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#21
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![]() What in your opinion or experience is the minimum aperture necessary for satisfying views of globular clusters and galaxies? Hmm . . . you did specify *minimum* didn't you? When asked in that manner my reply would be: The smallest telescope I happen to own -- 80mm. I find satisfaction in finding and identifying objects with small telescopes. Any visible details that might greet me from within an object would be looked upon as 'icing on the cake'. It is satisfying to find Globulars and Galaxies in a smaller scope but it seemed to me that the issue was about "viewing" them rather than finding them... jon |
#22
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My experience from this past Spring in Colorado actually made me think
about this very issue. Why? Well most seasons have easy-to-view objects, but Spring tends to be loaded with 'faint fuzzies.' I could locate many of these Messier objects, but little or no detail was visible in my 6" Newtonian. Those same objects in my friend's 12" SCT looked amazing, especially the globulars. This 'finding' of mine, dovetails nicely with the aperture sizes that sell in volume, but are still portable, i.e., those in the 8-12" range. Kirk What in your opinion or experience is the minimum aperture necessary for satisfying views of globular clusters and galaxies? Thanks, Bill Meyers |
#23
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Bill Meyers wrote in message ...
Hello, all, What in your opinion or experience is the minimum aperture necessary for satisfying views of globular clusters and galaxies? Well, this question is really quite hopeless as stated, but I'll do my best. For simplicity, I'll consider just four telescopes, all of which I've used fairly frequently, and which form a vaguely equally-spaced sequence: * 4-inch refractor * 8-inch reflector or catadioptric * 12.5-inch reflector * 17-inch reflector For viewing globular clusters, I'm never really satisfied unless I've resolved some stars. I can't really say just how many is enough; in fact, the view of a barely-resolved globular cluster has a charm of its own, with a dozen stars twinkling in and out of the halo as I apply averted vision. But on the whole, the more stars, the better. Of course, no amateur scope can resolve a globular cluster fully, like a Hubble photo, where you can count thousands of stars within a few arcseconds of the center. Next, I would divide globular clusters into four classes. The first class consists of 47 Tucanae and Omega Centauri, which are truly glorious in a 4-inch refractor under dark skies. The second class is what I would call the great globulars. Just which ones make the grade is a matter of taste, but anybody would include M5, M13, M22, NGC 6397, NGC 6752, and probably another dozen Messier and far- southern non-Messier globulars. These are pretty well resolved in a 4-inch refractor under dark skies, and they're really quite glorious in an 8-inch scope under dark skies. The third class is the major globulars, including most of the other Messier globulars and quite a few NGC globulars. An 8-inch scope may show a few stars in those, but it really takes a 12.5-inch scope under dark skies to do justice to them. And finally, there's all the other globular clusters in our galaxy, a motley assortment. A few of them are barely detectable even in a 17-inch, due mostly to heavy obscuration by galactic dust. On the whole, globular clusters survive light pollution pretty well, but they do require extra aperture to get views that are roughly equivalent to the dark-sky views. Under typical suburban conditions, I would move everything over one class. There, an 8-inch scope is just beginning to resolve the great globulars, and a 12.5-inch scope is required to do full justice to them. The story is quite different when it comes to galaxies. With a handful of exceptions, like M82, galaxies show very poorly in the presence of light pollution. Yes, you can get a decent view of M51's spiral arms in a big scope from one of the darker suburbs, but I still wouldn't call most galaxy views satisfactory unless the skies are reasonably dark. In discussing galaxies, I'll have to explictly exclude the two Magellanic clouds and our own Milky Way. All of those show some detail even to the unaided eye, and quite a lot of detail through tiny instruments. Steve O'Meara can obviously see a lot of galaxy structure in a 4-inch refractor, but for normal mortals, I think that 8 inches is the minimum. And even then, only a handful of galaxies show decently -- M31, M33, M51, M101, M83, M82, M66, maybe M81 under pristine skies. (I'm sure I've forgotten some.) Things improve quite a lot in a 12.5-inch scope. All of the galaxies listed above really begin to open up and show intricate detail, which an 8-inch scope just hints at. And a bunch more galaxies start to show tantalizing detail. But it takes a 17-inch scope to start to unlock the wider realm of galaxies -- and that's just the beginning. I've never seen a view of any galaxy in any scope, no matter how big, where I didn't wish for just a little more aperture -- or better yet, a lot more. - Tony Flanders |
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#25
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Tony Flanders wrote:
Steve O'Meara can obviously see a lot of galaxy structure in a 4-inch refractor, but for normal mortals, I think that 8 inches is the minimum. And even then, only a handful of galaxies show decently -- M31, M33, M51, M101, M83, M82, M66, maybe M81 under pristine skies. (I'm sure I've forgotten some.) If the 4 inch refractor is used at the proper power and under reasonably-dark skies (ZLM 6.0 or fainter), many people (other than Steve O'Meara) can see at least some structure or detail in a number of galaxies with averted vision. M31 begins to show some of its spiral structure in a low-power wide-field eyepiece, along with at least one of its dark lanes, although like most galaxies, it isn't all that bright. M51 will show a sort of "ring" structure hinting at its spiral nature, while M101 will also show some patchyness in its outer haze at low to moderate power. I can see a large diffuse patch in one end of M81, although it doesn't show the spiral arms in a 4 inch. M82 and M104 will show some dark lane-like structure, while a number of edge-on spirals like NGC 4565 will show their needle-like form fairly well. NGC 253 looks mottled, as does M33 (one arm starts to become visible), NGC 2903, M66 and a few others. As for an 8 inch, this aperture increases the number of galaxies which show at least some kind of detail by quite a bit, although with many of the fainter ones, any structure that is visible is mainly mottling, overall shape, star-like nucleii, or, in the case of near edge-on spirals, a dark lane. Observing galaxies is always a challenge, and learning how to tease out some of the detail that is visible is part of the fun. Clear skies to you. -- David W. Knisely Prairie Astronomy Club: http://www.prairieastronomyclub.org Hyde Memorial Observatory: http://www.hydeobservatory.info/ ********************************************** * Attend the 11th Annual NEBRASKA STAR PARTY * * July 18-23, 2004, Merritt Reservoir * * http://www.NebraskaStarParty.org * ********************************************** |
#26
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![]() "Sketcher" wrote in message ... On Thu, 23 Sep 2004 20:06:53 -0400, Bill Meyers wrote: What in your opinion or experience is the minimum aperture necessary for satisfying views of globular clusters and galaxies? Hmm . . . you did specify *minimum* didn't you? When asked in that manner my reply would be: The smallest telescope I happen to own -- 80mm. I find satisfaction in finding and identifying objects with small telescopes. Any visible details that might greet me from within an object would be looked upon as 'icing on the cake'. As long as a person doesn't have unrealistic expectations for what they ought to see with a given instrument they ought to be able to find the views satisfying. It shouldn't matter if they're using 8x42 binoculars or a major observatory telescope. Well that is a very honest opinion but lets face it, the average star party is loathy littered with every kind of Dob underthe sun..and that spells aperture aperture apeture. Most observers casual or otherwise just don't think like you. Except me. |
#27
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David Knisely wrote in message ...
