Deck 19: Origin of the Solar System and Extrasolar Planets

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Question
During Solar System formation, solid particles contracted from the gas of the nebula as it cooled.
Use Space or
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Question
The passing star hypothesis suggests that planets form in the rotating disks of gas and dust around young stars.
Question
Georges-Louis de Buffon was the first to propose that the Sun and planets formed when a large vortex contracted and condensed.
Question
Asteroids are the last of the icy planetesimals from the formation of the Solar System.
Question
The most important source for determining the age of the Solar System is by sampling a planet's core.
Question
Terrestrial planets grew slowly and the Jovian planets grew quickly.
Question
What are the small bits of rock and metal that collide with Earth's atmosphere?

A) meteors
B) comets
C) asteroids
D) meteorites
E) meteoroids
Question
Which term is described as small, icy bodies that orbit the Sun just beyond Neptune?

A) Kuiper belt objects
B) asteroid belt objects
C) Oort cloud objects
D) Jovian belt objects
E) Neptunian belt objects
Question
Astronomers consider the Solar System's Kuiper belt extending beyond the orbit of Neptune as an example of an old debris disk.
Question
The inner planets are composed of rock and metal, and the outer planets are rich in low-density gases such as hydrogen and helium.
Question
All the planets in the Solar System revolve in a clockwise motion.
Question
The dense disks of gas and dust such as those seen around the stars in Orion are sites where planets could be forming right now.
Question
Kuiper belt objects are small, rocky bodies orbiting beyond Mars.
Question
Asteroids are believed to be debris left over from the failure of a planet to form at a distance of about 3 AU from the Sun.
Question
Which best describes the appearance of an asteroid?

A) spherical in shape and covered with craters
B) spherical in shape with a volcanic surface
C) irregular in shape and covered with craters
D) irregular in shape with a volcanic surface
E) spherical in shape and smooth, dusty surface
Question
Jupiter and Saturn are so massive that they were able to grow by drawing in hot gas by gravitational contraction from the solar nebula.
Question
The first extrasolar planets discovered are small and have long orbital periods.
Question
The Kepler space telescope is searching for extrasolar planets by the transit method.
Question
Kuiper belt objects appear to be ancient planetesimals that formed in the outer Solar System but were never incorporated into a planet.
Question
Water vapor, methane, and ammonia were abundant in the solar nebula.
Question
Descartes' hypothesis of solar system formation was problematic because he did not understand the ____.

A) involvement of condensation
B) involvement of contraction
C) difference in the planets
D) involvement of gravity
E) gaseous properties of the Sun
Question
Planetesimals beyond the orbit of _____ failed to accumulate into a protoplanet because the gravitational field of _____ continuously disturbed their motion.

A) Neptune; Uranus
B) Jupiter; Mars
C) Earth; Saturn
D) Mars; Earth
E) Mars; Jupiter
Question
Which physical property in Laplace's nebular hypothesis could not explain the Sun's slow rotation?

A) angular momentum
B) angular diameter
C) gravitational pull
D) radiation pressure
E) electromagnetic energy
Question
What combination of forces releases the gas and dust of a comet when it approaches the Sun?

A) radiation pressure and electromagnetic energy
B) electromagnetic energy and solar wind
C) solar flares and nuclear fission
D) gravitational energy and solar wind
E) solar wind and radiation pressure
Question
What was the key physical property in determining the two categories of planets during solar system formation?

A) pressure
B) gravity
C) density
D) momentum
E) temperature
Question
The radioactive age of a rock is actually the length of time since the material in that rock was last ____.

A) formed
B) erupted
C) concentrated
D) melted
E) condensed
Question
Laplace's nebular hypothesis was problematic in that he could not explain ____.

A) the different types of planets
B) the rotational direction of the planets
C) how the Sun had
D) how one star could come within a close encounter of another star
E) how gravity was the dominant force of planet formation
Question
Which element represented most of the atoms in the early Universe?

A) helium
B) hydrogen
C) oxygen
D) carbon
E) nitrogen
Question
Numerous meteorites found on Earth originated from which planet?

A) Mercury
B) Venus
C) Mars
D) Jupiter
E) Saturn
Question
Which is the correct order of planetary object class during their formation?

