Term
| 5. Fusion is the process by which |
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Definition
| elements are transformed into heavier elements by nuclear reactions. |
|
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Term
| 5. A curious fact about the structure of the planet Jupiter, compared with the structure of Earth, is that it has |
|
Definition
| much greater mass but much lower average density. |
|
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Term
| 5. The most probable theory for the formation of the solar system is |
|
Definition
| the condensation of a nebula of hot gas into the Sun and planets. |
|
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Term
| 5. the condensation of a nebula of hot gas into the Sun and planets. |
|
Definition
| Many of the extrasolar planets are giant planets like Jupiter, orbiting at distances characteristic of terrestrial planets like Earth, where giant planets cannot form. |
|
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Term
| 5. The albedo of Mercury is about 0.1. This means that |
|
Definition
| Mercury reflects 1/10 of the sunlight falling on it. |
|
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Term
| 5. The albedo of Mercury is about 0.1. This means that |
|
Definition
| Mercury reflects 1/10 of the sunlight falling on it. |
|
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Term
| 5. What was the material from which the solar system formed? |
|
Definition
| nebula made mostly of hydrogen and helium gas but enriched in heavier elements from supernova explosions |
|
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Term
| 5. Where was all the hydrogen in the universe formed? |
|
Definition
| in the Big Bang, at the very beginning of the universe |
|
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Term
| 5. The manner in which the terrestrial planets formed was the |
|
Definition
| accretion of solid planetesimals containing mostly rocky material. |
|
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Term
| 5. The overall shape of the orbits of most of the planets in the solar system is |
|
Definition
| slightly elliptical, but nearly circular. |
|
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Term
| 5. What is the basic difference between comets and asteroids? |
|
Definition
| Comets are mostly composed of ices, whereas asteroids are mainly composed of rocks. |
|
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Term
| 5. The average density of a planet is |
|
Definition
| its total mass divided by its total volume. |
|
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Term
| 5. In our solar system, which of the following planets is NOT a member of the terrestrial group? |
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Definition
|
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Term
| 5. How do we measure the mass of an extrasolar planet? |
|
Definition
| We use Newton’s law of gravity, using the measured distance of the planet from its star and the planet’s gravitational pull on the star |
|
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Term
| 5. In the search for planets around other stars, which of the following possible lines of evidence has NOT yet been seen? |
|
Definition
| faint pinpoints of light slowly circling a star |
|
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Term
| 5. Which planet in our solar system has the largest mass? |
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Definition
|
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Term
| 6. Most of the mountain ranges on the Moon are the |
|
Definition
| circular edges and rims of large maria that have been formed by impacts from large objects. |
|
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Term
| 6. Earth’s magnetic field is most probably generated by |
|
Definition
| electric currents in Earth’s electricity-conducting molten core. |
|
|
Term
| 6. How was the Mid-Atlantic Ridge formed? |
|
Definition
| Molten rock pushed up from Earth’s interior and forced two crustal plates apart. |
|
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Term
| 6. What process created the lunar regolith? |
|
Definition
| cracking and pulverizing by meteoric bombardment |
|
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Term
