Astronomy Chapter 9
the major processes that heat the interiors of the terrestrial worlds are
(1) heat deposited as the planets were built from planetesimals; (2) heat deposited as the planets underwent differentiation; (3) heat released by radioactive decay
how large is an impact crater compared to the size of the impactor
10 times larger
How long, approximately, do geologists estimate it takes for the entire seafloor to be replaced due to plate tectonics?
200 million years
some of the oldest continental crust on Earth lies in
Northeastern Canada
why are there fewer large impact craters on the Earth's seafloor than on the continents?
Seafloor crust is younger than continental crust, so it has had less time in which to suffer impacts
The choices below describe four hypothetical planets. Which one would you expect to have the most features of erosion? (Assume the planets orbit a star just like the Sun and that they are all the same age as the planets in our solar system.)
Size: same as Venus. Distance from Sun: same as Mars. Rotation rate: once every 25 hours.
the choices below describe four hypothetical planets. which one's surface would you expect to be most crowded with impact craters? (Assume the planets orbit a star just like the Sun and that they are all
Size: same as the Moon. Distance from Sun: same as Mars. Rotation rate: once every 10 days.
which internal energy source produces heat by converting gravitational potential energy into thermal energy
accretion and differentiation
the three principal sources of internal heat of terrestrial planets are
accretion, differentiation and radioactivity
what kind of surface features may result from tectonics?
all of the above
what are the conditions necessary for a terrestrial planet to have a strong magnetic field?
both a molten metallic core and reasonably fast rotation
how have we been able to construct detailed maps of surface features on Venus
by using radar from spacecraft that were sent to orbit Venus
the core, mantle, and crust of a planet are defined by differences in their
composition
the main process by which heat flows upward through the lithosphere is
conduction
why is continental crust lower in density than seafloor crust?
continental crust is made from remelted seafloor crust and therefore only the lower-density material rises to form it
What drives the motion of the tectonic plates on Earth?
convection cells in the mantle
from center to surface, which of the following correctly lists the interior layers of a terrestrial world?
core, mantle, crust
which two properties are most important in determining the surface temperature of a planet
distance from the Sun and atmosphere
which of the following best describes the geological histories of the Moon and Mercury
early in their histories, they suffered many impacts and experienced some volcanism and tectonics, but they now have little geological activity at all
which of the terrestrial worlds has the strongest magnetic field
earth
which of the following is not evidence for plate tectonics on Earth?
existence of volcanoes
When we say that a liquid has a high viscosity, we mean that it
flows slowly like honey
steep-sided stratovolcanoes are made from lava that
has a high viscosity
shallow-sloped shield volcanoes are made from lava that
has a medium viscosity
volcanism is more likely on a planet that
has high internal temperatures
which internal heat source still generates heat within the terrestrial worlds today?
heat from radioactive decay
a planet is most likely to have tectonic activity if it has
high internal temperature
Ridges in the middle of the ocean are places where
hot mantle material rises upward and spreads sideways, pushing the plates apart
in general, which things below are affected by a magnetic field?
impact cratering, volcanism, tectonics and erosion
heat escapes from a planet's surface into space by thermal radiation. Planets radiate almost entirely in the wavelength range of the
infrared
what is the most important factor that determines the thickness, and therefore strength, or the lithosphere?
internal temperature
why does Earth have the strongest magnetic field among the terrestrial worlds?
it is the only one that has both a partially molten metallic core and reasonably rapid rotation
which of the following best describes convection?
it is the process in which warm material expands and rises while cool material contracts and falls
why does the moon have a layer of "powdery soil" on its surface
it is the result of countless tiny impacts by small particles striking the moon
You discover an impact crater that is 10 kilometers across. Which of the following can you conclude?
it was created by the impact of an object about 1 km across
which of the following has virtually no effect on the structure of a planet?
its magnetic field
which of the following most likely explain why Venus does not have a strong magnetic field?
its rotation is too slow
which of the following most likely explains why Venus does not have a global magnetic field like Earth?
its rotation is too slow
Based on all we know about the terrestrial worlds, what single factor appears to play the most important role in a terrestrial planet's geological density?
its size
which of the following is the underlying reason why Venus has so little wind erosion?
its slow rotation
what is the fundamental reason that Mars, unlike Earth, has become virtually geologically dead?
its small size compared to Earth
why does the Moon have a layer of powdery "soil" on its surface?
its the result of gradual erosion by micrometeorites striking the Moon
Valles Marineris is a
large canyon on Mars
how did the lunar maria form?
large impacts fractures the Moon's lithosphere, allowing lava to fill the impact basins
which of the following does not have a major effect in shaping planetary surfaces
magnetism
Which two factors are most important to the existence of plate tectonics on Earth?
mantle convection and a thin lithosphere
Most of the Moon's surface is densely covered with craters, but we find relatively few craters with lunar maria. What can we conclude?
maria formed after the heavy bombardment ended
the terrestrial planet cores contain mostly metal because
metals sank to the center during a time when the interiors were molten throughout
the cores of the terrestrial worlds are made mostly of metal because
metals sunk to the centers a long time ago when the interiors were molten throughout
The polar caps on Mars are composed of
mostly solid carbon dioxide and some water ice
suppose we had a device that allowed us to see Earth's interior. If we looked at a typical region of the mantle, what would we see happening?
not much--on human time scales, the mantle looks like solid rock
deep trenches in the ocean mark places where
one plate slides under another, returning older crust to the mantle
What process has shaped Earth's surface more than any other?
plate tectonics
what are the two geological features that appear to set Earth apart from all the other terrestrial worlds?
plate tectonics and widespread erosion
The geysers and hot springs of Yellowstone National Park result from
plumes of hot mantle rising in a hot spot within a plate
which internal energy source is the most important in continuing to heat the terrestrial planets today?
