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Reproduction of part or all of the contents of this document in any form is expressly prohibited other than for individual use only. All text, images and labels are property of Nimax Gmbh.

 

 

7. Using the accessories, a bit of math to 
understand how all it works. 

Using the accessories is easy and fun. To 
change magnification simply swap eyepieces. 
To get more magnification simply use the 
barlow lens. But how does all of this work? 
 

7.1. Power (magnification)

 

Your telescope has a focal length of 100mm. 
This is approximately the distance between 
the telescope lens and its focal point (very 
similar to the distance between the focus 
point of a loupe and the loupe lens). This is a 
very important feature, that allows to 
determine several interesting facts such as 
magnification. 

The magnification is determined by the 
telescope’s focal length and the used 
eyepiece. You probably noticed that the two 
supplied eyepieces are Plössl 25mm and Plössl 
10mm. This means that the Plössl 25mm is a 
25mm focal length eyepiece while the Plössl 
10mm is a 10mm focal length eyepiece. 

To determine the magnification just divide the 
telescope’s focal length by the eyepiece’s 
focal length. Let’s give an example for our 
telescope and the supplied eyepieces: 

Telescope’s focal length is 1000mm. 
Plössl 25 eyepiece’s focal length is 25mm. 

 

1000𝑚𝑚

25𝑚𝑚

= 40 𝑝𝑜𝑤𝑒𝑟

 

This means that the Plössl 25mm

 

eyepiece 

provides a 40x power (magnification). This 
seems low,  but when you try it, you will see a 
bright image with some (very good) details. 

7.2. Barlow Lens 

The barlow lens is a very interesting device. It 
is a negative lens, that multiplies the 
telescope’s focal length. So a 2x Barlow 
multiplies the original focal length by 2x, in 
this case 

1000𝑚𝑚 𝑥 2 = 2000𝑚𝑚

A 3x Barlow lens multiplies by 3x. 
Your telescope is supplied with a 2x Barlow 
lens. When used with the Plössl 25mm 
eyepiece you get 2x the power obtained 
before 

40 𝑝𝑜𝑤𝑒𝑟 𝑋 2𝑥 𝐵𝑎𝑟𝑙𝑜𝑤 = 80 𝑝𝑜𝑤𝑒𝑟

 

 

7.3. Erecting lens (not included)

 

The erecting lens gets you an upright image 
view with the telescope. It also adds some 
power like the barlow lens. The Erecting Lens 
provides an extra 1.5x power. 

7.4. Diagonal Mirror  

This diverts the light coming from the 
telescope to an angle of 45 or 90 degrees. It is 
useful because it provides a more confortable 
position when observing. 

Here are some examples on how to use the 
accessories. 

 

 

Some possible accessory combinations 

 

Terrestrial 

View 

Moon 

Deep Sky 

Jupiter and 

Saturn 

Barlow Lens 2x 

 

 

 

Yes 

Plössl 25mm Eyepiece 

 

 

Yes 

Yes 

Plössl 6.3mm Eyepiece 

 

Yes 

 

 

Power 

Does not apply 

153x 

40x 

80x 

 

Questions? Visit our website 

www.astroshop.eu

 and drop us a line* nimax Gmbh Otto-Lilienthal-Str. 9 D-86899 Landsberg am Lech

 

 

 

Summary of Contents for 90/1000 EQ-2

Page 1: ...of the contents of this document in any form is expressly prohibited other than for individual use only All text images and labels are property of Nimax Gmbh Instruction Manual Omegon AC 90 1000 EQ 2...

Page 2: ...orks The telescope should point to the object being observed The front lens inside the dew shield 1 figure 1 gathers the object s light and directs it to the eyepiece on the focuser side 6 figure 1 Ro...

Page 3: ...an for individual use only All text images and labels are property of Nimax Gmbh Figure 2 Tripod assembly Figure 3 Tray placement Figure 4 Adjust tripod s extension Figure 5 Place the equatorial mount...

Page 4: ...used sharp image easily For night use we suggest starting with an easy object The Moon is a big object easy to point at and train telescope pointing We suggest to use the Moon as a first target before...

Page 5: ...igure1 lights figure 4 and figure 5 A small red point is projected on the optical window 3 figure 1 This red point when aligned with the telescope allows precise pointing to objects To precise align t...

Page 6: ...xt images and labels are property of Nimax Gmbh Figure 15 Red dot lights when ON Figure 16 A red dot is projected on the optical window Figure 17 Turn azimuth adjustment knob to align finder Figure 18...

Page 7: ...possible so we have the widest field of view STEP 1 Figure 22 Looking through the finderscope it should be powered ON we see the same building but in this case the red dot and chimney are not centered...

Page 8: ...the battery Turn the potentiometer on and check if the red dot is now brighter When not in use the finderscope should always be powered OFF to prolong battery s life 6 How to use the equatorial mount...

Page 9: ...tracking Star s positions rotate slowly but surely in the night sky This is caused by the Earth s rotation Every 24 hours the Earth make a complete turn So does the night sky This means that when obs...

Page 10: ...djustment so that the inclination of the mount is the same as the latitude of observers For an observer in Munich the latitude is 48 degrees The inclination angle should be approximately 48 degrees Ma...

Page 11: ...the supplied eyepieces Telescope s focal length is 1000mm Pl ssl 25 eyepiece s focal length is 25mm 1000 25 40 This means that the Pl ssl 25mm eyepiece provides a 40x power magnification This seems lo...

Page 12: ...rve it when the Moon is not full Try the crescent Moon and look for features along the terminator between illuminated and dark surfaces 8 2 Jupiter is the biggest planet of our solar system It is also...

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