AsteriX. Pointing software for telescopes PDF Stampa E-mail




Built in the years '60, this telescope is located at our stellar station at Serra La Nave (mt 1750 asl).
In order to achieve a good level of automation of the pointing system, the original mechanics has been modifyed by our staff.
The original system of a.c. motors and gear-boxes was upgrated with only two brushless motors capable of running, with constant torque, up to 5000 rpm.
The same motor, therefore, allows a positioning of the telescope without jerks by a soft moving, up to a fast speed at the telscope of 1 degree for second.

For both axis of the telescope, the original transission system of endless screw & toothed wheel has been mechanically interfaced with two incremental encoders for a pointing with an accuracy better of 5 arcsec.

The "glue" between mechanics and software is electronics.

From the hardware of motors to the user's interface, the system has four levels of feedback: for the control the speed of the motors, the precision of their speed, their positioning and the position of the whole telescope.




A first level of supervision of the motors is performed by the Servo Amplifier with a Tachogenerator.
An intelligent motion controller (by Galil) performs a second and a third level of feedback with a digital control of the speed and the position of the telescope.

The supervising control is done by a Pentium @ 600 MHz Personal Computer. There the Asterix software check the position of the telescope and ensures that the requested star is into the observing field.





Here is a block diagram of the telescope motion control system.

The first level of feedback (the analogic) is drawn in brown.
The second level of feedback (the digital for speed) is drawn in red.
The third level of feedback (the digital for positioning) is drawn in orange.
The fourth level of feedback (the software for pointing) is drawn in yellow.



The Asterix program (written by Bruno Fedel in the 90's years and rearranged by S. Massaro in the 2000) performs the calculation of the position in the sky for a requested star (at a specific time) and ensures the positioning of the telescope near the star field.



Ultimo aggiornamento Martedì 04 Gennaio 2011 09:55