A) planetesimals, protoplanets, and planets
B) planets, planetesimals, and protoplanets
C) planetesimals, planets, and planetettes
D) protoplanets, planetesimals, and planets
E) planetesimals, planetettes, and planets
Question
From meteorite and lunar rock samples, astronomers have determined the age of the Solar System to be ____.

A) 4.6 million years
B) 10 million years
C) 2.4 billion years
D) 4.6 billion years
E) 8.4 billion years
Question
What is the process in planetary formation in which heavy metals settle to the core of the planet while lower density materials floated to the surface to form a crust?

A) separation
B) differentiation
C) gravitation
D) condensation
E) accretion
Question
Once a protoplanet reached a large mass, what is the next step for it to formally grow into a planet?

A) gravitational collapse
B) expanding
C) accretion
D) condensation
E) slowing momentum
Question
As a radioactive substance gradually decays, the abundance of daughter ____ gradually increases.

A) atoms
B) isotopes
C) elements
D) cells
E) nuclei
Question
Comets are composed of ____.

A) rock and dust
B) rock and metals
C) ice and metals
D) ice and dust
E) rock and gas
Question
According to solar nebula theory, what is the first step in planetesimal formation?

A) heating
B) flattening
C) accretion
D) condensation
E) gravitational collapse
Question
The outer planets are composed of ____.

A) rock and ice
B) ice and gas
C) metal and ice
D) high density metals
E) low density gas
Question
What astronomical object is the most important source for determining the age of our Solar System?

A) lunar rocks
B) Earth core samples
C) meteorites
D) meteors
E) asteroids
Question
Who was the first to propose solar system formation with gravity as a key component of the hypothesis?

A) Isaac Newton
B) René Descartes
C) Pierre-Simon de Laplace
D) Georges-Louis de Buffon
E) Emanuel Swedenborg
Question
The inner planets are composed of ____.

