Tuesday, November 14, 2017

Takahashi's TOA 150 takes on it's FS-152 ancestor By Jerry Wise

https://www.astromart.com/reviews/article.asp?article_id=657

From time to time, discussions spring up over this issue. The new triplet APOs usually come out on top with flawless color reproduction and great contrast. Several months ago the last new Takahashi FS-152 APO doublet showed up on Astromart. After a few Emails to Herb York (owner of Astromart), the FS-152 was on the way to the Lake Murray Observatory. Then another stroke of luck. A friend received a new Astro Physics 140 APO. Trouble was he just purchased a new Takahashi TOA-150 Triplet APO. A few more Emails and the APO triplet was on the way to too. While individual samples of an instrument will vary, these two OTAs seem good representative samples. No major problems, good star test and solid construction from a reputable manufacturer. Also, both are nearly new. 


Keeping everything on target, an AP-1200 mount was used for this evaluation Robin Casady's Triad bar with Losmandy and Casady clamping plates held the scopes. This allows both scopes to view and image the same object at the same time through the same air column. Between the two is a Tak FS-60c holding the CCD camera for the STV autoguider. On top of the FS-152 is a Tak FS-78 for some widefield imaging. 



Here are the specifications from various sources. Seems some specifications. for the TOA are hard to find or are outdated. I measured the weights of the TOA. It’s certainly a heavier scope. Especially with the 10 pound counterweight attached. 

SPECIFICATIONS for the FS-152 (Tube assembly only)



SPECIFICATIONS for the TOA-150 (Tube assembly only)



Goals:

I’ve heard a lot about false color in doublet APO designs so when I mention color I'm looking for a purple tint around the Moon's limb and white stars. It's very easy to see in an achromatic or even a run of the mill ED scope. Another item for comparison is sharpness. Some say a triplet APO is sharper than a doublet since the three primary colors come to a more precise focus. And then there is contrast. Fine APO doublets (especially fluorite doublets) have a reputation for very good contrast. . 

Some issues on the scopes: 

With any new products there is a chance for "issues"…. even with Takahashi APOs.

TOA 150: 

The focuser would not work at all with a camera and MaxBright diagonal. I took the cover off and shifted it slightly. This seems to work. It may have been binding the tension collar on the 10 to 1 side. 

The camera adjuster didn't work. You move it to match the position of the camera on the FS-152 and it wouldn’t tighten. Turns out the whole assembly was loose on the draw tube. Clamping the adjuster bolt down and tightening it was all it took to fix. 

When setup, this is a heavy scope. With the 10 pound counterweight, rings and a dovetail it’s nudging 50 pounds. With its sliding dew shield and smaller tube length it is still an easy scope to handle.

FS-152: 

Focuser drags to beat the band. I finally got it adjusted to "pull uphill" with a Tak diagonal and Canon DSL but the tube is very hard to move. This is with the focus knobs on either side. Makes me think I'm about to strip the drive gear. A lot of tinkering has it moving along well now. 

With rings the FS-152 is less than 30 pounds. But is it ever long. 54 inches before diagonal and extending the focus draw tube any length. The fixed dew shield also hurts portability. It’s not for an overhead bin in most airplanes. 

Cool down:

The TOA has a 10 pound counterweight attached to the rear of the scope. With the counterweight and the weight of the triplet lens cell cool down time would seem slower. The TOA did take longer to cool over several nights testing at various temps. drops. In order to quantify the rate, I used a RadTech thermometer and measured the surface temp of various points on the scope bodies in a three hour period. The lens temperature is from direct measurements of 4 points on the glass surface at the given time and averaged. The body temps are also four readings that are averaged. The FS-78 was easy to include and may help in comparing. For the TOA, the massive 10 pound counterweight circling the base of the scope also is included. I thought it would lag and hold the area of the scope it was in contact with at a higher temperature but it seemed to follow the temp drops in step with the other portions of the OTA. Larger scopes with more mass do indeed cool down at a slower rate. Even refractors. 



Visual:

Visually both perform well with the usual APO pinpoint stars and contrasty backgrounds. No problems with either on the Trapezium E and F stars, Alnitak's double (no flaring problems covering the double like I've seen on some other OTAs) and Mars looked great in both. (I know all this is easy stuff but if you can't do the easy stuff the hard stuff won’t be possible.) The triplet APO has the edge in fine color accuracy. Mars showed distinct markings and great color in the triplet while the doublet did not bring out the same detail and had a warm cast. Side by side with the same EPs (a Nagler 3-6 zoom really shows the detail here) comparisons were easy to make. The APO also seemed easier to focus or less critical finding precise focus even with the lower Focal ratio. Without them side by side over a long period I don't think I could rate one better than the other.

Even the legendary doublet contrast is not detectable using them side by side. However, the doublet FS-152 has a longer focal length. I’ve noticed longer focal length scopes don’t show as much contrast when compared to other shorter focal length scopes of the same construction/quality. The magnification dims contrast a bit under some seeing conditions and this may have affected the Mars observations. 

False color was checked on both OTAs using a variety of stars and EPs. At moderate power the results were the same in both with neither scope showing noticeable false color. I then put in an AP x2 barlow with a Nagler 3.5mm T6. This raised the magnification to 694 on the FS-152 and 628 on the TOA. The TOA going from outside focus to inside focus and back showed no false color. The FS-152 going from outside to inside and back showed minor greenish yellow on outside and minor purple false color on inside focus. As you approached focus on the doublet the color slowly diminished and when crossing exact focus the color seemed to melt away. At one very small sweet spot the doublet showed almost no false color. The triplet would be much easier to work with and less forgiving at these powers. However, seeing conditions would rarely permit this much magnification. 

At high power on the Moon, I went all around the limb moving through focus with both scopes. The TOA was rock solid with no visible color. The FS-152 doublet again showed a minimal green or purple tint as you traversed focus but again, right at focus, the color was very hard to detect. Using the Nagler 3.5mm I could just barely make out the faintest tinge of brownish green shading almost within the edge of the Moon at exact focus……. in both OTAs. The shading stayed with the EP and was not visible in a 7mm Nagler T6. Both showed remarkable detail and contrast with both EPs. 

The Double Double was also low in the sky and testing here would duplicate bad seeing conditions. Refractors are often said to beat seeing so this seemed a good object to have a look. Both scopes made the split/splits easily with the two Naglers. I then put in a 35mm Panoptic and couldn’t make the split in either scope. They were oblong but no clean split. Then a 10mm Pentax XW was tried on both scopes. With the target low in the sky the 152 doublet looked the cleaner split to me. Over and over I swapped the EP and moved through focus. The TOA was viewing at 110 power while the FS was at 120 with the 10mm Pentax. This might have had some influence but there was still less than 10% difference in magnification. Each time the close double just jumped out at you with both scopes but the 152 view was a tad clearer with just a bit darker background. A very pretty sight. 

I repeated similar test on both scopes over several clear nights. A week later under Moonless skies I did another star test for both. On Sirius they both looked great. Just a touch of color at 500 plus power in the doublet that seemed to go away at one critical focus spot. At a very small focus zone it would lose all color with a 10mm Pentax XW and all magnification positions of a Nagler 3-5 zoom. On progressively dimmer stars the diffraction patterns of both scopes were textbook. On Mars the FS doublet had just a hint of warm color while the triplet had lighter tints and was very natural looking. To my eye the triplet showed more detail and clarity. The legend of the doublet is well deserved and the best for it's time. But when Takahashi brought out the new and improved triplet.... it is an improvement. You pay for it in weight and cool down time but the benefits are there. Either one just beats anything I've tried yet for ease of use and results. The 6" APO has got to be the sweet spot of the market.

Imaging:

A few sample images are included below. Both scopes are easy to image with. The TOA has a much better camera angle adapter. The FS-152’s camera angle adapter has three small knurled knobs screwing into a “V” grove on the draw tube. The TOA’s angle adapter has one knob and a very positive feel. The FS-152 has slop when you loosen the knobs. I can’t help worrying about loss of critical focus when adjusting the FS-152. It seems to hold but doesn’t “feel” right when adjusting. For imaging, focusers are adequate on both after some adjustment. Nothing special and no special feel. A FeatherTouch or Moonlight upgrade would help both in the “Look and Feel” department. 

On a Canon DSLR size chip, the TOA needs a field flattener while the FS-152 stays sharp to the edge. While not as obvious visually with a widefield EP, you can see the oblong stars below. 


