How do you calculate a telescope’s image circle and field of view at infinity focus?
Asked 12/9/2012
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2 answers
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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
3
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
0
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.
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