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Sky Astro - CCD

Sky Astro - CCD

A site dedicated to astrophotography

  • ABOUT
  • IMAGES
    • Sites without light pollution
    • Site of extreme light pollution
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  • OBSERVATORY
  • EQUIPMENT
    • Personal equipment
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  • PREPARING FOR A SESSION
    • Astronomical calculations
    • Telescope collimation
    • Setting up the telescope
    • Find the polar axis of rotation
    • Make a PEC
    • Autoguiding
    • Focusing the camera
    • Suggested exposure times
    • Maximum exposure time in light pollution
    • Using narrow band filters ...
  • IMAGE ACQUISITION
    • The different image formats
    • Acquisition of images used for preprocessing
    • Acquisition of deep sky images
  • IMAGE PROCESSING
    • The different compositing methods
    • Image preprocessing
    • Processing deep sky images
    • Planetary image processing
    • LRVB technique
  • ADVANCED TREATMENTS
    • Create a synthetic green layer
    • Create a Synthetic Luminance Image
    • Correct the red-salmon color
    • Color balance using curves
    • Remove dust, colored pixels and other imperfections
  • FILES
  • RÉFÉRENCES
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CALCULATION OF THE FIELD OF VIEW OF AN EYEPIECE OR AN ASTRONOMIC CAMERA

Field of view of an eyepiece

Formula :

C '= Co / (F / f) * 60

C '= Field of view in minutes of arc
Co = Apparent field of the eyepiece in degrees
F = Focal length of telescope or telescope
f = focal length of the eyepiece

Here is an example :
Use of a 40 mm eyepiece offering an apparent field of 43o with a telescope with a focal length of 2 mm:

43 / (2000/40) * 60 = 51,6 ′ of arc

The eyepiece with this telescope will provide a field of view of 51,6 ′ of arc

CCD camera field of view

Formula :

S = 205 x P / FL

S = Field of view covered by one pixel in arc second
P = Physical dimension of a pixel in microns 
FL = Telescope focal length

It remains to multiply by the number of pixels in width and height. To convert to minutes of arc divide by 60.

Richard Beauregard
Sky Astro - CCD

Revised 2022/06/04

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