2
A
Fig. 44: Loosen control latch.
High latitude leg mounting hole.
Attachment knob.
Latitude control bar.
Fig. 45: High latitude leg mounting hole and corresponding attachment knob.
C
Fig. 46: Attach telescope to tripod.
However, owners who wish to perform astrophotography or use the Meade LPI or Deep Sky Imager (see PHOTOGRAPHY WITH MEADE’S AUTOSTAR SUITE, page 41, for more information) will find equatorial mounting indispensible to their needs.
Equatorial Mount
Equatorial mounting lines up the telescope’s polar axis with the North Celestial Pole (or the South Celestial Pole if observing in the southern hemisphere).
When using an equatorially mounted telescope, tracking (following) celestial objects is possible by turning on your ETX telescope's motor drive. The motor counteracts the Earth's rotation and keeps objects in the field of view of the eyepiece for
Equatorial Mounting Procedure
1.Assemble the tripod as described in Step #2 of How to Assemble Your Telescope and Tripod, page 12.
2.Loosen the latitude control latch (1, Fig. 44) and lift up the
3.Turn the tripod, so that the face of the
4.Line up the mounting hole on the base of the telescope labeled "High Latitude Leg" with the attachment knob that is closest to the latitude control bar (see Fig. 45). Line up the other mounting hole with the remaining attachment knob. Thread both attachment knobs into the base of the telescope. Tighten to a
5.Determine the latitude of your observing location from a road map, atlas or the
LATITUDE CHART FOR MAJOR CITIES OF THE WORLD, page 54. Loosen the latitude control latch (1, Fig. 47, on next page) and adjust the latitude control bar (4, Fig. 47) so that your observing site's latitude is just visible above the flat surface of the tripod head. Retighten the latch.
6.If you have not already done so orient the tripod leg (see Step #3 and 5, Fig. 48) so that it is pointing due North (if the location of Polaris, the North Star, is known, point the telescope directly at Polaris. Observers located in the Earth’s Southern Hemisphere must point the telescope due South).
7.The telescope is now equatorially mounted; the tripod must not be moved or else the alignment will be lost. Instead, use one of the following methods to move the telescope's optical tube to a desired celestial object.
(a)Loosen the vertical and/or horizontal locks (6 and 9, Fig. 1a and 1b) to permit the optical tube to be freely moved manually. Tighten the locks once you center on the object.
(b)With the horizontal and vertical locks in their “locked” positions, use the Arrow keys to move the optical tube.
Note: For most astronomical observing requirements, approximate settings of the telescope's latitude and
Using an Equatorially Mounted Telescope
Once your telescope is equatorially mounted, the telescope motor drive will keep a celestial object in the telescope eyepiece's field of view.
To Track a Star When Polar Mounted:
Make sure you have initialized your telescope before you try out this feature (see INITIALIZING AUTOSTAR, page 17).
1.Tighten the vertical and horizontal locks (6 and 9, Fig. 1a and 1b) if necessary.
2.Make sure that AutoStar is connected to the HBX port (C, Fig. 2) of the telescope’s computer control panel.
3.Flip the telescope power switch (A, Fig. 2) to the ON position.
The AutoStar screen displays a copyright message displays, followed by a short beep. Then AutoStar takes a few moments to start up the system.
4.A message displays that warns not to look at the Sun. At the end of this message, press the key prompted by AutoStar to signify that the message has been read and
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