What Was the Resolving Power of Green Bank's 300-ft Telescope?

AI Thread Summary
The resolving power of Green Bank's 300-foot telescope can be calculated using the formula resolving power = (wavelength in microns) / (diameter in meters), with the diameter approximately 91.44 meters. The discussion clarifies that H I refers to the neutral hydrogen line, which is crucial for determining the appropriate wavelength. The Raleigh limit, which is the diffraction limit in radians, is also noted as 1.22 times the wavelength divided by the diameter. Users can easily find the wavelength of the neutral hydrogen line through a quick online search. Understanding these concepts is essential for accurately assessing the telescope's capabilities.
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Question: Before it collapsed in 1989, Green Bank's 300-foot diameter telescope mapped the sky in H I. What was its resolving power?

I believe the formula you would use is resolving power = (wavelength in microns) / (diameter in meters)

So the diameter in meters would be about 91.44 m, but how do you know what the wavelength is? I guess I'm not sure what H I means...

Thanks for any help!
 
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Assuming the Raleigh limit the diffraction limit (in radians) is something like 1.22 wavelength/diameter (assuming wavelength and diamter are in the same units)

H1 is the neutral hydrogen line, astronomers have funny nomenclature, H1 is un-ionized hydrogen, H2 is singly ionized (H+)

You can look up the wavelength and frequency easily ( google "neutral hydrogen line" )
 
Dividing the dish diameter by wavelength gives you an idea of resolving power at any given wavelength.
 
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