Cameras and focus:

A Canon 20Da DSLR (Digital Single Lens Reflex) camera and a Happ Griffin modified Canon 350D DSLR are used on most objects. Where the extra IR response of the modified Canon 350D isn’t needed a stock Canon 350D may be used. Focus is set on both with a Stiletto focus aid and confirmed with the 20Da “live focus” feature at the FC-2 setting (most magnification). Focus is rechecked after every image run if the temperature is dropping. 

FS-152 image of the Double Cluster. Lower left magnification is of upper left portion of image.



TOA 150 image of the Double Cluster.



A side by side Moon Image:



Moon limb:



FS-152 Deerlick Group image with TOA-150 central galaxy superimposed.



Conclusion:

Overall, these things are so close it's scary. Just the smallest bit less color in the TOA. The camera adjuster is worlds better on the TOA. Functions like it should. The FS-152 camera adjuster is less secure and flops the diagonal when loose. The TOA is a nice size and has a weight similar to a Celestron 14” SCT. The FS-152 is huge and weighs similar to a Meade ETX. The FS-152 doublet is no longer in production so the used market is the only source. The TOAs are off the shelf available. A real plus when you want to get into the 6” APO world without a substantial wait. Which is my choice? I’d say either one. They are close enough to continue long term testing and comparing to other scopes before deciding. Maybe a slight edge to the TOA right now. But that FS-152 is just plain classy and cool. 

Astro-Physics 155 F/7 Starfire EDFS APO Refractor vs. Takahashi FS 152 F/8 APO Refractor

https://www.cloudynights.com/articles/cat/user-reviews/telescopes/140mm-refractors/astro-physics-155-f7-starfire-edfs-apo-refractor-vs-takahashi-fs-152-f8-apo-refractor-r866

The Current 'Big Guns':

This is a review and comparison of two of the larger and better currently available "APO" refractors. There are others that can be ordered, such as the Meade 6 and 7" APOs, but they have not fared well when viewed by others and do not command the respect of these two telescopes. The TMB refractors are coming on line, but only a handful of the 6" and larger TMB scopes are in this country, and none are currently available for testing. That leaves these two 6" APOs as the 'top of the heap' in refractors one is apt to encounter for sale, or to view at a star party. They are, in addition, both remarkably alike yet quite distinct at the same time.

Physical Description:

The Takahashi FS 152 is an air-spaced doublet, with the outer element composed of Fluorite and a focal length of f/8. The OTA is supposedly 54.75", but measured closer to 58" from the end of its rigidly mounted dew cap to the compression ring at the end of the focuser when I checked before I purchased a custom case. All of the 152s come with a rotating, 4" focuser. The OTA weighs 24 pounds.
The files with the photos of the 152 became corrupted, so I can't post a photo as part of this review. Picture an FS 102 or a 128 in your mind and then fatten and lengthen the tube. The tube is gloss white and the focuser, tube rings (a massive and expensive double ring and bridge assembly) and other mechanical parts are anodized in the traditional Takahahsi lime green.
The Astro-Physics 155 is an oil-spaced triplet, using super ED glass and a focal length of f/7. The OTA measures 41" with the dew cap stored in its retracted and reversed position. The OTA weighs 23 pounds in the EDFS version with the 2.7" focuser. (The EDF version uses a 4" focuser and comes standard with a field flattener. That version weighs 27 pounds.) The mechanical parts are black anodized, as can be seen in the attached pictures.
The difference in length is not as great as the statistics would indicate. The extra length of the Takahashi is caused in part by its fixed, non-removable and non-retractable dew cap. Once extended, the only real difference in length between these two 6" APOs is found in the slightly shorter, 'faster' focal length of the AP.
'Hefting' both scopes with the dew caps extended, there is little to chose from in feel. The slightly longer Tak feeling more nose-heavy even with the doublet objective versus the triplet lens assembly at the front of the AP. The Tak seemed a tad more awkward to maneuver than the AP, noticeable in mounting and dismounting the scope.
Fit and finish on both scopes was hard to fault. The AP I own is one of the older models with the smooth, glossy white finish. Compared to my 130 f/6 with the 'new' pebble-grain white finish, I prefer the older, smooth style. While both scopes look great, I would give the Tak the edge in ultimate finish, paint and mechanical, but with the AP nipping at its heels.
The Tak end cap is a piece of relatively heavy, cast (?) aluminum, with a removable disk at the center to let you 'stop down' the scope if you wish. The AP uses a plain, black- anodized end cap. While the Tak is wonderful to look at, it is overkill, and justs adds to the nose heavy feel of the scope. Point to AP for substance over style on this one. (Again, personal preference issue.)
The AP comes in a vinyl-covered, wooden case. A focal extender and 1.25" adapter comes with it. The Tak, a lot more money to start with, requires you to buy the case extra.

Use - Mechanical and other Non-optic Issues:

The Tak focuser is the clear winner here. Even though the AP is smooth, and I prefer the 2.7" for non-photographic use, the Takahashi 2.7" as I used on my 102 and 128 was simply more precise in feel than the excellent AP 2.7. The Tak 4" and the 4" AP (which I tried on a friend's EDF) are both noticeably more 'stickly' and take more effort to use, with the Tak coming on top here by a still-slim, but slightly more distinct margin.
The Tak uses the more traditional compression rings on the standard extension tubes. The AP offers its brass, internal compression rings on the standard 2"/1.25" adapters. Point for the AP. (I used an AP Maxbright 2" diagonal on both scopes, so the everyday use was a tie.)
The AP mounts with the traditional 'clamshell' rings, quite easy to use in an EQ mount or in the Gr-2 (Standard) as shown in the picture. Getting the OTA in and out is simplicity itself. Rings are fairly inexpensive.
The Tak uses an elaborate double ring, 'bridge' setup that is nearly $700 (!) and quite heavy. Getting the tube in and out, particularly at night, is a comparative nightmare , since the rings need to be carefully opened, the tube lifted out, and the entire assembly unnecessarily complex. Another point for the AP.
I owned the Takahashi first, trading the FS 128 and an EM 200 mount for the larger 152 and an NJP mount (having been told that the EM 200 was marginal for the longer and heavier Tak 6".) The NJP is a superb mount, and for photography with the 152, a clear 'win' for the Tak. However, I am purely a 'visual' guy and, courtesy of Uncle Sugar and the good ole US Army circa 1969, my back is not up to hefting anything too heavy. The NJP and the 152 was a beast to move and setup. The 152 tended to be used quite little since I was not usually in the mood to 'rassle' 50 or 60 pounds of mount, tripod, and then 24 pounds of scope out for a night of observing. Given my touchy back, I wanted an easier 6" to set up and use.
I acquired the 155 for some smaller scopes a friend wanted and cash. The idea was to get a 6" scope that I could use on an EQ mount if necessary (I have a G-11 and a Mi-250) or on an Alt-Az if I could find one that would hold a 6" and work reasonably well for visual.
That chance came a week after I got the 155. Shown below is the AP 155 set up on the APM Gr-2 (Standard) mount as reviewed elsewhere on this site. The mounting plate was purchased from Anacrotes, who sells it as a plate to use with their WYO refractors. I bought several, and have them set up with tube rings for my TMB 100 f/8, the AP 130 f/6, the TV 140, and the AP 155. As you can see from the photo, the plate attaches to the mounting head and goes on and off with two 7mm Allen bolts. Switching or mounting a scope is a two-minute job. Bolt in the appropriate plate and rings, open the rings, put in the OTA, and away you go.

The standard version of the GR-2 mount is rated at 25 pounds. The 155 worked fine, although it was clearly at the limit of what the standard version of this mount would hold. (I noted more vibration and a general 'touchy' feeling with the 155 that was absent when the lighter AP 130 and the TV 140 was used on this mount. It worked fine, but needed a second to settle down with a load at the ep end. It did settle down very quickly, however. The Deluxe version that is on its way to me should handle the 155 much better and will, according to what I have been told, be less sensitive to vibration as it is rated at 50 to 60 pounds rather than half that weight for the standard version.)
So the 155 would be a better scope for me to own for purely personal reasons. Now, what about the real test - optics?

Outside and Test:

(I acquired my 152 over the Winter, and had the chance to test it on the Gas Giants. The 155 arrived after they were long gone, so this commentary will restrict itself to deep sky and lunar.)
The Takahashi doublets have been treated with disdain by some as having 'too much color', lacking in the ultimate optical ability of the AP triplets, and otherwise simply not 'in the same league' as the Astro-Physics products. Starting out here, rather than at the end, I can say that whether the 152 I owned was an exception, and others are 'worse', I found the Tak to be an outstanding performer. I say that after having spent enough time using the AP 155 to compare these two scopes. As the 155 AP I now own was previously in the hands of a more experienced observer (who said it was a great example of the 6" AP) and as this same scope had been tested by a well-known optical designer at AstroFest a few years ago, and given his 'seal of approval', I know I don't own a 'dog.' So, assuming my Tak was typical of the 'breed', lets have a dog show.
The Tak does indeed cool down faster. Ed Ting's observations are correct. The AP has a fair amount of glass up there, and the oil-spaced objective needs a lot of time to come to equilibrium. Star testing the AP when the Tak was cooled down showed tube currents waffling through the image. Once both are 'ready', it is tough to pick one over the other.
Deep sky is also a toss-up. Both split doubles with contemptuous ease. Double Double and the Ring Nebula show almost the same through the same eps. Both scopes reach 'deep.' In comparison to a 5" scope (using the FS 128 I owned before and the 130 AP I own now as a benchmark) there is a better image scale and 'reach' that is very real and very noticeable. While neither scope can match a good Dob (my 11 EL Starmaster kicks both of these scopes in the chops on deep sky) deep sky, clusters, and doubles are sensational compared to smaller aperture refractors.
* * *
[A quick digression on aperture in refractors:]
Let me stop here to address the common rubric that while the step up from a 4" to a 5" refractor is quite noticeable, the step up from a 5" to a 6" is not the same magnitude. I agree as to the former, having experienced it myself when getting the FS 102 alongside the FS 128. However, and I am sorry to disappoint you when I say this, but while the difference in cost moving from a 5" to a 6" is a big step, so is the improvement in image scale and 'reach.' I have had the two AP scopes side by side, and the 155 is visually FAR more impressive than its smaller 5" brother. (The issue becomes muddied when the TV 140 comes into the mix. Yes, it has more 'oomph' than the 130, as I noted in my review. Does the 155 'walk on it?' No. There is a difference, but not as great as between the 130 and the 140 in a 'side by side.' Too tough to call.) Of course, as the price difference between the Tak 128 and the Tak 152 is nearly double, if not more, then the scorecard may indeed shift the decision back to the 5". The AP 5" and 6" are much closer in price, so the equation shifts the other way in that test, IMHO.
* * *
Lunar? AP wins. 'Sharpness' and contrast are a tossup. Both give stunning views and soak up stupid amounts of magnification. (Both would hold a 5mm Takahashi and a 2.5 Powermate on Plato. If I did my numbers right that is 695X for the Tak (1390 divided by 5 times 2.5) and 542 for the AP (1085 divided by 5 times 2.5 And that was condition limited, not optically limited.) Both scopes took magnification well. Contrast on both scopes was outstanding.
Why then does the AP 'win'? On really bright nights, the AP shows no color at or off the edge of the lunar disk. Stars just beyond and behind the Moon stand out with no 'bleed over.' The Tak did show just a trace at the edge.
Optically, the only real difference is that the Tak is a hair easier to snap into focus. Perhaps it is a characteristic of an oil-spaced versus an air-spaced system, but I noticed the same thing testing the TV 140 setup next to the AP 130 f/6. Neither AP is difficult to bring to focus, but the ari-spaced Takahashis and the TVs seem to snap in more 'crisply'. It is a bit easier to go past focus and then have to come back in the AP than the Tak. (I noticed the same testing my air-spaced triplet TMB 100 f/8, so I assume this is in fact simply something inherent in an air-spaced versus an oil-spaced design.) Having said that, however, it is indeed a completely minor point, and not a problem in 'real world' observing. Just a nit to pick, not a problem at all.

Conclusion:

Two great scopes. Everything you have heard about the 155 AP is true. However, forget all of the nonsense you heard about the 'big' Takahashi, it is bull. Both are comparable performers. I traded my 152 as part of the deal that brought the TV 140 to me. My decision to trade it, and acquire the AP in its place, was personal and not related to 'better' or 'worse' at all.
If you have read any of my other reviews, you know that I am fixated on mounting the largest possible refractor on an AltAz mount. The AP 155 EDFS is just a scoosh (yes Brian, it is a 'David' word, not to be found in the dictionary) smaller and lighter than the Tak - albeit attributable almost entirely to the nature of the dew cap and because of the smaller focuser. When a chance to get the TV 140 came up, and the other guy wanted the FS 152, I traded what could be replaced if I wanted to for something a whole lot harder to acquire. And, once the 155 was 'up and running' in the Gr-2 (and with the Gr-2 Deluxe on its way in) the 152 is simply a fond memory. But it is indeed a fond memory, and a scope you should consider if the opportunity arises.
The AP 155? Great scope. I am a novice in comparison to Todd Gross and Ed Ting. I echo everything they say about this remarkable 6" refractor. Also a scope you should consider if the opportunity arises.
It has been a privilege to own two of the best. I would be pleased to own either one again if the situation arose, and would urge the same if any of you find yourself in the market for a superb refractor.
As always, thank you for listening to my ruminations. 

4" Apochromatic Hyper Shootout by Daniel Mounsey

https://www.cloudynights.com/topic/100005-4-apochromatic-hyper-shootout/page-11#entry2381946

INTRODUCTION:

This review is only for the cloudynights. I have decided that I have no intent to share it anywhere else as long as CN wants to keep it, and the review can stay in it's unedited form. Today we will compare 4” refractors on an unprecedented level. We will reveal which ones were good, which ones were great, and which ones were at the absolute pinnacle in a side by side, visual shootout. This was a monumental task and I’m glad it’s finally over because after finishing it, you guys are on your own. There may be a number of clerical errors here and there, so forgive me, I wrote this myself and it's a lot to write.

I wonna thank Farah Payan for her strong support. I could never have done this without her. I’d also like to thank a great observing buddy of mine, June Trajano, who’s always participated in these types of tests over the years and offers valuable input for me. June and I have been observing for quite a while and I’ve always respected his opinion and critical eyes. I’d also like to thank Ridwan Angkasa for spending so much time conducting tests. Ridwan has an amazing ambition with visual testing and I have a great deal of respect for him. I’d also like to offer a special thanks to all the guys who assisted with loaning their telescopes in order to make this review a reality.

NOTICE

The reason this review was so delayed is because I had second thoughts about posting it. I have to set an example because of what I represent with cloudynights and this industry and it's a huge responsibilty to take on because of who I am. It is extremely difficult to go in open forum and lay it all on the line as I've done here. It is not my intent to bash any company and I've tried to be as constructive, yet critical as possible. This must be clearly stated.

THE CONTENDERS FOR THIS PARTICULAR REVIEW

Some of these refractors were tested side by side, while others were tested during other periods. In some cases we had multiples of the same model. This would allow us an opportunity to see how consistent they were. I’ve tested various other 4” refractors on numerous occasions, but they were not picked as part of this comparison. Note that OTA stands for (optical tube assembly).

Antares 4” F-15 achromat
Orion 100ED
Takahashi FS102 (lost count)
Takahashi FC100 (lost count)
Takahashi TSA102 (four units)
Takahashi FSQ106 “Q” (two units)
Televue NP101 (two units)
Televue 101
Televue 102IS
TMB102
TMB115
Vixen 103ED
Vixen 100ED
William Optics FLT110/TEC optic
William Optics FLT110/TMB optic design (two units)
William Optics Megrez 110

Some observers asked to have the Stellarvue refractors as part of this comparison and I was offered to barrow a couple. This review could be given an update if I set the time aside to do so and people want it enough. If there is a telescope you do not see here that you were interested in, don't worry too much. Many of today's refractors are coming from the same plants over seas with different names stamped on them with a few cosmetic changes. This is why new brands are popping up all over the place. If you still have questions on a 4" refractor not tested here, then I'll try and offer some insight if possible.

