GeNeral INSTruCTIONS Warning! Never observe the Sun directy through your telescope or its finder scope - permanent eye damage could result. The telescope is designed for visual observations of celestial objects and for astronomical photography. It requires careful treatment and some knowledge of astronomy. Only in this case the use of telescope will bring satisfaction to its owner.
INVeNTOry lIST Component Tal-1 Tal-150P Tal-150P8 TAL-1М Tal-2 Telescope finderscope: Polar axis finderscope equatorial mount: MT- with counter- weight 2.2 kg MT-C with counter- weight 2.2 kg MT-3S (MT-3S-2D) with counter-weight 2.2 kg (2 units) MT-3S (MT-3S-2D) with counter-weight 3.7 kg (2 units)
CONSTruCTION Of The TeleSCOPe The telescope consists of three main parts: - Optical tube assembly (OTA) (), - German equatorial mount (2), - A pier or tripod (3). The optical tube is a basic component of the telescope. It includes all main optical units such as a primary mirror, a diagonal mirror and a focuser.
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To provide the smoothness of TAL-1 telescope focuser, hold the left focus knob (1) with one hand and turn the right focus knob (2) clockwise (with a little effort) with other hand.
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Different models of telescopes are provided with different mounts. The mount MT-1 has manual slow- motion controls on both axes and is used with TAL-1 telescope. For the first sight-in on the object, loosen the telescope s Dec. and R.A.
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M T- 3 S m o u n t i s u s e d w i t h telescopes with primary mirror diameter of 150mm and above. The mount head has a clock drive embedded, which enables tracking of celestial objects with user defined speed.
PreParING TeleSCOPe fOr ObSerVaTIONS aSSeMblING The TeleSCOPe Take a pier (1) and legs (2) out of the package. Attach tightly three legs to the bottom point of the pier using the captive screws. The pier must not swing on the legs. Place the pier on a firm plain ...
Place the finderscope bracket (1) in the wedge slides for TAL- TAL-150P, and TAL-50P8 telescopes. Tal-1 and TAL-1M telescopes have finderscope bracket mounted directly on the OTA. Fix the finderscope with six thumbscrews (2). balaNCING The TeleSCOPe To provide a smooth motion of the telescope and reliable operation of equatorial mount drives, the balancing of the telescopes is required.
Keep in mind that if the telescope is not balanced properly, the clock drive periodic error will increase. alIGNING The fINDer SCOPe High magnification of the main telescope makes it difficult to find a required celestial object in the sky because of the small field of view. This is why the telescope is equipped with a low-power finder scope with a wide field of view.
POWer SuPPly aND haND CONTrOller Warning! always connect power supply to the mount using the power cord with power supply disconnected from the power outlet. use only original manufacturer s power supply fuse or analogue (consult your dealer). always disconnect all the power, if replacing the power supply fuse.
For MT-3S mount connect the hand controller to the socket (1). Then follow the same procedure as for MT-1C mounts. If the telescope is used in the Southern hemisphere, the directi- on of the clock drive rotation must be changed.
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For visual observations point the R.A. (polar) axis of the telescope towards. Polaris Polaris ( uMi). See the picture. α With this level of pointing accurary, very little use of the Dec. slow- motion control is necessary for Ursa Major celestial objects tracking.
CalIbraTING The SeTTING CIrCleS R.A. and Dec. axes have setting circles, which enable observer to locate an object in the sky by its celestial coordinates - right ascension (R.A.) and Declination (Dec.). Calibration of setting circles is done after polar alignment of the telescope. Level the Dec.
ObSerVaTIONS When using higher magnification not only the visible image size ap- pears larger in the telescope, but also blurring and distortion of the im- age, star twinkle, caused by atmosphere become more significant. To achieve maximum stability of the visible image and best performance of the telescope, all parts of the telescope need to reach thermal equilibrium with...
Use focus knobs to focus, when changing eyepieces. Provided eye- pieces give several magnification options for an observer. Tal-1; Tal-1M Plössl f'=25 mm Plössl f'=10 mm Tal-150P Plössl f'=25 mm Plössl f'=7.5 mm Tal-2; Tal-150P8 Plössl f'=25 mm...
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For higher magnification, use Bar- low lens with one of the eyepieces (see picture). 2 Barlow lens doubles magnification of the telescope. TAL-1; TAL-1М Plössl f'=25 mm, Plössl f'=10 mm, Barlow Barlow Tal-150P Plössl f'=25 mm, Plössl f'=7.5 mm,...
aSTrOPhOTOGraPhy For astrophotography with TAL- and TAL-1M telescopes mount a camera (1) on the camera holder (2), which is attached to the coun- terweight shaft. Fix the camera to the holder using the lock knob (3). As a long exposure is required for ...
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For astrophotography with TAL-2, TAL-150P and TAL-150P8 tele- scopes use the same procedure as described above. However prime focus photography is also available when using M42x1 objective thread cameras (M42x0.75 thread camera adapter is also supplied with the telescope). For the prime focus setup unscrew ...
MaINTeNaNCe In order to keep telescope in good operating condition one should provide good care and maintenance for the instrument. Please note that lens or mirror surfaces should be cleaned as infrequently as possible, only when absolutely necessary. Optics self-cleaning only permitted after expiration of manufac- turer limited warranty! Keep telescope clean and protect it from any physical damage.
COllIMaTION (alIGNMeNT) Of The OPTICS Collimation (alignment) of the optics is permitted only in case of absolute necessity, and after expiration of manufacturer limited warranty. In case of accidental mirrors misalignment or after cleaning optical parts, telescope collimation might be necessary. To inspect the view of the mirror ...
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the reflection of the secondary mir- ror with spider vanes will be out of center. For TAL-1 and TAL-1M collimation, loosen the three small screws that lock the primary mirror (). Then adjust the tilt of the primary mirror...
STOraGe The telescope must be kept in a clean, dry (humidity must not ex- ceed 80%), dust-free place with an ambient temperature between +5° and +40°C. Avoid collision and shaking of the telescope. It is prohibited to store acids, alkalis, and any chemically active ...
Appendix A Precise polar alignment for the MT-1 and MT-1C mounts For precise polar alignment for MT-1 and MT-1C mounts observe two bright stars in the west and in the east by turns, using the eyepiece f’=25mm with reticle. If during the observation of the star in the east it slowly shifts, so that you have to lower the top end of the telescope to follow it, then the northern (upper) side of the R.A.
Appendix B Double stars list for telescope image quality test Coordinates r. a. Declination Star Constellation 2000.0 2000.0 ° α Psc 4.3-5.3 .9" Pisces ° γ Cet 3.4-4.4 2.8" Cetus ° ζ Ori 2.0-4.2 2.5" Оrion ° α Gem 2.0-2.8 .8"...
Appendix C brightest stars visible in the Northern hemisphere Declination Visible r. a. Star Constellation 2000.0 magnitude 2000.0 0 h 08 m 2.07 m Alpheratz α And Andromeda ° h 09 m 2.07 m ° Mirach β And Andromeda 2 h 3 m .97 m Polaris...
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