Radio Astronomy — MCQs August 20, 2025 by u930973931_answers 50 Score: 0 Attempted: 0/50 Subscribe 1. Radio astronomy studies which type of electromagnetic waves? (A) Visible light (B) Radio waves (C) Infrared waves (D) X-rays 2. Who is regarded as the father of radio astronomy? (A) Isaac Newton (B) Karl Jansky (C) Galileo Galilei (D) Edwin Hubble 3. The first detection of cosmic radio waves was made in: (A) 1928 (B) 1931 (C) 1938 (D) 1945 4. The largest single-dish radio telescope is located in: (A) USA (B) China (C) Russia (D) Chile 5. The name of China’s giant radio telescope is: (A) FAST (B) Arecibo (C) VLA (D) GMRT 6. The Arecibo telescope was located in: (A) Puerto Rico (B) Mexico (C) Brazil (D) Spain 7. Radio telescopes are usually built in: (A) Cities (B) Deserts or remote areas (C) Mountain peaks (D) Ocean shores 8. The Very Large Array (VLA) is located in: (A) Texas (B) New Mexico (C) Arizona (D) California 9. The world’s largest radio telescope array project is called: (A) ALMA (B) SKA (C) FAST (D) VLA 10. SKA stands for: (A) Solar Kinetic Array (B) Square Kilometre Array (C) Sky Knowledge Aperture (D) Space Kinematic Array 11. Which type of radiation passes easily through clouds and atmosphere, making ground-based observations possible? (A) X-rays (B) Gamma rays (C) Radio waves (D) Ultraviolet rays 12. Radio waves from space are usually detected with: (A) Lenses (B) Metal dishes (C) Mirrors (D) Prisms 13. What was the first astronomical object detected in radio waves? (A) Sun (B) Moon (C) Jupiter (D) Milky Way Galaxy 14. The discovery of pulsars was made using: (A) Optical telescope (B) Radio telescope (C) Infrared telescope (D) X-ray telescope 15. Pulsars were first discovered by: (A) Jocelyn Bell Burnell (B) Edwin Hubble (C) Karl Jansky (D) Subrahmanyan Chandrasekhar 16. Radio interferometry improves: (A) Sensitivity (B) Magnification (C) Resolution (D) Brightness 17. The process of combining signals from multiple radio telescopes is called: (A) Dispersion (B) Interferometry (C) Diffraction (D) Reflection 18. The Atacama Large Millimeter Array (ALMA) is located in: (A) Australia (B) Chile (C) South Africa (D) India 19. Which planet in our Solar System is a strong source of radio waves? (A) Mars (B) Saturn (C) Jupiter (D) Venus 20. The cosmic microwave background radiation was discovered in: (A) 1955 (B) 1965 (C) 1972 (D) 1980 21. Who discovered the cosmic microwave background radiation? (A) Jansky and Reber (B) Penzias and Wilson (C) Hubble and Humason (D) Bell and Hewish 22. Which part of the day is best for radio astronomy? (A) Morning (B) Noon (C) Day and night equally (D) Only at night 23. Why do radio telescopes have large dishes? (A) To magnify objects (B) To collect faint radio signals (C) To reduce distortion (D) To block sunlight 24. Which of the following can be studied with radio astronomy? (A) Pulsars (B) Quasars (C) Galaxies (D) All of the above 25. The first radio telescope built by Grote Reber was in: (A) 1937 (B) 1945 (C) 1952 (D) 1960 26. A major challenge in radio astronomy is: (A) Gravity (B) Light pollution (C) Radio frequency interference (D) Telescope weight 27. The unit of frequency used in radio astronomy is: (A) Hertz (B) Decibel (C) Magnitude (D) Arcsecond 28. Quasars were first identified through: (A) Optical astronomy (B) Radio astronomy (C) Infrared astronomy (D) Ultraviolet astronomy 29. The Parkes radio telescope is located in: (A) South Africa (B) Australia (C) Canada (D) Brazil 30. Radio waves are: (A) High frequency, short wavelength (B) Low frequency, long wavelength (C) Medium frequency, medium wavelength (D) Variable frequency 31. Which type of celestial object was first studied in detail using radio astronomy? (A) Comets (B) Stars (C) The Sun (D) Black holes 32. VLBI stands for: (A) Very Large Binary Imaging (B) Very Long Baseline Interferometry (C) Variable Light Beam Interference (D) Visible Light Band Imaging 33. The first pulsar discovered was nicknamed: (A) Little Star (B) LGM-1 (Little Green Men) (C) Cosmic Beam (D) Radio Star 34. Radio galaxies emit most of their energy in: (A) Visible light (B) Radio waves (C) Infrared rays (D) X-rays 35. Which telescope collapsed in 2020? (A) FAST (B) Arecibo (C) VLA (D) ALMA 36. The wavelength range of radio astronomy is approximately: (A) 1 mm to 10 km (B) 1 nm to 100 µm (C) 100 km to 1000 km (D) 0.1 µm to 700 nm 37. The Indian GMRT stands for: (A) Giant Microwave Research Telescope (B) Giant Metrewave Radio Telescope (C) Global Magnetic Radio Telescope (D) Galactic Microwave Reflecting Telescope 38. Radio telescopes can operate: (A) Only in space (B) Only at night (C) Day and night from Earth (D) Only underwater 39. Which technique allows global networks of radio telescopes to work together? (A) Diffraction (B) VLBI (C) Reflection (D) Refraction 40. The strongest natural radio source in the sky is: (A) The Sun (B) The Moon (C) Jupiter (D) The Milky Way center 41. Radio waves travel at the speed of: (A) Sound (B) Light (C) Electrons (D) Gravity 42. Why is space-based radio astronomy less common than optical astronomy? (A) Radio waves penetrate Earth’s atmosphere (B) It is too costly (C) Radio waves are blocked by atmosphere (D) Satellites cannot detect radio waves 43. Which Nobel Prize was awarded for the discovery of pulsars? (A) Physics (B) Chemistry (C) Astronomy (D) Medicine 44. Radio quasars appear as: (A) Very faint optical objects but strong radio sources (B) Bright visible stars (C) Moving asteroids (D) X-ray bursts 45. Which band of frequencies is often protected for radio astronomy? (A) X-band (B) L-band (C) Hydrogen line (21 cm) (D) K-band 46. The 21 cm radio line corresponds to: (A) Hydrogen atoms (B) Helium atoms (C) Oxygen molecules (D) Carbon atoms 47. Radio astronomy played a key role in proving: (A) Heliocentric theory (B) Expansion of the Universe (C) Gravitational lensing (D) Space travel 48. Which telescope is part of the Event Horizon Telescope (EHT) project? (A) ALMA (B) FAST (C) Parkes (D) VLA 49. Radio astronomy can detect signals from: (A) Stars (B) Galaxies (C) Planets (D) All of the above 50. The main challenge in building the Square Kilometre Array is: (A) Cost and international collaboration (B) Telescope weight (C) Lack of materials (D) Small dish size