APO Services Page

By: Apo  09-12-2011
Keywords: telescope

                This section will list some extra reading material for now.

                              

       

                   

               Specifications for Apochromatic Lenses 1. Optical component surface finishDimensions of scratches and points shall not exceed the following values:
Scratches Width, not more than 0.04mm.
Total length, mm, not more than 3mm.
Points Diameter no more than 0.4mm.
Quantity no more than 0.5 clear aperture.
Accumulation of defects diameter of a limited area, 5mm.
Total area of scratched and points no more, square mm 1 The total scratch length and the point quantity that are close on width and diameter to the maximum permissible shall not exceed the following values:
Scratches Width, 0.02 mm.
Total length, mm, not more than 2mm.
Points Diameter, mm 0.3.
Quantity, no more than 0.2 clear aperture. Scratches and points with the following dimensions are disregarded:
Scratch width, not more, 0.004 mm
Point diameter, not more, 0.01 mm2. Anti-reflection coating requirementsNon-uniformity of coating interference coloration, which doesn't degrade characteristics of coating optical parameters and doesn't affect output characteristics of a lens, is permissible on anti-reflection surfaces of optical elements.3. Bubbles and inclusions requirementsPermissible dimensions of bubbles and inclusions:
In lens material bubbles and inclusions of no more than 0.3mm in size are allowable , and a number of bubbles of diameter 0.03mm to 0.3mm in each lens shall not exceed 3 pieces.
These do not affect optical performance in any way.

                       A Tale of Two Astronomers                                                                       By Allister St. ClaireOnce upon a time there lived two amateur astronomers, Alfred and Steve. Alfred and Steve both entered the astronomy hobby 1 year ago. Both purchased their first telescope from the same hobby store in their area. In fact, they purchased the same first telescope, a 90mm f/10 achromat on a sturdy EQ mount with an RA motor drive.From here our budding astronomers diverge on separate courses through the hobby.Alfred's TaleAlfred grabs his observing book and owner's manual and is out observing the first night. He uses the books to teach himself the names of constellations and bright stars. The night sky transforms from a chaos of bright lights to an ordered system of constellations and asterisms. Soon he is able to navigate the skies like he navigates the streets of his town.Alfred finds the telescope awkward to use at first. There are so many steps to remember; find object in finder, find it in the eyepiece, tighten the RA access, engage the drive and focus the eyepiece. However, as with any skill, practice makes perfect. Soon the individual steps blur into unconscious movements of his hands. Alfred graduates to using a star atlas with an accompanying guide. He's now taken to recording his evening observations in a simple log. Double stars are a particular delight. Alfred eagerly scans each constellation on his atlas for double star listings. Time passes and the telescope becomes like a trusted friend. Alfred knows the magnifications of his 2 eyepieces and barlow by heart. He's able to quickly find any object plotted in his Atlas as long as it's within the light grasp of his telescope. His familiarity with the telescope is now to the point where he doesn't need a light to find the RA and DEC axis locks, motor drive engagement clutch or centering the finder. The telescope has now become an extension of Alfred's desire and skill to observe.After 1 year Alfred is convinced of two things. First, astronomy is an amazing hobby invoking feelings of awe about the universe. Second, his telescope is the best telescope in the world. Looking back on 12 months of observing with it, the telescope has never let him down.Steve's TaleSteve's been involved in a number of hobbies over the years. Like Alfred, he makes an impulse buy. However, unlike Alfred, Steve's smart. He knows it's important to read up on his purchase and the hobby in general. Steve logs online and finds a telescope review site and reads the two reviews on his telescope. With a sinking feeling Steve learns his scope will show secondary color, have an upper magnification ceiling of 140x and is awkward to use due to it's long focal length. Steve spends the first month learning both the constellations and looking for the issues with his scope that the reviews informed him about. With dismay Steve views the secondary color on brighter objects. To determine the extent of the secondary color, Steve views stars of dimmer magnitudes. From this he determines where the threshold is for the secondary color. He also tests the upper magnification of the scope and finds it falls apart at around 130x!After the first month Steve admits he was a "sucker" on his first telescope purchase. He now reads the telescope review site with a vengeance. He reads and digests review after review. Steve learns optical terms, company names and simple methods for testing the optics of a telescope.Another month passes. Steve orders his second telescope, a 4" apochromatic refractor on an alt-az mount. Ahhh - this will be the perfect telescope.The new Apo arrives. A proud Steve is out observing with it the first evening. He hasn't learned the constellations or bright stars yet as he was field testing the sucker telescope for his first month in the hobby. No matter, he will learn them now.He will as soon as he completes star testing his new APO. Steve's "smart" and doesn't just drop $3000 on a new telescope without testing the optics. His first night out and Steve realizes that to star test his new APO he will needed a driven mount so he can compare the star images with those in his new star testing book.Back online and a week of reading mount reviews. Steve learns all about drive error, PEC, dual axis drives and other telescope mount terms. An order is placed and several days later his new mount arrives. Out comes his APO for it's second night in the backyard (Steve's been busy reading mount reviews) and Steve realizes he will need quality eyepieces for the high magnifications needed for star testing.Back online and 2 weeks of reading eyepiece reviews ...Time passes and Steve's read reviews stating 4" of telescope aperture is too small for "serious" observing. This kicks off not only another round of reading reviews, but now he's intensely engaged in posting on the astronomy forums. Boy, he won't make the mistake of buying a telescope that's too small. Steve's smart.Over the next year Steve buys, tests and sells an 8" sct, 10" dob, 18" dob, 12" GOTO SCT and a 6" APO. Given that the price commitment for each scope is increasing, Steve reads and researches his potential purchases with greater and greater thoroughness. Test sessions with each telescope take on the atmosphere of a tax audit. With so much money riding on each purchase, Steve must be certain the telescope is without flaws.After 1 year, Steve is convinced of two things. First, astronomy is an expensive hobby. Second, unless you are "smart", you will be suckered into owning and using some 90mm beginner's scope.

