? MYSTERY ? EDMUNDS ? 6" CASSEGRAIN ?
#101
Posted 23 June 2014 - 12:23 PM
#115
Posted 23 June 2014 - 12:56 PM
Looks great. So what do the images look like ? I haven't finished my DK. Got busy restoring the local high schools 10" Cave Cass. mount and dome.
- Dave
#116
Posted 23 June 2014 - 01:21 PM
Tom,
Looks great. So what do the images look like ? I haven't finished my DK. Got busy restoring the local high schools 10" Cave Cass. mount and dome.
- Dave
Before I did the paint and finish... This winter I had it out for star test and star collimation Dave those test proved to be very good ..tooo cold to mess around too long outside. Think I did swing around and check out JUP real quick It looked good too. then back in the house. I took all the optics out to do the paint and finish ,reassembled and did a bench collimation last week. have to get it out to test and star collimate again soon I hope .then I'll have better weather conditions to play around,, then in the dead of winter
#117
Posted 23 June 2014 - 02:00 PM
#118
Posted 23 June 2014 - 02:03 PM
#119
Posted 23 June 2014 - 02:16 PM
I cannot for the life of me understand why noone (or darned few anyway) makes a classical Cassegrain like that anymore.
It's awfully long (slow) for a classical Cass. I'd think it more likely to be a D-K. The reason we don't see very many classical Cassegrains is that very nearly the same performance can be had by relaxing the mirror curves to a slower D-K, making a more affordable instrument. Or the primary can be pushed into a hyperboloid at a modest increase in cost and similar performance can be had in a much faster package. Both alternatives are much more popular than the original, which offers the least bang of the three for the buck.
#120
Posted 23 June 2014 - 02:58 PM
#121
Posted 23 June 2014 - 03:31 PM
Dall Kirkhams are easier to make so more popular. Since the primary is an ellipse is has less correction then a parabola and the same test techniques can be used to make it as one uses to make a parabola. The secondary mirror is a convex sphere. Since a sphere has no optical axis you can grind a larger disk that is easy to handle then cut out the ssmaller secondary from it. When it comes to testing, the concave "tool" used to grind the convex secondary can be polished, figured and tested just like making any other sphere then used as a test plate to check the figure of the convex secondary by contact interference. So the testing the secondary is much easier as well. If your making a number of optical sets you can grind and figure a large enough disk to cut out the needed number of secondaries from just the one disk.
What you lose in a Dall Kirkham is off axis performance. It has much more coma then a classic Cass so the useable field of view is much smaller.
- Dave
#122
Posted 23 June 2014 - 07:52 PM
The reason why you don't see classic Cassegrains is the difficulty in making the convex hyberbolic secondary.
Don't think so. Other designs (RC, ACF, others) use hyperboloid secondaries and are still are much more common then the classical Cass. Even the RC, with not one but two hyperboloid mirrors is far more common. The CC is at the worst point in the performance/difficulty-to-produce curve. I liked mine (a Takahashi) but it wasn't a good value.
#123
Posted 23 June 2014 - 08:27 PM
#124
Posted 23 June 2014 - 08:31 PM
#125
Posted 23 June 2014 - 09:38 PM
I really like how you polished the finder instead of painting it. Very nice indeed.
Thanks Gerald, I was going for that UNI-CORN-ISH look