Showing posts with label Tips and Tricks. Show all posts
Showing posts with label Tips and Tricks. Show all posts

Thursday, October 31, 2013

"Cartes Du Ciel" (CdC): Grid Settings

One thing that irks me to no end in CdC from day one is the grid spacing: When you zoom in, the grid lines jump around, as the grid spacing changes. One possibility would be 30°, 15°, 5°, 1°, 0°30' and 0°15'.

But the default grid spacing is 20°, 15°, 10°, 5°, 2° and so on – which is utterly utterly UTTERLY braindead.

But, do not fret! One can change the settings!

But fuck you very much, there are bugs: Because once you start to set the grid spacing to sensible values, the grid lines start to appear horizontally and vertically at different zoom levels. Seriously, WTF?

But that isn't the worst bug, not by far! At certain zoom levels the grid lines disappear completely! Instead, the "compass rose" appears for no apparent reason whatsoever… (at least here on my Macintosh). I think it is a problem when the grid spacing does not change from one so called "field of view number" to the next – but I could not quite nail the problem. Changing the field of view for a "field of view number" moves things around.

Before I started to curse, I initially wanted to simply write down how to set the grid spacing to sensible values – but it didn't seem possible, so I had to vent some air.

But after some fiddeling I managed to cobble together some working settings (the working values might change with different versions, as the code handling the grid spacing seems buggy…).

Setup > Chart, coordinates > Field of vision

Set the following values:

Field Number "From" value
1 0.75 (was 0.50)
2 1.0
3 2.0 (was 1.5)
4 5.0
5 10.0
6 30.0 (was 20.0)
7 45.0
8 90.0
9 180.0
10 310.0

Setup > Chart, coordinates > Grid spacing

Set the following values:

Field Number "Declination grid" value
0 +00 05 00
1 +00 15 00
2 +00 30 00
3 +00 30 00
4 +02 30 00
5 +05 00 00
6 +15 00 00
7 +15 00 00
8 +15 00 00
9 +45 00 00
10 +45 00 00

For me, these values result in a halfway useful grid being displayed most of the time. Occasionally the jumps between zoom levels are not smooth, but hey…

[Update] I hate CdC. Now that I have set the grid spacing to sensible values, I can now see the grid moving relative to the stars when I scroll around with the cursor! WTF? This is a cesspool. The code for displaying the grid in CdC seems to be horribly buggy.

"Cartes Du Ciel" (CdC): Setting Star Catalogs And Limiting Magnitudes

While there are some quite irksome UI particularies in Cartes Du Ciel, I find the software somewhat useful (considering it is free!) and haven't found an free alternative (and I don't expect to find anything better).

One thing I had to change is the amount of stars visible: It was far too few, and I could not related the view through my scope with the display by CdC. I was looking for the "tail" in the Pleiades, but wasn't able to find it. For these faint stars to become visible, one hast to change some settings:

Setup > Chart, coordinates > Object filter > Deep sky filter

Set "Limiting magnitude" to 13 for "Field of vision number" 1 to 4 – the rest should be fine. I don't know if 13 is the best choice, but for me it works OK (and it should show somewhat more than I can see with my scope).

Setup > Catalog > CdC stars

Make sure these two are selected:
  • "Extended Hipparcos" (min 0 to max 10, cat/xhip)
  • "Tycho 2" (min 0 to max 5, cat/tycho2)
The last one has apparently replaced the "Hubble Guide Star Catalog".

With these changes, one should see more stars, and get a view that resembles more the view through the scope.

Saturday, October 19, 2013

Improving My Chinese-Build 6-inch f/5 Newtonian Telescope (Mainly Cooling)

I am currently looking into ways how to get the maximum performance of my cheap "light-bucket" 5.9-inch Newton scope, with minimal resources. Unfortunately – as with all affordable Chinese-build scopes – it is far from being "well-designed" and has several shortcomings, some of which should be addressed.

First of all, there are some points that might need addressing to get the maximum performance (the "last ten percent"), but which I will probably not do:
  • Increase the Fully Illuminated Field. The position and size of the secondary are such that only the central on-axis point is fully illuminated (and only just about). But then again the obstruction through the secondary is small (about 25%), so for visual use this should be fine.
  • Wider Tube. At the moment the tube is just a whee bit larger then the mirror – the diameter of the tube is about 170mm (6.7 inch, haven't properly measured it yet), with the mirror diameter (hopefully) being 150mm (5.9 inch). A wider tube might aid the cooling, but that would mean a complete rebuild – but in that case I would probably try some sort of portable design or even some ultra-light Dobsonian design for that scope.
  • Thinner Spider Vanes. These things are thick! Cast metal, baby! But probably the spikes won't bother me…
But if I wanted a perfect scope, I should start by getting a perfect mirror (and probably a larger one at that!), because my mirror is most certainly not top notch. So as my time&energy&money are limited (and as I will not buy a better mirror), next are some points which should be reasonable, and which I will therefore address:
  • Focuser shifting. While I have addressed this already, the focuser is now too stiff and I need to readdress this problem once more.
  • Baffling. I will have to add some felt in to focuser tube and opposite the focuser, and possibly baffle(s) in the focuser and at the mirror cell. Plus the secondary's holder is made from shiny plastic – I should baffle this as well.
  • Cooling. This is at the moment the most obvious problem: Tube currents despite ample cool down time.
With regards to focuser shifting, I will have to see what I will come up with.