A) rock and ice
B) ice and gas
C) rock and gas
D) metal and ice
E) rock and metal
Question
Match between columns
small, irregular icy bodies found orbiting beyond Neptune
asteroids
small, irregular icy bodies found orbiting beyond Neptune
meteor
small, irregular icy bodies found orbiting beyond Neptune
Terrestrial planets
small, irregular icy bodies found orbiting beyond Neptune
Kuiper belt objects
small, irregular icy bodies found orbiting beyond Neptune
comets
small, irregular icy bodies found orbiting beyond Neptune
Jovian planets
small, irregular icy bodies found orbiting beyond Neptune
protoplanets
small, irregular icy bodies found orbiting beyond Neptune
Planetesimals
small, irregular icy bodies found orbiting beyond Neptune
hot Jupiters
small, irregular icy bodies found orbiting beyond Neptune
extrasolar planets
the inner four rocky planets of our Solar System
asteroids
the inner four rocky planets of our Solar System
meteor
the inner four rocky planets of our Solar System
Terrestrial planets
the inner four rocky planets of our Solar System
Kuiper belt objects
the inner four rocky planets of our Solar System
comets
the inner four rocky planets of our Solar System
Jovian planets
the inner four rocky planets of our Solar System
protoplanets
the inner four rocky planets of our Solar System
Planetesimals
the inner four rocky planets of our Solar System
hot Jupiters
the inner four rocky planets of our Solar System
extrasolar planets
piece of dust or tiny rock burning in a planet's atmosphere
asteroids
piece of dust or tiny rock burning in a planet's atmosphere
meteor
piece of dust or tiny rock burning in a planet's atmosphere
Terrestrial planets
piece of dust or tiny rock burning in a planet's atmosphere
Kuiper belt objects
piece of dust or tiny rock burning in a planet's atmosphere
comets
piece of dust or tiny rock burning in a planet's atmosphere
Jovian planets
piece of dust or tiny rock burning in a planet's atmosphere
protoplanets
piece of dust or tiny rock burning in a planet's atmosphere
Planetesimals
piece of dust or tiny rock burning in a planet's atmosphere
hot Jupiters
piece of dust or tiny rock burning in a planet's atmosphere
extrasolar planets
extrasolar Jovian worlds that have been found orbiting close to their parent stars
asteroids
extrasolar Jovian worlds that have been found orbiting close to their parent stars
meteor
extrasolar Jovian worlds that have been found orbiting close to their parent stars
Terrestrial planets
extrasolar Jovian worlds that have been found orbiting close to their parent stars
Kuiper belt objects
extrasolar Jovian worlds that have been found orbiting close to their parent stars
comets
extrasolar Jovian worlds that have been found orbiting close to their parent stars
Jovian planets
extrasolar Jovian worlds that have been found orbiting close to their parent stars
protoplanets
extrasolar Jovian worlds that have been found orbiting close to their parent stars
Planetesimals
extrasolar Jovian worlds that have been found orbiting close to their parent stars
hot Jupiters
extrasolar Jovian worlds that have been found orbiting close to their parent stars
extrasolar planets
planets orbiting stars outside of our Solar System
asteroids
planets orbiting stars outside of our Solar System
meteor
planets orbiting stars outside of our Solar System
Terrestrial planets
planets orbiting stars outside of our Solar System
Kuiper belt objects
planets orbiting stars outside of our Solar System
comets
planets orbiting stars outside of our Solar System
Jovian planets
planets orbiting stars outside of our Solar System
protoplanets
planets orbiting stars outside of our Solar System
Planetesimals
planets orbiting stars outside of our Solar System
hot Jupiters
planets orbiting stars outside of our Solar System
extrasolar planets
the outer four gaseous planets of our Solar system
asteroids
the outer four gaseous planets of our Solar system
meteor
the outer four gaseous planets of our Solar system
Terrestrial planets
the outer four gaseous planets of our Solar system
Kuiper belt objects
the outer four gaseous planets of our Solar system
comets
the outer four gaseous planets of our Solar system
Jovian planets
the outer four gaseous planets of our Solar system
protoplanets
the outer four gaseous planets of our Solar system
Planetesimals
the outer four gaseous planets of our Solar system
hot Jupiters
the outer four gaseous planets of our Solar system
extrasolar planets
icy bodies with "tails" on a extreme elliptical orbit
asteroids
icy bodies with "tails" on a extreme elliptical orbit
meteor
icy bodies with "tails" on a extreme elliptical orbit
Terrestrial planets
icy bodies with "tails" on a extreme elliptical orbit
Kuiper belt objects
icy bodies with "tails" on a extreme elliptical orbit
comets
icy bodies with "tails" on a extreme elliptical orbit
Jovian planets
icy bodies with "tails" on a extreme elliptical orbit
protoplanets
icy bodies with "tails" on a extreme elliptical orbit
Planetesimals
icy bodies with "tails" on a extreme elliptical orbit
hot Jupiters
icy bodies with "tails" on a extreme elliptical orbit
extrasolar planets
small, irregular rocky bodies mostly found between Mars and Jupiter
asteroids
small, irregular rocky bodies mostly found between Mars and Jupiter
meteor
small, irregular rocky bodies mostly found between Mars and Jupiter
Terrestrial planets
small, irregular rocky bodies mostly found between Mars and Jupiter
Kuiper belt objects
small, irregular rocky bodies mostly found between Mars and Jupiter
comets
small, irregular rocky bodies mostly found between Mars and Jupiter
Jovian planets
small, irregular rocky bodies mostly found between Mars and Jupiter
protoplanets
small, irregular rocky bodies mostly found between Mars and Jupiter
Planetesimals
small, irregular rocky bodies mostly found between Mars and Jupiter
hot Jupiters
small, irregular rocky bodies mostly found between Mars and Jupiter
extrasolar planets
coalescing planetesimals that eventually become planets
asteroids
coalescing planetesimals that eventually become planets
meteor
coalescing planetesimals that eventually become planets
Terrestrial planets
coalescing planetesimals that eventually become planets
Kuiper belt objects
coalescing planetesimals that eventually become planets
comets
coalescing planetesimals that eventually become planets
Jovian planets
coalescing planetesimals that eventually become planets
protoplanets
coalescing planetesimals that eventually become planets
Planetesimals
coalescing planetesimals that eventually become planets
hot Jupiters
coalescing planetesimals that eventually become planets
extrasolar planets
solid bits of matter that will eventually be made into protoplanets
asteroids
solid bits of matter that will eventually be made into protoplanets
meteor
solid bits of matter that will eventually be made into protoplanets
Terrestrial planets
solid bits of matter that will eventually be made into protoplanets
Kuiper belt objects
solid bits of matter that will eventually be made into protoplanets
comets
solid bits of matter that will eventually be made into protoplanets
Jovian planets
solid bits of matter that will eventually be made into protoplanets
protoplanets
solid bits of matter that will eventually be made into protoplanets
Planetesimals
solid bits of matter that will eventually be made into protoplanets
hot Jupiters
solid bits of matter that will eventually be made into protoplanets
extrasolar planets
Question
Which best describes the transit method?

