Adaptive Optics — MCQs August 20, 2025 by u930973931_answers Score: 0 Attempted: 0/50 Subscribe 1. What is the main purpose of adaptive optics in astronomy? (A) To increase telescope magnification (B) To correct atmospheric distortion in real time (C) To reduce chromatic aberration in lenses (D) To block light pollution 2. Atmospheric turbulence causes what effect in ground-based telescopes? (A) Redshift (B) Blurred and twinkling images (C) Stronger magnification (D) Longer wavelengths 3. Adaptive optics uses: (A) Movable mirrors that adjust rapidly (B) Fixed mirrors with coatings (C) Thick lenses (D) Space-based telescopes only 4. The distorted wavefront of light is corrected by: (A) Secondary eyepiece (B) Deformable mirror (C) Diffraction grating (D) Polarimeter 5. What type of sensor is used to measure atmospheric distortions? (A) Spectrograph (B) Wavefront sensor (C) Photometer (D) CCD camera 6. Adaptive optics systems typically use what to provide a reference point in the sky? (A) Natural guide stars (B) Telescope mounts (C) Black holes (D) Supernovae 7. When no bright natural star is available, adaptive optics use: (A) Artificial guide stars created by lasers (B) Satellite reflections (C) Radio signals (D) Planetary moons 8. Laser guide stars are produced by exciting atoms in which layer of the atmosphere? (A) Troposphere (B) Stratosphere (C) Mesosphere (D) Ionosphere 9. Sodium atoms in the atmosphere are excited with lasers to create: (A) Artificial stars for wavefront sensing (B) Stronger reflections (C) Radio signals (D) Infrared radiation 10. Adaptive optics primarily improves a telescope’s: (A) Light-gathering power (B) Angular resolution (C) Focal length (D) Aperture size 11. The first astronomical adaptive optics systems were developed around: (A) 1940s (B) 1970s (C) 1990s (D) 2000s 12. Which country’s military research originally advanced adaptive optics? (A) USA (B) Germany (C) Japan (D) Russia 13. The main limitation adaptive optics solves for ground-based telescopes is: (A) Telescope weight (B) Atmospheric seeing (C) Mirror polishing (D) Star distance 14. Adaptive optics can make ground-based telescopes rival: (A) Radio observatories (B) Space telescopes like Hubble (C) Infrared satellites only (D) Amateur telescopes 15. In astronomy, “seeing” refers to: (A) Telescope magnification (B) Blurring from atmospheric turbulence (C) Field of view (D) Brightness of stars 16. The speed of deformable mirror adjustments is usually: (A) Once per second (B) Hundreds to thousands of times per second (C) Every hour (D) Once a night 17. Multi-conjugate adaptive optics use: (A) A single wavefront sensor (B) Several deformable mirrors at different altitudes (C) Larger telescope mounts (D) Gravitational lenses 18. Extreme adaptive optics (ExAO) are designed mainly for: (A) Detecting galaxies (B) Direct imaging of exoplanets (C) Measuring distances (D) Observing black holes only 19. Which major telescope is known for pioneering adaptive optics in astronomy? (A) Hale Telescope (B) Keck Observatory (C) Hubble Space Telescope (D) Greenwich Telescope 20. Adaptive optics is less useful for which type of telescope? (A) Ground-based optical (B) Ground-based infrared (C) Space telescopes (D) Large reflectors 21. Wavefront sensors compare incoming starlight to: (A) Laser beams (B) Reference wavefronts (C) Telescope aperture size (D) Mirror curvature 22. Which type of wavefront sensor is most widely used in adaptive optics? (A) Hartmann sensor (B) Shack-Hartmann sensor (C) Michelson sensor (D) CCD sensor 23. The main challenge for adaptive optics in visible light is: (A) Faster correction speeds needed (B) Too many mirrors (C) No available detectors (D) Weak diffraction 24. Adaptive optics corrections are performed in: (A) Real time (B) After image processing (C) Telescope construction (D) Space only 25. Which technology is sometimes combined with adaptive optics for sharper images? (A) Photometry (B) Interferometry (C) Spectroscopy (D) Polarimetry 26. Ground-layer adaptive optics (GLAO) corrects for: (A) Upper atmosphere distortions only (B) Turbulence close to Earth’s