Mel Bartels has something to say about baffling:
Proper baffling ensures that no unwanted light enters the focuser. There is a baffle just below the focuser and a baffle opposite the diagonal. The focuser baffle is particularly important.  Both are covered with Edmund Scientific black felt. The primary is also baffled, just in front of the glass, and totally enclosed in ultra flat black. It is an impressive demonstration to shine a powerful flashlight on any part of the scope, and discover that your observing buddy looking through the eyepiece with his eye cupped cannot tell you when you have the light on or off. The goal in baffling a minimalist ultra light is to block every ray of light not coming from the primary mirror. Extra baffling to absorb secondary reflections from the baffles is used in high performance refractors, but this is a luxury we can forego since the flashlight test is quite convincing when using light trapping felt or velvet.
With regards to cooling, the simplest way is to add a fan is at the rear. There are more elaborate ways of cooling (and the first order of business is keep the primary mirror as thin as possible), but these methods are overkill for my puny 6-incher: One could add a fan in front of the primary, blowing on the primary. Or one could add a fan at the side, creating a laminar flow across the front face of the primary, and scrubbing that darned boundary layer of the primary. Best would be to actively cool the primary through some attached machinery (cooling pipes, peltier elements, and somesuch black magic).

Bah humbug, too complicated and not needed for my scope. (Though I would love for a bigger mirror to combine electronically controlled peltier elements at the rear of the primary, with a laminar flow across the front face of the primary – should make one heck of a good scope I'd reckon.)

Instead I will stick to putting a fan to the rear end of my scope, and call it a day. But should it act as an "rear exhaust", sucking out warm air? Or should it be a "rear intake", blowing cold air at the back of the primary?


Advantage Disadvantage
"Rear Exhaust" – Motor heat is kept away from the primary
– Better scrubs that boundary layer off the primary (maybe)
– Less dirt in the tube (maybe)
– Less efficient cooling of the primary
– Increases the dew-risk for the secondary (maybe)
– Works against the natural convection (possibly maybe more turbulent)
"Rear Intake" – More efficient cooling of the entire rear face of the primary
– Keeps dew away from the secondary (maybe)
– Works with the natural convection, not against it (should be less turbulent, maybe)
– Motor warms the air
– Sucks in more dirt from the ground (maybe)
– Not so good in scrubbing the boundary layer off the primary (maybe)

So I will go for the "rear intake" solution, and mount it on "some sort of circular mask" so the fan is decoupled from the scope, and air is forced in. With a 6-inch diameter primary I count on the glass being 2-inch or less, so it should be enough to cool it from the rear.

What I dread is adding batteries, cables, connectors and the like – it will complicate the setup, and I already hate the thought of it. And I need to take care of my powersource, change/charge the batteries – bah!

And to add a fan I have to take the scope apart, I guess…

Tuesday, October 1, 2013

Indoor Astronomy

One thing you hear from time to time is: Astronomy can't be done indoors. Well, I say Bah Humbug! to that.

Well of course the quality of the images is better if you schlep yourself and your astronomical gear outside. First of all you don't have the window panes between your fine astronomical instrument and the astronomical object you want to observe. As you probably do not have windows made out of a multi-coated, λ/4 polished, BK7 glass (or better), the image will be somewhat degraded by the window panes. But even if you do open the window, the temperature difference between inside and outside will lead to thermal currents which can degrade the image. And of course the portion of sky one can see is limited.

Having said that, you can do astronomy from indoors. In summer I observed Saturn with its majestic rings from inside. I opened the windows half an hour before I started observing and I didn't notice any problems.

Then in the last month I observed through the closed window and got quite nice views of the Moon at around 60x magnification.

And on Sunday I saw the Pleiades just fine from inside at 12x magnification.

Of course, the fainter and the smaller something is, the less likely it is to be viewable from inside. Conversely the less difficult an object is, the more likely it is to be viewable from inside. If you can go outside to observe, than by all means do it! But sometimes there are reasons to stay inside (staying outside in the cold is not good my health) and then it is good to do astronomy from indoors.
    [Update 2013-10-23] I have to report that I tried yesterday to observe Jupiter from indoors, through the closed window and it was not good. The disc was not resolved sharply, and the two visible jovian moons were turned into smudges (the other two moons were transiting Jupiter, or close to the limb, I take it). So low magnification is OK from indoors (say for open star clusters, or the Moon), but trying to do any "serious" astronomy through a common window-pane is not the way to go :-D

Secondary Mirror Too Small: Regain Lost Aperture With An Barlow?

    [Update 2013-10-13] On second (third? fourth?) thought, I don't think this works like that. The Barlow lens would need to be before the secondary to recover lost aperture.
By now, I have two Newton telescopes with an "undersized" secondary mirror (won't illuminate full primary mirror), and I just realized:

If you use an Barlow with these scopes, then more of the primary becomes visible.

The closer the Barlow's lens is to the secondary, the more pronounced the effect is – so a "Shorty" Barlow is not as good as one with a long barrel. (Though the optimum for spherical mirrors would be a good "Bird-Jones" corrector.)

And one needs to make sure that the Barlow itself does not introduce vignetting itself…