A) observing changes in the brightness of the star when the orbiting planet crosses in front of the star
B) observing the magnification of a distant star's brightness by gravitational lensing when an extrasolar planet passes precisely between Earth and a background star
C) observing the back-and-forth motion that can be measured from Doppler shifts in a star's spectrum
D) observing the intensity of brightness from a newborn distant star
E) observing the magnification of a distant planet when it passes closely to our Solar System
Question
Explain the Jovian problem and some possible answers to why there are so many Jovian planets found around stars.
Question
Almost every solid surface in the Solar System is covered with _______________, most of which formed during a period of heavy bombardment.
Question
Which method does the Kepler space telescope use to detect extrasolar planets?

A) Doppler method
B) microlensing method
C) wobble method
D) transit method
E) astrometric method
Question
Which space observatory uses the transit method to detect extrasolar planets?

A) Hubble
B) Kepler
C) Spitzer
D) Chandra
E) Voyager
Question
Explain the steps involved in clearing a nebular of its interstellar material that stopped planetary formation.
Question
The Jovian planets formed beyond the _______________, where water vapor, methane, and ammonia could freeze to form ice particles.
Question
Why do Terrestrial planets not have rings?

A) Terrestrial planets rotate in the opposite direction of the Sun.
B) Terrestrial planets do not have large enough masses to retain particles in rings.
C) Terrestrial planets have a core too rich in heavy metals to retain rings.
D) Terrestrial planets are too close to the Sun to support a ring system.
E) Terrestrial planets are not gaseous bodies.
Question
Which hypothesis was out-ruled by the solar nebular theory?

A) planet accretion hypothesis
B) imploding cloud hypothesis
C) passing star hypothesis
D) condensation hypothesis
E) catastrophic hypothesis
Question
A collection of small, icy bodies are found in the _______________ orbiting in the outer fringes of our Solar System
Question
What do scientists believe created the asteroid belt during Solar System formation?
Question
The Kepler mission has found a lot more of ______________ than Earth-like extrasolar planets.
Question
A large _______________ makes it easier for a planet to hold onto orbiting ring particles.
Question
Which statement best describes an extrasolar planet?

A) A planet that orbits closely to the Sun in our Solar System.
B) A new planet not previously accounted for within our Solar System.
C) A planet smaller and icier than the other planets in our Solar System.
D) A planet discovered orbiting another star outside of our Solar System.
E) A planetary body that orbits just beyond Neptune.
Question
Outline the three steps to the solar nebular theory.
Question
All the planets revolve around the Sun in a(n) _______________ direction.
Question
Explain why the passing star hypothesis was problematic.
Question
Explain the two sources of heat that "melted" a planet during its formation.
Question
Which theory best describes today's current thinking about the birth of a solar system?

A) Big Bang theory
B) Solar Nebular theory
C) Condensation theory
D) Theory of Relativity
E) Passing star theory
Question
The process of _______________ depends partly on the presence of short-lived radioactive elements whose rapid decay would have released enough heat to melt the interior of planets.
Question
During the growth of planetesimals to protoplanets, could the planetesimals have collided into one another? Why or why not?
Question
Explain the four internal processes that gradually destroy a solar nebula.
Question
The _______________ supposes that planets form in the rotating disks of gas and dust around young stars.
Question
According to the solar nebula theory, Earth and the other planets of the Solar System formed billions of years ago as the Sun _______________ from a cloud of interstellar gas and dust.
Question
The _______________ of a radioactive substance is the time it takes for half of the parent isotope atoms to decay into daughter isotope atoms.
Question
Jupiter and Saturn are so massive they were able to grow by drawing in cool gas by _______________ from the solar nebula.
Question
Outline a simple model of planet building.
Question
In the inner solar nebula, only metals and silicates could form solids, so the _______________ planets grew slowly.
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Deck 19: Origin of the Solar System and Extrasolar Planets
1
During Solar System formation, solid particles contracted from the gas of the nebula as it cooled.
False
2
The passing star hypothesis suggests that planets form in the rotating disks of gas and dust around young stars.
False
3
Georges-Louis de Buffon was the first to propose that the Sun and planets formed when a large vortex contracted and condensed.
False
4
Asteroids are the last of the icy planetesimals from the formation of the Solar System.
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k this deck
5
The most important source for determining the age of the Solar System is by sampling a planet's core.
Unlock Deck
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6
Terrestrial planets grew slowly and the Jovian planets grew quickly.
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7
What are the small bits of rock and metal that collide with Earth's atmosphere?