COLOR CORRECTION AND CONTRAST HYPE

There are a good number of observers who appear to be under the impression that refractors, which exhibit some minor false color on stars, have less contrast than ones that doesn’t. I can assure you this is not always the case and in my opinion, it sends a red flag about the observer’s judgment and experience regarding the true quality of the telescope. There are various other factors, which could also potentially influence the contrast. One of the things I look at is the amount of spherical aberration the optic has or whether there are zones in the star test. There are give and takes to all the possibilities in fact there is no such thing as an optic that doesn’t have an aberration. Even eyepieces can introduce false color. How much of it we are willing to accept is probably what matters most, therefore I wouldn’t suggest you write a refractor off because someone tells you it exhibits a bit of false color.

I’ve seen a surprising amount of experienced observers do this without even qualifying the instrument in a number of other important ways to be sure about the true quality of the telescope. I will also tell you that there are even long achromats with wonderful contrast that very few have had the opportunity to look through. A decent refractor that is properly made has the potential to produce beautiful image quality on deep sky and planets whether it’s a doublet or triplet. I don’t want to give the impression that having excellent color correction is not an important factor but more so, to help prevent beginners and even some experienced observers from being so overly critical with it, that it clouds their overall judgement and it has easily proven to do so in many cases. If I had two refractors, which produced good images and one of them had less false color than the other, then of course, I’d pick the one that had less false color.

OH MY, THERE’S A SPECK OF DUST IN MY NEW OPTIC

The psychological effect of a few dust particles, which have absolutely no effect on optical quality are far less important than the possibility that the optic you already possess, may be that extra special scope out of the batch. In other words, you are blowing a perfectly good opportunity, which very few have, to discover that you may or may not already have an exceptionally great optic. In my opinion it’s a foolish mistake to send a new telescope back because of a few specs of dust without even testing it for something far more damaging called spherical aberration. Unfortunately though, there are some cases where the amount of dust is unacceptable as you are about to see.

JUDGING CONTRAST

I would describe contrast as a striking dissimilarity in pigmentation between features. Pretend we have two telescopes of equal aperture. Should we assume that because one telescope yields a darker background, that automatically means it has higher contrast? In my opinion no. Assuming both telescopes are of equal aperture, it’s quite possible that one instrument may not be transmitting as much light at the eyepiece for whatever the reason and you could mistakenly interpret that to mean it has higher contrast. A better way to test for contrast is to point both telescopes a star cluster for example and observe how the fainter stars appear in each instrument. If one telescope is revealing the faintest stars just as brightly as the other instrument and it still yields a darker background, then it’s probably safe to say it has higher contrast.

HOW DO YOU KNOW YOU HAVE A GREAT OPTIC?

The simple answer is that you don’t no matter what kind of glass it has. Even for opticians, it can be difficult to fully predict how well the glass will behave when exposed to various climates in the field when the telescope is under scrutiny. I’ve tested unacceptable refractors from all the best companies in the world that range from 80mm to 200mm. In some cases, very few of the same brand of refractor will perform exactly the same. I’m sure it’s similar to the way two of the same brand of guitars sound to a purist. They may sound very close, but very few will sound exactly the same.

THOMAS BACK’S STAR TESTING ESSAY

I personally prefer not to state how bright a star should be or what magnification you should use during the star test, there are too many variables involved here. With that said, you will have to feel out what works best in your particular case, but one of the best essays I’ve seen was written by Thomas Back of TMB Optical who sadly, is no longer with us. I strongly urge you to take the time to read this, and you will have a better understanding of what to expect out of your own refractor. Back also explains the importance of using color filters during the star test in certain refractors.

http://www.tmboptica...d.asp?cat_id=31

HOW I TEST OPTICS USING THE AIRY DISC

There are a number of things that should also be considered but in my opinion, this one plays a significant role on how I judge an optic and this is one of the things I examine. Just about any refractor can reveal an airy disc when the air stability is good, even if the optic has a number of optical aberrations, but there’s an exception. What you don’t want to see is that extraneous junk around the airy disc while the star is in focus regardless of whether it's a doublet, triplet or quadruplet. The same rules apply to all of them. This unfocused light will have a direct effect on how much sharpness and contrast a planet will appear to have at higher magnifications.

The airy disc is simply the concentrated light from a star, focused to a single point in the eyepiece. What you should see is the airy disc, along with a few faint and ill defined outer rings, which trickle in and out while being viewed through Earth’s atmosphere but this will also depend on the brightness of the star and the seeing conditions. This is the sign of an excellent optic in its purist visual state. Whenever I examine the quality of any refractor on a good night, this is one of the things I’m looking for when the star is in focus.

THE STAR TEST AND UNDER-CORRECTION

You'll notice that I focus on this quite a bit because it's common to see it. Under-correction occurs when light rays from the outer parameter of the optic converge inward faster or closer than light rays from the central area. The symptom is typically a fuzzier picture with a brighter central core and a less prominent outer ring while outside of focus. Over-correction is just the opposite.

One can tell if too much under-correction exists, even while focusing on a planet, it doesn’t even have to be a star! Two refractors may appear very close to the same under the seeing conditions most observers endure, but there are still going to be slight and possibly even severe differences in sharpness and contrast on the better nights of seeing which purists will appreciate at higher magnifications.

IS UNDER-CORRECTION COMMON

Yes. It’s very common for an optic to have some degree of under-correction, in fact a refractor simply by its nature will usually be in this state as it acclimates closer to the surrounding temperature and even then, it can exist, so don't panic every time you see this. The key is learning how much is acceptable. Some of the highest quality refractors in the world will show some degree of this while they acclimate.

A good 8” triplet can take as long as three, whopping hours before reaching its best spherical correction, depending on the temperature drop and the behavior of the glass. When a refractor reaches this state, that’s when it really begins to shine and the most subtle planetary features come alive! I’ve even seen the same instrument produce slightly different star tests on different nights because of the different climates the optics must endure. Even eyepieces can influence the star test, so I’d suggest you approach this with a very open mind and take your time. I personally prefer Naglers for star testing on axis.

Test your telescope over the course of several nights and examine how the optic behaves on average when the temperature and seeing conditions are still in question. It’s frustrating when impatient observers expect results right away. Bad seeing conditions can mimic aberrations or under-correction because as you rack the focus out, the rings are typically focused over turbulent air which can smear them. Jet streams and bad seeing can easily be verified by pointing the telescope at the Moon or planets. Rack the focus slightly outward and you will probably see a jet stream flowing across the field.

WHAT ABOUT OPTICAL CERTIFICATES

I remember a person who was adimant about getting an optical certificate with his refractor. I could tell he didn’t have much experience evaluating optics himself and any visual observer who knows this, soon finds out that a document doesn’t necessarily answer this question. Many observers seek answers in optical certificates in order to feel justified in paying the big bucks, or they just think it will determine whether they have a good optic or not. If that were the case, then there are some odd certificates floating around. In my opinion, this is something you should learn to do on your own. As for me, optical certificates serve little purpose. I can test the telescope myself over the course of a few nights, depending on the conditions and tell quite easily if it’s actually as good as the papers claim.

I’ve seen optics, which may seem impressive on a document go astigmatic in the winter seasons. On paper, everything looks nice but glass usually has a personality of its own when exposed to varying temperatures. What takes no prisoners is good seeing, steady temperatures, determination, guts, skill, patience and a keen eye because in reality, these are the things you'll need in order to see what a scope can really dish out. If you don’t think your eyes are keen enough, then I see little reason to be so obsessed with the issue. What you don’t see wonte hurt.

WHICH IS BETTER, DOUBLET OR TRIPLET

Any refractor that is properly made, has the potential to deliver fine images regardless of whether it’s a doublet, triplet or quadruplet design based on my personal experiences with all of them. I would not concern myself with the topic of extra glass but more so, the issue of the steep, curved shapes of the glass. By this I mean that having all these pieces of glass working in harmony with eachother to extreme tight tollorances as they do, is a monumental achievement when it's pulled off! Today’s coatings and figuring technology are absolutely amazing when you think about it.

My leaning towards longer doublets has more to do with their behavior under climate change and the forgiveness they have regarding collimation. Triplets are nearly impossible to realign, should the elements accidentally shift out of place even just a tiny bit. There is absolutely no room for error. Doublets are user friendly and adjustments between the elements themselves can even be made at home in some cases. Ridwan Angkasa actually does this.

WARM VS. COLD

This is one of the main issues I addressed some years back in a planetary eyepiece review because I noticed that it was constantly being overlooked by even some of the most experienced observers in the world and it was a topic that was not tapped into yet, or at least as far as I know. I also believe that the topic needs some scientific study but from a visual standpoint, I’ll express what takes place. There are some cases where either the glass or possibly the coatings will influence the images seen in a telescope or an eyepiece. I have come to find that most purists have a bias for cold images.