| 6. Craters are not apparent on Earth at the present time in the abundance seen on the Moon because |
|
Definition
| plate tectonics has returned cratered surface layers into Earth’s interior, and weathering has obliterated the more recent craters. |
|
|
Term
| 6. Subduction on Earth is the process by which |
|
Definition
| dense material sank while lighter material rose to the surface during the early geological history of Earth. |
|
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Term
| 6. What is the most likely cause of the smooth and relatively crater-free surfaces of lunar maria? |
|
Definition
| The lava in these basins flowed in the relatively late geological history of the Moon, after the period of major bombardment. |
|
|
Term
| 6. What is a typical speed of drift for a continent sliding over Earth’s surface? |
|
Definition
| a few centimeters per year |
|
|
Term
|
Definition
| meandering, canyonlike valleys. |
|
|
Term
| 6. Which of the following mechanisms is most likely to have taken place while Earth was molten to form the present structure of Earth? |
|
Definition
| Heavy elements sank to the center under gravity while lighter materials rose to the surface and solidified into rocks. |
|
|
Term
| 6. Which of the following observations have been made about the Moon that will be very helpful (if they prove true) as humans begin to plan for its colonization? |
|
Definition
| discovery of evidence of water (as ice) that can be used for the support of life, the growth of food, and as fuel if it is split into hydrogen and oxygen by sunlight |
|
|
Term
| 6. What is the basic structure of Earth’s interior? |
|
Definition
| solid iron inner core, molten iron outer core, rocky mantle, lighter rocky crust |
|
|
Term
| 6. Why does the temperature in the stratosphere increase with increasing altitude? |
|
Definition
| The stratosphere is heated by solar ultraviolet radiation absorbed by the ozone layer. |
|
|
Term
| 6. In its orbit around Earth, the Moon |
|
Definition
| keeps the same side toward Earth. |
|
|
Term
| 6. Where did the majority of the large amount of carbon dioxide (CO2) from the second major atmosphere to form on the early Earth end up? |
|
Definition
| still in the atmosphere, but the quantity of nitrogen and oxygen has since risen to make these constituents the most abundant and relegate carbon dioxide to a minor constituent |
|
|
Term
| 6. The Moon rotates synchronously as it orbits Earth, always keeping one side pointed toward Earth, because |
|
Definition
| of the effect of the gravitational pull of Earth on the tidally induced bulge on the Moon. |
|
|
Term
| 6. If Earth is known to have an average albedo of 0.37, what percentage of the sunlight hitting Earth is absorbed by it? |
|
Definition
|
|
Term
| 6. The troposphere of Earth is the |
|
Definition
| atmospheric layer closest to the ground. |
|
|
Term
| 6. Which of the following theories is now considered to be the most likely for the formation of the Moon? |
|
Definition
| collision-ejection theory, where an interplanetary collision knocked material into orbit around Earth that eventually formed into the present-day Moon |
|
|
Term
| 6. Auroras on Earth are caused by |
|
Definition
| high-energy charged particles from the magnetosphere guided by Earth’s magnetic field into polar regions of the atmosphere. |
|
|
Term
| The two conditions that appear to be necessary for the generation of a powerful magnetic field in planets that are NOT present simultaneously on Mercury are |
|
Definition
| rapid rotation and a molten iron core. |
|
|
Term
| “This planet has a large iron core, a heavily cratered surface, and no atmosphere.†Which planet in our solar system fits this description? |
|
Definition
|
|
Term
| Which of the following statements best describes our current understanding of the Valles Marineris? |
|
Definition
| The valley system formed primarily by cracking and faulting of the Martian surface, but some valleys at the eastern end appear to have been carved by water. |
|
|
Term
| The conditions on the surface of Venus are |
|
Definition
| a high-pressure, high-temperature, carbon dioxide atmosphere. |
|
|
Term
| What significant evidence is there for the idea that large quantities of water once flowed on the planet Mars? |
|
Definition
| deep, winding canyons and flood plains |
|
|
Term
|
Definition
