Spectroscopy — MCQs August 20, 2025 by u930973931_answers 50 Score: 0 Attempted: 0/50 Subscribe 1. What is spectroscopy primarily used for in astronomy? (A) Measuring distances (B) Analyzing light to determine composition (C) Observing planets directly (D) Measuring gravity 2. Which law explains how light spreads into a spectrum through a prism? (A) Snell’s law (B) Newton’s law (C) Kirchhoff’s law (D) Kepler’s law 3. Who first demonstrated that white light could be split into colors using a prism? (A) Galileo Galilei (B) Isaac Newton (C) Joseph Fraunhofer (D) Robert Hooke 4. The dark lines in the solar spectrum are called: (A) Emission lines (B) Fraunhofer lines (C) Spectral bands (D) Absorption rays 5. Which type of spectrum is produced by hot, dense objects like stars? (A) Absorption spectrum (B) Emission spectrum (C) Continuous spectrum (D) Broken spectrum 6. An emission spectrum is produced when: (A) A hot gas emits light at specific wavelengths (B) A solid object absorbs light (C) Light passes through a prism (D) A gas blocks radiation 7. Absorption spectra are formed when: (A) Hot dense objects emit light (B) Cool gas absorbs certain wavelengths (C) A prism scatters light (D) Stars reflect light 8. Kirchhoff’s first law of spectroscopy states: (A) Hot dense bodies produce continuous spectra (B) Cool gases emit absorption lines (C) Hot gases emit continuous spectra (D) All stars show emission lines 9. Spectral lines are unique because they: (A) Depend only on star size (B) Identify chemical elements (C) Vary randomly (D) Change daily 10. Which element’s spectral lines were first observed in the Sun before being found on Earth? (A) Helium (B) Hydrogen (C) Oxygen (D) Lithium 11. The study of Doppler shift in spectra helps astronomers measure: (A) Mass of a star (B) Distance to galaxies (C) Motion toward or away from Earth (D) Temperature of planets 12. A redshift in a galaxy’s spectrum indicates that the galaxy is: (A) Moving toward Earth (B) Stationary (C) Moving away from Earth (D) Rotating 13. A blueshift in a star’s spectrum means: (A) The star is moving away (B) The star is moving closer (C) The star is cooling (D) The star is dimming 14. What type of spectroscope uses a diffraction grating? (A) Newtonian (B) Modern spectroscope (C) Refractor (D) Polarimeter 15. The resolving power of a spectroscope refers to its ability to: (A) Gather light (B) Distinguish close spectral lines (C) Show colors (D) Measure distances 16. Which instrument separates light more efficiently than a prism? (A) Lens (B) Diffraction grating (C) Mirror (D) Eyepiece 17. Hydrogen’s spectral lines in the visible region are called: (A) Fraunhofer lines (B) Balmer series (C) Paschen series (D) Lyman series 18. The Lyman series of hydrogen lies in which region? (A) Visible (B) Infrared (C) Ultraviolet (D) X-ray 19. The Paschen series of hydrogen lies in which region? (A) Infrared (B) Visible (C) Ultraviolet (D) Radio 20. Which law explains the relationship between wavelength, frequency, and speed of light? (A) Planck’s law (B) Wien’s law (C) c = λν (D) Ohm’s law 21. Wien’s displacement law relates a star’s: (A) Radius to luminosity (B) Temperature to peak wavelength (C) Mass to brightness (D) Motion to spectrum 22. According to Planck’s law, hotter objects emit: (A) Longer wavelengths (B) More radiation at shorter wavelengths (C) Only visible light (D) Only infrared radiation 23. The Zeeman effect in spectroscopy refers to: (A) Splitting of spectral lines in a magnetic field (B) Broadening of lines due to motion (C) Redshift of light (D) Cooling of gases 24. Spectral line broadening can be caused by: (A) Temperature and pressure (B) Mounting of telescope (C) Light pollution only (D) Random dust 25. Which element