Quote:
Originally Posted by alistairsam
i read somewhere that the losmandy mounts have a resolution of 1/2 arc sec based on the encoders on motor shaft and subsequent gear reduction which is quite high as they use servo motors in a closed loop.
|
This is roughly what the resolution for accurate tracking should be - at the RA shaft.
However, because of subsequent reduction (and PE introduced by it) this final resolution is pretty meaningless, because you still have PE introduced by subsequent reduction and this could be much larger (5-10arcsec for very good mounts) and unless it is not compensated in the software, you can't use it for long time exposures with long FL lenses, where you need sub-arcsec tracking accuracy.
Again, don't confuse time increments with angle, expressed in arcsec.
I mentioned earlier:
Quote:
... it is 3arcmin on both axes. The difference you are mentioning for RA is because for RA unit we use time (meaning, it takes 12 sec of time for the sky to rotate by 3arcmin in angle units)
|
So, the sky rotates for 15arcsec (angle, at celestial equatror) for 1 sec (in time).
The resolution of encoder needs to be at least 1arcsec (Angle, based on 1m FL, 5.7um pixel size), and that is 1296000 ticks at RA shaft.
The same goes for accuracy - if you have the above resolution, but overall PE introduced by subsequent reductor is +-10arcsec, you will see this on your photo as elongated star image, spread over ~10 pixels in E-W direction.
That is why I think that for good closed loop system you need the encoder with such accuracy and resolution (1 arcsec or better, directly on the RA shaft - and this is very expensive encoder).
Or, you can have encoder on the motor shaft, but the subsequent PE must be compensated somehow.. and the most efficient way is auto guiding.