How do you calculate a telescope’s image circle and field of view at infinity focus?

Asked 12/9/2012

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I’m trying to understand the geometry behind image circle / sensor coverage for prime-focus astrophotography, rather than just using an online calculator.

My setup is a Celestron NexStar 130 SLT (130 mm aperture, 650 mm focal length) with a Nikon D80 attached via T-ring/T-adapter. I’ve also used a 2× Barlow to reach focus. How can I calculate, at near-infinity focus, the projected image size or field of view on the sensor from the telescope’s focal length and sensor dimensions?

I’d like the underlying formula so I can compare how different telescopes would perform on the same camera sensor.

Originally by Photography Stack Exchange contributor. Source · Licensed CC BY-SA 4.0

Photography Stack Exchange contributor

13y ago

2 Answers

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I am not sure about the answer to Would the image circle size decrease if I was able to ditch the Barlow lens?

But if you look at the JavaScript of that page you will see

var sensorw = "Sensor Width"
var sensorh = "Sensor Height"
var maxres  = "Max Res"
var focleng = "Focal Length"

var thisF = sensorw * 3438/focleng;
var thisF2 = sensorh * 3438/focleng;
var thisF3 = sensorw * 3438/focleng * 60/maxres;
var thisF4 = focleng/Math.sqrt(sensorw * sensorw + sensorh * sensorh);

Values:

  • thisF = Arc Min of Sky- Width:
  • thisF2 = Arc Min of Sky- Height:
  • thisF3 = Arc Seconds/Pixel:
  • thisF4 = Magnification (X):

This is how that page calculates it

Originally by user5052. Source · Licensed CC BY-SA 4.0

user5052

13y ago

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AI Answer

Generated from our catalog & community — verify before relying on it.

At infinity focus, you can treat the optical system geometrically: the image forms at the focal plane, and the focal length sets the mapping between sensor size and angular field.

For a sensor dimension S and focal length F:

tan(theta) = S / F

So:

theta = arctan(S / F)

For practical camera/telescope field of view, the small-angle approximation is often used:

field of view ≈ sensor size / focal length

with units converted to radians, or in arcminutes using:

FOV (arcmin) ≈ sensor size × 3438 / focal length

Apply that separately to sensor width, height, or diagonal.

This tells you how much sky fits on the sensor. A larger focal length gives a smaller field of view.

Important: this is not quite the same as the true illuminated image circle of a telescope, which also depends on the optical design. But for calculating what angular field your sensor records at infinity focus, focal length and sensor size are the key inputs.

Also, if a Barlow is used, the effective focal length increases by its actual magnification, which can be higher than the nominal 2× depending on spacing. That would make the field of view smaller.

UniqueBot

AI

13y ago

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