Pathways to Astronomy 5Th Edition By Steven Schneider – Test Bank
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Sample Test
Part 3 Test Bank – The Solar System
 
There are ___ moons more massive than Pluto …
 
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   1.  | 
  
   There are ___ moons more massive than
  Pluto or Eris. 
 The moons are Ganymede, Io, Europa, Callisto, Titan, Triton
  and our Moon.    | 
 
 
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These are bodies nearly the same size as Plu…
 
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   2.  | 
  
   These are bodies nearly the same size
  as Pluto and beyond Neptune’s orbit: ___. 
 Trans-Neptunian Objects.    | 
 
 
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A term for ices which means they can evapor…
 
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   3.  | 
  
   A term for ices which means they can
  evaporate easily is ____. 
 Will be ice or liquid in Earth’s environment.    | 
 
 
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As far as the planets are concerned, the so…
 
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   4.  | 
  
   As far as the planets are concerned,
  the solar system could be described as a thin rotating disk because 
  | 
 
 
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Uranus is tilted into its orbital plane.
 
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   5.  | 
  
   Uranus is tilted into its orbital
  plane.  | 
 
 
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TNOs are primarily made of ices.
 
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   6.  | 
  
   TNOs are primarily made of ices.  | 
 
 
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The average time for an atom to decay is cal…
 
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   7.  | 
  
   The average time for an atom to decay
  is called its _________. 
 Time it takes for half of the parent atoms to decay to their
  daughters.    | 
 
 
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Kant and Laplace proposed this theory of the…
 
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   8.  | 
  
   Kant and Laplace proposed this theory
  of the Solar System formation: _____. 
 Gas cloud flattened and created the solar system.    | 
 
 
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These atoms have the same number of protons…
 
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   9.  | 
  
   These atoms have the same number of
  protons but differing numbers of neutrons. 
 If the number of neutrons gets too large it can become
  radioactive.    | 
 
 
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The solar system was born from
 
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   10.  | 
  
   The solar system was born from 
  | 
 
 
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Meteorites are small chunks of asteroids …
 
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   11.  | 
  
   Meteorites are small chunks of
  asteroids that have landed on the Earth.  | 
 
 
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One of the reasons that Mercury has little o…
 
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   12.  | 
  
   One of the reasons that Mercury has
  little or no atmosphere is its small mass.  | 
 
 
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Dusty and gaseous material orbiting a star i…
 
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   13.  | 
  
   Dusty and gaseous material orbiting a
  star is called a(an) _____. 
 Many pictures have now been taken of these to help our
  research.    | 
 
 
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Planets orbiting stars other than…
 
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   14.  | 
  
   Planets orbiting stars other than the
  Sun are called _____. 
 Each day the number increases.    | 
 
 
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A new theory about many planets orbiti…
 
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   15.  | 
  
   A new theory about many planets
  orbiting other stars is they formed and then ______ to their present
  position. 
 This theory also may explain many things about our solar
  system.    | 
 
 
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The Doppler shift method of detecting exopl…
 
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   16.  | 
  
   The Doppler shift method of detecting
  exoplanets is possible because 
  | 
 
 
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The largest majority of planets found around…
 
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   17.  | 
  
   The largest majority of planets found
  around other stars are earthlike in their masses.  | 
 
 
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We use the Doppler Shift Method to detect ex…
 
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   18.  | 
  
   We use the Doppler Shift Method to
  detect exoplanets.  | 
 
 
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The Earth’s magnetic field is caused by
 
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   19.  | 
  
   The Earth’s magnetic field is caused by 
 The rotation of the Earth and its warm molten iron core make
  the dynamo possible.    | 
 
 
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The process of ______________ creates motion…
 
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   20.  | 
  
   The process of ______________ creates
  motion inside the Earth. 
 Expanding, hotter, lighter materials rise and dense materials fall.    | 
 
 
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This is the more scientific name for the pro…
 
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   21.  | 
  
   This is the more scientific name for
  the process of continental drift: 
 Tecton in Greek is to build.    | 
 
 
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Mountain ranges on the Earth are formed by
 
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   22.  | 
  
   Mountain ranges on the Earth are formed
  by 
  | 
 
 
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Olivine is sometimes carried to the surface …
 
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   23.  | 
  
   Olivine is sometimes carried to the
  surface of the Earth by volcanoes.  | 
 
 
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Rocks on the Earth are primarily silicates.
 
