Skip to content

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.

Advertisements
No comments yet

Leave a Reply

Fill in your details below or click an icon to log in:

WordPress.com Logo

You are commenting using your WordPress.com account. Log Out / Change )

Twitter picture

You are commenting using your Twitter account. Log Out / Change )

Facebook photo

You are commenting using your Facebook account. Log Out / Change )

Google+ photo

You are commenting using your Google+ account. Log Out / Change )

Connecting to %s

%d bloggers like this: