NAME _______________________________________________

Astronomy 121

MW class
Final


Write your name on the test and the Scantron form. Write your student ID number in the appropriate area and bubble in the appropriate numbers on the Scantron form. When you finish the exam, turn in the test and the Scantron form at the front desk.




























Multiple Choice Questions (100 questions--2 points per question). Select the best answer.



1. Aristarchus showed that the distance from the Earth to the Sun was much larger than the size of the Moon's orbit by _____ .
2. The heliocentric theory for the Solar System was first proposed by _____ .
3. Of the following, which has not been used to probe the interior of a planet?
4. Comparative planetology _____ .
5. The concept of the Celestial Sphere was originated by _____ .
6. The altitude of the North Celestial Pole (NCP) above the horizon _____ .
7. A large reason why the Heliocentric theory was not accepted for more than 1,700 years was _____ .
8. A newly discovered comet has an orbit of size 4 astronomical units. What is its orbital period?
9. The large rotating interstellar medium cloud that formed the Solar system, _____ as it contracted.
10. The Center-of-Mass of the Solar System lies _____ .
11. For an observer in Eugene, a day with equal hours of daylight and darkness occurs _____ .
12. Suppose Mars was on the Celestial Meridian at midnight last night. When will Mars next be on the Celestial Meridian at midnight?
13. Copernicus explained the lack of observed Annual Trigonometric Parallax by _____ .
14. The Celestial Equator is _____ .
15. Yesterday I went outside and saw star Z rise at around 8 p.m. One month ago, when did star Z rise?
16. Pluto is ____ .
17. The day with the greatest number of hours of daylight for an observer in Santiago, Chile is _____ .
18. Tycho Brahe's observations _____ .
19. Which of the following must all theories for the formation of our Solar System explain?
20. Which of the following is a FALSE statement about the motions of the planets?

21. According to Copernicus, retrograde motion _____ .
22. Kepler's third law (the Harmonic Law) may be applied to ______ .
23. The daily rising and setting of celestial objects is due to _______ .
24. The Solar day is longer than the sidereal day because _______ .
25. The seasons at mid-northern latitudes are caused by _____ .
26. In the Condensation Theory for the formation of the Solar System, there is a natural explanation for _____ .
27. The Titius-Bode Relation led to the discovery of _____ .
28. Our understanding of the motion of the planets in our Solar System was finally considered complete after _____ .
29. The composition of the interior of Jupiter is most similar to _____ .
30. Jovian planets _____ .
31. The planet with the largest uncompressed density is _____ .
32. The Sun _____ .
33. The Moon _____ during a total Solar eclipse.
34. Protoplanets started to form _____ .
35. Spring tides (the highest high tides) occur _____ .
36. On the vernal equinox, _______ .
37. The rotation period of the Earth ______ tidal forces exerted by the Moon on the Earth.
38. An observer on the Moon is looking at the Earth. The Earth is full. What is the phase of the Moon?
39. Terrestrial planets _____ than are Jovian planets.
40. The conditions in the current atmosphere of Mars are _______ .
41. When Mars was young, its climate was believed to be similar to the current climate of the Earth. Its atmosphere then evolved to what it is today. The current wisdom says that this was because of _______ .
42. The searches for extra-Solar planets that have yielded the most discoveries of planets were based on the detection of _____ .
43. The Jovian-like planets found in extra-Solar planetary systems _____ .
44. Continental plate make up about _____ of the surface of the Earth.
45. Of the following, which suggests that Mars has a permafrost layer?
46. In the Greenhouse Effect on Earth, carbon dioxide traps _____ in the atmosphere
47. Of the following, which would you expect to show the most active geology today?
48. The asthenosphere and lithosphere of the Earth are defined by _____ .
49. S waves are seismic waves. S waves ______ .
50. The Greenhouse Effect _____ .
51. The current atmospheres of the Terrestrial planets are _______ .
52. The majority of the Moon's surface is best described as _______ .
53. Continental plates on the Earth _______.
54. The Tharsis region on Mars _______ .
55. Uranium 235 decays to lead 207 with a half-life of around 700,000 years. A rock contains one-eighth of its original uranium. How old is the rock?
56. The reason the atmospheres of Venus and Earth have followed such different evolutionary paths is _____ .
57. Of the following, which best describes the planet most likely to have an atmosphere?
58. The early atmosphere of Venus may have been as hot as 2,700 F because _____ .
59. The impact that formed the Caloris basin on Mercury also formed the _______ .
60. Near a subduction zone, we expect _______ .
61. A transform fault is _____ .
62. The bulk of the carbon dioxide initially present in the atmosphere of the young Earth _______ .
63. Of the following statements about Venus, which is NOT correct?
64. The Valles Marineris _____ .
65. Lunar maria _______ .
66. Strong evidence that the Moon was geologically active in the past comes from the ____ .
67. The Ozone layer on the Earth ________ .
68. The Hawaiian island chain _______ .
69. The interior of the Earth was significantly heated by _____ .
70. The mountains found on the Moon were formed _____ .
71. The newly discovered planets _____ .
72. The oldest rocks on the Earth are a little more than _____ old, according to radioactive age dating.
73. Compared to the side of the Moon facing the Earth, the Lunar backside has _____ .
74. The density of the Moon is most similar to _____ .
75. What theory of the Moon's origin is favored by most astronomers today?
76. The surface of Mercury bears the strongest resemblance to _____ .
77. The cratering density in the Lunar highlands and maria tells us that _____ .
78. Earth and Venus are often called sister planets. In what ways are Venus and the Earth most alike? Earth and Venus have similar _____ .
79. A large difference between Mars's northern hemisphere and its southern hemisphere is _____ .
80. The Moon has been geologically dead for the last _____ .
81. The belts of Jupiter are best described as _____ .
82. The three cloud layers of Jupiter are composed of ______ .
83. The most massive planet in our Solar System is _____ .
84. The storm-like feature(s) primarily found near 20o N latitude on Jupiter _____ .
85. Jupiter is noticeably flattened in shape because ____ .
86. Of the following planets, which radiates the most energy compared to what it receives from the Sun?
87. The belt and zone structure on Saturn is more muted in color than Jupiter's because _____ .
88. If I am south of the equator on the Earth and I drop a ball from the top of a tall tower, the object ______ .
89. The different colors of the belts and zones on Jupiter and Saturn arise because the clouds _____ .
90. The Great Red Spot ______ .
91. The clouds in the atmosphere of Saturn form in the _____ of Saturn.
92. Kepler's Second Law of Planetary Motion _____ .
93. The Great Red Spot sits in the southern hemisphere of Jupiter and rotates in the counter-clockwise sense. These imply that it _____ .
94. Uranus and Neptune are much less massive than Jupiter and Saturn because _____ .
95. The atmosphere of Saturn is composed primarily of _____ .
96. Saturn's bands, ovals, and flow patterns are driven by _____ .
97. The large magnetic fields of Jupiter and Saturn _____ .
98. The source of the excess heat radiated by Saturn is(are) _____ .
99. The coolest clouds in Jupiter's atmosphere are _____ in color.
100. The equator-to-pole circulation on Saturn is broken into counter-streaming belts and zones by _____ .