In What Wavelength Range Was Interferometry First Routinely Used
Question: What is the purpose of adaptive optics?
Answer: to eliminate the distorting effects of atmospheric turbulence for telescopes on the ground
Question: True or false: A radio telescope and an optical telescope of the same size have the same angular resolution.
Answer: False
Question: What does better angular resolution mean?
Answer: you can see smaller details
Question: True or false: X rays from astronomical objects can only be detected from telescopes in space.
Answer: True
Question: What is interferometry?
Answer: It is the analysis of interference patterns of light from different telescopes to enable combining the light into one image.
Question: Telescopes operation at this wavelength must be cooled to observe faint astronomical objects
Answer: extreme infrared
Question: The largest effective telescope, created by radio interferometry, is the size of
Answer: the earth.
Question: What do we mean by the diffraction limit of a telescope?
Answer: It is the best angular resolution the telescope could achieve with perfect optical quality and in the absence of atmospheric distortion.
Question: Improving the spectral resolution of a spectrograph comes at the expense of
Answer: increased exposure time
Question: Which of the following is not a good reason to place observatories on remote mountain tops?
Answer: to be able to observe at radio wavelengths