Warm is simply a term used to describe an optic that has a slight coffee tone or yellowness, while cold represents a bright, white or crystal clear image that is completely neautral. We can think of cold as favoring the blue while warm favors the yellow. For most deep sky targets, I prefer an optic that produces cold images, with the exception of viewing Jupiter in particular and sometimes Saturn but it also depends on the magnifications used, particularly with the rings.

If you take an 82 wratten light blue filter and view Jupiter, you’ll notice that Jupiter’s equatorials belts will become darker and therefore you may interpret that as having more contrast. But, there’s a negative trade off that must be considered. The trade off comes at the cost of losing some of the color fidelity the planet has to offer because Jupiter’s belts now take on a more monochrome appearance. This is one of the reasons why I actually don’t like images to be cold while viewing Jupiter. I still use Televue plossls as a planetary eyepiece for Jupiter because they are slightly warm. They are the only eyepieces in production that have a warmer tint to them while the Clave of Paris are the warmest I’ve ever seen. Telescopes behave in the same manner.

Some observers misunderstand how filters behave because they just expect them to make features pop into view. In order for a filter to work, the feature under scrutiny needs to be visible to some reasonable degree first before the filter can accentuate it. I personally can’t stand filters because most of them are so much darker than they need to be and many of them ghost too much, probably because they need good coatings. With filters being as dark as they are, they take away the natural color and beauty planets have to offer. There are some cases where highly experienced visual observers like Carlos Hernandez or Sol Robbins benefit from them and that makes perfect sense because they're more interested in documenting a specific feature and filters can sometimes help in this case.

I sometimes use a very special 48mm warming filter and a #82 light blue filter for planets made by B+W optics of Germany. They are the only brand of filters I use. Other than that, I don’t use color filters at all. I often use the warming filter on Jupiter and don't always have to be as concerned whether or not the eyepiece produces the warmth I want. Every observer is different, so it just depends on what you like.

CHECK YOUR DIAGONAL

Being involved sales, it doesn’t take long to notice what people are sold on. As soon as they hear the term 99% dialectric! they automatically assume it’s a great diagonal. This has become a big marketing strategy. Observers should be aware that many of these diagonals are mass produced over seas and just because it’s a dialectric diagonal doesn’t mean it has a smooth figure or that the application of the coatings is great either. This is often overlooked because people have become so obsessed with hearing the term “dialectric”! The precision or accuracy of the glass should not be ignored and the telescope is only as good as its weakest link. I'm not suggesting you become obsessed with this, I'm merely indicating you be aware of it. Not everyone can afford special diagonals.

The only diagonals we used for this particular comparison were two different Vernonscope diagonals and two Everbrite diagonals from Televue. My personal favorites are the Vernonscope models and the Baader Planetarium prism. This opinion is based on a number of very careful side by side comparisons that are not part of this review. No other diagonals were to be used in this comparison only because I wanted to keep everything as simple as possible. Sometimes we would even switch them around just to see if they introduced any positive or negative results. They were all very good.

EYEPIECES

Since I’ve been pretty impressed with the Pentax XW line and Nagler T6 series lately, I decided that they would be the only eyepieces used for this comparison and no others, mainly because of their short focal lengths and comfortable eye relief for these evaluations, particularly the XW’s. Focal lengths ranged anywhere from 3.5mm on up to 13mm. By the way, I highly recommend plossls or high quality orthos with good glass and optical coatings for planetary observations.

WHY I PREFER LIGHT POLLUTION

These tests all took place from a bright city. Observers often think that light pollution hinders planetary observations and it's probably the biggest myth of all time in astronomy. I actually prefer light pollution while viewing planets, it’s more soothing on the eyes and in some cases I’ll even leave an ambient light on as long as it’s not shining directly into the eyepiece. The reason I do this sometimes is to help prevent my eyes from becoming dark adapted. One of the worse things to have is a dark adapted eye while viewing planets. There are technical reasons for this. My perception of color and sharpness are usually improved this way and the best views of planets I’ve ever encountered were right at sundown, as soon as the planets first become visible and no stars are even visiable. This helps reduce light scatter, caused from overwhelming contrast and sharpens planetary edges. This fact has also been shared by many expert planetary
observers.

LETS GET DOWN TO BUSINESS

On the evening of February 24th 2007, June, Ridwan and myself set out on a quest to find some answers about today’s 4” apochromats. The tests would continue for the next year. This particular night would grant us seeing that was an 8.5 on a scale of 1-10 and it would be Ridwan’s first night under real steady skies. Although Ridwan was new to these comparisons, his eyes are alarmingly trained since he's a professional wedding photographer and teaches me more about colors then I'll ever understand. We had several apochromats from various companies.

ANTARES 4” F-15 ACHROMAT vs. ORION 100ED

We started our first comparison with the more affordable models here. The Antares achromat is a pretty scope to look at with its 1500mm focal length. I don’t know what it is with these two scopes, we just had so much fun with them. There’s a feeling of history I get when I look at the Antares 4” F-15, which is the intension Antares has. We first started out by giving all the scopes some ample time to settle down. We then paired the two scopes up side by side on an EM200 mount. We used an 11mm T6 and 7mm XW in the Antares to get 136x and 214x on Saturn while the 100ED had a 7mm XW and 5mm XW to give 143x and 200x. We would play with the magnifications and switch out eyepiece to clarify any issues like warmth or coldness in the image.

The first thing that surprised us all was how sharp the Orion ED100 was on Saturn. The Antares gproduced a more natural and beautiful warmth to the image, so we switched to the Pentax XW’s to see if the Nagler had any influence on this and it was definitely the optic of the telescope itself. The Orion 100ED continually pumped out a tighter and sharper image and this really surprised us all. If anything, I would have expected the Antares to at least equal or slightly surpass the 100ED in sharpness. We switched diagonals for clarification too. Even with the Orion 100ED at slightly higher magnifications, it was still about 7% or 10% sharper than the Antares in my apparent visual estimation and everyone agreed. Some observers say you can't see a 7% difference, oh well. June and I were both still impressed with the appearance of a more natural or colorful appearance in the Antares, but this was purely cosmetic and I actually prefer this effect more so on
Jupiter.

We also noticed that the background in the Antares was definitely darker than the 100ED, as if it had more contrast, but the moons around Saturn were not as obvious and we would soon find out it was not a gain in contrast, but more so, an actual loss of light from lack of better optical coatings in my opinion, at least on this particular unit. I believe that if the Antares had better optical coatings, it would have taken it up another notch in performance. I looked at the objective coatings and noticed they were very thin and it was easy to see my own reflections in them. A good amount of multi coatings makes it harder to see your own reflections. The moons around Saturn in the 100ED were more distinct while they appeared dim or in & out with the Antares. Over all, we agreed that the Orion 100ED was the winner here. Honestly, the Orion is fantastic for the money and an absolute bargain in my opinion. The color correction in both scopes were good, with
the Antares having a slight bit more of false color. This can sometimes fluctuate with the seeing but it was a steady night overall. June and I really loved the Antares and I'll bet that if we had another unit, it's quite possible that it could have done better. I would still highly recommend the Antares and would be happy to own one myself.

1st place Orion 100ED, 2nd place Antares 4" F-15

VIXEN 103ED vs. VIXEN 100ED

Vixen’s been around for a long time. I’ve always liked their older fluorite 102’s and even their 102 achromats back in the day. If you can find one, I highly recommend them. Those ones carried the Celestron name but were true Vixen’s underneath and observers should not under estimate them either. The Vixen 100ED doublet is basically the same scope as the Orion 100ED with different cosmetics but each one happened to perform very similar, which is quite an accomplishment if you ask me. The 103ED is another thing in itself. The 795mm F-7.7 103ED is Vixen’s flagship model at twice the price of the 100ED. When comparing the two scopes on Saturn, there were some interesting differences worth mentioning but we all still had some mixed thoughts here. We pushed the 103ED to 160x and the 100ED to 143x and 200x. We later found that the color correction was a bit better in the 103ED compared to the 1000mm F-10 100ED. The images were also noticeably brighter, probably due to better coatings, but what we really found odd was the background contrast, noticed by Ridwan. For some strange reason, the field of view around the very edges were greyer in the 103ED, then got darker going inward and brighter around the planet.

