Star Testing Astronomical Telescopes, 2nd Ed. [By Suiter]
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Title: Star Testing Astronomical Telescopes, 2nd Edition - A Manual for Optical Evaluation and Adjustment
Author(s): Harold Richard Suiter
Other Info: 6.0" by 9.0", 428 pages, Hardbound, 2 lb item wt.
It is not often that a book opens the eyes of a whole generation of amateur astronomers—but the first edition of Dick Suiter’s Star Testing Astronomical Telescopes was just such a book. By giving its readers a simple, sensitive, and reliable test for optical performance, he enhanced the observing experience of every amateur astronomer who took its lessons to heart. Whether you were a novice or expert, Star Testing was important because it told you how to get the most from your telescope.
What makes the star test so great is that it’s both very easy and very sensitive. The star test is so simple that you probably use it already without being aware of it. When focusing an instrument you probably roll the eyepiece back and forth a couple times before settling on the sharpest position. If the telescope is well figured, collimated properly, and the air is steady, best focus lies midway between two identical out-of-focus disks. Without even thinking about it, you just know that appearance means good optics.
To perform the test, you simply observe a star with a moderately high-power eyepiece, giving careful consideration to the image on both sides of focus. The patterns you see in the focused and out-of-focus star images tell you whether your telescope is aligned for maximum performance, whether the atmosphere is steady, when the telescope has cooled, and when it is ready to do its best.
I have known Dick Suiter for about twenty-five years, since I met him at a star party in Ohio and subsequently asked him to write a short article about star testing for Astronomy magazine. His ability to meld abstruse theory with practical observing has always impressed me, and now, in this second edition, he has produced once again a spectacular blend of theory and practice.
In the Foreword to the first edition, I told readers how star testing helped me to get top-notch performance from my 20-inch ƒ /5 Dobsonian, back in the days when not many people had experience with telescopes of that aperture. Star testing revealed tube currents, so I added a fan; it revealed a bit of spherical aberration, and I had the primary refigured. With the help of star testing, I tuned up my big Dob to give excellent lunar and planetary images. During the 1988 opposition of Mars, for example, not only did I see Deimos and Phobos for the first time, but I also enjoyed the best views I’d ever had of the planet itself.
In the years since this book first appeared, I think that the increasing number of amateurs who routinely star test telescopes has exerted a powerful but subtle influence on the telescope industry. When the first edition of Star Testing came out, it was not particularly uncommon, at a star party, to accept a proud owner’s invitation to look through a new telescope—only to find yourself thinking, “Oh my gosh, does this person realize the telescope has major problems?” Over time, I am sure that amateurs who routinely star test every instrument they look through have given a few proud telescope owners a few bad nights, and that has resulted in bad days for some dealers and manufacturers. But the net result is that today, the astronomical public expects—and gets—a far better telescope than they did some twenty years ago. All because Dick Suiter taught us what to look for in a star image.
What impresses me most about this second edition is that what was already good has become even better. With great care, Dr. Suiter has improved the visual fidelity of the figures by computing effects for the whole range of wavelengths visible to the eye. He has tested differing computational schemes against one another to verify his results. He has carefully compared the complex aberrations found in real telescopes with the pure aberrations found in theory—and he demonstrates that they match.
Star Testing is a resource that should be on the shelf where you keep your most-often-used astronomy books. Toss it into your observing kit along with eyepieces, Oreo cookies, and packs of instant hot chocolate. Read it; absorb it; read it again. Star testing is an integral part of observing.
You will benefit when you become sensitive to your telescope’s optical performance. If you find that it has a few problems—and what telescope does not?—it is best to deal openly with them. Would-be astronomers who refuse to acknowledge such problems tend to stop using their instruments, and eventually their interest in astronomy. Once you recognize that a problem exists, you can possibly use the star test to correct it. Often, it’s nothing that careful collimation will not solve. If your telescope has properly adjusted and excellent optics, the star test will confirm that fact—and you are free to turn your attention to observing the splendors of the heavens.
Richard Berry
Lyons, Oregon
More About this BookMany observers harbor misgivings about their telescope. The manufacturer may have guaranteed accuracy to “one-quarter wavelength” or as “diffraction-limited” but most telescope users have, at best, only a hazy idea of how to personally verifying such claims. Sure, there are ways to check the accuracy of individual components but for many they are hard to understand or require costly reference optics and other test equipment. Besides, telescope users are interested in the performance of the entire optical train, not just the main optical element.
