| The Takahashi Mewlon 210 Telescope |
The Takahashi Mewlon 210 is not a Schmidt-Cassegrain. It is a Dall-Kirkham design which sports a prolate ellipsoid primary and a spherical secondary mirror. It is a Cassegrain focus. See ATM-Page Dall-Kirkham Information. This design makes for mirrors that are easier to grind, but it results in fields that are usually more curved than that of a SCT and showing more coma. At least, this is what the various books on telescope optics have to say about it. This scope is an f/11 with 210mm of useful aperture. The mirror is really a 220mm diameter but is masked, presumably to reduce aberrations. It would thus be good for planetary and Lunar studies. With an optional focal reducer, one could use it for deep sky visual and CCD imaging projects (my goal).
The Mewlon 210 is painted Takahashi off-white with the familiar Takahashi green for the mirror cell and hardware. The visual back and 1.25" adapter are black anodized aluminum with matte black interior. The visual back accepts standard 2" equipment, while the 1.25" adapter is the Takahashi compression ring device which accepts all standard 1.25" equipment without marring the finish with set screws. The dust cover is a leatherette material which fits nicely over the tube's front end. One will want to keep this on whenever not observing, since this is an open-tube design. Looking down the tube will reveal the 4-vane spider holding the secondary mirror. The interior is a rough matte black as is the spider and all other exposed hardware. I can see that I will not have to go in with a paint brush to touch up any missed spots of shiny metal. Through the center of the primary mirror is a long light baffle to enhance contrast. The secondary mirror has a shorter light baffle as well. Along the bottom of the outside of the tube is the dovetail wedge to which the Takahashi mount clamp attaches. There is some slide travel available for fine balancing. Most of the weight is in the rear with the primary mirror. One of the nice features of the Mewlon is the attached 7x50 finder and bracket. Their finders are the best I have ever used. The finder bracket is so firmly attached that Takahashi actually tells the user to hoist the scope around by it! Now, that is a finder!

Here is a look down the tube at the primary mirror. The primary mirror
is really 220mm in diameter but only 210mm is clear aperture. The
edge is masked off to reduce the coma common in this scope design.
Behind the name-plate are three collimation screws for the secodary mirror.
The name plate just unscrews from the housing.

A closer look down the tube shows the primary mirror light baffle.
This adds to the spectacular contrast that this scope delivers.
Note that the interior of the baffle is also baffled with ridges
to prevent internal reflections. To the right of this image is
the secondary mirror and its light baffle.

Here is the business end of the telescope. A standard Takahashi
visual back is brought to a standard 2" holder. Inserted into that
is a 1.25" compression ring eyepiece holder. The zenith prism and
eyepiece are not provided.

Here is a closeup image of the famed heavy-duty finder. This is a
7x50mm finder with superb optics. The finderscope is rigidly attached
to the telescope tube. The manual actually states that one
should life the tube by the finder! Yes - it is true, and it works.


The star seems to show a bit of misalignment with the optics, but remember that the CCD chip itself is not centered on the optical axis. Still, I think that there is a bit of collimating to do. The optics are very very good. There is no problem there. All the stars in M-13 were resolved to shimmering diamonds sparkling on a velvety black background. No problems there at all. A 40mm Plossl makes a fine wide field view, while I was using a 10mm and 3mm Radian on the Moon without any difficulty. The Moon showed marvelous contrast and no ghosting whatsoever. Of course, there is no false color to be seen here. Having seen the Moon so well visually, I decided to take the following CCD image series to show the capabilities of these optics:
This is Rupes Recta and the surrounding area. My best image of this
taken with a C-8 can be seen Here. There is no comparison:

This is the area of Aristoteles, Eudoxus, and Mare Frigoris:

This is the Eratosthenes and Montes Apenninus region:

Many will worry about the focus mechanism: It uses the same method as the ubiquitous commercially available SCTs. In other words, with the Mewlon 210, the primary mirror is moved to reach focus. Is there image shift? Yes, but only a slight amount. There is so little shift, that objects did not fall off of an ST-7's CCD when drastic focus moves were made in both directions. It is a great improvement over the other telescopes which use the same method. Those looking to buy a larger diameter Mewlon should note that all the larger models (250+) focus by moving the secondary mirror via a small electric motor with a hand control. This is nice, especially for imagers, but there is no manual focus mode available when the batteries run dry.
Final thoughts? The Mewlon 210 is an extraordinary telescope. I would recommend it to anyone, especially visual observers. It has enough light gathering ability to keep someone busy for a lifetime. The optics are crisp and clean. The telescope is light and easily carried. Maintenance might be higher with an exposed mirror. If you are an imaging nut, then be prepared to jump through some hoops and do some research to get the correct equipment. Enjoy! Telescopes are great fun!
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Last Modified: 3/19/03 8:55p
This page:© Copyright 2005 by John A. Blackwell