A) meteors
B) comets
C) asteroids
D) meteorites
E) meteoroids
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Unlock for access to all 69 flashcards in this deck.
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8
Which term is described as small, icy bodies that orbit the Sun just beyond Neptune?

A) Kuiper belt objects
B) asteroid belt objects
C) Oort cloud objects
D) Jovian belt objects
E) Neptunian belt objects
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9
Astronomers consider the Solar System's Kuiper belt extending beyond the orbit of Neptune as an example of an old debris disk.
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10
The inner planets are composed of rock and metal, and the outer planets are rich in low-density gases such as hydrogen and helium.
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11
All the planets in the Solar System revolve in a clockwise motion.
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12
The dense disks of gas and dust such as those seen around the stars in Orion are sites where planets could be forming right now.
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13
Kuiper belt objects are small, rocky bodies orbiting beyond Mars.
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14
Asteroids are believed to be debris left over from the failure of a planet to form at a distance of about 3 AU from the Sun.
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15
Which best describes the appearance of an asteroid?

A) spherical in shape and covered with craters
B) spherical in shape with a volcanic surface
C) irregular in shape and covered with craters
D) irregular in shape with a volcanic surface
E) spherical in shape and smooth, dusty surface
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16
Jupiter and Saturn are so massive that they were able to grow by drawing in hot gas by gravitational contraction from the solar nebula.
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17
The first extrasolar planets discovered are small and have long orbital periods.
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18
The Kepler space telescope is searching for extrasolar planets by the transit method.
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19
Kuiper belt objects appear to be ancient planetesimals that formed in the outer Solar System but were never incorporated into a planet.
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20
Water vapor, methane, and ammonia were abundant in the solar nebula.
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21
Descartes' hypothesis of solar system formation was problematic because he did not understand the ____.

A) involvement of condensation
B) involvement of contraction
C) difference in the planets
D) involvement of gravity
E) gaseous properties of the Sun
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k this deck
22
Planetesimals beyond the orbit of _____ failed to accumulate into a protoplanet because the gravitational field of _____ continuously disturbed their motion.

A) Neptune; Uranus
B) Jupiter; Mars
C) Earth; Saturn
D) Mars; Earth
E) Mars; Jupiter
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23
Which physical property in Laplace's nebular hypothesis could not explain the Sun's slow rotation?

A) angular momentum
B) angular diameter
C) gravitational pull
D) radiation pressure
E) electromagnetic energy
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24
What combination of forces releases the gas and dust of a comet when it approaches the Sun?

A) radiation pressure and electromagnetic energy
B) electromagnetic energy and solar wind
C) solar flares and nuclear fission
D) gravitational energy and solar wind
E) solar wind and radiation pressure
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25
What was the key physical property in determining the two categories of planets during solar system formation?

A) pressure
B) gravity
C) density
D) momentum
E) temperature
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k this deck
26
The radioactive age of a rock is actually the length of time since the material in that rock was last ____.

A) formed
B) erupted
C) concentrated
D) melted
E) condensed
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Unlock Deck
k this deck
27
Laplace's nebular hypothesis was problematic in that he could not explain ____.

A) the different types of planets
B) the rotational direction of the planets
C) how the Sun had
D) how one star could come within a close encounter of another star
E) how gravity was the dominant force of planet formation
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Unlock for access to all 69 flashcards in this deck.
Unlock Deck
k this deck
28
Which element represented most of the atoms in the early Universe?

A) helium
B) hydrogen
C) oxygen
D) carbon
E) nitrogen
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29
Numerous meteorites found on Earth originated from which planet?

A) Mercury
B) Venus
C) Mars
D) Jupiter
E) Saturn
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k this deck
30
Which is the correct order of planetary object class during their formation?

A) planetesimals, protoplanets, and planets
B) planets, planetesimals, and protoplanets
C) planetesimals, planets, and planetettes
D) protoplanets, planetesimals, and planets
E) planetesimals, planetettes, and planets
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31
From meteorite and lunar rock samples, astronomers have determined the age of the Solar System to be ____.

