I agree, the 150 achro will be used for dso mainly even though i have read people with the 750mm fl say it isnt bad on planets and the moon, given it being a fast scope.
About your SV503 80ed, I purchased my starfield 80mm as an apo, it clearly states it is an apo whereas the sv503 is not? If you know something i do not know regarding this as the price of the starfield was $887(in us dollars, i did conversion). Can they sell a telescope and advertise it as an apo when it is not? As i have looked on their website and a number of stores and it states it is an apo
I assumed at first that your 80mm was an ED doublet very similar to mine. But your comment has made me look at it more closely. It is indeed sold as an ED doublet, but they do include the term APO in the description. However, when we go to review the characteristics of the doublet they do not specify what kind of lenses it uses.
In ED doublets, the crown component is usually made of a special type of glass, sometimes with very expensive natural fluorite (calcium fluoride), or more frequently with synthetic fluorides. Lenses with these materials have the property of generating a very low dispersion of white light in its different wavelengths, or colors (hence the acronym "ED", extra-low dispersion). However, within ED lenses there are several different qualities, in fact, they are characterized by their Abbe numbers, which is a standardized indicator of the refractive index of any kind of lens, and in the case of crown lenses it ranges from approximately V=60 to V=95: the higher the V (Abbe number), the higher the refractive quality and the more expensive the lens. For example, doublets that incorporate a FPL-53 lens (V=94.96) are more expensive than those that incorporate a FPL-51 lens (V=81.61).
Why is it important to know this data? Because precisely one of the main aberrations that refractors suffer (although not the only one) is chromatic aberration (CA), which manifests itself in the form of colored halos (generally purple) around bright objects, as in the case of nighttime observation of the main planets, first magnitude stars or the Moon. The evolution of refractor lenses has always sought to reduce to a minimum the presence of this "false color" in the image (whether visual or photographic). With the invention of the achromatic doublet around the middle of the 18th century (positive crown lens + negative flint lens) it was possible to reduce to practically zero the so-called primary color spectrum, which, broadly speaking, was the very notable chromatic aberration generated by the archaic single-lens objective of, for example, Galileo's telescope. With the achromatic doublet it was also possible to greatly improve the sharpness and contrast of vision. Even so, the so-called secondary color spectrum persisted, which was (is) a remnant of CA that the (achromatic) doublet is not able to eradicate... although it can minimize it with very high focal ratios.
To control the secondary color spectrum at moderate focal lengths, the triplet objective was developed approximately a century later. It consisted of three lenses and was much more complex to build than the doublet. If the achromatic doublet bring two wavelengths (usually in the blue and red colors, that is, from the extremes of the visible spectrum) to the same focal plane, the triplet was capable of bringing three wavelengths in the blue, green and red region. These types of objectives were called apochromatic, or, to simplify, APO, which basically means "colorless." They were characterized by minimizing practically to 0 the chromatic aberration generated by the telescope tube objective. CA not only generates those unwanted color fringes around bright objects or details, but also reduces to some extent the sharpness and contrast of the view. So, although the achromatic telescope already offered very good views compared to the old Galileo, Kepler or Huygens telescopes, the apochromatic telescope improved these performances even further and, in addition, achieved this without the need to increase the focal ratio of the system. But about 60 years ago, new lens manufacturing materials appeared whose exceptional refractive properties gave new life to the old doublet objective, the ED lenses. The use of this type of low light dispersion lenses provides a control of the CA "similar" or close to that which a triplet objective can give, that is, it can minimize the secondary spectrum to practically 0. For this reason, telescopes with ED lenses are sometimes given the title of APO. But they are also often referred to as semi-APO, or simply ED.
Strictly speaking, from the point of view of chromatism, an APO refractor is one that can bring three wavelengths to the same focal plane. It is not stated whether this should be achieved with two, three, four or five lenses. Is it possible that a doublet with a high-quality ED element and an optimized construction design could do it? It seems to be. I think the SW 100ED Evostar is a good example of this. In fact, FLO doesn't promote it as APO (https://www.firstlig...pro-outfit.html), but Astronomics does (https://astronomics.com/collections/refractors/products/sky-watcher-evostar-100ed-100mm-f-9-ed-doublet-apochromatic-refractor?_pos=8&_fid=4df15ba87&_ss=c). I would say that visually it is practically impossible to find any false color in the views it offers. Likewise, I think we have all heard of triplets that, just because they are triplets, do not guarantee APO status, simply because their build quality is not fully optimized.
Finally, on the issue of the coveted APO label, I must also say that there is a certain amount of marketing involved, and it has become more of a "hook" for the buyer than a meaningful description of the optical quality of the refractor. If not, and considering that the Sky Watcher Evostar 100ED doublet is APO, what difference can there be then with the SW triplet Esprit 100, which is supposedly the "authentic" APO, apart from a difference of more than a thousand dollars, a lower focal ratio and a larger field of view? Well, there has to be a difference, and this is where the "crux" of the matter often lies. In visual observation, as far as chromaticity is concerned, there is probably no difference at all. And from a photographic point of view, much more sensitive to remnants of the secondary spectrum, the triplet, which also has an ED element of the same quality as the doublet, may, with a much lower focal ratio, give a better result. Furthermore, something similar is likely to happen with other non-chromatic aberrations that are also present in refractors and that are relevant in photography, such as field curvature, spherical aberration or comatic aberration. For this reason, some doublets are often classified as APO, provided that they are used primarily for visual purposes, and for this reason astrophotographers often use triplets, quadruplets or even quintuplets instead of doublets, since they normally guarantee a higher degree of correction in photographic shots at low or very low focal ratios.
In the case of your Starfield, since the type of ED lens used in the doublet is not indicated, it is likely to be an FPL-51, FCD-1 or equivalent, that is, a "basic" type of ED lens. By "basic" I do not mean "bad", but simply that it will probably not be one of those with the highest Abbe number, that is, one with the highest refractive index. Generally, the lower the dispersion index of an ED lens, the more expensive it is and the more they state this in the description in order to justify the price of the optical tube. That said, you don't have to worry too much about this kind of thing either, since "one lens does not make a spring". You always have to evaluate the whole picture, and this includes another lens (in the case of the doublet), the design of the lens, the quality of the overall construction of the tube and also of the lenses and their cell, etc., etc. In the end, optical quality and therefore viewing quality is a very complex issue involving many variables, which often can only be really evaluated in practice or experience.
I hope I haven't bored you. Here is this thread if you want to learn more:
https://www.cloudyni...y-ed-refractor/
Edited by Japetus Eye, 30 January 2025 - 12:03 PM.