re stuck where we are. So, ever since the dawn of telescopic astronomy, the art of observing has been the art of using your eye to the utmost of its ability.
Using telescopes takes a little time..soon you will be able to go out and look through your scope and see things you missed just the night before, you’ll become accustomed to the telescope and your eyes will quickly adapt to this ‘new’ way of seeing. Everyone goes through this and everyone I know remarks on how easy it is to pick up the skill!
When looking through the telescope, focus and refocus with care. A good observer is always fiddling with the focus, trying to get it just a hair sharper. Many people find it best to keep both eyes open, since squinting strains the working eye. You can cover the “off” eye with one hand.
Don’t expect to see right away everything an astronomical object has to offer.
The first look always shows less than comes out with continued scrutiny. This is true whether your subject is a dim galaxy that can hardly be told from the blackness of space, or detail on the Moon or a planet where the light is almost blindingly bright.
One reason it takes time to see detail is the unsteadiness of the Earth’s atmosphere. Celestial objects constantly shimmer and boil when viewed at high power, due to weak but ever-present heat waves in the air around and above us. The severity of this shimmering — called the atmospheric seeing — varies from night to night and often from minute to minute.
As you watch an object quiver and churn, unsuspected detail will flicker into view during quick moments of stability when the view sharpens up, only to fade out again before you know it. The skilled observer learns to remember these good moments and ignore the rest. The quality of the atmospheric seeing is most important when viewing bright objects at high power, but it can influence the visibility of faint ones too.
The main reason it takes time to see detail, however, has to do not with the atmosphere but with the eye and mind. Wringing everything possible out of very distant views means learning new visual skills that involve active, concentrated effort.
You’ll discover that the eye’s picture of a difficult object builds up rather slowly. First one detail is noticed and fixed, and you think there’s nothing more to be seen. But after a few minutes another detail becomes evident, then another.
To convince yourself of this, look at a piece of sky with the naked eye and try to spot faint stars. Some will be visible right away; others take a few seconds to come out. When no more appear, most people would quit trying. But keep at it for a few minutes. Chances are some more will glimmer into view in places you would have sworn were blank. After a while you’re seeing at least half a magnitude fainter than at first.
The planet Mars is another classic example of this effect. For the beginner taking a first look with a small telescope, Mars ranks as the most disappointing object in the sky. It’s just a tiny, featureless, orange fuzzball. The beginner steps aside to let an experienced Mars observer look in the eyepiece. Silence. “There’s the north polar cap…. That big dark area in the south must be Mare Erythraeum. Okay, I’ve got Sinus Meridiani…. There’s a cloud patch on the western limb….”
The beginner looks again. Nothing but a fuzzball. Well, maybe there is a bit of brightness at the north edge crawling around in the poor seeing, and the fuzziness isn’t a perfectly uniform orange, but these hardly seem like things worth noticing. Nevertheless, the next time the beginner looks he or she won’t be quite a beginner, and the bright spot and dark area will come into view more readily.’
Record what you see
An excellent way to train yourself to see better is to make sketches. These don’t have to be works of art; the idea is just to record details in your notebook more directly than you can with words. Star fields require no artistic talent whatsoever, but by sketching a field that contains a faint asteroid or outer planet, you can identify the intruder be checking back in the next few days or weeks and seeing which one changes position.
For practice sketching planets, try drawing the Moon with the naked eye. If you have reasonably sharp or well-corrected vision, the Moon shows much more detail to the naked eye than any planet will in a telescope! Make a semicircle a couple of inches in diameter by tracing some round object and then draw the terminator exactly as you see it on the Moon. Carefully add the major dark areas with pencil shading, then look for finer markings. By now you’ll be seeing much more detail on the Moon’s face than you ever thought possible without optical aid.
The lesson is clear,” wrote the British author James Muirden in The Amateur Astronomer’s Handbook, long a classic: “No opportunity should be lost to train the eye to work with the telescope; to observe the same object with different powers so as to see the effect of magnification; to try to see faint stars; and to draw planetary markings.
In the beginning, to be sure, this may all seem to be wasted effort; the observing book will fill up with valueless sketches and brief notes of failure. But this apparently empty labor is absolutely essential; for, as the weeks pass, a steady change will be taking place.
Objects considered difficult or impossible to see will now be discerned at first glance, and fainter spectres will have taken their place. Indeed, these former features will now be so glaringly obvious that the observer may suppose that some radical improvement has occurred in the observing conditions. But the credit belongs entirely to the eye.”