Photometry — MCQs August 20, 2025 by u930973931_answers 50 Score: 0 Attempted: 0/50 Subscribe 1. What is photometry in astronomy mainly concerned with? (A) Measuring wavelengths of light (B) Measuring the intensity or brightness of light (C) Splitting light into spectra (D) Measuring star distances 2. The basic unit of luminous intensity in photometry is: (A) Watt (B) Lumen (C) Candela (D) Lux 3. Which unit represents luminous flux? (A) Lux (B) Lumen (C) Candela (D) Joule 4. What does “lux” measure in photometry? (A) Total energy output (B) Illuminance on a surface (C) Spectral distribution (D) Angular size 5. In astronomy, photometry is most often applied to measure: (A) Surface temperature of planets (B) Brightness variations of stars (C) Shape of galaxies (D) Motion of planets 6. The apparent brightness of a star decreases with: (A) Increasing mass (B) Increasing distance (C) Higher temperature (D) Larger size 7. The standard system of magnitudes in photometry was introduced by: (A) Ptolemy (B) Hipparchus (C) Galileo (D) Newton 8. In the magnitude scale, a difference of 5 magnitudes corresponds to a brightness factor of: (A) 50 (B) 100 (C) 10 (D) 500 9. Which modern photometric system uses filters like U, B, V? (A) Johnson photometric system (B) Hipparchus system (C) Sloan survey system (D) Hubble filters 10. The “V” filter in UBV photometry corresponds to: (A) Infrared (B) Visible green-yellow light (C) Ultraviolet (D) X-ray 11. Bolometric magnitude measures: (A) Brightness in visible light only (B) Total radiation across all wavelengths (C) Brightness in X-rays (D) Reflectivity of planets 12. The absolute magnitude of a star is defined as its brightness at: (A) 5 parsecs (B) 10 parsecs (C) 50 parsecs (D) 100 parsecs 13. The apparent magnitude of a star depends on: (A) Distance and intrinsic luminosity (B) Color only (C) Radius only (D) Surface gravity only 14. A lower magnitude number means a star is: (A) Dimmer (B) Brighter (C) Further away (D) Cooler 15. Photomultiplier tubes and CCDs are used in photometry as: (A) Spectrum analyzers (B) Light detectors (C) Diffraction gratings (D) Radio receivers 16. The main advantage of CCDs in astronomical photometry is: (A) They are small (B) They provide high sensitivity and digital data (C) They split light into colors (D) They are cheaper than lenses 17. Differential photometry measures: (A) Differences in spectral lines (B) Brightness of a star relative to a comparison star (C) Stellar distances (D) Light speed variations 18. Which type of stars are most commonly studied with photometry for brightness variations? (A) Main sequence stars (B) Variable stars (C) Neutron stars (D) White dwarfs 19. Eclipsing binary stars can be studied effectively using: (A) Interferometry (B) Photometry (C) Polarimetry (D) Spectroscopy 20. Light curves are graphs of: (A) Spectrum vs wavelength (B) Brightness vs time (C) Distance vs velocity (D) Temperature vs luminosity 21. The discovery of exoplanets using the transit method depends on: (A) Gravitational pull on the star (B) Small dips in stellar brightness (C) Radio emission variations (D) Changes in star temperature 22. The Kepler Space Telescope used: (A) Spectroscopy (B) Photometry (C) Polarimetry (D) Interferometry 23. Photoelectric photometry was a major advancement because it: (A) Used lenses instead of mirrors (B) Replaced visual estimates with electronic measurements (C) Allowed magnification (D) Introduced spectrographs 24. Atmospheric effects on photometry include: (A) Redshift (B) Extinction and scattering (C) Doppler effect (D) Radiation pressure 25. Which technique corrects for atmospheric effects in photometry? (A) Adaptive optics (B) Radio interferometry (C) CCD cooling (D) Lens correction 26. The color index (B–V) in photometry is a measure of: (A) Distance (B) Temperature (C) Luminosity (D) Mass 27. A star with a negative (B–V) color index is likely: (A) Very cool (B) Very hot and blue (C) Yellow like the Sun (D) A red giant 28. The magnitude scale in photometry is: (A) Linear (B) Logarithmic (C) Quadratic (D) Exponential 29. Which effect causes the apparent brightness of stars to vary due to Earth’s atmosphere? (A) Refraction (B) Scintillation (twinkling) (C) Chromatic aberration (D) Doppler shift 30. Stellar variability is often classified using: (A) Photometric light curves (B) Diffraction gratings (C) Mount types (D) Eyepiece magnification 31. Standard stars in photometry are used to: (A) Detect galaxies (B) Calibrate brightness measurements (C) Observe comets (D) Reduce light pollution 32. A bolometer in photometry measures: (A) Radio signals (B) Total radiation including infrared (C) Optical magnitudes only (D) X-ray emissions 33. Photometry across different filters is called: (A) Broadband photometry (B) Narrowband spectroscopy (C) Colorimetric analysis (D) Reflection photometry 34. Narrowband photometry is useful for: (A) Measuring continuum light (B) Studying specific emission or absorption lines (C) Imaging galaxies (D) Correcting telescope focus 35. CCD saturation in photometry occurs when: (A) Too much light fills a pixel (B) Too little light reaches the detector (C) A star is too distant (D) Telescope is misaligned 36. Which noise source affects photometric accuracy? (A) Photon noise (B) Thermal noise (C) Readout noise (D) All of the above 37. The term “signal-to-noise ratio” in photometry refers to: (A) Ratio of magnitudes (B) Strength of signal compared to noise level (C) Light curve slope (D) Magnification level 38. Ground-based photometry is limited by: (A) Telescope size only (B) Atmospheric turbulence and absorption (C) Mirror quality (D) Lens coatings 39. Space-based photometry avoids: (A) Absorption and atmospheric distortion (B) Gravitational effects (C) Temperature variations of stars (D) Radiation from galaxies 40. Which mission revolutionized photometry by detecting thousands of exoplanets? (A) Hubble (B) Spitzer (C) Kepler (D) Chandra 41. The TESS mission focuses on: (A) Measuring stellar spectra (B) Large-scale photometry of nearby stars (C) Radio wave collection (D) Infrared mapping 42. The brightness of a variable star that changes periodically is often plotted as a: (A) Spectral diagram (B) Hertzsprung-Russell diagram (C) Light curve (D) Magnification graph 43. Photometry helps determine the albedo of planets, which means: (A) Rotation speed (B) Reflectivity (C) Mass (D) Magnetic field 44. Stellar flares are detected using: (A) Photometric brightness variations (B) Polarization changes (C) Radio pulses (D) Gamma-ray bursts 45. Which type of variable stars were used as “standard candles” for distance measurement? (A) Pulsars (B) Cepheid variables (C) White dwarfs (D) Red dwarfs 46. RR Lyrae stars are important in photometry because they: (A) Have predictable brightness variations (B) Emit strong radio waves (C) Are supernovae (D) Show strong X-ray lines 47. Photometry across multiple wavelengths helps determine a star’s: (A) Spectrum lines only (B) Temperature and energy output (C) Distance only (D) Magnetic field 48. Which effect in photometry occurs when light is absorbed by Earth’s atmosphere at certain wavelengths? (A) Atmospheric extinction (B) Doppler shift (C) Zeeman effect (D) Light scattering only 49. Photometric redshift estimation uses: (A) Color changes in galaxy light (B) Magnification effects (C) Radio mapping (D) Binary star eclipses 50. The main advantage of photometry over spectroscopy is: (A) Higher detail on spectral lines (B) Simplicity and ability to observe many stars quickly (C) Use of diffraction gratings (D) Measurement of chemical elements directly