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

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SUMMARY

The resolving power of Green Bank's 300-foot telescope, prior to its collapse in 1989, can be calculated using the formula resolving power = (wavelength in microns) / (diameter in meters). The telescope's diameter is approximately 91.44 meters. The relevant wavelength for H I, which refers to the neutral hydrogen line, can be easily found through online resources. The diffraction limit, or Raleigh limit, is defined as 1.22 times the wavelength divided by the diameter, providing a clear method for determining the telescope's resolving power.

PREREQUISITES
  • Understanding of the formula for resolving power in astronomy
  • Familiarity with the concept of diffraction limits
  • Knowledge of the neutral hydrogen line (H I) and its significance
  • Basic skills in unit conversion (meters to microns)
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  • Research the wavelength of the neutral hydrogen line for precise calculations
  • Explore the concept of diffraction limits in radio astronomy
  • Learn about the historical significance of Green Bank's 300-foot telescope
  • Investigate other telescopes and their resolving power comparisons
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Astronomers, astrophysics students, and anyone interested in radio telescope technology and its applications in mapping celestial objects.

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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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