It’s not unusual to see a bit of light scatter around a planet, but the overall contrast did not appear as uniform across the entire field of view. We switched eyepiece focal lengths and diagonals to be sure, and it was coming from the scope. No matter what we did, the contrast was not uniform in the 103ED and this was the only telescope in this review that did that. Regardless, we all really enjoyed both these scopes and highly recommend them. During the evaluations, June gave a slight edge to the image in the 103ED because the light through-put was a bit better and even though the contrast was not as uniform across the field, the overall planetary color contrast was still a bit better than the 100ED and we all agreed.

The most astonishing thing though was some of us were still impressed with what appeared to be a slightly sharper image in the 100ED at 200x. Even at this higher magnification, it was a bit sharper than the 103ED at 160x! I was pretty surprised, especially since they both had ample time to cool down. I just can’t help but think what an amazing value these little 100ED’s are. Both of these scopes were fabulous though. Unfortunately I did not bring a different 103ED to the shootout, but I might test them both again.

So far, we have this particular Vixen 103ED, Vixen 100ED and Orion 100ED tied for 1st place and the Antares in 2nd place.


WILLIAM OPTICS FLT110-TEC vs. TELEVUE 102IS

This particular apo from William Optics utilizes an oil/gel spaced triplet lens made by TEC and is housed in an OTA by William Optics. We had a few other OTA 's set up on this particular evening. One was a Televue 102IS, Televue NP101 and a TSA102 from Takahashi. The first target was the Trapezium in Orion's nebula. From my location, there’s quite a bit of light pollution and I'm limited to about magnitude 4.5 naked eye visibility, but as I stated before, the seeing was excellent. The FLT110-TEC has a bit more light grasp than the other scopes but there’s a twist to this, so hang tight. The first time I looked through this instrument, I knew this comparison was elevated to another level. The contrast was stunning and we could resolve six stars in the trapezium as clean, little airy discs with no junk around them at 143x. Ridwan wasn’t able to see the E and F components at first, but once he was shown a diagram
from Burnham’s Celestial Handbook, he immediately saw them. Most observers will tell you that it makes a difference when you train your eyes where to look.

Next, we fired the Televue 102IS at the trapezium using magnifications of 125x and 176x. Although we could still discern the E and F components, none of us were as impressed with the image as the stars trickled in and out of focus. In other words, the airy discs did not appear to be as pronounced in the TV102IS. On a more scrutinized level, there was noticibly less light concentrated in them and a bit more scattered outside. The contrast was also not nearly as striking as it was in the FLT110-TEC and everyone agreed.

The four brighter components revealed airy discs in the TV102IS, but they were still not as defined as they were in the FLT110-TEC and it was obvious that it was not caused by the slight differences in aperture, but more so, the actual optical quality. Most of the stars energy should be concentrated into that airy disc. We used various magnifications in both instruments and the results were conclusive. BTW, the airy disc and fainter, ill-defined rings in the FLT110-TEC appeared text book perfect!

We then fired both scopes at Saturn and once again, the FLT110-TEC clearly prevailed. It revealed a sharper image overall and a staggering 20% more contrast than the TV102 in our apparent visual estimation. This was obvious while observing the subtle, but darker belts on Saturn, as well as the rings. The TV102 looked softer in comparison. This was unquestionably a direct result of the scattered light we noticed around the airy disc during the in-focus star test. In case you are curious to know, the TV102IS did exhibit some minor false color on Saturn while it was harder to detect in the FLT110-TEC.

This now pushed the FLT110-TEC into 1st place, with the Vixen 103ED, Vixen 100ED and Orion 100ED in 2nd place, the TV102IS in 3rd place and the Antares 4" F-15 in 4th place.

Now I realize that some of you may be shocked to see the TV102IS behind the 100ED scopes, but there is no bias in this review. We called it like we saw it and I'm sure that had I tested another TV102, the results probably would have been better. I've actually tested other TV102's that were actually better than this particular one, but we did not have them for testing side by side at the time.

WILLIAM OPTICS FLT110-TEC vs. TELEVUE NP101

Next, It was time to compare Televue’s flagship NP101 to the FLT110-TEC. During our tests, the color correction on brighter stars was a tad better in the NP101 but once again, the in-focus star test was slightly superior in the FLT110-TEC. The NP101 produced an airy disc which was surrounded by less light scatter than the TV102, but still more than the FLT110-TEC. We then fired both scopes at the Trapezium using 154x in the NP101 and 143x in the FLT110-TEC. We could see all six stars in both scopes but once again, the contrast was still noticeably superior in the FLT110-TEC. I seriously began to wonder if we even had anything that was better than this incredible optic from TEC and I can definitely say it is one of the finest 4” apochromats I’ve ever tested and Ridwan had a keeper since it belonged to him.

We then compared Saturn in both scopes. The NP101 was magnified 154x while the FLT was at 205x and 143x. Over all, the contrast and picture was still superior in the FLT110-TEC again! The surface features simply stood out more clearly and the background was darker and prettier to all of us. When we examined the edge of the rings, the hard and defined outlines were a bit more evident in the FLT110-TEC. You may own an NP101 and see that the edge of Saturn’s rings look really sharp, but remember that everything is relative. When you’re comparing scopes side by side at this level, you would understand. This particular NP101 that belongs to June exibits a tad of over-correction while the FLT110-TEC exhibited a tad of under-correction.

So far, our test results kept the FLT110-TEC in 1st place, with the NP101 in 2nd place, while the rest were pushed into third, fourth and so on.

TELEVUE NP101 vs. TELEVUE 101

This particular review was conducted when Jupiter was visible at a different time from the rest of these comparisons. We’ll get back to the other scopes again but let’s compare these two Televue refractors first. To this day, some observers ask about how these two Televue's compare. The NP101 is the latest version, which is supposed to have improved glass and it does in fact have a shorter physical dimension, but the focal length, 540mm's remains the same.

During careful testing using Jupiter as the primary target, the images in the older TV101 were actually a tad better in contrast when compared to the newer NP101. This occurred after a side by side with two different NP101’s in particular at 216x and 154x. The contrast just seemed a bit better in the older TV101 no matter how the tests were done, even after we had switched diagonals an eyepieces to be sure, but it was still pretty close.

As it stands, we had the FLT-110-TEC in 1st place, with the (very close) TV101 and NP101 in 2nd place and so on.

Televue 101 vs. TAKAHASHI FSQ106 “Q”

Now I realize this review is about comparing planets and stars at high magnification, but you've gotta see the star fields in these scopes in order to appreciate how good they really are with long, wide field eyepieces. The wide field vistas are beautiful. The Takahashi “Q” is a 530mm tank that packs a punch but in reality, this scope is more of an astrograph even though can use it visually, but it's really overkill. There were two units I tested. The first one Ridwan and I star tested was for Markus Ludes of APM telescopes before sending it to Germany. It exibited just a bit of under-correction while the second unit exibited just a bit of over-correction. The issue here as that this is an extremely sophisticated optical system for visual observations, and it's quite temperature sensative. The pictures taken with these scopes are sensational and Televue's NP101 and TV101 are very nice in this area as well.

The NP101, TV101 and the Takahashi “Q” are all, four element designs. Ridwan and myself made some very careful visual comparisons with the “Q” using my own, personal TV101 on the Double cluster in Perseus with a 22mm Panoptic and a 20mm XW. We were surprised at how close the image quality was, including the edge sharpness and we even switch out eyepieces since there are slight differences with the. In all, they were pretty kneck and kneck. Both Ridwan and myself could see that the contrast in the “Q” was slightly better. It wasn’t much but it was there. It amazes me how Televue and Takahashi make 4 elements scopes this good.

I saw one of the most memorable views of Saturn ever with the little “Q”. The seeing was absolutely breathtaking at home and I set my Televue Binovue up with it using a pair of 19mm Panoptics and a 3.8x barlow. Although this only produced 106x, the image was amazing, and to see Saturn floating in space with all this glorious space around it, it was something I’ll just never forget! That night I spent three hours on and off just staring at it and invited two neighbors over to see how beautiful it looked. I could hardly pry them from the bino. They’d never seen anything like it before. I’m sure the TV101 would have produced a beautiful image as well that night but it was on a different occasion.

