| a. By measuring the angle the sun made with the vertical at a time when it was known to be directly overhead in a distant city. | ||
| b. By measuring the difference in height of the North Star above the horizon from cities a known distance apart. | ||
| c. By observing a ship entering port and measuring the amount of mast becoming increasingly visible as the ship traveled a known distance toward the port. | ||
| d. By determining the size of the shadow of the earth on the moon during a lunar eclipse. | 
| a. Plato believed in a geocentric universe while Aristotle believed in a heliocentric universe. | ||
| b. Plato believed the earth was flat while Aristotle believed it was a sphere. | ||
| c. Plato believed that only reason could lead to true knowledge while Aristotle believed that observation and classification could lead to true knowledge. | ||
| d. Plato believed that the material world was the highest form of reality while Aristotle believed in a higher form from which the material world was only an imperfect copy. | 
| a. The causes of the phases of the moon. | ||
| b. The causes of eclipses. | ||
| c. The approximate circumference of the earth. | ||
| d. All of the above. | 
| a. Earthly objects were composed of combinations of four basic elements. | ||
| b. Atoms were the basic components of earthly objects. | ||
| c. The earth was spherical in shape. | ||
| d. The laws governing the heavens were different from those governing the earth. | 
| a. It just seemed like common sense. | ||
| b. There was no sensation that we lived on an object that was in motion. | ||
| c. The shifting positions of the stars in the sky due to parallax were not observed. | ||
| d. All of the above. | 
| a. Celestial equator. | ||
| b. North celestial pole. | ||
| c. Celestial sphere. | ||
| d. Ecliptic. | 
| a. When the moon falls in the shadow of the earth. | ||
| b. When the moon falls in the shadow of the sun. | ||
| c. When the earth falls in the shadow of the moon. | ||
| d. When the earth falls in the shadow of the sun. | 
| a. About one week. | ||
| b. About two weeks. | ||
| c. About three weeks. | ||
| d. About four weeks. | 
| a. The distance from the earth to the sun varies throughout the year. | ||
| b. The axis of rotation of the earth is not perpendicular to the orbit of the earth around the sun. | ||
| c. The energy output of the sun varies throughout the year. | ||
| d. Ocean currents carrying heat to the southern and northern hemispheres alternate throughout the year. | 
| a. That solar eclipses only occur during a new moon. | ||
| b. That lunar eclipses only occur during a full moon. | ||
| c. That eclipses do not occur every new or full moon. | ||
| d. Both A and B above. | 
| a. Autumnal equinox. | ||
| b. Winter solstice. | ||
| c. Spring equinox. | ||
| d. Summer solstice. | 
| a. It is closer to the sun than the earth is. | ||
| b. It is roughly the same distance from the sun as the earth is. | ||
| c. It is farther from the sun than the earth is. | ||
| d. None of the above. The relative distances from the sun to the earth and waxing gibbous moon vary throughout the year. | 
| a. Both considered knowledge of the material world to be important. | ||
| b. Both believed the universe to be geocentric. | ||
| c. Both were dominated by religious authorities. | ||
| d. Both were times of political stability. | 
| a. The attitude toward science improved in the Late Middle Ages. | ||
| b. Many of the scientific writings of the Greco-Roman era were recovered in the Late Middle Ages. | ||
| c. The rate of literacy increased in the Late Middle Ages. | ||
| d. The model of the universe changed to the heliocentric model in the Late Middle Ages. | 
| a. The use of trigonometry and spherical geometry. | ||
| b. The preservation of ancient Greek and Roman scientific texts. | ||
| c. The replacement of Roman numerals with Arabic numerals. | ||
| d. Advances in optics and the invention of the telescope. | 
| a. By the rotation of the celestial sphere. | ||
| b. By the rotation of the earth. | ||
