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the equatorial mount
is designed
for pointing the telescope at the
celestial objects and tracking their
movement.
MT-3S
(MT-3S-2D) mount consists of
two axes square with each other: the
polar axis and the axis of declination.
There is a mounting plate with OTA
rings on the top point of the declination
axis, and a counter-weight shaft with
counter-weights on the other side.
It is possible to place all types of the
mounts on a pier or tripod.
The mount head has a clock drive
embedded, which enables tracking
of celestial objects with user defined
speed.
The speed is set by a hand controller
and has three tracking rates: solar,
lunar and stellar, as well as two
additional correction speeds - acce-
leration and deceleration at 50%.
Hand controller has a night light
lamp.
For the first sight-in on the object,
loosen the telescope’s Dec. and
R.A. locks (2) and move the
telescope to center an object in the
field of view.
The fine alignment is done by manual
Dec. slow-motion controls (2) on
Dec. axis, and R.A. slow-motion
controls (3) embedded into the
clock drive.
The polar axis has embedded polar
axis finderscope (optional) (5) and
is fixed in a tripod (pier) mounting
head with a latitude dial.
m o u n t m T - 3 S - 2 D h a s a
drive according to the axis of
declination.