surface (C) Cosmic rays (D) Star brightness changes 27. The European Extremely Large Telescope (E-ELT) will rely heavily on: (A) Large refracting lenses (B) Adaptive optics (C) Space-based optics (D) Radio antennas 28. Adaptive optics benefits infrared astronomy because: (A) Infrared light is unaffected by turbulence (B) Longer wavelengths need less correction (C) It increases telescope size (D) It reduces mirror cost 29. Which space agency has invested heavily in adaptive optics for ground telescopes? (A) NASA (B) ESA (C) JAXA (D) ISRO 30. The Gemini Planet Imager uses adaptive optics for: (A) Radio galaxy surveys (B) Direct imaging of exoplanets (C) Stellar distance measurements (D) Solar observations 31. Adaptive optics also finds applications in: (A) Medicine (ophthalmology) (B) Agriculture (C) Mining (D) Architecture 32. What limits the field of view in adaptive optics systems? (A) Laser brightness (B) Anisoplanatism (correction valid only in a small area) (C) Telescope mount (D) CCD resolution 33. Pyramid wavefront sensors are an alternative to: (A) Deformable mirrors (B) Shack-Hartmann sensors (C) CCD detectors (D) Spectrographs 34. The main disadvantage of laser guide stars is: (A) They cannot work at night (B) They do not measure tip-tilt motion accurately (C) They require space telescopes (D) They damage mirrors 35. Adaptive optics improves telescope resolution close to the: (A) Rayleigh limit (diffraction limit) (B) Magnification limit (C) Brightness limit (D) Extinction limit 36. Which adaptive optics technique combines multiple laser guide stars? (A) Ground-layer AO (B) Multi-conjugate AO (C) Lucky imaging (D) Speckle interferometry 37. “Lucky imaging” is an alternative method to AO that: (A) Selects sharpest short-exposure images (B) Uses lasers for correction (C) Avoids CCDs (D) Relies on radio waves 38. The main power requirement of adaptive optics systems comes from: (A) Cooling CCDs (B) Running fast actuators and sensors (C) Telescope tracking (D) Eyepiece magnification 39. Deformable mirrors in AO are controlled by: (A) Hand adjustments (B) Computer-driven actuators (C) Telescope mounts (D) Laser beams directly 40. The AO system at Keck Observatory improved imaging of: (A) Exoplanets and the Galactic center (B) Comets only (C) Earth’s atmosphere (D) Radio galaxies 41. What is the typical size of deformable mirrors in adaptive optics? (A) A few centimeters (B) A few meters (C) Several kilometers (D) Microscopic only 42. How does adaptive optics affect spectroscopy? (A) Provides sharper input light for better spectral resolution (B) Removes spectral lines (C) Reduces telescope size (D) Eliminates need for gratings 43. Which large telescope will use adaptive optics to directly observe Earth-like planets? (A) Thirty Meter Telescope (TMT) (B) James Webb Space Telescope (C) Hubble Space Telescope (D) Arecibo Observatory 44. Multi-object adaptive optics (MOAO) corrects: (A) One star only (B) Several objects in different directions simultaneously (C) Only galaxies (D) Only planets 45. Adaptive optics requires very fast computing because: (A) Corrections must keep pace with changing turbulence (B) Stars rotate quickly (C) CCDs work slowly (D) Telescopes move too fast 46. In medical applications, AO is used to: (A) Improve MRI scans (B) Correct for distortions in retinal imaging (C) Enhance X-ray imaging (D) Reduce ultrasound noise 47. The first successful AO system for astronomy was installed on a: (A) Radio telescope (B) Ground-based optical telescope (C) Space telescope (D) Satellite array 48. Adaptive optics cannot correct distortions caused by: (A) Earth’s atmosphere (B) Telescope vibrations (C) Galactic dust absorption (D) Optical misalignment 49. Extremely Large Telescopes (ELTs) will depend on AO because: (A) Larger mirrors are more affected by turbulence (B) AO reduces telescope size (C) AO eliminates need for mounts (D) AO makes telescopes cheaper 50. The ultimate goal of adaptive optics in astronomy is to achieve: (A) Higher magnification (B) Diffraction-limited resolution from the ground (C) Infinite brightness (D) Unlimited telescope size