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| Telescope Object Library |
| LOCAL= 12:00:00 SIDE = 14:00:00 |
| 01/01/00 _ |
| Telescope Object Library |
WARNING:: At this point the fork arm of the telescope will start to slew to an hour angle that approximates the position of Polaris for the current time and date. It is possible (and has happened with regularity) for the black serial cord connecting the fork arm to the main panel to get wrapped around the main dial and stuck between the RA dial and the fork arm.
DO NOT LET THIS HAPPEN !!! The added resistance will cause a slippage in the worm gears and the alignment process will have to be repeated from scratch. I recommend holding this black cable in one's hand while the telescope is slewing to Polaris (or any other time it looks as if this cable may get wrapped around the telescpe).
If extreme pointing precision is required one may switch at this point between the superplosal eyepeice and a smaller eyepeice. One may even go as far as to use the luminated retical eyepeice, but this requires refocusing the telescope and usually one can use the 16 mm eyepeice and acheive excellent results.
Method Two
This method is useful if you are doing research on stars that are not listed under any of the catalogues in the control panel's database (which only consists of a few thousand stars). We have used this method while researching RR Lyrae variables.
document last revised 6/5/98 by Andrew Kinard