| c. By the revolution of the sun about the earth. | ||
| d. By the revolution of the earth about the sun. | 
| a. Kepler's heliocentric model was able to provide calculations that matched the observed orbits of the planets. | ||
| b. Galileo's telescopic observations disproved many features of Ptolemy's geocentric model. | ||
| c. Newton's theory of gravity was compatible with a heliocentric model but not with a geocentric one. | ||
| d. All of the above. | 
| a. It required epicycles to account for the motion of the planets. | ||
| b. It had planets revolving in elliptical orbits. | ||
| c. It was the first to suggest that the earth revolves around the sun. | ||
| d. It included a force of gravity to keep the planets in their orbits. | 
| a. Kepler's laws are observational facts while Newton's law is a theoretical interpretation. | ||
| b. Kepler's laws are theoretical interpretations while Newton's law is an observational fact. | ||
| c. Both Kepler's laws and Newton's law are theoretical interpretations. | ||
| d. Both Kepler's laws and Newton's law are observational facts. | 
| a. Nicolaus Copernicus | ||
| b. Galileo Galilei | ||
| c. Johannes Kepler | ||
| d. Isaac Newton | 
| a. Nicolaus Copernicus | ||
| b. Galileo Galilei | ||
| c. Johannes Kepler | ||
| d. Isaac Newton | 
| a. Nicolaus Copernicus | ||
| b. Galileo Galilei | ||
| c. Johannes Kepler | ||
| d. Isaac Newton | 
| a. Nicolaus Copernicus | ||
| b. Galileo Galilei | ||
| c. Johannes Kepler | ||
| d. Isaac Newton | 
| a. The Bohr model has most of the mass of the atom in the nucleus. | ||
| b. The electrons are no longer located in the nucleus. | ||
| c. The energy of the atom is quantized. | ||
| d. The electrons no longer orbit the nucleus. | 
| a. It was the first to explain how chemical reactions occur. | ||
| b. It was the first to include electrons as a constituent of the atom. | ||
| c. It was the first to explain atomic spectra. | ||
| d. It was the first to recognize that most of the mass of the atom was concentrated in a tiny nucleus at the center of the atom. | 
| a. It was the first to explain how chemical reactions occur. | ||
| b. It was the first to include electrons as a constituent of the atom. | ||
| c. It was the first to explain atomic spectra. | ||
| d. It was the first to recognize that most of the mass of the atom was concentrated in a tiny nucleus at the center of the atom. | 
| a. Small. | ||
| b. Spherical. | ||
| c. Indivisible. | ||
| d. Matter. | 
| a. The bending of light around an obstacle. | ||
| b. The fact that light travels slower in water than it does in air. | ||
| c. Constructive and destructive interference. | ||
| d. All of the above. | 
| a. The photoelectric effect. | ||
| b. The bending of light around an obstacle. | ||
| c. The scattering of X-rays by electrons. | ||
| d. The transition of an atom from a lower energy state to a higher one. | 
| a. Infrared, visible, X-ray, ultraviolet, gamma, radio. | ||
| b. Radio, ultraviolet, visible, infrared, X-ray, gamma. | ||
| c. Radio, infrared, visible, ultraviolet, X-ray, gamma. | ||
| d. Radio, infrared, visible, ultraviolet, gamma, X-ray. | 
| a. Radio waves. | ||
| b. Sound waves. | ||
| c. Gamma rays. | ||
| d. Ultraviolet radiation. | 
| a. It is in the state with the highest energy. | ||
| b. It can emit but not absorb a photon. | ||
| c. It can absorb but not emit a photon. | ||
| d. It can either emit or absorb a photon. | 
| a. It was the first to explain how chemical reactions occur. | ||
| b. It was the first to include electrons as a constituent of the atom. | ||
| c. It was the first to explain atomic spectra. | ||
| d. It was the first to recognize that most of the mass of the atom was concentrated in a tiny nucleus at the center of the atom. | 
| a. By applying Newton's law of gravity to stars in nearby spiral nebulae. | ||
| b. By applying Kepler's laws to planets found in nearby spiral nebulae. | ||
| c. By applying the inverse square law to stars of known luminosity in nearby spiral nebulae. | ||
| d. By analyzing the atomic spectra of stars in nearby spiral nebulae. | 