| irregularly shaped, cratered, and grooved. |
|
|
Term
| Why has Mercury become locked into a 3-to-2 spin orbit coupling instead of a 1-to-1 coupling like the Moon around the Earth? |
|
Definition
| Mercury’s orbit is very eccentric, so its orbital speed varies while its rotation rate remains constant, preventing a 1-to-1 lock. |
|
|
Term
| The severe atmospheric conditions that quickly destroyed spacecraft that soft-landed on the surface of Venus were |
|
Definition
| high temperatures, high pressures, and corrosive acid clouds and mist. |
|
|
Term
| What is the principal reason we have no volcanoes on the Earth anywhere near the size of Olympus Mons? |
|
Definition
| Because of tectonic activity on the Earth, a volcano does not sit over the same spot for long periods and continue to grow. |
|
|
Term
| Temperatures on the surface of Mercury are seen to fluctuate between very cold 100 K (–173°C) and extremely hot 700 K (427°C). What does this measurement indicate about conditions on Mercury? |
|
Definition
| The planet is close to the Sun, has no atmosphere to maintain heat from the Sun, and is rotating. |
|
|
Term
| In view of the present surface and atmospheric conditions on Mars, why would there be no liquid water on its surface? |
|
Definition
| The very low atmospheric pressure would allow the water to boil and evaporate rapidly. |
|
|
Term
| The reason that very few impact craters are seen on Venus compared with the Moon is believed to be that |
|
Definition
| lava flows and surface melting have covered all but the most recent craters. |
|
|
Term
|
Definition
|
|
Term
| What is the main reason that the greenhouse effect has been much more effective in raising the surface temperature on Venus than in raising the surface temperature on the Earth? |
|
Definition
| Carbon dioxide, which traps heat from the planet’s surface, is the major component in the very dense Venusian atmosphere, while it is a only a minor constituent of the Earth’s. |
|
|
Term
| 7. How have we obtained samples of Martian rocks? |
|
Definition
| Rocks were blasted off Mars by impacts and landed on Earth as meteorites. |
|
|
Term
| 7. Mercurys iron core takes up approximately what fraction of the volume of the planet? |
|
Definition
|
|
Term
| 7. What is the Caloris Basin? |
|
Definition
| multiringed impact basin on Mercury |
|
|
Term
| 7. There are many reasons why a multiday hiking trip on foot through the Valles Marineris on Mars would not be advisable, at least not without suitable protection. Which of the following conditions would NOT be a concern? |
|
Definition
| oppressively high atmospheric pressure |
|
|
Term
| 7. The Martian magnetic field is |
|
Definition
| weak and localized, not at all like the global magnetic field of the Earth. |
|
|
Term
| 8. Triton, the giant moon of Neptune, differs from all other major moons of the planets because |
|
Definition
| it orbits in a retrograde direction, opposite to the planets rotation. |
|
|
Term
| 8. Which planetary satellites are known to have plumes of gas escaping through their surfaces? |
|
Definition
|
|
Term
| 8. Jupiters mass makes up what fraction of the total mass of the planetary system, excluding the Sun? |
|
Definition
|
|
Term
| 8. How was Neptune discovered? |
|
Definition
| by a careful application of Newtons laws to the somewhat irregular motions of Uranus |
|
|
Term
| 8. One interesting feature of Jupiters rotation is the fact that |
|
Definition
| regions of Jupiter at different latitudes appear to rotate at different rates. |
|
|
Term
| 8. The specific and unique property of water that was responsible for the large-scale surface features dark polygons surrounded by heavily grooved and lighter terrain”on Ganymedes surface is |
|
Definition
| the fact that it expands when it freezes. Water squeezed out from beneath old, dark ice expanded to produce the lighter, raised terrain |
|
|
Term
| 8. Which planetary satellite shows strong evidence of disruption by an impact at some time in its history and of subsequent partial reassembly and reshaping by self-gravity? |
|
Definition
|
|
Term
| 8. The major gaps in the rings of Saturn are most likely to be caused by |
|
Definition
| combined gravitational forces from Saturn and its moons that deflect the paths of particles that stray into the gaps. |
|
|
Term