              Star Testing Astronomical Telescopes

                                    DEFINITIONS

Highest Useful Magnification This is the highest visual power a telescope can achieve before the image becomes too dim for useful observing (generally at about 50x to 60x per inch of telescope aperture). However, this power is very often unreachable due to turbulence in our atmosphere that makes the image too blurry and unstable to see any detail.
On nights of less-than-perfect seeing, medium to low power planetary, binary star, and globular cluster observing (at 25x to 30x per inch of aperture or less) is usually more enjoyable than fruitlessly attempting to push a telescope's magnification to its theoretical limits. Very high powers are generally best reserved for planetary observations and binary star splitting. Small aperture telescopes can usually use more power per inch of aperture on any given night than larger telescopes, as they look through a smaller column of air and see less of the turbulence in our atmosphere. While some observers use up to 100x per inch of refractor aperture on Mars and Jupiter, the actual number of minutes they spend observing at such powers is small in relation to the number of hours they spend waiting for the atmosphere to stabilize enough for them to use such very high powers.

Therefore... any time you see brand new $200 scopes advertising capabilities of 525x and the like, know full well that it is the mathematical capability of the combined pieces, not what will happen in the real world.

Limiting Magnitude This is the magnitude (or brightness) of the faintest star that can be seen with a telescope. The larger the number, the fainter the star that can be seen.
An approximate formula for determining the visual limiting magnitude of a telescope is 7.5 + 5 log aperture (in cm). Keep in mind that this formula does not take into account light loss within the scope, seeing conditions, the observer’s age (visual performance decreases as we get older), the telescope’s age (the reflectivity of telescope mirrors decreases as they get older), etc. The limiting magnitudes specified by manufacturers for their telescopes assume very dark skies, trained observers, and excellent atmospheric transparency – and are therefore rarely obtainable under average observing conditions. The photographic limiting magnitude is always greater than the visual (typically by two magnitudes).

Focal Length This is the length of the effective optical path of a telescope or eyepiece (the distance from the main mirror or lens where the light is gathered to the point where the prime focus image is formed). Focal length is typically expressed in millimeters.
The longer the focal length, the higher the magnification and the narrower the field of view with any given eyepiece. The shorter the focal length, the lower the magnification and the wider the field of view with the same eyepiece.

Focal Ratio This is the "speed" of a telescope’s optics, found by dividing the focal length by the aperture. The smaller the f/number, the lower the magnification, the wider the field, and the brighter the image with any given eyepiece or camera.
Fast f/4 to f/5 focal ratios are generally best for lower power wide field observing and deep space photography. Slow f/11 to f/15 focal ratios are usually better suited to higher power lunar, planetary, and binary star observing and high power photography. Medium f/6 to f/10 focal ratios work well with either.

An f/5 system can photograph a nebula or other faint extended deep space object in one-fourth the time of an f/10 system, but the image will be only one-half as large. Point sources, such as stars, are recorded based on the aperture, however, rather than the focal ratio – so that the larger the aperture, the fainter the star you can see or photograph, no matter what the focal ratio.

Resolution This is the ability of a telescope to separate closely-spaced binary stars into two distinct objects, measured in seconds of arc. One arc second equals 1/3600th of a degree and is about the width of a 25-cent coin at a distance of three miles!
In essence, resolution is a measure of how much detail a telescope can reveal. The resolution values on our website are derived using the Dawes’ limit formula. Dawes’ limit only applies to point sources of light (stars). Smaller separations can be resolved in extended objects, such as the planets. For example, Cassini’s Division in the rings of Saturn (0.5 arc seconds across), was discovered using a 2.5” telescope – which has a Dawes’ limit of 1.8 arc seconds! The ability of a telescope to resolve to Dawes’ limit is usually much more affected by seeing conditions, by the difference in brightness between the binary star components, and by the observer’s visual acuity, than it is by the optical quality of the telescope.

Aperture This is the diameter of the light-gathering main mirror or objective lens of a telescope.
In general, the larger the aperture, the better the resolution and the fainter the objects you can see.
 

  Astronomy Technologies Astro-Tech Ritchey-Chrétien Optics

                                                         Optical features of this Astrograph . . .