If the 4 inch refractor is used at the proper power and under reasonably-dark skies (ZLM 6.0 or fainter), many people (other than Steve O'Meara) can see at least some structure or detail in a number of galaxies with averted vision. You're absolutely right -- it's all a matter of how much detail you want. Even a 60mm scope is big enough to classify most of the Messier galaxies as spiral versus elliptical with a reasonably high degree of confidence, and M31 is obviously a spiral to the naked eye. Not that you can see the spiral arms, but no elliptical galaxy could possibly have that shape and that kind of central condensation. Josh Roth here at S&T told me that he recently glimpsed M33's spiral arms using an O-III filter in his 60mm refractor, and 60mm is certainly enough to see the emission area NGC 604 in that galaxy. I've heard of people seeing M31's dust lanes in hand-held binoculars, although I'm sure that feat is far beyond me. - Tony Flanders |
#28
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Total Mikal posted:
Well that is a very honest opinion but lets face it, the average star party is loathy littered with every kind of Dob underthe sun..and that spells aperture aperture apeture. Is this a problem? -- David W. Knisely Prairie Astronomy Club: http://www.prairieastronomyclub.org Hyde Memorial Observatory: http://www.hydeobservatory.info/ ********************************************** * Attend the 11th Annual NEBRASKA STAR PARTY * * July 18-23, 2004, Merritt Reservoir * * http://www.NebraskaStarParty.org * ********************************************** |
#29
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#30
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Per Erik Jorde posted:
Even a 60mm scope is big enough to classify most of the Messier galaxies as spiral versus elliptical with a reasonably high degree of confidence, and M31 is obviously a spiral to the naked eye. Not that you can see the spiral arms, but no elliptical galaxy could possibly have that shape and that kind of central condensation. You are exaggerating _grossly_ on both acounts, IMO. First, a small scope (most scopes, really) typically shows just the central hub of spiral galaxies, and these are not much differen from ellipticals. Second, one only has to glance over at neighboring M110 to see an elliptical galaxy that looks very similar to the naked eye view of M31. Well, he might be exagerating a little, but a good 60mm refractor when used at a *low* enough power under reasonably dark skies will show M31 and its much fainter extended outer haze. Its core region is usually the only thing which shows up well at the moderate powers that many of the common "department store" refractors use, but drop that power to 20x and the faint vaguely patchy outer extensions become quite easy to see, along with the marked dropoff of light intensity along the northwest side marking the location of the first major dark lane. This kind of brightness profile (small brighter nuclear region and extended faint outer haze) is enough to show that M31 is a spiral galaxy, although it does not show what kind it is nor does it show much of the arm structure. M110 on the other hand does not show the kind of smaller and markedly brighter central core which would hint at it being a spiral. Its smooth edges, slowly increasing brightness level with decreasing distance from the center, and the lack of a smaller fairly well-defined brighter (but non-stellar) core indicate that it is probably an elliptical galaxy, an impression which is confirmed with larger apertures. It is quite easy to use the overall brightness profile of galaxies which show little other structure to get at least an idea of whether they are spirals or ellipticals. In addition, with an 8 or 10 inch telescope, I can usually tell what kind of galaxy I am looking at for a *large* number of galaxies as faint as 13th magnitude (or sometimes fainter). With that aperture, I can usually see at least some indications of structure (mottling or irregular edges, small bright nucleii, dark lanes) that can point to the object being a spiral without necessarily seeing the spiral arms. Of course, with a ten inch, there are a number of galaxies which will visibly show the spiral structure, so for those at least, there is little doubt of the classification. Even without those, the brightness profile is sometimes enough on its own to tell whether a galaxy is an elliptical or a spiral. Clear skies to you. -- David W. Knisely Prairie Astronomy Club: http://www.prairieastronomyclub.org Hyde Memorial Observatory: http://www.hydeobservatory.info/ ********************************************** * Attend the 11th Annual NEBRASKA STAR PARTY * * July 18-23, 2004, Merritt Reservoir * * http://www.NebraskaStarParty.org * ********************************************** |
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