A) 4.6 million years
B) 10 million years
C) 2.4 billion years
D) 4.6 billion years
E) 8.4 billion years
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Unlock Deck
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32
What is the process in planetary formation in which heavy metals settle to the core of the planet while lower density materials floated to the surface to form a crust?

A) separation
B) differentiation
C) gravitation
D) condensation
E) accretion
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Unlock for access to all 69 flashcards in this deck.
Unlock Deck
k this deck
33
Once a protoplanet reached a large mass, what is the next step for it to formally grow into a planet?

A) gravitational collapse
B) expanding
C) accretion
D) condensation
E) slowing momentum
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34
As a radioactive substance gradually decays, the abundance of daughter ____ gradually increases.

A) atoms
B) isotopes
C) elements
D) cells
E) nuclei
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Unlock Deck
k this deck
35
Comets are composed of ____.

A) rock and dust
B) rock and metals
C) ice and metals
D) ice and dust
E) rock and gas
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k this deck
36
According to solar nebula theory, what is the first step in planetesimal formation?

A) heating
B) flattening
C) accretion
D) condensation
E) gravitational collapse
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k this deck
37
The outer planets are composed of ____.

A) rock and ice
B) ice and gas
C) metal and ice
D) high density metals
E) low density gas
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38
What astronomical object is the most important source for determining the age of our Solar System?

A) lunar rocks
B) Earth core samples
C) meteorites
D) meteors
E) asteroids
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Unlock for access to all 69 flashcards in this deck.
Unlock Deck
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39
Who was the first to propose solar system formation with gravity as a key component of the hypothesis?

A) Isaac Newton
B) René Descartes
C) Pierre-Simon de Laplace
D) Georges-Louis de Buffon
E) Emanuel Swedenborg
Unlock Deck
Unlock for access to all 69 flashcards in this deck.
Unlock Deck
k this deck
40
The inner planets are composed of ____.