| a. By measuring the distances to several spiral nebulae. | ||
| b. By showing that the shapes of spiral nebulae were similar to our galaxy. | ||
| c. By measuring the redshifts in the radiation from spiral nebulae. | ||
| d. By measuring the diameters of spiral nebulae and showing that they were about the same size as our galaxy. | 
| a. They are both observational facts. | ||
| b. They are both theoretical interpretations of observational facts. | ||
| c. Hubble's Law is an observational fact and the expansion of space is its theoretical interpretation. | ||
| d. The expansion of space is an observational fact and Hubble's Law is its theoretical interpretation. | 
| a. No dark matter has charge. | ||
| b. Dark matter does not emit or absorb electromagnetic radiation. | ||
| c. Dark matter is not a constituent of atoms. | ||
| d. All of the above. | 
| a. Stars, galaxies, voids, clusters, superclusters. | ||
| b. Stars, galaxies, clusters, voids, superclusters. | ||
| c. Stars, voids, galaxies clusters, superclusters. | ||
| d. Stars, galaxies, clusters, superclusters, voids. | 
| a. That stars in more distant galaxies are younger than those in closer galaxies. | ||
| b. That the distant galaxies are moving away from us through space. | ||
| c. That space is expanding. | ||
| d. That gravity can lengthen the wavelength of light. | 
| a. Recessional velocity and redshift. | ||
| b. Recessional velocity and distance. | ||
| c. Redshift and size. | ||
| d. Recessional velocity and age. | 
| a. The greater the time light from a distant galaxy spends traveling toward us, the more spread out the wavelengths of the light. | ||
| b. The expansion of space slows down the light from distant galaxies in direct proportion to their distance. | ||
| c. The intensity of light from distant galaxies is reduced in direct proportion to their distance. | ||
| d. The more distant a galaxy is, the farther back in time the light we see left the galaxy. | 
| a. Galaxies, clusters, and superclusters, but not stars. | ||
| b. Clusters and superclusters, but not stars or nearby galaxies. | ||
| c. Superclusters, but not stars, nearby galaxies, or clusters. | ||
| d. None of the above. Everything in the universe obeys Hubble's Law. | 
| a. In the central bulge of the galaxy. | ||
| b. In the halo of the galaxy. | ||
| c. In the disk, about 2/3 of the way from the center of the galaxy. | ||
| d. In the disk, at the edge of the galaxy. | 
| a. The age of the universe was discovered to be finite. | ||
| b. The realization that elements heavier than helium were produced in the interiors of stars. | ||
| c. The interpretation of Hubble's Law that space is expanding. | ||
| d. The discovery of the cosmic background radiation. | 
| a. They were aware of Gamow's prediction and set out to discover the radiation. | ||
| b. They were not aware of Gamow's prediction but were aware of Dicke's prediction and set out to discover the radiation. | ||
| c. They were unaware of any prediction and believed that they were the first to make a connection between the radiation and the big bang model. | ||
| d. They were unaware of any prediction and did not realize what they had discovered until later. | 
| a. The age of the universe. | ||
| b. Whether or not the space was expanding. | ||
| c. The large-scale structure of the universe. | ||
| d. All of the above. | 
| a. That space was expanding and the existence of the cosmic background radiation. | ||
| b. That space was expanding and that the early universe was nearly pure hydrogen and helium. | ||
| c. That space was expanding and the universe had a finite age. | ||
| d. That the early universe was nearly pure hydrogen and helium and the existence of the cosmic background radiation. | 
| a. He was the first to predict it. | ||
| b. He was not the first to predict it, but he did independently predict it. | ||
| c. He was a member of the team that discovered it. | ||
| d. He was the first to measure its temperature. | 
| a. George Gamow. | ||
| b. Edwin Hubble. | ||
