Shane LaPierre's ATM Pages! |
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The Benefits of a Large Dobsonian There are two words that summarize the benefits of a large Dobsonian: simplicity and aperture. Simplicity because there's nothing that's quite as easy as hand-pushing a Dobsonian around the sky at your leisure, and aperture because these scopes are big enough so that there's no trouble seeing what you want to see. Want to see the Ring Nebula? No problem, even the central star is readily observable at a dark site. The shape of the Swan Nebula is... well, like a swan! You will get lost observing in the Realm of the Galaxies because there are more galaxies visible through your telescope than are plotted on Uranometria!
When you have a large aperture telescope, you have to do a little more than you may with your 80 mm ShortTube. Here's some of the things that I have noted that require my attention:
Telrad: Need I say more? With a Telrad you can see where you're pointing, and then just peer through the eyepiece. If you mount it near the eyepiece, it may tower over you when you're on the ground. But that's not a problem. The Telrad allows you to use it even if you're several feet away as you peer "through" the device towards your target. It's not important to be close, just as long as you can see the red circles, you can point your telescope to within 1/2 degree anywhere in the sky. Low Power Eyepiece: I use a 40 mm wide angle eyepiece (Pentax 40mm XL) in the main telescope when I'm trying to find things. For brighter objects I can sweep, and the 20" aperture will pick up all of the Messiers, for Traditional Finder: I use an 8x50 finder on mine, and I find it to be useful. I can see M33 through it on a good night in my backyard, and for at least 1/2 of the Messiers it's the ideal way to center your target. Just be sure to provide a means of keeping the dew off. In the picture on the right, you can see I have a couple of spray-paint lids rubber-banded to the finder mount. You can just pop them on and off without fear of losing them in the dark. A Jumbo-Sized Finder: Picture this... mounted along-side or piggy back the main telescope is a jumbo finder that is as large as a standard telescope. I've got an 8" that I can mount alongside the 20", and the idea is to allow the observer to see those faint objects that only a legitimate telescope can see. During testing of the 8" mirror, when only the jumbo finder's optical tube was completed, I found I was able to scan without a mount at 27X magnification with 2 1/3 degree field of view. This is a textbook rich-field machine. Couple that with 8" of light gathering capability and you'll be able to point your large Dobsonian at anything! At the Connecticut Star Party 2000, I had the scope set up that way for the whole weekend. Someone would be observing through the 20", and someone else through the 8". It made for a fun time. Jumbo Finder! Star Hopping: A Dobsonian telescope may seem disadvantaged, but in many ways it is much simpler to use than a traditional equatorial mounted telescope. For example, I recently was helping an observer using a 6" Newtonian on a German Equatorial Mount (GEM.) to verify a field of view with M95, M96 and M105, three galaxies in the constellation Leo. He had something in the field of view, but it was very cumbersome turning the manual controls, first North or South, then East or West. And to be honest with you I wasn't totally sure which way I was going... Needless to say I was not as successful as usual considering I consider star-hopping old hat. You can learn these odd motions, but a Dobsonian can be easily "mastered" in an hour or less. Once you master the reversed motions, you simply nudge the scope in the direction you want to move it and it responds by moving in both axes. This makes finding objects much simpler if you are not using setting circles, so if you plan on tracking down your own objects a Dobsonian is an ideal instrument. There are not too many limitations to Dobsonians anymore, but let's be fair and talk about what they don't do... at least easily: Automatic Tracking of the Stars: Most Dobsonians don't track the stars, so it is required that the user keep up with the object as the earth turns. If you have never used a telescope before you may be surprised to hear that the earth spins fast enough for this to be a problem, but if you ever get a chance to look through one then you will realize it's a matter of 30 seconds or less before the object has moved or is completely out of view. The simple solution is to simply nudge the scope ever 15 seconds or so. It gets pretty easy after a while, and can even be done at powers of 500+ although it is a little tricky.
Viewing at the Zenith Equatorial telescopes have a tough time viewing near the North Celestial Pole (by the North Star), and Dobsonians have a problem near the zenith (straight overhead). This area is called "Dobson's hole". The reason for this problem is the telescope may need to be moved around azimuth pivot many degrees to make a small adjustment in position. The good news is with practice it's not that bad. A few degrees away from the zenith make a big difference, as do the quality of the bearings. In addition, with a large scope it's just so high! You have to be ready to climb a ladder and be sure not to drop anything. The Problem My 20" optical tube weighs in at over 125 pounds, but a solid wooden tube would weigh even more, and a cardboard tube would simply be too big to manage. The aluminum trusses allow disassembly of the optical tube assembly into more manageable components, but the truss tube allows external light to sneak into the eyepiece. The Light Shroud A popular way to deal with a part of the problem is to get a light shroud. This is a material (such as ripstop nylon or spandex ) "skirt" that goes around the trusses when the tube is assembled. I own one, and it is useful for blocking light. It does, however, make the entire telescope suceptible to breezy conditions so there are nights that it is not practical to utilize a shroud. Secondary Baffle Just as important as a shroud, is a baffle on the upper side of the secondary cage. I use a piece of Kydex that gets velcroed to the secondary cage. Focuser Baffle Another significant method of blocking off-axis light is the focuser baffle. Cut out a piece of plastic about 3 inches in diameter, and cut about 1 3/4 inch hole in its center. Align this with the center of the focuser inside the secondary cage, and figure out a way to secure it. This helps keep a lot of the stray light from entering your focuser. |