Frequently Asked Questions (FAQ)
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Mirror holder size |
Number of lugs
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0.75" to 2.48" |
One lug for all tube sizes. |
bigger than 2.48" |
Two lugs for all tube sizes. |
As a general rule, this isn't possible. The overhang ('A' dimension in the graphic) is predetermined by our tooling. However, you do not have to drill the spider mounting holes in your tube with high precision, as there is about 1/2" of total adjustment travel (i.e., +/- 1/4") to accommodate for measuring tolerances and other variables.
The exception to this are the spiders designed to be direct replacements for commercial telescopes. Those are designed with an 'A' dimension that matches the scope so no new holes in the tube are required.
We can typically ship secondary mounts in 1-3 weeks of your order.
Yes, we sell spider and mirror holder subassemblies separately, but be aware that these two components work together to allow for collimation. (The collimation screws are in the spider hub, while the clutch disk and semi-flexible shaft are part of the mirror holder.) In other words, one part without the other probably won't work unless you have a custom design in mind. For the same reason, our holders will not work in other manufacturer's spider designs. If you need either a spider or holder to replace a damaged component, please contact us for details.
Off-the-shelf bolt solutions for thumbscrew adjustment are to be strictly avoided. The problem is that standard bolts of sufficient length do not have threads fully formed along the entire bolt length. If you turn the screws in too much, the non-threaded portion of the bolt shaft will begin to engage the brass thread inserts in the spider hub. Once this happens, the entire spider is usually ruined, as you can't get the bolt back out without spinning out the thread insert. The insert and the bolt bind together.
The other problem is that most plastic thumbscrew heads have a diameter that's too large, and they will partially protruding into the light path. This is a particular problem for the 1.83" and 2.60" sizes, since the spider hub is nearly the same size as the secondary mirror.
We offer custom-designed finger adjusting screws as an option. They are fully-threaded aluminum shafts with precision ground tips and custom heads designed for your fingers in the dark. See our options page for more details.
Many of our products are very black and don't photograph well. The 3D rendered images show far more detail. That said, we do include a few traditional photographed images to show that the real product matches the virtual one closely.
The antidew heater is recommended for observers who frequently stay up well past midnight when dew is most likely to form, or live in a region where dew is a more persistent problem. Also, secondary mirrors in open truss-style cages tend to dew up more frequently than closed tube telescopes.
Any DC power source with a voltage of 13 volts or less will work with the antidew heater. The heater can be used at full voltage to clear dew that has been allowed to form, but only about 1/3 to 1/2 of this voltage is required to keep dew from forming. To lengthen the battery life, we recommend a solid-state controller like the Kendrick Controller to throttle down the power consumption of the antidew heater.
There are several ways to attach power wires to the two conductive vanes. It can be done externally or hidden inside the tube. More information can be found in the instruction manual for heated spiders.
Offsetting the secondary is the practice of shifting the secondary mirror away from the focuser by a small amount so that its geometric center is no longer in the center of the tube. From a purely optical standpoint, offsetting has no effect on optical quality, collimation, or vignetting. Incorporating offset will do no harm, but there is no optical benefit either. The only consequence of not offsetting is that the optical axis (i.e., where the scope's mirror is pointed) will not be perfectly parallel the tube's center axis.
If you have a Newtonian mounted a German equatorial mount (GEM) then offsetting will ensure the optical axis is parallel with the telescope tube's axis. Depending on the GOTO system, this can potentially reduce slewing/pointing errors. For Dobsonian mounted telescopes - even those with a GOTO system - having the two axis parallel is not important.
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Protostar, P.O. Box 368 New Albany, Ohio 43054 U.S.A. 614-375-3146
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