| 8. The requirement(s) for the generation of a powerful magnetic field in a Jovian planet (e.g., Jupiter, Saturn) appear(s) to be a |
|
Definition
| liquid metal interior and relatively rapid rotation. |
|
|
Term
| 8. The Roche limit around a planet is defined as the |
|
Definition
| distance at which a planet creates tides on its moons surface high enough to pull its moon apart. |
|
|
Term
| 8. Neptunes high cirrus clouds consist of |
|
Definition
|
|
Term
| 8. Which characteristic of Jupiters satellite Io makes it different from 8. any other known satellite in the solar system? |
|
Definition
| Io is volcanically active, with gas plumes and lava flows. |
|
|
Term
| 8. The ocean water that is predicted to occur below the surface of Jupiters moon Europa is kept unfrozen by heat from |
|
Definition
| tidal distortions of the moon by the combined gravity of Jupiter and the other moons. |
|
|
Term
| 8. The surface of Callisto, the outer Galilean moon of Jupiter, can best be described as |
|
Definition
| relatively smooth, with a great many impact craters and one large basin created by an asteroid impact. |
|
|
Term
| 8. What causes the banded structure on Jupiters visible surface as seen from the Earth? |
|
Definition
| breaking up by underlying mountain ranges of the strong eastward flow caused by Jupiters rapid rotation |
|
|
Term
| 8. What characteristic of Saturns satellite Titan makes it different from any other known satellite in the solar system? |
|
Definition
| Titan has a permanent and dense atmosphere. |
|
|
Term
| 8. What gives Uranus its blue-green coloration? |
|
Definition
| absorption of red light by methane gas |
|
|
Term
| 8. The internal structure of the two largest Jovian planets (from the center outward) is a(n) |
|
Definition
| rocky core, a liquid “ice†layer, a liquid metallic hydrogen and helium layer, and an ordinary hydrogen and helium gaseous layer. |
|
|
Term
| 8. Saturn is less massive than Jupiter but almost the same size. Explain. |
|
Definition
| The smaller mass exerts less gravitational force and is unable to compress the mass as much as in Jupiter. |
|
|
Term
| 8. Which of the following effects is now thought to be the most likely cause for the inclinations of spin axis of several of the planets such as Uranus (and even the Earth) to their orbital planes? |
|
Definition
| major collision with another planetlike body |
|
|
Term
| 9. How large does the coma, or gas cloud surrounding a comet nucleus, become when it reaches its closest point to the Sun? |
|
Definition
| about 106 km, as big as the Sun |
|
|
Term
| 9. Most of the asteroids of the solar system move around the Sun between the orbits of which planets? |
|
Definition
|
|
Term
|
Definition
| a flat or donut-shaped distribution of distant comets around the Sun, extending out about 500 AU. |
|
|
Term
| 9. What mechanism controls the direction in which a comets ion tail is aligned in space? |
|
Definition
| flow of solar wind past the comets head |
|
|
Term
| 9. What is the typical distance between asteroids in the asteroid belt? |
|
Definition
|
|
Term
| 9. A piece of rock from outer space that reaches Earth’s surface after surviving a fiery passage through Earths atmosphere is known as a(n) |
|
Definition
|
|
Term
| 9. Stony iron meteorites are believed to |
|
Definition
| originate from differentiated asteroids (in which iron sank to the center). |
|
|
Term
| 9. What is considered to be the most likely origin of the comets in the Oort cloud? |
|
Definition
| The comets in the Oort cloud formed near the orbits of Uranus and Neptune and were flung outward by the gravitational influence of these two planets. |
|
|
Term
| 9. If you were standing on Pluto, how often would you see the satellite Charon rise above the horizon each day? |
|
Definition
| once every 2 days because Charon orbits in the same direction Pluto rotates but more slowly |
|
|
Term
|
Definition
| small particle of interplanetary dust burning up and glowing as it enters Earths atmosphere. |
|
|
Term
| 9. The Allende meteorite contained an abundance of 26Mg, an isotope of magnesium. What is the significance? |
|
Definition
| 26Mg is the stable product of the decay of radioactive 26Al. The 26Al from which the 26Mg formed was probably produced in a nearby supernova explosion about the time the solar system was formed. |
|
|
Term