What is really needed is a test that can be used at the observing site, so that all the problems that impact on a telescope's performance can be diagnosed. Isn't there a simpler and more complete way than the complicated shop tests? Yes, the star test is such a method. It uses the entire working telescope. It is not a poor substitute or a work-around that uses bits and pieces of the optical system. It is the oldest and most sensitive of the optical tests—an inspection of the diffraction image itself.
Star-test results apply to the complete imaging performance of the telescope. The star test is lightning-fast and requires only a good high-power eyepiece. It tests the telescope for precisely what it was meant to do. Bad or poorly-aligned instruments fail the star test unambiguously. The star test often allows you to correct the optical difficulty immediately in the field, when you might be frantic to have your telescope perform well to observe a once in a lifetime event.
While the star test has been around for centuries learning it has often been hampered by messy mathematics and its visual nature. Most people who use it have learned it at the elbow of a patient Master. In this book, Dick Suiter becomes your Master. He carefully shields you from difficult diffraction theory and uses advanced computer generated graphics to show you the appearance of each aberration. Again and again, you will look at Dick's graphics and say “I've seen that before. So that's what it was!” The star test is a powerful but inexpensive way of obtaining better resolution and contrast. With this book most observers will find that they don't need a new telescope because they now can test, diagnose and fix the one they have. Using Star Testing Astronomical Telescopes as a guide, your telescope will perform to the best of it's abilities and perhaps it will show images better than you would have believed possible.
Title: Star Testing Astronomical Telescopes, 2nd Edition - A Manual for Optical Evaluation and Adjustment
Author(s): Harold Richard Suiter
Other Info: 6.0" by 9.0", 428 pages, Hardbound, 2 lb item wt.
It is not often that a book opens the eyes of a whole generation of amateur astronomers—but the first edition of Dick Suiter’s Star Testing Astronomical Telescopes was just such a book. By giving its readers a simple, sensitive, and reliable test for optical performance, he enhanced the observing experience of every amateur astronomer who took its lessons to heart. Whether you were a novice or expert, Star Testing was important because it told you how to get the most from your telescope.
What makes the star test so great is that it’s both very easy and very sensitive. The star test is so simple that you probably use it already without being aware of it. When focusing an instrument you probably roll the eyepiece back and forth a couple times before settling on the sharpest position. If the telescope is well figured, collimated properly, and the air is steady, best focus lies midway between two identical out-of-focus disks. Without even thinking about it, you just know that appearance means good optics.
To perform the test, you simply observe a star with a moderately high-power eyepiece, giving careful consideration to the image on both sides of focus. The patterns you see in the focused and out-of-focus star images tell you whether your telescope is aligned for maximum performance, whether the atmosphere is steady, when the telescope has cooled, and when it is ready to do its best.
I have known Dick Suiter for about twenty-five years, since I met him at a star party in Ohio and subsequently asked him to write a short article about star testing for Astronomy magazine. His ability to meld abstruse theory with practical observing has always impressed me, and now, in this second edition, he has produced once again a spectacular blend of theory and practice.
In the Foreword to the first edition, I told readers how star testing helped me to get top-notch performance from my 20-inch ƒ /5 Dobsonian, back in the days when not many people had experience with telescopes of that aperture. Star testing revealed tube currents, so I added a fan; it revealed a bit of spherical aberration, and I had the primary refigured. With the help of star testing, I tuned up my big Dob to give excellent lunar and planetary images. During the 1988 opposition of Mars, for example, not only did I see Deimos and Phobos for the first time, but I also enjoyed the best views I’d ever had of the planet itself.
In the years since this book first appeared, I think that the increasing number of amateurs who routinely star test telescopes has exerted a powerful but subtle influence on the telescope industry. When the first edition of Star Testing came out, it was not particularly uncommon, at a star party, to accept a proud owner’s invitation to look through a new telescope—only to find yourself thinking, “Oh my gosh, does this person realize the telescope has major problems?” Over time, I am sure that amateurs who routinely star test every instrument they look through have given a few proud telescope owners a few bad nights, and that has resulted in bad days for some dealers and manufacturers. But the net result is that today, the astronomical public expects—and gets—a far better telescope than they did some twenty years ago. All because Dick Suiter taught us what to look for in a star image.