| c. George Lemaitre. | ||
| d. Arno Penzias. | 
| a. Lemaitre's theory concerns the current universe while Gamow's concerns the early universe. | ||
| b. In Lemaitre's theory, the universe was infinitely old, while in Gamow's, it had a finite age. | ||
| c. Gamow's theory made testable predictions while Lemaitre's did not. | ||
| d. In Gamow's theory, the early universe was hot and dense, but in Lemaitre's, it was cool and dense. | 
| a. Protons and neutrons, atoms, nuclei. | ||
| b. Nuclei, atoms, protons and neutrons. | ||
| c. Protons and neutrons, nuclei, atoms. | ||
| d. Atoms, protons and neutrons, nuclei. | 
| a. Sunlight scattered by dust in the Solar System. | ||
| b. Radioactive material found naturally all over the earth's surface. | ||
| c. Light from the other stars in our galaxy. | ||
| d. A remnant of the early universe. | 
| a. Essentially the same as it is today. | ||
| b. Essentially the same as it is today for the elements lighter than iron, but the very heavy elements had not yet been produced. | ||
| c. Mostly heavier elements because they had not yet had a chance to break down into the lighter elements. | ||
| d. Essentially pure hydrogen and helium. | 
| a. The universe became cool enough for helium nuclei to form. | ||
| b. The temperature of the universe suddenly increased due to the heat of the cosmic background radiation. | ||
| c. Stars and galaxies began to form. | ||
| d. The universe went from an ionized state to a neutral gas. | 
| a. Its temperature is a few degrees above absolute zero. | ||
| b. It comes from the direction of the center of the universe. | ||
| c. It lies in the radio region of the electromagnetic spectrum. | ||
| d. It forms a continuous spectrum. | 
| a. The temperature of the universe. | ||
| b. The density of the universe. | ||
| c. The relative strengths of the forces producing the structure. | ||
| d. Both A and C above. | 
| a. Dark matter, dark energy, atoms. | ||
| b. Dark energy, atoms, dark matter. | ||
| c. Dark energy, dark matter, atoms. | ||
| d. Atoms, dark energy, dark matter. | 
| a. Dark energy plays a significantly greater role now than it did in the early universe. | ||
| b. Electromagnetic radiation and neutrinos made significant contributions to the content of the early universe, but they are insignificant at the present time. | ||
| c. Both now and in the early universe, dark matter was a more significant component of the universe than ordinary matter. | ||
| d. All of the above. | 
| a. 4.6 billion years. | ||
| b. 10 billion years. | ||
| c. 13.7 billion years. | ||
| d. Approximately 20 billion years. | 
| a. Dark energy produces a universal repulsive force which tends to speed up the expansion of space. | ||
| b. Dark energy is the energy that caused the big bang. | ||
| c. Dark energy is a consequence of dark matter. | ||
| d. All of the above. | 
| a. In the earlier history, the expansion of space was slowing down because of gravity, but now it is accelerating because of dark energy. | ||
| b. The force of attraction on the universe by gravity has decreased with time, but the force due to dark energy has been constant since the beginning of the universe. | ||
| c. Einstein's theory of gravity, which included the cosmological constant, could explain both gravity and dark energy. | ||
| d. All of the above. | 
| a. The age of the universe. | ||
| b. The contents of the universe at the time of the formation of the cosmic background radiation. | ||
| c. The existence of dark energy. | ||
| d. Strong evidence that the geometry of the universe is flat. | 
| a. Gravity produces a force while dark energy does not. | ||
| b. Gravity has a tendency to slow the expansion of space while dark energy tends to speed it up. | ||
| c. Dark energy caused the initial expansion of space while gravity is working against expansion. | ||
| d. Gravity has been present since the beginning of the universe while dark energy came into existence only after stars and galaxies formed. | 
| a. The energy emitted per unit surface area in the visual region. | ||