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   24.  | 
  
   Rocks on the Earth are primarily
  silicates.  | 
 
 
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Where our weather takes place:
 
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   25.  | 
  
   Where our weather takes place: 
 Comes from trepan meaning all mixed up.    | 
 
 
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This gas is thought to have destroyed the o…
 
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   26.  | 
  
   This gas is thought to have destroyed
  the ozone layer in the Antarctica: 
 When UV hits CFC it releases chlorine which then destroys the
  ozone layer.    | 
 
 
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This effect is a force created by rotating b…
 
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   27.  | 
  
   This effect is a force created by
  rotating bodies: 
 Veers to the right in the Northern Hemisphere.    | 
 
 
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Oxygen began to appear in the Earth’s atmosphere 2.4 billion
years ago due to
 
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   28.  | 
  
   Oxygen began to appear in the Earth’s
  atmosphere 2.4 billion years ago due to 
  | 
 
 
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The stratosphere is about 12 km above the Ea…
           
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   29.  | 
  
   The stratosphere is about 12 km above
  the Earth’s surface.  | 
 
 
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Global warming over the last century is due …
 
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   30.  | 
  
   Global warming over the last century is
  due primarily to the ozone decrease in our atmosphere.  | 
 
 
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The origin of the moon is thought to be best…
 
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   31.  | 
  
   The origin of the Moon is thought to be
  best explained by _____. 
 Proto Moon and proto Earth collided.    | 
 
 
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Craters on the Moon are created mostly by _…
           
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   32.  | 
  
   Craters on the Moon are created mostly
  by _____. 
 Most craters are caused by accretion formation of the planet.    | 
 
 
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The Marias on the Moon are primarily this t…
 
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   33.  | 
  
   The Marias on the Moon are primarily
  this type of rock: ______. 
 Basalt is a dark volcanic rock.    | 
 
 
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Mountains on the Moon were formed by
 
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   34.  | 
  
   Mountains on the Moon were formed by 
  | 
 
 
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The Marias are newer areas on the Moon.
 
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   35.  | 
  
   The Marias are newer areas on the Moon.  | 
 
 
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The far side of the Moon is primarily cover…
 
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   36.  | 
  
   The far side of the Moon is primarily covered
  by craters.  | 
 
 
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This spacecraft is the first to visit Mercur…
 
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   37.  | 
  
   This spacecraft is the first to visit
  Mercury since 1975: 
 The name implies Mercury Surface, Space Environment,
  Geochemistry and Ranging    | 
 
 
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Caloris Basin is about _____ km across.
 
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   38.  | 
  
   Caloris Basin is about _____ km across. 
 May be largest crater in solar system.    | 
 
 
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Large ____ are found on Mercury, similar to…
 
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   39.  | 
  
   Large ____ are found on Mercury,
  similar to cliffs on Earth. 
 May be caused by the shrinking of the core.    | 
 
 
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Mercury makes one complete rotation in ____…
 
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   40.  | 
  
   Mercury makes one complete rotation in
  ________ of a revolution around the Sun. 
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Relative to the stars, the rotation of Mercu…
 
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   41.  | 
  
   Relative to the stars, the rotation of
  Mercury is about 59 days.  | 
 
 
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Mercury takes 225 days to revolve around the…
 
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   42.  | 
  
   Mercury takes 225 days to revolve
  around the sun.  | 
 
 
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The primary component of Venus’ atmosphere is ____.
 
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   43.  | 
  
   The primary component of Venus’
  atmosphere is ____. 
 Carbon dioxide makes up about 95 percent of the atmosphere.    | 
 
 
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Venus rotates slowly and is _____.
 
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   44.  | 
  
   Venus rotates slowly and is _____. 
 Rotates in 243 days backwards.    | 
 
 
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The molecule in the atmosphere of Venus tha…
 
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   45.  | 
  
   The molecule in the atmosphere of Venus
  that is responsible for its high temperature, due to the greenhouse effect,
  is 
  | 
 
 
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Many craters were found on Venus.
 
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   46.  | 
  
   Many craters were found on Venus.  | 
 
 
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Pancake volcanoes are blistered uplifts on V…
 
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