If you are considering either of these scopes, the Televue has a more narrow tube assembly because it uses flocking instead of baffles like the Q. The Q on the other hand is extremely short but it's like a little Sherman tank and it's pretty heavy. For visual applications, there's less need for such sophisticated optics and the more simple the optics are, the more well behaved they usually are under climate change.

As it currently stands, we have the FLT110-TEC in 1st place, with the FSQ Q, TV101 and NP101 all pretty close in 2nd place and so on.

WILLIAM OPTICS FLT110-TEC vs. WILLIAM OPTICS FLT110-TMB

Now this would be an interesting comparison. Once again, the FLT110-TMB is an air spaced triplet, designed by TMB, but the optics are by William Optics. I had second thoughts about how I was going to present this particular refractor because there were four problems right from the go. I think people should know that I wasn’t going to share this at first but read on.

The first problem occurred when my crew and I first examined the optic on the William Optics FLT110-TMB. I will try and post photos. It’s not at all unusual to see a little bit of dust inside of the inner optic when a refractor is new, but this optic was nothing like that. The entire inner optic was caked with dust as if it had literally been sitting on an optical bench for weeks on end and was just put into the OTA. I asked the guys to look at it and they were stunned at how caked the dust was.

The second problem was the 2” to 1.25” visual adapter that came with the OTA. There was so much slop when it was placed in the focuser, we could actually jiggle it inside. Although we didn;t use it, we still checked it. Understand that William Optics has a very smart and unique tapered design on the barrels of their adapters, but there was still something wrong here. The third issue was the focuser, which kept slipping back when the tube was pointed upwards. Whenever we tightened the tension screw, it would prevent it from slipping, but would not allow us to adjust focus upward. I realize that there are some other screws which require some tools to adjust it, but I have to ask myself, for a $2800 OTA, why wasn’t this already done at the factory and what about all the other inconsistencies?

The next and worst problem of them all was the optic itself. It had been cooling for three hours while we evaluated the other refractors. There was so much spherical aberration outside of focus, it stayed all night long. When the scope was pointed at Saturn, we could see a nasty glow around the planet and something was surely wrong and it wasn’t the dust but more so, the severe aberrations in the star test. The in-focus star test revealed a very tiny airy disc with lots of scattered light all around it. This is what happens to the airy disc when alot of the light is not concentrated in it. This was a case of major spherical aberration. I decided to notify William Optics about the problems.

I wanted to give them a chance to fix the issues because I felt it was the right thing to do before presenting this review and I even told them I was using it for a review. After explaining the problems with William Optics, I was told that I would receive a new and proper OTA that would be inspected. We finally got the second unit in for testing and inspected it. The first thing I checked for was the dust inside and once again, it was caked with it, just like the first one but in various other parts of the glass inside. I'll post pictures of this one too. The new 2” to 1.25” adapter fit better though and the focuser was adjusted properly but then came the worst. We set the scope out to cool for two full hours and once again, it had a severe amount of under-correction, so much in fact, that the images were very soft at higher magnifications of around 180x to 200x and I could see that nasty glow around Saturn again. At this point, it was like bringing
a pocket knife to a gun fight when comparing it to the FLT110-TEC. It’s quite possible that the spacing of the optics was the culprit. I brought this issue up with William Yang in New York at the North Eastern Astronomical Forum, better known as NEAF. He explained that improper spacing of the elements was most likely the cause.

I’m not here to bash anyone, but I gave William Optics the opportunity to replace the first scope and even said it was for my review, and in my opinion, they were given a fair opportunity to correct it. I will let you now that out of every scope that was tested in this review, the FLT110-TMB was the least favorable. The optics in both FLT110-TMB’s were unacceptable and should never have even left the factory this way, especially at $2800. I love the fantastic TEC model we tested though, which sadly is no longer available.

We still have the FLT110-TEC in 1st place , the FSQ, TV101, NP101 in 2nd place, the Vixen 103, 100ED, Orion 100ED in 3rd place, TV102IS in 4th place, Antares in 5th place and the FLT110-TMB in last place.

WILLIAM OPTICS MEGREZ-110 (Indipendant test)

The Megrez 110 is a doublet apo from WO with a focal ratio of F-5.95. This new refractor wasn't actually part of this review until recently, when I had an opportunity to test it. A friend of mine had indicated that he actually had a Meade 80ED that was consistantly outperfroming it on the planets and he couldn't understand why. After acquiring the Megrez to test it myself in order to find out, I noticed that it was a bit out of collimation, but the biggest problem were zones, due to rough surface polishing and there was also some false red color, which is another story. This, combined with major spherical aberration really put me off. This was the third William Optics refractor for this review with diplorable optics. Getting these scopes serviced was also quite a challenge. This scope was placed last with the FLT110-TMB.

WILLIAM OPTICS FLT110-TEC vs. TAKAHASHI TSA102

It was time to compare the fantastic FLT110-TEC against Takahashi’s flagship 4”, the TSA102. The focal length is 816mm, which is almost identical to its FS102 predecessor at 820mm’s. The TSA102 utilizes an air spaced triplet with top of the line glass, also called FPL-53. The star test in our unit was real impressive at 233x on Procyon. The in focus star revealed a perfect airy disc, with a few faint and ill-defined rings around it, which trickled in an out a bit with the very slight fluctuations in the atmosphere. It was a beautiful sight and absolutely textbook. The seeing was fantastic and one of the most memorable sights was Sirius at low magnification in the TSA102. It literally looked like a brilliant, light blue diamond on a perfectly uniform back ground without a trace of false color!

We then fired both scopes at the Trapezium in Orion. Right from the get go, we knew that this comparison was elevated to an unprecedented level of performance. All six stars in the trapezium were clearly visible TSA102 and the contrast was absolutely breathtaking in comparison to the other scopes! Even Ridwan was beside himself and I was scratching my head. It was pulling out the faintest stars and the in-focus color correction was flawless at 164x.I immediately went over to the FLT110-TEC and altered the magnifications from 143x to 204x and was absolutely astonished that even as good as it was, the contrast in the Tak was even better by an incredible 10% to 15% in our visual estimation. I suggested we switch out the diagonals for fun. June compared the two scopes in silence new the outcome.

We then pointed both scopes at Saturn. Once again, we were all beside ourselves! At 233x, the image in the Tak was easily just as bright but, there was a hardness to it like no other and it was crystal clear, without a trace of false color. You have to remember that the FLT110-TEC had beaten every single scope up to this point, so it was quite astonishing to see. Ridwan was so impressed with the TSA102, he literally sold his the wonderful FLT110-TEC just two days later, before we could even complete the comparison and purchased his very own TSA102. You had to be there to truly understand what we were all going through on the incredible night. It was like watching the greatest boxing match in history! Dispite the fact that I’ve tested countless 4” apochromats, I can honestly say that I’ve never encountered anything quite like the TSA102. It simply amazes me that an optic can be made this well.

This now easily put the TSA102 in 1st place and the incredible FLT110-TEC into 2nd position and so on.

TAKAHASHI TSA102 vs. TAKAHASHI TSA102

It was time to compare the best of the best. Ridwan decided to bring his new TSA102 over for visual testing. We had two of every Pentax XW eyepiece for the comparison. We decided to test the two scopes on Rigel, side by side at 166x and 233x. We were all surprised to see how different the star tests were. In the original TSA, there was just a hair of under correction and to our amazement with Ridwan’s, there appeared to be savere over correction in his model. Something was definitely wrong and I knew this was not at all typical of Takahashi! Both under correction and over correction are forms of spherical aberration but over-correction is worse. As the optic acclimates, it can either stay or move further and further away from proper spherical correction. It’s better for an optic to be slightly under-corrected because it will usually improve as it acclimates closer to ambient temperature.

We then decided to compress the rings around the airy disc and there was a noticeable difference. The two rings around the airy disc in Ridwan’s TSA looked heavier and the airy disc was noticibly smaller from light not being as concentrated in it. We then fired both telescopes at Saturn and the results were conclusive. The contrast was much better in the original TSA102. In Ridwan’s TSA, we could see some scattered light around Saturn and it didn’t look as sharp. This was obviously a direct result of what we saw during the star test. I know how great the quality control is with Takahashi. Most of the Takahashi's I've tested are absolutely wonderful scopes, so anything could have happened here and as I stated before, things can occur with the best brands. The unit was immediately returned for a new one without any hassles at all. I would also like to say something about how Art at TNR deals with these situations. If he even hears anything like this, the first words out of his mouth are, send it back! Art can't stand the idea that any of his scopes are not working correctly and that's the best thing one can do. This now put one of the TSA'a at the back of the line.

