Gravitational Wave Astronomy — MCQs August 20, 2025 by u930973931_answers 50 Score: 0 Attempted: 0/50 Subscribe 1. Gravitational waves were first directly detected in which year? (A) 2014 (B) 2015 (C) 2016 (D) 2017 2. The first direct detection of gravitational waves was announced by: (A) LISA (B) LIGO (C) Virgo (D) Einstein Telescope 3. Who first predicted the existence of gravitational waves? (A) Isaac Newton (B) Albert Einstein (C) Stephen Hawking (D) Galileo Galilei 4. Gravitational waves are ripples in: (A) Time only (B) Space only (C) Space-time fabric (D) Matter 5. The Nobel Prize in Physics 2017 for gravitational waves was awarded to: (A) Kip Thorne, Rainer Weiss, Barry Barish (B) Einstein, Hawking, Feynman (C) Penrose, Genzel, Ghez (D) Chandrasekhar, Fowler, Bethe 6. The main sources of detectable gravitational waves are: (A) Pulsars (B) Binary black holes and neutron star mergers (C) Solar flares (D) Supernova neutrinos 7. LIGO consists of how many detectors? (A) One (B) Two (C) Three (D) Four 8. The two LIGO detectors are located in: (A) Washington and Louisiana (B) California and Texas (C) New York and Florida (D) Arizona and Nevada 9. Virgo, a gravitational wave detector, is located in: (A) Germany (B) France (C) Italy (D) Switzerland 10. The LISA mission is a planned gravitational wave detector in: (A) Underground labs (B) Space (C) Antarctica (D) Ocean floor 11. The interferometer arms of LIGO are how long? (A) 1 km (B) 2 km (C) 4 km (D) 10 km 12. Gravitational waves travel at the speed of: (A) Sound (B) Light (C) Slower than light (D) Faster than light 13. Which astrophysical event produced the first observed gravitational wave GW150914? (A) Supernova explosion (B) Binary black hole merger (C) Neutron star collision (D) Pulsar rotation 14. The event GW170817 was associated with: (A) Black hole merger (B) Neutron star merger (C) Supernova (D) Pulsar emission 15. Gravitational wave astronomy opened a new era called: (A) Neutrino astronomy (B) Multi-messenger astronomy (C) Particle astrophysics (D) Radio astronomy 16. The sensitivity of gravitational wave detectors depends on: (A) Arm length and laser power (B) Temperature only (C) Earth’s rotation (D) Cosmic rays 17. Which type of black holes are most commonly detected by LIGO? (A) Supermassive black holes (B) Stellar-mass black holes (C) Primordial black holes (D) Intermediate black holes 18. What happens to space-time when gravitational waves pass through it? (A) Expands and contracts (B) Heats up (C) Breaks apart (D) Stays unchanged 19. Which other signal was detected alongside GW170817? (A) Gamma rays (B) Neutrinos (C) Cosmic rays (D) X-rays only 20. What type of interferometer is used in LIGO? (A) Mach-Zehnder (B) Fabry–Pérot Michelson (C) Sagnac (D) Twyman-Green 21. The strain measured by LIGO is of order: (A) 10^-3 (B) 10^-9 (C) 10^-18 (D) 10^-25 22. The Einstein Telescope is a proposed: (A) Radio telescope (B) Underground gravitational wave detector (C) Neutrino detector (D) X-ray observatory 23. The KAGRA detector is located in: (A) USA (B) Japan (C) India (D) Germany 24. Which Indian project will join the global network of gravitational wave detectors? (A) LIGO-India (B) INDIGO (C) ASTROSAT (D) SKA 25. Gravitational waves can test which aspect of physics? (A) Quantum chromodynamics (B) General relativity (C) Special relativity (D) Nuclear decay 26. Gravitational waves from inflation in the early universe are called: (A) Primordial gravitational waves (B) Relic neutrinos (C) Dark energy waves (D) Solar gravitational waves 27. Which black hole merger produced the heaviest final black hole observed so far? (A) GW150914 (B) GW190521 (C) GW170817 (D) GW190412 28. The polarization of gravitational waves can be used to test: (A) Einstein’s equations (B) Alternative theories of gravity (C) Dark matter models (D) Neutrino physics 29. The frequency band of LIGO sensitivity is approximately: (A) 0.01 – 1 Hz (B) 10 – 10,000 Hz (C) 100 kHz – 1 MHz (D) 1 MHz – 1 GHz 30. Which cosmic objects emit continuous gravitational waves? (A) Pulsars with asymmetry (B) Supernovae (C) Neutron star mergers (D) Black hole binaries 31. Which detection method complements gravitational wave astronomy? (A) Electromagnetic observations (B) Neutrino detections (C) Cosmic ray studies (D) All of the above 32. The main noise source in LIGO at low frequencies is: (A) Seismic noise (B) Thermal noise (C) Shot noise (D) Cosmic rays 33. The space-based LISA detector will primarily detect: (A) Stellar-mass black holes (B) Supermassive black hole mergers (C) Neutron star mergers (D) Pulsars 34. Which kind of astrophysical event could produce both gravitational waves and neutrinos? (A) Neutron star mergers (B) Pulsars (C) Cosmic ray showers (D) Gamma-ray bursts 35. Which effect limits ground-based detectors at high frequencies? (A) Thermal noise (B) Seismic vibrations (C) Quantum shot noise (D) Earth’s magnetic field 36. The global network of gravitational wave detectors improves: (A) Sensitivity only (B) Source localization (C) Laser stability (D) Detector arm length 37. What are tidal deformabilities measured in GW170817 used for? (A) Dark energy models (B) Nuclear matter equation of state (C) Dark matter detection (D) Photon mass limits 38. Which observatory detected the electromagnetic counterpart of GW170817? (A) Hubble Space Telescope (B) Fermi Gamma-ray Space Telescope (C) Swift Observatory (D) All of the above 39. The gravitational wave signal from a binary inspiral is called: (A) Chirp (B) Echo (C) Pulse (D) Ring 40. Which type of waves are gravitational waves? (A) Scalar (B) Vector (C) Tensor (D) Longitudinal 41. What happens to black holes after merging in terms of gravitational wave signal? (A) Inspiral (B) Merger (C) Ringdown (D) All of the above 42. Which constant is crucial in calculating gravitational radiation? (A) Planck constant (B) Speed of light (C) Gravitational constant (D) Both B and C 43. Which wave property carries energy away from systems? (A) Amplitude (B) Frequency (C) Gravitational wave strain (D) All of the above 44. Which black hole merger detection challenged known mass ranges? (A) GW150914 (B) GW190521 (C) GW170817 (D) GW190425 45. The time delay between gravitational waves and light from GW170817 was about: (A) Seconds (B) Minutes (C) Hours (D) Days 46. Gravitational waves confirm that black holes are: (A) Hypothetical objects (B) Real astrophysical objects (C) White dwarfs (D) Neutron stars 47. Which detector is proposed to be triangular in design with 10 km arms? (A) Virgo (B) Einstein Telescope (C) KAGRA (D) LISA 48. What is the unit of gravitational wave strain? (A) Newton (B) Joule (C) Dimensionless (D) Meter per second 49. Which type of astronomy benefited most from GW170817? (A) Gamma-ray astronomy (B) Optical astronomy (C) Radio astronomy (D) All of the above 50. Gravitational wave astronomy is expected to reveal: (A) Hidden black holes (B) Early universe physics (C) Neutron star interiors (D) All of the above