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GazOC

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Posts posted by GazOC

  1. On 23/10/2020 at 01:54, John said:

    It's somewhere between FPL-51 and FPL-53 in terms of potential for CA control but remember that the glass used in the mating element plus the figure and polish of the lenses is equally important.

     

    Not much chance of forgetting it, John. You can pretty much guarantee that someone will make that comment every time a thread is started about glass types 😉

    • Haha 1
  2. Hi all,

    I was looking at dipping my toes back into a bit of lunar/ planetary imaging and was dead set on getting a ZWO ASI 290MC camera but then saw this from QHY. Does anyone have any experience or views on it?

     

    https://www.modernastronomy.com/shop/cameras/lunar-planetary/qhy-lunar-planetary/qhy5iii462c-planetary-and-nir-imaging-camera/

     

    It seems an attractive option with the far IR sensitivity as I definitely want to go down the OSC route for planetary but would also like the advantages mono gives for lunar imaging.

  3. 3 hours ago, Nair al Saif said:

    The evostar was it an achro or an ed and why was it better?

    It was the achromat. I didn't have them both side by side but I'm pretty sure I had them at the same Jupiter opposition (it was ~15 years ago so I can't be sure). 

    The 127 gave clearly better views of Jupiter than the 120 and I've always regarded the planet as the acid test for refractors.

    Ironically, given the question, I sold the 127 when I bought an ED120 which rendered the achromat a bit redundant

  4. 11 hours ago, mikeDnight said:

    Here goes:  There's another thing to consider also and that's the amplification factor of the secondary mirror. I seem to remember from years back that an F2 primary with a 5X amplifying secondary, creating a F10 system, doesn't amplify the heat errors by 5X, but by 25X. (5X^2). So thermal equilibrium is much more difficult to achieve in a catadioptric system using an amplifying secondary, or even with an open Cassegrain design. What puzzles me though, is that a Maksutov always seems to perform better, presenting sharper stars and higher definition than a SCT. Why? I have no idea! Perhaps it's that awful Schmidt corrector plate that's responsible for those cotton wool star images and drunken planetary views?? 

    I'm working on being more sensitive. How am I doing?👍👎

    The reason I've read is that, while in an ideal world there's no reason a Mak/Cass should outperform a SCT, it's easier to accurately mass produce the Mak corrector than it is the SCT corrector so the customer is more likely to get better quality optics.

     

    (Disclaimer: I am not a telescope manufacturer) 😉

  5. @John I tried to find one but couldn't but if you can locate a similar diagram for an ED doublet or an achromat it may show the idea more clearly 

    Depending on how the designer has chosen to set up scope the focus point for the wavelength at the blue end of spectrum will be further apart from the on the vertical scale  from where the red/ green wavelengths come to focus than it is the example above. This is the CA you see at the eyepiece 

     

    • Like 1
  6. 1 hour ago, JamesF said:

    I've just had a quick look at my (blue Skywatcher) 127 Mak.  I reckon the clear aperture of the corrector alone is no more than 118mm.  119mm at the very most.

    James

    I've taken the corrector out my blue Mak and made a couple of *very quick* measurements. 

    The clear aperture of the front of the corrector seems to be 127mm, the back of the corrector is harder to measure but the ID of the cell is 133-134mm with a ~3mm lip all around near the corrector so somewhere very near 127mm.

    I wish I'd have measured the primary when I had the thing stripped a few weeks ago as that is often given as the reason for the restricted aperture but haven't got the stomach to attempt that job again 

  7. 2 minutes ago, John said:

    Thanks Gaz - I'm glad I was not imagining it !

    So I wonder just what Synta / Skywatcher did actually change to increase the effective aperture ?. Maybe nothing and the tales of the 180's operating at less than 180mm are myths ?

     

     

    The mirror is oversized and there's lot of space in between the mirror and the tube so I can't see that being the problem

     

    To me, that leaves the baffle coming out of the primary (realistically the secondary baffle isn't going to knock off 10mm from the effective aperture) as the only possible culprit but  whoever designed that part has made sure it tapers in as it gets closer to the secondary. 

    Just MHO but I'd be surprised if Skywatcher redesigned the scope to give it an extra 10mm aperture and then said nothing about it ? 🤷

    • Like 1
  8. 1 hour ago, John said:

    I've seen a thread somewhere on the original gold tube 180 which showed that it has a primary the same diameter as the more up to date one that @Captain Magenta took apart recently. Is there some other modification that would increase the effective aperture such as a re-designed secondary baffle ?

     

    That'll be me 😉

    The mirror is 200mm. It could be that that baffle coming out of the primary is cutting out light but it looks very carefully graduated in width as it approaches the primary

     

    Someone has put a lot of thought into the width of the baffle at any given point. That's not to say they've not just got it wrong but they've not just stuck a tube on and hoped it's correct 

    • Like 1
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