What impresses me most about this second edition is that what was already good has become even better. With great care, Dr. Suiter has improved the visual fidelity of the figures by computing effects for the whole range of wavelengths visible to the eye. He has tested differing computational schemes against one another to verify his results. He has carefully compared the complex aberrations found in real telescopes with the pure aberrations found in theory—and he demonstrates that they match.
Star Testing is a resource that should be on the shelf where you keep your most-often-used astronomy books. Toss it into your observing kit along with eyepieces, Oreo cookies, and packs of instant hot chocolate. Read it; absorb it; read it again. Star testing is an integral part of observing.
You will benefit when you become sensitive to your telescope’s optical performance. If you find that it has a few problems—and what telescope does not?—it is best to deal openly with them. Would-be astronomers who refuse to acknowledge such problems tend to stop using their instruments, and eventually their interest in astronomy. Once you recognize that a problem exists, you can possibly use the star test to correct it. Often, it’s nothing that careful collimation will not solve. If your telescope has properly adjusted and excellent optics, the star test will confirm that fact—and you are free to turn your attention to observing the splendors of the heavens.
Richard Berry
Lyons, Oregon
More About this BookMany observers harbor misgivings about their telescope. The manufacturer may have guaranteed accuracy to “one-quarter wavelength” or as “diffraction-limited” but most telescope users have, at best, only a hazy idea of how to personally verifying such claims. Sure, there are ways to check the accuracy of individual components but for many they are hard to understand or require costly reference optics and other test equipment. Besides, telescope users are interested in the performance of the entire optical train, not just the main optical element.
What is really needed is a test that can be used at the observing site, so that all the problems that impact on a telescope's performance can be diagnosed. Isn't there a simpler and more complete way than the complicated shop tests? Yes, the star test is such a method. It uses the entire working telescope. It is not a poor substitute or a work-around that uses bits and pieces of the optical system. It is the oldest and most sensitive of the optical tests—an inspection of the diffraction image itself.
Star-test results apply to the complete imaging performance of the telescope. The star test is lightning-fast and requires only a good high-power eyepiece. It tests the telescope for precisely what it was meant to do. Bad or poorly-aligned instruments fail the star test unambiguously. The star test often allows you to correct the optical difficulty immediately in the field, when you might be frantic to have your telescope perform well to observe a once in a lifetime event.
While the star test has been around for centuries learning it has often been hampered by messy mathematics and its visual nature. Most people who use it have learned it at the elbow of a patient Master. In this book, Dick Suiter becomes your Master. He carefully shields you from difficult diffraction theory and uses advanced computer generated graphics to show you the appearance of each aberration. Again and again, you will look at Dick's graphics and say “I've seen that before. So that's what it was!” The star test is a powerful but inexpensive way of obtaining better resolution and contrast. With this book most observers will find that they don't need a new telescope because they now can test, diagnose and fix the one they have. Using Star Testing Astronomical Telescopes as a guide, your telescope will perform to the best of it's abilities and perhaps it will show images better than you would have believed possible.
Title: Star Testing Astronomical Telescopes, 2nd Edition - A Manual for Optical Evaluation and Adjustment
Author(s): Harold Richard Suiter
Other Info: 6.0" by 9.0", 428 pages, Hardbound, 2 lb item wt.
It is not often that a book opens the eyes of a whole generation of amateur astronomers—but the first edition of Dick Suiter’s Star Testing Astronomical Telescopes was just such a book. By giving its readers a simple, sensitive, and reliable test for optical performance, he enhanced the observing experience of every amateur astronomer who took its lessons to heart. Whether you were a novice or expert, Star Testing was important because it told you how to get the most from your telescope.
What makes the star test so great is that it’s both very easy and very sensitive. The star test is so simple that you probably use it already without being aware of it. When focusing an instrument you probably roll the eyepiece back and forth a couple times before settling on the sharpest position. If the telescope is well figured, collimated properly, and the air is steady, best focus lies midway between two identical out-of-focus disks. Without even thinking about it, you just know that appearance means good optics.
To perform the test, you simply observe a star with a moderately high-power eyepiece, giving careful consideration to the image on both sides of focus. The patterns you see in the focused and out-of-focus star images tell you whether your telescope is aligned for maximum performance, whether the atmosphere is steady, when the telescope has cooled, and when it is ready to do its best.