| b. The energy emitted per unit area over all wavelengths. | ||
| c. The energy radiated per second over all wavelengths. | ||
| d. The energy radiated over the lifetime of a star. | 
| a. From 100 to 1/100 solar luminosities. | ||
| b. From 1,000 to 1/100 solar luminosities. | ||
| c. From 10,000 to 1/1,000 solar luminosities. | ||
| d. From 1,000,000 to 1/10,000 solar luminosities. | 
| a. A high-mass main sequence star. | ||
| b. A low-mass main sequence star. | ||
| c. A white dwarf. | ||
| d. A red giant. | 
| a. A high-mass main sequence star. | ||
| b. A low-mass main sequence star. | ||
| c. A white dwarf. | ||
| d. A red giant. | 
| a. Upper left-hand region. | ||
| b. Upper right-hand region. | ||
| c. Lower left-hand region. | ||
| d. Lower right-hand region. | 
| a. A mixture of gas and liquid that, because of its high density, behaves more like a solid. | ||
| b. A very hot gas composed mostly of hydrogen and helium atoms. | ||
| c. A completely ionized state (a plasma) that behaves like a gas. | ||
| d. A mixture of mostly hydrogen and helium that, because of high pressure, behaves like a liquid. | 
| a. The more luminous a star the greater its apparent brightness. | ||
| b. The apparent brightness of a star decreases in direct proportion to the distance. | ||
| c. The apparent brightness of a star decreases with the square of the distance. | ||
| d. None of the above. The apparent brightness depends only on the distance of a star and is not related to its luminosity. | 
| a. It is a plot of the luminosity of a star versus its surface temperature. | ||
| b. Different regions of the diagram represent different stages in the evolution of a star. | ||
| c. The location of a star on the diagram provides information about the size of the star. | ||
| d. All of the above. | 
| a. It becomes hotter and more luminous. | ||
| b. It becomes cooler and more luminous. | ||
| c. It becomes hotter and less luminous. | ||
| d. It becomes cooler and less luminous. | 
| a. It becomes hotter and more luminous. | ||
| b. It becomes cooler and more luminous. | ||
| c. It becomes hotter and less luminous. | ||
| d. It becomes cooler and less luminous. | 
| a. The big bang. | ||
| b. Planetary nebula. | ||
| c. Supernovae. | ||
| d. Both A and C. | 
| a. Carbon. | ||
| b. Silicon. | ||
| c. Iron. | ||
| d. Uranium. | 
| a. Changes in the chemical composition of the core. | ||
| b. Changes in the density of the core. | ||
| c. Changes in the mass of the star. | ||
| d. Changes in the luminosity of the star. | 
| a. Nuclear fusion of hydrogen. | ||
| b. Nuclear fusion of heavier elements. | ||
| c. Heat energy left over from its earlier evolution. | ||
| d. A white dwarf is a dead star; it no longer radiates energy. | 
| a. Iron core, implosion, neutron core, explosion. | ||
| b. Implosion, iron core, explosion, neutron core. | ||
| c. Neutron core, iron core, implosion, explosion. | ||
| d. Iron core, neutron core, implosion, explosion. | 
| a. Because the fusion reactions occur at extremely high temperatures. | ||
| b. Because hydrogen nuclei have the smallest mass of all elements. | ||
| c. Because the helium produced is less massive than the hydrogen that produced it. | ||
| d. Because the helium produced is more massive than the hydrogen that produced it. | 
| a. In the sun, undergoing fusion. | ||
| b. Part of the planet earth. | ||
| c. Part of a star that is now dead. | ||
| d. Part of the material that had emerged from the big bang. | 
| a. The loss of six hydrogen and the gain of two helium. | ||
| b. The loss of six hydrogen and the gain of one helium. | ||
| c. The loss of four hydrogen and the gain of two helium. | ||
| d. The loss of four hydrogen and the gain of one helium. | 
| a. Solar heating. | ||
| b. Continental drift. | ||
| c. Radioactive decay. | ||
| d. The burning of coal and other energy-rich compounds deep in the interior of the earth. | 
| a. 24 days. | ||
| b. 36 days. | ||
| c. 48 days. | ||
| d. 60 days. | 
| a. That it formed by co-accretion at the same time the earth formed. | ||