A) rock and ice
B) ice and gas
C) rock and gas
D) metal and ice
E) rock and metal
Unlock Deck
Unlock for access to all 69 flashcards in this deck.
Unlock Deck
k this deck
41
Match between columns
small, irregular icy bodies found orbiting beyond Neptune
asteroids
small, irregular icy bodies found orbiting beyond Neptune
meteor
small, irregular icy bodies found orbiting beyond Neptune
Terrestrial planets
small, irregular icy bodies found orbiting beyond Neptune
Kuiper belt objects
small, irregular icy bodies found orbiting beyond Neptune
comets
small, irregular icy bodies found orbiting beyond Neptune
Jovian planets
small, irregular icy bodies found orbiting beyond Neptune
protoplanets
small, irregular icy bodies found orbiting beyond Neptune
Planetesimals
small, irregular icy bodies found orbiting beyond Neptune
hot Jupiters
small, irregular icy bodies found orbiting beyond Neptune
extrasolar planets
the inner four rocky planets of our Solar System
asteroids
the inner four rocky planets of our Solar System
meteor
the inner four rocky planets of our Solar System
Terrestrial planets
the inner four rocky planets of our Solar System
Kuiper belt objects
the inner four rocky planets of our Solar System
comets
the inner four rocky planets of our Solar System
Jovian planets
the inner four rocky planets of our Solar System
protoplanets
the inner four rocky planets of our Solar System
Planetesimals
the inner four rocky planets of our Solar System
hot Jupiters
the inner four rocky planets of our Solar System
extrasolar planets
piece of dust or tiny rock burning in a planet's atmosphere
asteroids
piece of dust or tiny rock burning in a planet's atmosphere
meteor
piece of dust or tiny rock burning in a planet's atmosphere
Terrestrial planets
piece of dust or tiny rock burning in a planet's atmosphere
Kuiper belt objects
piece of dust or tiny rock burning in a planet's atmosphere
comets
piece of dust or tiny rock burning in a planet's atmosphere
Jovian planets
piece of dust or tiny rock burning in a planet's atmosphere
protoplanets
piece of dust or tiny rock burning in a planet's atmosphere
Planetesimals
piece of dust or tiny rock burning in a planet's atmosphere
hot Jupiters
piece of dust or tiny rock burning in a planet's atmosphere
extrasolar planets
extrasolar Jovian worlds that have been found orbiting close to their parent stars
asteroids
extrasolar Jovian worlds that have been found orbiting close to their parent stars
meteor
extrasolar Jovian worlds that have been found orbiting close to their parent stars
Terrestrial planets
extrasolar Jovian worlds that have been found orbiting close to their parent stars
Kuiper belt objects
extrasolar Jovian worlds that have been found orbiting close to their parent stars
comets
extrasolar Jovian worlds that have been found orbiting close to their parent stars
Jovian planets
extrasolar Jovian worlds that have been found orbiting close to their parent stars
protoplanets
extrasolar Jovian worlds that have been found orbiting close to their parent stars
Planetesimals
extrasolar Jovian worlds that have been found orbiting close to their parent stars
hot Jupiters
extrasolar Jovian worlds that have been found orbiting close to their parent stars
extrasolar planets
planets orbiting stars outside of our Solar System
asteroids
planets orbiting stars outside of our Solar System
meteor
planets orbiting stars outside of our Solar System
Terrestrial planets
planets orbiting stars outside of our Solar System
Kuiper belt objects
planets orbiting stars outside of our Solar System
comets
planets orbiting stars outside of our Solar System
Jovian planets
planets orbiting stars outside of our Solar System
protoplanets
planets orbiting stars outside of our Solar System
Planetesimals
planets orbiting stars outside of our Solar System
hot Jupiters
planets orbiting stars outside of our Solar System
extrasolar planets
the outer four gaseous planets of our Solar system
asteroids
the outer four gaseous planets of our Solar system
meteor
the outer four gaseous planets of our Solar system
Terrestrial planets
the outer four gaseous planets of our Solar system
Kuiper belt objects
the outer four gaseous planets of our Solar system
comets
the outer four gaseous planets of our Solar system
Jovian planets
the outer four gaseous planets of our Solar system
protoplanets
the outer four gaseous planets of our Solar system
Planetesimals
the outer four gaseous planets of our Solar system
hot Jupiters
the outer four gaseous planets of our Solar system
extrasolar planets
icy bodies with "tails" on a extreme elliptical orbit
asteroids
icy bodies with "tails" on a extreme elliptical orbit
meteor
icy bodies with "tails" on a extreme elliptical orbit
Terrestrial planets
icy bodies with "tails" on a extreme elliptical orbit
Kuiper belt objects
icy bodies with "tails" on a extreme elliptical orbit
comets
icy bodies with "tails" on a extreme elliptical orbit
Jovian planets
icy bodies with "tails" on a extreme elliptical orbit
protoplanets
icy bodies with "tails" on a extreme elliptical orbit
Planetesimals
icy bodies with "tails" on a extreme elliptical orbit
hot Jupiters
icy bodies with "tails" on a extreme elliptical orbit
extrasolar planets
small, irregular rocky bodies mostly found between Mars and Jupiter
asteroids
small, irregular rocky bodies mostly found between Mars and Jupiter
meteor
small, irregular rocky bodies mostly found between Mars and Jupiter
Terrestrial planets
small, irregular rocky bodies mostly found between Mars and Jupiter
Kuiper belt objects
small, irregular rocky bodies mostly found between Mars and Jupiter
comets
small, irregular rocky bodies mostly found between Mars and Jupiter
Jovian planets
small, irregular rocky bodies mostly found between Mars and Jupiter
protoplanets
small, irregular rocky bodies mostly found between Mars and Jupiter
Planetesimals
small, irregular rocky bodies mostly found between Mars and Jupiter
hot Jupiters
small, irregular rocky bodies mostly found between Mars and Jupiter
extrasolar planets
coalescing planetesimals that eventually become planets
asteroids
coalescing planetesimals that eventually become planets
meteor
coalescing planetesimals that eventually become planets
Terrestrial planets
coalescing planetesimals that eventually become planets
Kuiper belt objects
coalescing planetesimals that eventually become planets
comets
coalescing planetesimals that eventually become planets
Jovian planets
coalescing planetesimals that eventually become planets
protoplanets
coalescing planetesimals that eventually become planets
Planetesimals
coalescing planetesimals that eventually become planets
hot Jupiters
coalescing planetesimals that eventually become planets
extrasolar planets
solid bits of matter that will eventually be made into protoplanets
asteroids
solid bits of matter that will eventually be made into protoplanets
meteor
solid bits of matter that will eventually be made into protoplanets
Terrestrial planets
solid bits of matter that will eventually be made into protoplanets
Kuiper belt objects
solid bits of matter that will eventually be made into protoplanets
comets
solid bits of matter that will eventually be made into protoplanets
Jovian planets
solid bits of matter that will eventually be made into protoplanets
protoplanets
solid bits of matter that will eventually be made into protoplanets
Planetesimals
solid bits of matter that will eventually be made into protoplanets
hot Jupiters
solid bits of matter that will eventually be made into protoplanets
extrasolar planets
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42
Which best describes the transit method?

