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How it works

The PiKon is a telescope that uses 3D printed parts and a Raspberry Pi with camera to capture images.

Newtonian Reflecting Telescope

 

A conventional (Newtonian) reflecting telescope uses a concave mirror (objective) to form an image which is then examined with an eye piece. So that you don’t get your head in the way while viewing, there is a 45 degree mirror placed in the telescope tube and the eye piece is mounted on the side with a focusing rack.

Visualtelescope3

In the PiKon design, the Raspberry Pi camera is placed in the tube with no 45 degree mirror. The size of the camera printed circuit board (PCB) is 24mm x 24mm, about the same size as the 45 degree mirror.

The lens of the Raspberry Pi camera is removed, exposing the camera sensor. The objective mirror is 4.5 inches diameter (113mm) and a focal length of about 600mm.

The telescope is operated using a Raspberry Pi computer, keyboard and monitor. Full details are in our assembly instructions.

The PiKon telescope has a magnification factor of about x160.

Slide26

We’ve worked that out based on a standard 35mm film camera. A 50mm lens there gives a x1 magnification. A 100mm lens gives a x2 magnification. The focal length of the objective mirror in the PiKon is 800mm. So, for 35mm film that would give a magnification of x16. But the Raspberry Pi Camera sensor is just one tenth the size of a 35mm film frame. So effectively the magnification is increased by a factor 10 to x160.

Slide27

Another way of thinking about the power of the telescope is the angle of field of view. If we place a 3.6mm wide sensor at the focal point of an 800mm lens, it subtends and angle of view of about a quarter of a degree. The moon subtends an angle of about half a degree at your eye ball, so we’d expect the PiKon to have a field of view that could capture about half of the moon. And that’s just what we get:

moon2-500x375

What is the limit of magnification?

The ultimate magnification of the PiKon is limited by something called Airy Disks. These are circular halos of light which surround a point image in the telescope. They are caused by defraction effects which depend on the size of the objective mirror and limit the ultimate useful magnification.

http://en.wikipedia.org/wiki/Airy_disk

The rule of thumb is that maximum useful magnification is 60 times the size of the mirror (in inches) or 2.2 times (in mm). The PiKon prototype has a mirror diameter of 4.5 inches or 113mm, which means its maximum useful magnification is x270.

4 Comments

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  1. Christian #
    June 15, 2019

    Hi,

    this is a very nice project! I’m currently building one myselfe.
    Could you please explain why you have to remove the lense from the camera?

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    • June 15, 2019

      First you need to hold the camera (small plastic box with lens) with pointed nose pliers. Then with a second pair of pointed nose pliers, grip the circular lens mount and twist anti clockwise. It is fitted with a screw thread which has been fixed by Lock Tight.
      If all else fails, score a ‘v’ across the lens fitting and twist with a sharp screw driver.

      Like

      • Christian Rajek #
        June 16, 2019

        Thanks for your comment. Actually, the camera comes with a tool to remove the lens or change the focus.
        But this is not the aswer to my question. I know how to remove the lense from the camera. I would like to know why it has to be removed. What would be the difference if the lens would be left in place, what are the benefits of removing the lens.

        Like

      • June 16, 2019

        If you can get the lens to rotate in the body of the camera, then remove it by turning it anti-clockwise until it comes out. The reason that you need to remove the lens is because the mirror forms the image on the camera sensor instead of the camera lens. If you leave the camera lens in, it will not focus.

        Like

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