| 9. The cause of the meteor showers seen at regular times each year on Earth is most probably |
|
Definition
| Earth moving through the remnant dust and rock fragments of an old comet that are orbiting the Sun in the comets old orbit. |
|
|
Term
|
Definition
| are very much like ordinary silicate rocks. |
|
|
Term
| 9. The most likely origin of the dirty snowballs that become comets when they are deflected into orbits that bring them closer to the Sun is the |
|
Definition
| Kuiper belt and Oort cloud surrounding the solar system. |
|
|
Term
| 9. Interplanetary material |
|
Definition
| falls on Earth at the rate of several hundred tons per day, mostly as micrometeoroids. |
|
|
Term
| 10. The order of the layers or parts of the Sun, as radius increases, is |
|
Definition
| radiative zone, convection zone, photosphere, chromosphere, corona. |
|
|
Term
| 10. The temperature of the Sun’s photosphere is |
|
Definition
|
|
Term
| 10. The major feature that distinguishes a sunspot from other regions on the Sun is |
|
Definition
| its very powerful magnetic field. |
|
|
Term
| 10. One particular feature of the solar corona is its |
|
Definition
|
|
Term
| 10. Which occurrence led astronomers to the conclusion that the temperature of the gases in the solar corona was very high? |
|
Definition
| detection of emission lines from highly ionized elements like iron |
|
|
Term
| 10. Spectral lines observed in the granules seen at the center of the Sun’s disk are |
|
Definition
| blueshifted near the center of the granule and redshifted near the edge of the granule. |
|
|
Term
| 10. In the thermonuclear process that is thought to heat the Sun, the nuclei of which chemical elements are converted to other nuclei to produce the requisite energy? |
|
Definition
| Hydrogen is converted to helium. |
|
|
Term
| 10. Any object will collapse under its own weight unless something stops it. In an ordinary star like the Sun, this collapse is prevented by |
|
Definition
| gas pressure inside the star. |
|
|
Term
| 10. What is the cause of the sunspot cycle on the Sun? |
|
Definition
| Subsurface magnetic fields are twisted by the Sun’s differential rotation and break through the surface as sunspots, then gradually cancel each other and return below the surface. |
|
|
Term
| 10. How does the number of sunspots on the Sun vary with time? |
|
Definition
| The number of sunspots varies relatively regularly, with a period of about 11 years. |
|
|
Term
| 10. Recent solar neutrino experiments have confirmed the suspicion that the explanation for the apparent shortfall in neutrino detection rates over the last 30 years is that |
|
Definition
| 2/3 of the solar neutrinos transform into types of neutrinos that were undetectable by old detection techniques. |
|
|
Term
| 10. The strength of the magnetic field in a sunspot is estimated from Earth by |
|
Definition
| observing the wavelength splitting of atomic spectral lines by the Zeeman effect. |
|
|
Term
| 10. Where would you expect to find spicules? |
|
Definition
| as small but rapidly erupting gas jets in the atmosphere of the Sun |
|
|
Term
| 10. The solar wind is made up primarily of |
|
Definition
| hydrogen nuclei and electrons, some He nuclei. |
|
|
Term
| 10. Apart from the helium nuclei and energy that are produced in proton-proton reactions in the Sun’s core, what are the other by-products? |
|
Definition
| positive electrons (positrons), gamma rays, and neutrinos |
|
|
Term
| 10. In what fundamental way does the overall solar magnetic field differ from that of Earth? |
|
Definition
| The solar field lies just beneath the surface, while Earth’s field passes through the whole Earth. |
|
|
Term
| 10. Coronal holes are thought to be the source of |
|
Definition
|
|
Term
| 10. The word chromosphere refers to a |
|
Definition
| layer in the Sun’s atmosphere. |
|
|
Term
| 10. Over the course of a sunspot cycle of about 11 years, the regions of sunspot occurrence on the Sun move |
|
Definition
| equatorward, moving from 30° to 10° latitude. |
|
|
Term
| 10. If a solar flare produces an X-ray outburst and also triggers a coronal mass ejection (CME), what will be the arrival times of these components, referenced to the time of occurrence on the Sun? |
|
Definition
| The X rays arrive about 8 minutes after the flare, while the CME material arrives after about 2 days. |
|
|