Ritchey-Chrétien Optical Design: The Astro-Tech astrograph is a true Ritchey-Chrétien (RC) reflector optical system. Unlike a Maksutov-Cassegrain or Schmidt-Cassegrain catadioptric scope (that uses simple spherical mirrors and corrector lenses), or Newtonian reflectors (that use a coma-producing parabolic primary mirror), the Astro-Tech RC is a Cassegrain-type two-mirror optical system that uses a concave hyperbolic primary and a convex hyperbolic secondary mirror to form its images. These sophisticated and difficult-to-make mirrors combine to produce images at the Cassegrain focus at the rear of this Astro-Tech scope that are free from coma and spherical aberration, with a smaller spot size, over a much wider field than conventional Newtonians or catadioptrics. The images are likewise free from the chromatic aberration found in refractors and some catadioptrics. Because of this wide coma-free field, small spot size, and relatively fast focal ratio, the Ritchey-Chrétien design is particularly well suited to wide field astrophotography, rather than visual observing. For imaging, the RC is the optical system of choice for most of the major professional observatory imaging telescopes built in the last half-century. For example, the Hubble Space Telescope, the twin 10-meter Keck telescopes in Hawaii, and the four 8.2 meter telescopes of the Very Large Telescope array in Chile are all Ritchey-Chrétiens. For serious amateur astrophotographers without NASA’s optical budget, an Astro-Tech RC is very likely the imaging system of choice. Fully Multicoated Quartz and BK7 Mirrors: The primary mirror of the 6” Astro-Tech is first-quality BK7 optical glass, while the 8” and larger Astro-Tech RCs use primary mirrors of low thermal expansion quartz for maximum focus stability during long exposure imaging sessions. Both 6” RC mirrors are vacuum-coated with enhanced aluminum for high reflectivity and over coated with a durable layer of silicon monoxide (quartz) for long life. The 8” and larger mirrors are dielectric coated for long life and reflectivity approaching 99%+. Computer Designed and Fabricated Optics: To keep the cost of each Astro-Tech RC so reasonable when compared to competitive RC scopes, the computer-optimized Astro-Tech hyperboloid mirrors are automatically ground and finished to very high tolerances using custom-made computerized mirror grinding machines. This precision computer control guarantees an exact repeatability of figure from mirror to mirror that is difficult to achieve using more costly conventional hand figuring. After grinding and polishing, each mirror is individually tested using a Zygo interferometer to assure that it meets or exceeds its specified surface accuracy. Frill-Free Design: To further keep its cost reasonable, an Astro-Tech RC does away with most of the bells and whistles found on competitive scopes that add little to their performance (but much to their cost). For example, Astro-Tech front and rear cells are first die-cast, then CNC machine-finished, rather than completely CNC machined from raw stock at considerably greater expense but no significant improvement in performance as is the case with other RCs. Glare stops in the optical tube are a molded insert, rather than machined aluminum, resulting in a significant savings in cost at no appreciable difference in performance. The Astro-Tech scopes use an external manual dual-speed Crayford focuser, rather than the considerably more complicated and much more costly motorized movable secondary mirror system that other manufacturers use for focusing. The result of the Astro-Tech no-frills approach is genuine Ritchey-Chrétien wide-field performance at a fraction the cost of other commercial RC systems. While the mechanical bells and whistles may be limited in an Astro-Tech RC, an Astro-Tech scope still has the high precision flat field/coma-free true Ritchey-Chrétien optics that are the most important reason for buying an RC scope.                                             Mechanical Features Of This Telescope’s Optical System . . .Fixed Primary Mirror with Computer Optimized Primary and Secondary Baffling: Unlike traditional Cassegrain designs that move the primary mirror fore and aft along the central baffle tube in order to achieve focus (which can lead to image shift as the mirror position is adjusted) each Astro-Tech RC primary mirror is fixed. The Astro-Tech is focused externally by means of a dual-speed 2” Crayford-style focuser on the rear cell, thereby eliminating a Cassegrain’s moving mirror image shift during focusing. Molded field stops are installed along the interior of the optical tube to effectively prevent stray off-axis light from reaching the image plane, resulting in improved contrast. In addition multiple glare-stop microbaffles on the inner surfaces of the primary mirror baffle tube and the secondary mirror light shield further prevent off-axis light from reaching the image plane, resulting in still further improved contrast. Collimatable Secondary Mirror: Since the primary mirror of an Astro-Tech RC is fixed in position, only the secondary mirror can (or needs to) be collimated. This makes it easy to keep the Astro-Tech RC optics aligned for peak performance. Collimation adjustments to the secondary mirror are made by adjusting the three collimating screws in the back of the secondary mirror holder. Cooling Fan: The open tube RC design allows for fast cool-down of the primary and secondary mirrors. Built-in fans on the rear cell of the 10” and larger scopes increases the air-flow around the optics to achieve still quicker “cool down” times of the larger primary mirrors. The 6” and 8” scopes do not have primary mirror cooling fans, as their mirrors are small enough to cool down quickly without any external aid.

The information in this article was current at 06 Dec 2011

Keywords: telescope