radioactivity
many scientists suspect that Venus has a stronger and thicker lithosphere than Earth. If this is true, which of the following could explain?
the high surface temperature that has "baked out" all the liquid water from Venus's crust and mantle
which of the following regions was the result of plumes of hot mantle rising in a hot spot within a plate?
the islands of Hawaii
which of the following is not generally true of all the terrestrial world lithospheres?
the lithosphere is broken into a set of large plated that float upon the softer rock below
Under what circumstances can differentiation occur in a planet?
the planet must have a molten interior
which of the following does not provide evidence that Mars once had abundant liquid water on its surface?
the presence of canali, discovered in the late 1800s by Giovanni Schiaparelli and mapped by Precival Lowell
what observational evidence supports the idea that Mercury once shrank by some 20 kilometers in radius?
the presence of many long, tall cliffs
Which of the following does not provide evidence that Mars once had flowing?
the presence of vast canals discovered in the late 1800s by Giovanni Schiaparelli and mapped by Percival Lowell
What is differentiation in planetary geology
the process by which gravity separates materials according to density
in the context of planetary geology, what do we mean by outgassing?
the release by volcanism of gases that had been trapped in a planetary interior
the lithosphere of a planet is the layer that consists of
the rigid rocky material of the crust and uppermost portion of the mantle
Why are there fewer large craters on the seafloor than on the continents?
the seafloor crust is younger than the continental crust
when we see a region of a planet that is not as heavily cratered as other regions, we conclude
the surface in the region is younger than the surface in more heavily cratered regions
which of the following best describes why the smaller terrestrial worlds have cooler interiors than the larger ones?
they have relatively more surface area compared to their volumes
why do we think Mercury has so many tremendous cliffs?
they were probably formed by tectonic stresses when the entire planet shrank as its core cooled
Which two geological processes appear to have been most important in shaping the present surface of venus?
volcanoes and tectonics
which of the following is an example of convection
warm air expanding and rising while cooler air contracts and fall
the relatively few craters that we see within the lunar maria
were formed by impacts that occurred after those that formed most of the craters in the lunar highlands
Rank the five terrestrial worlds in order of size from smallest to largest
Moon, Mercury, Mars, Venus, Earth
Why is Earth's continental crust lower in density than seafloor crust?
Continental crust is made as the lowest-density seafloor crust melts and erupts to the surface near subduction zones
which of the following worlds have the thinnest lithospheres?
Earth and Venus
which of the following places is the result of volcanoes erupting over a hot spot in the mantle?
Hawaii
Recent evidence suggests that Mars once had a global magnetic field. Assuming this is true, which of the following could explain why Mars today lacks a global magnetic field like that of Earth?
Mar's interior has cooled so much its molten core layer no longer undergoes convection
which of the following show evidence of ancient river bed?
Mars
Spacecraft have landed on all the terrestrial worlds except
Mercury
all of the following statements about Venus are true. Which one offers evidence of a global repaving about a billion years ago?
Venus has relatively few impact craters and these craters are distributed fairly evenly over the entire planet
What are the basic requirements for a terrestrial world to have a global magnetic field?
a core layer of molten, convecting material and sufficiently rapid rotation
How fast do plates move on Earth?
a few centimeters per year
on average, how fast do the plates move on Earth
a few centimeters per year
Based on its surface features, the most important event on Venus in the past billion years or so was
a global "repaving" that erased essentially all the surface features that had existed earlier
suppose we use a baseball to represent earth. on this scale, the other terrestrial worlds (Mercury, Venus, the Moon and Mars) would range in size approximately from that of
a golf ball to a baseball
Olympus Mons is
a huge shield volcano on Mars
the reason that small planets tend to lose interior heat faster than larger planets is essentially the same as the reason that
a large baked potato takes longer to cool than a small baked potato
a terrestrial world's lithosphere is
a layer of relatively strong, rigid rock, encompassing the crust and part of the mantle
in the context of plate tectonics, what is a subduction zone
a place where a seafloor plate is sliding under a continental plate
Olympus Mons is
a shield volcano on Mars
what is basalt
a type of rock that makes relatively low-viscosity lava
which of the following best describes the lunar maria?
relatively smooth, flat plains on the Moon
how does seafloor crust differ from continental crust
seafloor crust is thinner, younger and higher in density
how does seafloor crust differ from continental crust?
seafloor crust is thinner, younger, and higher in density
The choices below describe four hypothetical planets. Which one would you expect to have the hottest interior? (Assume the planets orbit a star just like the Sun and that they are all the same age as the planets in our solar system.)
size: same as the moon. distance from sun: same as mars. rotation rate: once every 10 days.
The Caloris Basin on Mercury covers a large region of the planet, but few smaller craters have formed on top of it. From this we conclude that
the Carolis Basin formed toward the end of the solar system's period of heavy bombardment
what type of stresses broke Earth's lithosphere into plates?
the circulation of convection cells in the mantle, which dragged against the lithosphere
which of the following describes tectonics?
the disruption of a planet's surface by internal stresses
which of the following describes volcanism
the eruption of molten rock from a planet's interior to its surface
which of the following describes impact cratering
the excavation of bowl-shaped depressions by asteroids or comets striking a planet's surface
which of the following describes impact cratering?
the excavation of bowl-shaped depressions by asteroids or comets striking a planet's surface
which of the following is not an example of tectonics?
the gradual disappearance of a crater rim as a result of wind and rain
what are the circumstances under which convection can occur in a substance?
when the substance is strongly heated from underneath
What do we mean when we say that the terrestrial worlds underwent differentiation?
when their interiors were molten, denser materials sank toward their centers and lighter materials rose toward their surfaces