TAKAHASHI TSA102 vs. TAKAHASHI TSA102 PART II

We now had a new TSA unit in our possession and made another comparison. Right from the get go, we could see that the new unit was fantastic! Both telescopes performed beautifully and we decided to keep comparing the two. I looked at June and Ridwan and said well? Everyone agreed that the images were practically identical but with a very slight edge going to the original TSA but still, both were absolutely nothing short of sensational and were clearly superior to the other scopes we tested no doubt. I know anybody would have been happy with either of the optical units. We then aquired a fourth TSA102 from a friend of mine name Chris Woodell. Once again, I was utterly impressed and it had just a hair of undercorrection when acclimated. Absolutely state of the art apos!

TAKAHASHI TSA102 vs. TAKAHASHI FS102

It was now time to compare the TSA102 to my favorite 4” apochromat of all time, the Takahashi FS102 and BTW, I also love the FC100. The FS102 has a fantastic reputation. There were a couple of interesting things we noticed between these telescopes when we compared them side by side. First, the overall background contrast was practically indistinguishable in both telescopes while viewing Saturn. The only difference noticible about the TSA and the FS was that the FS had a tiny bit of false color on some brighter stars and the images were just a tad bit warmer. Regardless of these comments, the TSA102 and the FS102 were pretty much neck an neck.

The FS102's incredibly low price of around $1500 to $1700 on the used market is an absolute bargain but most of all, they are the most consistent refractors I’ve ever tested and unfortunately I’ve lost count of how many that is. The fact that they are doublets, makes them very temperature friendly and they are very light weight, making them easy to mount. The winner? Read on......

TAKAHASHI FS102 vs. Televue NP101 (Daytime test)

Many people have asked how these two differ in day light. I'll never forget the day we spent during an afternoon with some friends comparing these two scope using some XW's in both scopes. High magnifications are not required but the main thing we wanted to see is the differences in warmth. People have often advocated that the FS102's are just a tad warm but you never realize how cold it is until you compare it to the NP101. Every single observer that was there that day didn't even question which scope was which. The Televue is actually warmer by quite a margin in daylight. Sharpness appeared the same at these magnifications but the color contrast accurracy on objects goes to the FS102 and everyone agreed.

NP101 vs. VIXEN 100ED (Temperature acclimating test)

Don't draw any conclusions until you read this whole paragraph. None of us will ever forget this night. Remember, now that the ED100 is a doublet and the NP101 is a four element design. While viewing Saturn with June's NP101, a friend of ours named Kelvin brought his Vixen 100ED to the Topanga observing site. When we all started viewing Saturn in both scopes, everyone aggreed that the 100ED was winning hands down because it was noticably sharper. The image of Saturn was flaring in the NP101 right on axis. This is a symtom of cool down. I told June it's most likely not cooled enough, but Kelvin enjoyed the better view in his Vixen 100ED at least another hour until the NP101 finally stabalized and it was all over. Everything about the NP101 was nicer but it just comes to show how long it takes doublets and multi element designs like the NP101 to start working at full thrust.

TAKAHASHI FS102 vs. FC100

If you want to put your stars on a diet, then get either one of these. Many observers have asked to have these two compared and this is something I made a point to do for you. The main difference between the FS102 and the FC100 from an optical aspect is mainly the placement of the flourite element. In the case of the FS102, the element resides at the front while on the FC, it resides "behind" the front element. The decision to go with the flourite element up front in the later FS model had more to do with optical coating applications and this is obvious when looking at the coatings on each OTA. In the FS, the coatings looks dark, while the FC looks somewhat thinner. Is there a visual difference? Yes, but they are very similar and I’ve actually compared them on several occasions and this is all I could notice.

In one particular case about seven years ago, my buddy Jim M. and I were viewing Jupiter at Charlton Flats next to Mt. Wilson using a pair of Takahashi 5mm LE eyepieces and Vernonscope diagonals. I’ll never forget being so frustrated with my FS102 this night. The seeing was so stable that I could actually see the slight pulsations from the stepper motors in my Losmandy GM8 mount. Jim had an old Vixen Super Polaris mount for his FC and it was tracking as smooth as a whip! At approximately 165x in both scopes, the images were just a tad sharper in the FC and I looked at Jim and suggested we exchange diagonals and still, the image was a tad sharper in his FC and both of us could see it.

Eventually I said this has got to be coming from the stepper motors in my GM8, so we turned the drive off and I watched the planet drift across and through the axis. When this happened, I immediately went over to the FC and looked into the eyepiece and still, it was still a tad sharper! No matter what we did with exchanging the eyepieces and diagonals, the FC prevailed just slightly. Another noticeable difference between the two though was the actual color of the belts on Jupiter. They looked just a tad more vibrant or pronounced in the FS and I liked this better. This probably happened because of the coatings in the FS, I really don't know. I highly doubt most observers would have been able to detect much difference between these OTA’s unless they had the conditions we had to allow it. Both scopes are fantastic and there are probably slight differences in all of them. We’re talking about A+, A and A-. That’s still extremely excellent either way you slice it.

Since all these OTA’s are so consistent, I would take this comparison with grain of salt because most of the nights I’ve compared them, the differences were not even worth noting.

TAKAHASHI TSA102 vs. TMB102 vs. TMB115

All these scopes are triplets. While attending NEAF in 2007, I noticed that Markus Ludes had a TMB102 and an TMB115 on his table. I acquired both units and couldn’t wait to test them. Both came in the exact same size tubes except one optic is bigger than the other. I realize this is supposed to be a comparison between 4" scopes but I thought I’d share my experience with the TMB115 and the TMB102. I allowed both OTA's plenty of time to settle down. After comparing the two units, I actually liked the planetary views better in the TMB102. It just wasn’t as good as the 102 and it showed. Upon inspection of the star test in the TMB115, I noticed some very slight zones and this revealed itself on the planets as well. The contrast was just not quite as good.

This comparison between the original TSA102 and the TMB102 will forever remain engraved in my memory because even before we compared them, I had spent a good amount of time star testing the TMB102 and viewing planets with it and I knew it was an absolute gem! June and I conducted this next comparison ourselves. We used a set of Pentax XW eyepieces and both scopes went head to head. To our astonishment! with both OTA’s trained on Jupiter, neither June or myself could possibly distinguish any difference at all between the two. We switched diagonals and eyepieces and the contrast, brightness and sharpness were literally identical. To be honest with you, I don't really focus on what kind of glass any of these scopes use. I just test them visually and call it like I see it but according to Tom Trusock, the TMB102 actually uses OK-4 glass, and as I stated before, the TSA102 uses FPL-53 and both were absolutely fantastic! Hands down, these OTA’s represent the pinnacle of the refractor world and in my opinion, you could not find a better 4”, anywhere in the world.

About the only potential drawback to the TMB is that it's quite a tank and it uses a composite tube material that could introduce some tube currents in fast dropping temperatures. Dormant materials like this are fine, but in a closed tube like this, it may not be the best way to go in certain climates. At no time however, was this an issue during my tests at sea level.

When this review was completed, I boxed the orginal TSA102 back up and I kept it for someone I thought would really appreciate it and until presenting this review, he has no idea he owns it. About two months after this particular shootout was completed, a man asked for my assistance in getting a really great refractor with a mount and all the accessories. The most important thing was that he didn’t nag at all about prices like so many others often do. He was a very humble man, especially since he forked out so much hard earned money. It was for this very reason that I picked him the best 4” I ever saw in my life. The Serial number for this TSA102 is #06121 and now belongs to Tamiji Homma.

THE WINNERS AND TOP PICKS IN THIS SHOOTOUT

1st place - Takahashi TSA102 and TMB102.

2nd place - Takahashi FS102/FC100, WO FLT110-TEC.

3rd place – Takahashi FSQ106 "Q", Televue 101 and Televue NP101.

4th place - Vixen 103ED, Vixen 100ED and Orion 100ED.

5th place – Televue 102IS.

6th place - Antares 4” F-15 achromat.

7th place – Takahashi TSA102, only one unit out of four. William Optics FLT110-TMB, William Optics Megrez 110.

Good seeing!
Daniel Mounsey AKA Doctor D

For Sunshine.
Sep 4, 2008