dominates stellar spectra? (A) Oxygen (B) Hydrogen (C) Iron (D) Helium 26. Spectroscopy allows astronomers to determine a star’s: (A) Diameter only (B) Composition, temperature, motion (C) Age only (D) Distance only 27. Which instrument records spectra electronically in modern astronomy? (A) Photographic plates (B) CCD detectors (C) Human eye (D) Film cameras 28. Which effect explains why moving stars change spectral wavelength? (A) Doppler effect (B) Compton effect (C) Photoelectric effect (D) Zeeman effect 29. A binary star system is often detected by observing: (A) Brightness only (B) Periodic shifts in spectral lines (C) Shape of the star (D) Size of planets 30. Spectroscopy can be used to study exoplanets by: (A) Observing their shapes (B) Detecting absorption lines in star light (C) Measuring telescope aperture (D) Using magnification 31. Stellar classification is based on: (A) Size and mass (B) Spectral lines and temperature (C) Distance and motion (D) Shape and density 32. The spectral classes of stars follow which sequence? (A) O, B, A, F, G, K, M (B) A, B, C, D, E, F, G (C) M, G, F, K, O, A, B (D) G, K, F, M, O, B, A 33. Which spectral type corresponds to the Sun? (A) A-type (B) F-type (C) G-type (D) K-type 34. Molecules in space are detected using which type of spectroscopy? (A) Optical spectroscopy (B) Radio spectroscopy (C) X-ray spectroscopy (D) Gamma spectroscopy 35. Infrared spectroscopy is useful for studying: (A) Cold interstellar dust and molecules (B) Hot plasma only (C) Nuclear reactions (D) Radio galaxies 36. X-ray spectroscopy is important for studying: (A) Planetary atmospheres (B) Black holes and neutron stars (C) Cold gas clouds (D) Optical galaxies 37. Gamma-ray spectroscopy helps detect: (A) Radio waves from stars (B) High-energy nuclear processes (C) Planetary surfaces (D) Stellar magnitudes 38. What are absorption bands in planetary spectra mainly caused by? (A) Atomic hydrogen (B) Atmospheric molecules (C) Stellar winds (D) Sunspots 39. Doppler spectroscopy is widely used in astronomy for: (A) Discovering exoplanets (B) Measuring star brightness (C) Estimating distances (D) Analyzing galaxy shapes 40. Spectroscopy shows that quasars are: (A) Close stars (B) Extremely distant objects with redshift (C) Small planets (D) Normal galaxies 41. Spectral energy distribution (SED) shows: (A) Total radiation output vs wavelength (B) Distance vs brightness (C) Temperature vs pressure (D) Mass vs volume 42. Which type of spectroscopy measures polarization of light? (A) Polarimetry (B) Fluorescence spectroscopy (C) Photoemission spectroscopy (D) Raman spectroscopy 43. Raman spectroscopy involves scattering of: (A) Radio waves (B) X-rays (C) Photons by molecules (D) Gamma rays 44. Ultraviolet spectroscopy is important for studying: (A) Cold planets (B) Hot young stars and interstellar gas (C) Black holes (D) Radio galaxies 45. Which type of spectrum do cool stars with molecules show? (A) Continuous only (B) Absorption bands (C) Emission only (D) Radio pulses 46. Stellar radial velocities are measured using: (A) Proper motion (B) Doppler shifts in spectra (C) Star brightness changes (D) Telescope mounts 47. Metallicity of a star is determined through: (A) Brightness (B) Spectral absorption lines (C) Position in sky (D) Motion in orbit 48. Which technique uses multiple telescopes to study spectra at high resolution? (A) Spectral blending (B) Interferometry (C) Reflection (D) Refraction 49. Spectral classification also indicates a star’s: (A) Distance (B) Surface temperature (C) Mass only (D) Radius only 50. The first woman to make major contributions in stellar spectroscopy and classification was: (A) Annie Jump Cannon (B) Marie Curie (C) Jocelyn Bell Burnell (D) Caroline Herschel