| b. That it formed by breaking away from the earth because of the very high spin rate of the early earth. | ||
| c. That it formed in a different location in the Solar System and was later gravitationally captured by the early earth. | ||
| d. That it formed by accretion of material eject as a result of a collision between the earth and a massive object. | 
| a. The earth formed from the gravitational collapse of gas and dust. | ||
| b. The earth formed from the accretion of small rock-like bodies. | ||
| c. The earth formed from material that was pulled from the sun by a passing star. | ||
| d. The earth formed from the breakup of a much larger body. | 
| a. Outgassing. | ||
| b. Comet bombardment. | ||
| c. Accretion. | ||
| d. Both A and B. | 
| a. There is now much more carbon dioxide because of burning coal and gasoline. | ||
| b. Most of the present oxygen has been added by photosynthesis in plants. | ||
| c. Biological activity has removed most of the nitrogen present at that time. | ||
| d. The atmosphere was primarily carbon dioxide at that time but it has since dissolved in the oceans. | 
| a. It did not explain the rotation of the planets or the sun. | ||
| b. It did not explain the formation of the planets and the flatness of the Solar System. | ||
| c. It did not explain the rotation of the sun and the formation of the planets. | ||
| d. It did not explain the rotation of the planets and their nearly circular orbits around the sun. | 
| a. The sun and the Jovian planets have similar compositions. | ||
| b. The terrestrial planets are composed of rocky-metallic materials. | ||
| c. The earth is the only planet with oxygen in its atmosphere. | ||
| d. The satellites of the Jovian planets are rocky-metallic-icy in composition. | 
| a. 50 thousand years. | ||
| b. 5 million years. | ||
| c. 5 billion years. | ||
| d. 14 billion years. | 
| a. The similarity between humans and chimpanzees. | ||
| b. The diversity and distribution of species. | ||
| c. The existence of datable fossils. | ||
| d. The fact that virtually all scientists believe in it. | 
| a. Australopithecus afaransis. | ||
| b. Australopithecus africanus. | ||
| c. Homo erectus. | ||
| d. Homo habilis. | 
| a. The ability to walk erect. | ||
| b. Cranial capacity. | ||
| c. An opposable thumb. | ||
| d. Differences in the structure of the teeth. | 
| a. Africa. | ||
| b. The Far East. | ||
| c. The Middle East. | ||
| d. Northern Europe. | 
| a. Amphibians, primates, fish, reptiles. | ||
| b. Fish, amphibians, reptiles, primates. | ||
| c. Amphibians, fish, reptiles, primates. | ||
| d. Fish, reptiles, amphibians, primates. | 
| a. Walk on two legs. | ||
| b. Use tools. | ||
| c. Produce works of art. | ||
| d. Migrate out of Africa. | 
| a. It produced organic compounds such as amino acids. | ||
| b. It produced cell-like structures known as microspheres. | ||
| c. It produced simple living organisms. | ||
| d. It proved that life began in the oceans. | 
| a. Its main-sequence lifetime. | ||
| b. The region near its surface where it is cool enough for molecules to exist. | ||
| c. The range of distances from the star between 0.75 and 1.25 AU. | ||
| d. The range of distances from the star where water can exist as a liquid. | 
| a. The number of habitable planets in the galaxy at the present time. | ||
| b. The number of planets in the galaxy where life exists at the present time. | ||
| c. The number of planets in the galaxy with technological civilizations at the present time. | ||
| d. The number of planets in the universe with technological civilizations at the present time. | 
| a. We have shown that we are the only intelligent life in the galaxy. | ||
| b. We have been in radio contact for some time with extraterrestrial civilizations. | ||
| c. It has been established that at least some UFOs represent extraterrestrial contacts. | ||
| d. It is widely accepted that there are billions of earthlike planets in the galaxy, but the existence of other forms of intelligent life is still uncertain. |