A) observing changes in the brightness of the star when the orbiting planet crosses in front of the star
B) observing the magnification of a distant star's brightness by gravitational lensing when an extrasolar planet passes precisely between Earth and a background star
C) observing the back-and-forth motion that can be measured from Doppler shifts in a star's spectrum
D) observing the intensity of brightness from a newborn distant star
E) observing the magnification of a distant planet when it passes closely to our Solar System
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43
Explain the Jovian problem and some possible answers to why there are so many Jovian planets found around stars.
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44
Almost every solid surface in the Solar System is covered with _______________, most of which formed during a period of heavy bombardment.
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45
Which method does the Kepler space telescope use to detect extrasolar planets?

A) Doppler method
B) microlensing method
C) wobble method
D) transit method
E) astrometric method
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46
Which space observatory uses the transit method to detect extrasolar planets?

A) Hubble
B) Kepler
C) Spitzer
D) Chandra
E) Voyager
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47
Explain the steps involved in clearing a nebular of its interstellar material that stopped planetary formation.
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48
The Jovian planets formed beyond the _______________, where water vapor, methane, and ammonia could freeze to form ice particles.
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49
Why do Terrestrial planets not have rings?

A) Terrestrial planets rotate in the opposite direction of the Sun.
B) Terrestrial planets do not have large enough masses to retain particles in rings.
C) Terrestrial planets have a core too rich in heavy metals to retain rings.
D) Terrestrial planets are too close to the Sun to support a ring system.
E) Terrestrial planets are not gaseous bodies.
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50
Which hypothesis was out-ruled by the solar nebular theory?

A) planet accretion hypothesis
B) imploding cloud hypothesis
C) passing star hypothesis
D) condensation hypothesis
E) catastrophic hypothesis
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51
A collection of small, icy bodies are found in the _______________ orbiting in the outer fringes of our Solar System
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52
What do scientists believe created the asteroid belt during Solar System formation?
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53
The Kepler mission has found a lot more of ______________ than Earth-like extrasolar planets.
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54
A large _______________ makes it easier for a planet to hold onto orbiting ring particles.
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55
Which statement best describes an extrasolar planet?

A) A planet that orbits closely to the Sun in our Solar System.
B) A new planet not previously accounted for within our Solar System.
C) A planet smaller and icier than the other planets in our Solar System.
D) A planet discovered orbiting another star outside of our Solar System.
E) A planetary body that orbits just beyond Neptune.
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56
Outline the three steps to the solar nebular theory.
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57
All the planets revolve around the Sun in a(n) _______________ direction.
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58
Explain why the passing star hypothesis was problematic.
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59
Explain the two sources of heat that "melted" a planet during its formation.
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60
Which theory best describes today's current thinking about the birth of a solar system?

A) Big Bang theory
B) Solar Nebular theory
C) Condensation theory
D) Theory of Relativity
E) Passing star theory
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61
The process of _______________ depends partly on the presence of short-lived radioactive elements whose rapid decay would have released enough heat to melt the interior of planets.
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62
During the growth of planetesimals to protoplanets, could the planetesimals have collided into one another? Why or why not?
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63
Explain the four internal processes that gradually destroy a solar nebula.
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64
The _______________ supposes that planets form in the rotating disks of gas and dust around young stars.
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65
According to the solar nebula theory, Earth and the other planets of the Solar System formed billions of years ago as the Sun _______________ from a cloud of interstellar gas and dust.
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66
The _______________ of a radioactive substance is the time it takes for half of the parent isotope atoms to decay into daughter isotope atoms.
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67
Jupiter and Saturn are so massive they were able to grow by drawing in cool gas by _______________ from the solar nebula.
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68
Outline a simple model of planet building.
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69
In the inner solar nebula, only metals and silicates could form solids, so the _______________ planets grew slowly.
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