background image

Part I: Introduction 

 

Part I : Introduction 

Sky-Watcher  Quattro-200  ST:  Sky  at  Night  magazine  group  test 
winner scoring 89% 

The superb Skywatcher Quattro-200 ST telescope OTA has beaten all the 
opposition  to  win  best  in  class  in  the  November  2011  Sky  at  Night 
magazine. 

The  most  acclaimed  feature  of  the  Quattro  200 
astrograph  is  the  knife-edge  baffle  system.  The 
Quattro's tube is lined with a set of nine internal baffle 
rings. Their main purpose is to cut down on stray light 
entering  the  telescope  tube,  greatly  helping  to 
improve image contrast. 

The Quattro is fitted with a Crayford-style focuser with 
tension adjustment, focus-lock and a 10:1 dual-speed 
fine focusing, and also comes with a 2-inch fitting that 
has  a  T-thread  on  its  external  side.  This  allows  a 
sturdy  connection  to  be  made  between  scope  and 
camera with the right adaptor ring. 

The primary and secondary mirrors are made of Low 
Expansion  Borosilicate  Glass,  for  near  zero  thermal 
expansion. 

The  impressive  0.5  mm  Ultra-Thin  secondary  mirror 
vanes  ensure  minimal  thermal  accumulation  and 
reaches thermal equilibrium in no time. 

The  secondary  mirror  support  is  mounted  offset,  for 
perfect optical collimation. 

Optimized  for  astrophotography,  with  its  baffle  system  and  parabolic  primary  optics  with  a 
very  fast  f/4  focal  ratio,  the  Quattro  200  is  designed  for  exceptional  wide-field,  deep-space 
imaging  performance.  Even  faint  galaxies  and  nebulas  exhibit  stunning  detail  with  limited 
exposure time when photographed with a CCD imager or DSLR camera. 

The Quattro  200  is  proposed  with  two  options for  the  tube:  Standard Tube  (ST  series)  and 
Carbon  Fiber  (CF  series)  for  astrophotographers  dealing  with  long  to  very  long  exposure 
times.  The  Carbon  Fiber  series  can  remain  in  focus  for  a  longer  period  of  time  and  long 
exposure images will stay clear and in focus. 

 

 

 

NEVER  USE  YOUR  TELESCOPE  TO  LOOK  DIRECTLY  AT  THE 

SUN. PERMANENT EYE DAMAGE WILL RESULT. 

 

NEVER USE AN EYEPIECE-TYPE SOLAR FILTER. 

 

NEVER USE YOUR TELESCOPE TO PROJECT SUNLIGHT ONTO 

ANOTHER  SURFACE;  THE  INTERNAL  HEAT  BUILD-UP  WILL 

DAMAGE THE TELESCOPE OPTICAL ELEMENTS. 

 

USE  A  PROPER  SOLAR  FILTER  FIRMLY  MOUNTED  ON  THE 

FRONT OF THE TELESCOPE FOR VIEWING THE SUN.  

 

WHEN  OBSERVING  THE  SUN,  PLACE  A  DUST  CAP  OVER 

YOUR  FINDERSCOPE  OR  REMOVE  IT  TO  PROTECT  YOU 
FROM ACCIDENTAL EXPOSURE. 

 

NEVER LET A TELESCOPE POINTING THE SUN UNATTENDED. 

 

 

 

Summary of Contents for Quattro-200 CF

Page 1: ...Quattro 200 ST CF Newtonian Astrograph INSTRUCTION MANUAL Copyright Sky Watcher QT200 F 140618V1 EN...

Page 2: ...eyepiece is provided with my telescope Is it normal 4 Why is no coma corrector proposed as standard 4 What does Sky Watcher propose for the Quattro series as accessories 4 Aligning the finder scope 5...

Page 3: ...equilibrium in no time The secondary mirror support is mounted offset for perfect optical collimation Optimized for astrophotography with its baffle system and parabolic primary optics with a very fa...

Page 4: ...cap for the 1 10 speed reduction s knob Assembling the finder scope 1 Carefully remove the rubber O ring from the finder scope bracket Position the O ring into the groove on the finder scope tube 2 Lo...

Page 5: ...r different purposes a standard low magnification eyepiece to check if the object is inside the field of view a high magnification eyepiece to observe Moon details and planets and many more usages wer...

Page 6: ...ed in and out of focus When focus is reached lock it in position with the knurled ring Fig 1 NEVER LOOK DIRECTLY AT THE SUN WITH THE FINDER SCOPE IT COULD IMPAIR DEFINITIVELY YOUR VISION When the find...

Page 7: ...plate Fig 2 2 simply unscrew the 11 4 inches tube Fig 2 1 form the 11 4 inches adapter Reassembling the 11 4 inches adapter can easily be done by following the preceding steps in reverse order 1 Asse...

Page 8: ...turn the 1 10 knob one way or the other until the image is perfectly sharp Fig 5 3 4 Tighten the locking screw Fig 5 1 if a heavy load is attached The image usually has to be finely refocused over tim...

Page 9: ...l image quality When looking at a bright star the star image given by your telescope should be symmetrical a central dot with diffraction rings centered on this white dot see Fig 2 Be patient to consi...

Page 10: ...lancing the tube with a heavy image train In Newtonian reflectors the secondary mirror intercepts the light and points it out the side of the tube at right angles to the tube through the eyepiece This...

Page 11: ...nsion by using the large thumbscrew below the focuser as shown in Fig 8 A correct tension allows to smoothly focusing but doesn t let the imaging train move due to gravity When in focus and centered d...

Page 12: ...econds Light Gathering Power Compared to Human Eye 858 x Fully Illuminated Field 44 mm 1 7 in Optical Tube Length 730 mm 28 74 in Optical Tube Weight ST Tube 9 5 kg 21 lbs Optical Tube Weight CF Tube...

Page 13: ...support available alongside with the list of distributors and dealers worldwide on our worldwide internet site http www skywatcher com Sky Watcher offers this product with the best available quality i...

Reviews: