
15" f/4.5 Teeter Dob
#1
Posted 26 October 2005 - 06:20 AM
#2
Posted 26 October 2005 - 10:22 AM
#3
Posted 26 October 2005 - 01:24 PM
#4
Posted 26 October 2005 - 01:53 PM
#5
Posted 26 October 2005 - 02:30 PM
#6
Posted 26 October 2005 - 03:11 PM
#7
Posted 26 October 2005 - 10:47 PM
Clear Skies,
Larry
#8
Posted 28 October 2005 - 03:05 PM

The mirror in this particular scope (R.F. Royce) is just phenomenal. It's just about as big as Royce likes to go and I have a hard time believing this mirror came in at his bottom line of 0.95 Strehl, it's certainly much much better than that. I would applaud Royce right here and now, but my hands are quite tired from doing that every time I look through a scope with his mirror in it.

Take care,
Rob Teeter
Owner, Teeter's Telescopes
#9
Posted 28 October 2005 - 04:20 PM

#10
Posted 29 October 2005 - 03:23 AM
They are being placed slightly closer together as a small slice of the mirror was not getting direct airflow. So the name plate and some handles are being placed different.
Yes - but I was wondering how *high* they were in the box with respect to the mirror.
I have a similar setup, with the fans' bottom 2cm higher than the mirror's face, and if I set them up pulling air, I have to put a baffle at the top of the circumference to avoid them pulling air mainly from the top of the mirror box (instead of from the face of the mirror). I'm wondering if they may not just have been placed slightly too high (not that I'm going to change things now that it works - just wondering. The drawback to the baffles is that I can no longer transport the secondary cage in the mirror box).
#11
Posted 29 October 2005 - 08:55 PM
I don't understand why you used the phrase "even though". Would a larger f/ ratio make a difference?
I ask this because the November issue of Astronomy magazine makes a big deal of the views through a public f/7 31" Newtonian, but much less of a deal of a f/4.5 30" Newtonian.
#12
Posted 02 November 2005 - 08:06 PM
The difference is that 1)its harder- to figure a faster mirror to high precision (High Strehl)
2)Collimation becomes so critical in a fast scope that often they do not perform at their full potential. 3) Keeping the secondary small in a fst scope is a bit more tricky.
However these are merly challenges and not insurmountable obsticles a fast, well colimated Royce, Zambuto etc. will deliver fantastic planetary images under goo conditions.