I am still waiting for the finder bracket I ordered to attach a Tak 5X30 finder scope I already own to my just purchased Tac FS-102 NSV. It is due to be delivered tomorrow. But being impatient to test out my new APO, I used a Styrofoam block as a spacer and taped the finder to the telescope as a stop-gap solution. Its pointing accuracy was sufficient to allow objects to be seen in the telescope's field of view at 32 power.
I also took out my diminutive 4 inch Meade SCT for comparison, as it is the only other 4 inch telescope I own. Viewing through this tiny treasure earlier this evening reaffirmed my belief that its optics are not just good, but shockingly so!
While the telescopes cooled, I pointed them at the moon for views at 100 to 125 power. While the FS-102 was much brighter, as expected, and sharper, the little Meade came closer the Takahashi's level of sharpness than anyone would have any right to expect. I had to look at very faint and intricate features to really to see the differences in sharpness.
Don't get me wrong, the Tak was bitingly sharp, and its superior contrast made subtle details more distinct. But on a high contrast object like the moon, the resolution of the micro Meade was something to behold! And how about this...?
Last night I pushed the punchy little Meade to 286 power for a peek at Eta Orionis, a double with a separation of 1.5 to 1.7 arc seconds. Even though the seeing was not perfect, the double was cleanly split, with no flaring and dark sky between the components. I have separated even closer doubles on occasion, and the double-double is laughably easy.
After the telescopes had fully cooled, I pointed both toward Polaris for some impromptu star-testing. The Meade displayed one of the most aesthetically beautiful star images I have ever seen! By aesthetically beautiful, I don't mean optically perfect, like was displayed by the Tak FS-102. I just mean visually impressive.
In the Meade, the stellar disk was hard and round, and was surrounded by a very distinct and perfectly circular diffraction ring. It was the visibility and intensity of this ring, resulting from the SCT's large central obstruction, that made the image so striking.
On the other hand, the image in the Tak was, to use a somewhat worn-out cliche, textbook perfect. The diffraction ring was much fainter, and the central disk much brighter and more intense, as would be expected in an optically perfect, unobstructed system.
I finished out the evening using the FS for peeks at Alberio and Almach. Both were indescribably lovely, their colors intense and true.
I stand by my previous posts extolling the virtues of beautifully corrected achromats, but I must confess I am having to re-adjust my understanding of just what is possible in a refractive optical system!
Sincerely,
Steve
Edited by Steve Allison, 17 October 2018 - 02:29 AM.