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Voyager 3

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Posts posted by Voyager 3

  1. 3 hours ago, Don Pensack said:

    Yes.  There are multiple reasons:

    1) magnification.  A 1" separation at 180x is an effective 3' separation.

    2) resolution.  1' is about the limit of resolution for the human eye.  A 4.5" telescope can resolve a 1" separation!

    3) exit pupil.  Visual acuity is higher when the pupil used is smaller than the dark adapted pupil.  A 2-3mm exit pupil behind the eyepiece will allow your eye to resolve better than the full dark adapted pupil diameter.

    Far fewer aberrations in the eye can be seen.

     

    Many years ago, someone posted a chart I'll try to remember:

    1' of arc--the limit of human vision

    3' of arc--the typical limit for a person with good, but not superb, vision

    4' of arc--the average resolution without strain--fairly easy for most experienced observers.

    8' of arc--an easy resolution for the average eye without perfect correction of vision--just about everyone can see this easily.

    How that translates:

    a star with a 1" separation will be seen as double by the person with a resolution of:

    1' at 60x

    3' at 180x

    4' at 240x

    8' at 480x.

     

    Perhaps that will give you an insight into why people need such radically different magnifications to split close double stars.

    I can see ε Lyrae as double with the naked eye with glasses on.  In a scope, that translates to 78x to see all 4, and that is close to accurate--I can see all 4 stars at 83x fairly easily.

    An easy split by everyone, though, might require 209x.  Certainly, seeing them all is much easier at the higher magnification.

    People's eyes differ a lot, and scope quality and seeing can interfere as well, so there is no set magnification to see any double star.

     

     

    And as you may know the ∆ mag of the double can affect the resolution even though it's not a direct factor . It is the direct result of the size of the airy disc .

    Evenly matched pairs are a good test for resolving power of eyes / telescope / seeing . 

    • Like 1
  2. I wanted to know why you northerners always complain about low elevation of planets in recent times . So one day in early August , I cooled the dob and pointed the scope soon after it got dark . Jupiter would have been at 10-15° altitude . 

     

    My first reaction was no thanks . Bam ! What a blurry mess . The interesting thing was , the blurry , seeing effect was much more prominent and disturbing than the very mild bluish-reddish AD . Mind you , I never view the planets that low and I've never seen AD before on planets to be that much prominent , but still it wasn't the major factor in the poor views of Jupiter and Saturn . Fortunately I didn't feel the requirement of ADC , at least for my eyes , equipment and location .

    Now now I feel pity for folks who live much Norther than me . Luckily this trend will improve in the coming years ;) .

    • Like 1
  3. I remembered this thread in mind and I tried yesterday . I was easily able to tell Ganymede and Callisto were much larger than background stars ( and other 2 moons for that matter ) . I later checked SkySafari and confirmed that both the semi-point sources were indeed Ganymede and Callisto. It was a bit difficult to tell the extended nature of Io and Europa as one would expect from their sizes . 

    It's fun and I recommend you try to see which are the moons comparing them to background stars before checking it with the software ! 

    I used just 96× as seeing was bad but the lower power helped mitigating it . GRS too was visible ! 

    • Like 1
  4. 3 hours ago, John said:

    The O-III is worth having for the Veil Nebula complex alone. There really is so much to see there :icon_biggrin:

    A UHC will show it but an O-III is has much more impact.

    A good rich field refractor , a dark site , an OIII filter can keep anyone busy for a lifetime . The Veil nebula bubble helps too . 😀

  5. 52 minutes ago, Jiggy 67 said:

    ……..It’s neck and neck!!  Nothing to split between the UHC and 0III !!…….🤣😀

    Then getting both the filter at the same time is the best solution to please all of us . :evil: 

     

    Just kidding , buy either of them first , keeping in mind that you will be buying the other eventually . If you really get into this hobby and have a good dark site , a H-beta filter will be a good tertiary filter . 

  6. If you will be getting both , then get the UHC first . It is more universal and will give a huge boost for the more famous nebulae like M8 , M17 , M42 , M16 etc . 

     

    The  get the OIII for use with some supernova remnants , wolf -rayet excitation nebulae , large planetary nebulae etc . 

    • Like 1
  7. 7 hours ago, Astro_Nic said:

    Thanks - will take a look at the APM 9mm

    It's weird as all the beginner guides say get barlows to reduce number of eyepieces, yet all the advice seems to be to not to bother......

    So say I get all 100 degree APMs - what targets would I use for each of the sizes - 5mm, 9mm, 13mm and 30mm ?  Is that a good spread?  340x, 170x, 123x, 53x ?

    What's the main difference between OIII and UHC filters?  Do you use both at once or just one at a time?

    Are the APMs suitable for binoviewers if I went that way?  

     

    Thanks!

    You will be using a Paracorr II / paracorr for the best correction to use with 100° stuff . It adds 1.15× to the FL/ Focal ratio . 

     

    So I take the FL as 1878 . 

    Here is your spread with 30mm ( UFF )-13mm-9mm-4.75mm( really a 4.75mm approximately and not a 5mm ) . The 30mm can be substituted by the 20mm XWA  , if your site is light polluted . 

    62× - 144× - 208× - 395×  . 

    As you can see this is a good set until you reach the 9mm . It's a really big jump from 9mm to 4.75mm . 

    A 6mm Ethos fits right in at 313× , but the 7mm APM XWA will also be a good step up at 268× . 

    Now it looks like 

    62× - 144× - 208× - 268× - 395× . 

    Basically you may still need to fill the gap between 7mm and 4.7mm but it is down the list . A coma corrector like the paracorr II must be your first purchase . This assumes you already have good collimation tools . 

     

  8. 7 hours ago, JeremyS said:

    CCD is cooling, but thin high stuff has come in. 

    Will probably put my 0.06m refractor out later.

    Approximately 10 nanosecond cooldown time

    Noooo ! It is 0.00000001 second cool down time :headbang2: .

    • Haha 1
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