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Alan W. Craft wrote:
Correct me if I'm wrong, but shouldn't the focal length of the telescope in conjunction with the f.l. of the eyepiece, that is, the magnification, determine whether or not a telescope is fast or slow? The terms "fast" and "slow" come, as you may know, from photography, where they roughly express how quickly a lens will properly expose film. The lower the f-ratio (or t-ratio, if they differ significantly), the shorter the exposure need be. There are two factors involved: 1. The light-gathering power of a lens or telescope is, to first order, proportional to the area of the aperture. There are secondary considerations--light throughput, central obstruction, and so on--but these probably do not equate to more than a 25 percent difference in linear aperture. 2. The image scale--that is, the linear size of the image at the focal point (more properly, focal plane) of the lens or telescope--is proportional to the focal *length* of the lens or telescope. With these two factors in mind, consider two telescopes: a 4-inch f/12 and an 8-inch f/6. Both telescopes have a 48-inch focal length, so they both have identical image scales. For example, if you were to put a piece of ground glass at the focal plane of both telescopes, and you pointed them at the Moon, both pieces of ground glass would depict a little Moon approximately 0.4 inches across. Since the Moon is about half a degree across, we might say that the image scale is 0.8 inches per degree in both scopes; more usually, we use mm and say that the image scale is 20 mm per degree. However, because the 8-inch has twice the aperture, it gathers about four times (2 squared) the light. Four times as much light is put into the same size image, so that the image of the Moon on the ground glass in the 8-inch scope is four times as intense as the image on the ground glass in the 4-incher. If you were to put pieces of film in place of the ground glass, the film would be exposed four times as quickly in the 8-inch scope as it would be in the 4-inch. Next, consider a third scope: an 8-inch f/12. (A fairly long scope, unless it's a folded design like an SCT, but never mind that for now.) This scope has a focal length of 96 inches, twice as long as the other two scopes, so its image scale is twice that of the others. A piece of ground glass at its focal plane will show an image of the Moon about 0.8 inches across. Its image scale is therefore about 1.6 inches or 40 mm per degree. Now, in comparison with the 8-inch f/6, it gathers just as much light, but because the image of the Moon covers four times as much area, the image is only one-fourth as intense. On the other hand, in comparison with the 4-inch f/12, it gathers four times as much light, but that larger amount of light is spread out over four times the area, so that the image at the focal plane is just as intense in the 8-inch f/12 as it is in the 4-inch f/12. To summarize, then, scopes of the same focal *length* have the same image scale. In contrast, scopes of the same focal *ratio* have the same image intensity. This in turn determines how fast they will expose a piece of film and gives rise to the terms fast (low focal ratio, meaning more light spread out over a smaller image, so more intense illumination) or slow (high focal ratio, meaning less light spread out over a larger image, so less intense illumination). While an 8" f6 would be considered fast when compared to an 8" f10, the same 8" f6 would at the same time be equitable in "speed" to a 4" f12, and therefore considered slow. To continue my thought: However, when a scope is used visually, the chief consideration is aperture, not focal ratio. The larger the aperture, the more light gathered, and the brighter the image at any particular magnification. To be sure, an 8-inch f/6 requires an eyepiece half as long in focal length as an 8-inch f/12, in order to achieve the same magnification, but what of that? A simple 2x Barlow will suffice. The image will look pretty much the same in an 8-inch f/6 at 100x and an 8-inch f/12 at 100x, all other things such as optical quality being equal. On the other hand, at 100x, the view in the 4-inch f/12 will look significantly dimmer--one-fourth as bright, in fact. Such slowness is precisely what I am trying so desperately to avoid, and in order to use the telescope for comet-hunting and widefield DSO observation, while at the same avoiding glaring instances of coma and exacting collimations. If what you want is wide true field of view, and you are willing to live with less aperture, then you want a combination of short focal length and wide focuser. For example, the Pronto has a focal length of just 480 mm and a 2-inch focuser. That yields a maximum true field of view of around 5 degrees--quite wide. Of course, the larger the aperture, the more you will see in any given field of view, but it is pretty hard to make a high-quality fast scope of significant aperture. Brian Tung The Astronomy Corner at http://astro.isi.edu/ Unofficial C5+ Home Page at http://astro.isi.edu/c5plus/ The PleiadAtlas Home Page at http://astro.isi.edu/pleiadatlas/ My Own Personal FAQ (SAA) at http://astro.isi.edu/reference/faq.txt |
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