I have known Dick Suiter for about twenty-five years, since I met him at a star party in Ohio and subsequently asked him to write a short article about star testing for Astronomy magazine. His ability to meld abstruse theory with practical observing has always impressed me, and now, in this second edition, he has produced once again a spectacular blend of theory and practice.
In the Foreword to the first edition, I told readers how star testing helped me to get top-notch performance from my 20-inch ƒ /5 Dobsonian, back in the days when not many people had experience with telescopes of that aperture. Star testing revealed tube currents, so I added a fan; it revealed a bit of spherical aberration, and I had the primary refigured. With the help of star testing, I tuned up my big Dob to give excellent lunar and planetary images. During the 1988 opposition of Mars, for example, not only did I see Deimos and Phobos for the first time, but I also enjoyed the best views I’d ever had of the planet itself.
In the years since this book first appeared, I think that the increasing number of amateurs who routinely star test telescopes has exerted a powerful but subtle influence on the telescope industry. When the first edition of Star Testing came out, it was not particularly uncommon, at a star party, to accept a proud owner’s invitation to look through a new telescope—only to find yourself thinking, “Oh my gosh, does this person realize the telescope has major problems?” Over time, I am sure that amateurs who routinely star test every instrument they look through have given a few proud telescope owners a few bad nights, and that has resulted in bad days for some dealers and manufacturers. But the net result is that today, the astronomical public expects—and gets—a far better telescope than they did some twenty years ago. All because Dick Suiter taught us what to look for in a star image.
What impresses me most about this second edition is that what was already good has become even better. With great care, Dr. Suiter has improved the visual fidelity of the figures by computing effects for the whole range of wavelengths visible to the eye. He has tested differing computational schemes against one another to verify his results. He has carefully compared the complex aberrations found in real telescopes with the pure aberrations found in theory—and he demonstrates that they match.
Star Testing is a resource that should be on the shelf where you keep your most-often-used astronomy books. Toss it into your observing kit along with eyepieces, Oreo cookies, and packs of instant hot chocolate. Read it; absorb it; read it again. Star testing is an integral part of observing.
You will benefit when you become sensitive to your telescope’s optical performance. If you find that it has a few problems—and what telescope does not?—it is best to deal openly with them. Would-be astronomers who refuse to acknowledge such problems tend to stop using their instruments, and eventually their interest in astronomy. Once you recognize that a problem exists, you can possibly use the star test to correct it. Often, it’s nothing that careful collimation will not solve. If your telescope has properly adjusted and excellent optics, the star test will confirm that fact—and you are free to turn your attention to observing the splendors of the heavens.
Richard Berry
Lyons, Oregon
More About this BookMany observers harbor misgivings about their telescope. The manufacturer may have guaranteed accuracy to “one-quarter wavelength” or as “diffraction-limited” but most telescope users have, at best, only a hazy idea of how to personally verifying such claims. Sure, there are ways to check the accuracy of individual components but for many they are hard to understand or require costly reference optics and other test equipment. Besides, telescope users are interested in the performance of the entire optical train, not just the main optical element.
What is really needed is a test that can be used at the observing site, so that all the problems that impact on a telescope's performance can be diagnosed. Isn't there a simpler and more complete way than the complicated shop tests? Yes, the star test is such a method. It uses the entire working telescope. It is not a poor substitute or a work-around that uses bits and pieces of the optical system. It is the oldest and most sensitive of the optical tests—an inspection of the diffraction image itself.
Star-test results apply to the complete imaging performance of the telescope. The star test is lightning-fast and requires only a good high-power eyepiece. It tests the telescope for precisely what it was meant to do. Bad or poorly-aligned instruments fail the star test unambiguously. The star test often allows you to correct the optical difficulty immediately in the field, when you might be frantic to have your telescope perform well to observe a once in a lifetime event.
While the star test has been around for centuries learning it has often been hampered by messy mathematics and its visual nature. Most people who use it have learned it at the elbow of a patient Master. In this book, Dick Suiter becomes your Master. He carefully shields you from difficult diffraction theory and uses advanced computer generated graphics to show you the appearance of each aberration. Again and again, you will look at Dick's graphics and say “I've seen that before. So that's what it was!” The star test is a powerful but inexpensive way of obtaining better resolution and contrast. With this book most observers will find that they don't need a new telescope because they now can test, diagnose and fix the one they have. Using Star Testing Astronomical Telescopes as a guide, your telescope will perform to the best of it's abilities and perhaps it will show images better than you would have believed possible.