ASTR p2

  1. The Great Red Spot of Jupiter has been observed since
    the 1600s.
  2. **The basic energy source in the interior of the Sun is the nuclear energy derived from the fusion of
    hydrogen into helium
  3. **Which of the following is a problem inherent to individual radio telescopes?
    poor angular resolution
  4. The temperature of the solar photosphere is about
    5,800 K.
  5. The Zeeman effect describes what changes in spectral lines?
    Line splitting due to intense magnetic fields
  6. In general, the Jovian planets differ from the terrestrial planets in several important features. Which of the following is not one of these features?
    (less dense, more massive, longer rotation periods, considerably larger in size)
    longer rotation periods
  7. What is the average length of time from one time of sunspot maximum on the Sun until the next time of sunspot maximum?
    11 years
  8. **Two forms of electromagnetic radiation that penetrate Earth's atmosphere are
    Visible light and radio waves
  9. Where are the main belt asteroids generally found in the solar system?
    Between the orbits of Mars and Jupiter
  10. The light from the visible surface of the Sun comes from which atmospheric layer?
    Photosphere
  11. What natural barrier tries to prevent two protons from combining?
    Electromagnetic repulsion
  12. Asteroids associated with the Lagrange points in the orbit of Jupiter are called
    Trojan asteroids
  13. The dark appearance of sunspots indicates that they are ______ the surrounding surface of the Sun.
    cooler than
  14. **The four giant moons of Jupiter were discovered by
    Galileo
  15. The only satellite in the solar system known to have a dense atmosphere is _________. It is one of the satellites of Saturn
    Titan
  16. Which of the following properties is constant for all types of electromagnetic waves?
    speed
  17. **Which of the following is a problem inherent to individual radio telescopes?
    They have poor angular resolution.
  18. **Which kind of process, as a net result, supplies the energy of our Sun?
    Hydrogen atoms are converted to helium through fusion.
  19. Observation of the shift of a star's spectrum toward the red or the blue enables us to determine the star’s
    radial velocity.
  20. Name the second most abundant element in the Sun.
    Helium
  21. Which of the following is one of the many contributions Galileo Galilei made to astronomy?
    He used a telescope to observe the heavens, thereby reinforcing the notion of heliocentricity.
  22. **Where are asteroids generally found in the solar system?
    Between the orbits of Mars and Jupiter
  23. If you view a hot star through a cool cloud of gas, what sort of spectrum are you likely to see?
    Absorption
  24. **The temperature of the solar photosphere is about
    5,800 K.
  25. Adaptive optics are used to correct what problem?
    Atmospheric turbulence
  26. **The amount of light reflected by a planet or other object is its
    albedo
  27. **The Zeeman effect describes what changes in spectral lines?
    Line splitting due to intense magnetic fields
  28. How was Uranus discovered?
    By accident, by an astronomer who was conducting a sky survey
  29. Suppose you are at the Tropic of Cancer, which has a latitude of 23.5°. The altitude of the north celestial pole as seen from your position is:
    • 23.5°
    • (same number - the altitude of the north celestial pole is always the same as your latitude)
  30. The planet that rotates on its axis with a period almost identical to that of the Earth is
    Mars
  31. Suppose you see the Moon in the sky one evening. The next evening, it will have moved
    to the east
  32. In 1928 the International Astronomical Union divided the entire sky into ______ officially recognized constellations.
    88
  33. **What is the primary ingredient in the Earth's atmosphere?
    Nitrogen
  34. Which of these is LEAST important to an astronomer for observing stars?
    magnifying power
  35. The absolute magnitude of a star is defined to be the apparent magnitude that the star would have if it were at a standard distance of ______ parsec(s).
    10
  36. The apparent magnitude of the Sun is about
    -27
  37. Which of the following would be considered to be a correct spectral type and luminosity class for our Sun?
    G2V
  38. A parsec is defined as the distance to an object which has a parallax of _____ second(s) of arc.
    1
  39. A fifth-magnitude star is times brighter than a fifteenth-magnitude star.
    10,000
  40. If you view a typical star with a spectrograph, what type of spectrum are you likely to observe?
    Absorption
  41. The luminosity of a star is a unique measure of its
    total energy output
  42. Which of these is the greatest distance?
    1 parsec
  43. All F-type stars have approximately the same
    temperature
  44. The absolute magnitude of the Sun is about
    +5
  45. **The spectrum of a typical gaseous nebula illuminated by an early B-type star is
    an emission spectrum.
  46. An eighth-magnitude star is times brighter than a tenth-magnitude star.
    6 3/10
  47. A telescope of large aperture is better than one of small aperture because of
    greater resolving power
  48. Which two ingredients are needed to make an emission nebula?
    Hot stars and interstellar gas
  49. Stars which are just forming (protostars) radiate most of their energy and are most commonly detected in
    infrared
  50. **What is NOT thought to be approximately the same for each star in a cluster?
    mass
  51. **What inevitably forces a star like the Sun to evolve away from the main sequence?
    It builds up a core of helium
  52. **What is the most important physical characteristic in determining the time that a given star spends on the main sequence?
    Mass
  53. **A galactic cluster is young if
    it has an H-R diagram that resembles a complete main sequence.
  54. The H-R diagram is a plot of
    luminosity versus spectral type.
  55. Another term for luminosity
    absolute magnitude
  56. Spectral type is based on...
    temperature
  57. **What inevitably forces a star like the Sun to evolve away from being a main sequence star?
    It builds up a core of helium
  58. Which of the following definitely does NOT agree with present theories of stellar evolution?
    • [the misconception that] more massive stars evolve more slowly than the less massive stars
    • (Actually, the bigger the star, the more rapidly they evolve.)
  59. **A galactic cluster is young if
    it has an H-R diagram that resembles a complete main sequence.
  60. **What is the most important physical characteristic in determining the time that a given star spends on the main sequence?
    Mass
  61. **The spectrum of a typical gaseous nebula illuminated by a B-type star is
    an emission spectrum
  62. Which of the following are not intrinsic type variable stars?
    Eclipsing binaries
  63. If we know only the period for a Cepheid variable star, we can estimate its
    absolute magnitude
  64. A binary system cannot be seen as an eclipsing system if
    its orbital plane is perpendicular to the line of sight.
  65. Spectroscopic studies of Cepheids show that their changes in brightness are correlated with changes in
    size
  66. The masses of stars other than the Sun would be unknown without the study of
    binary stars
  67. The distances to the nearby galaxies like M33 in Triangulum are based primarily on observations of the periods of the which can be seen in these nearer galaxies.
    Cepheid variable stars
  68. **Stars which are just forming (protostars) radiate most of their energy and are most commonly detected in
    infrared
  69. The variable star delta Cephei is a classic example of a/an
    classical Cepheid
  70. The type of intrinsic variable stars known as stars have periods ranging from a few hours to one day and are often found in globular clusters. They are sometimes referred to as cluster variables. They are often used to estimate distances to globular clusters.
    RR Lyrae
Author
katiedr96
ID
340251
Card Set
ASTR p2
Description
for ASTR
Updated