ASTR 102 - TEST - MC08 & SA&TF

What percentage of the mass of the solar nebula consisted of elements other than hydrogen and helium?
A) 0 percent
B) 0.1 percent
C) 2 percent
D) 20 percent
E) 80 percent

C) 2 percent

Where did the elements heavier than hydrogen and helium come from?
A) They were produced in the Big Bang.
B) They evolved from hydrogen and helium shortly after the Big Bang.
C) They were produced inside stars.
D) They were produced inside dense interstel

C) They were produced inside stars.

Why did the solar nebula heat up as it collapsed?
A) Nuclear fusion occurring in the core of the protosun produced energy that heated the nebula.
B) As the cloud shrank, its gravitational potential energy was converted to kinetic energy and then into ther

B) As the cloud shrank, its gravitational potential energy was converted to kinetic energy and then into thermal energy.

Why did the solar nebula flatten into a disk?
A) The interstellar cloud from which the solar nebula formed was originally somewhat flat.
B) The force of gravity pulled the material downward into a flat disk.
C) As the nebula cooled, the gas and dust settl

D) It flattened as a natural consequence of collisions between particles in the nebula, changing random motions into more orderly ones.

What happened during the accretion phase of the early solar system?
A) Atoms and molecules in the gas bonded together and solidified.
B) Particles grew by colliding and sticking together.
C) The solar nebula differentiated into metals inside of the frost

B) Particles grew by colliding and sticking together.

According to our theory of solar system formation, why do all the planets orbit the Sun in the same direction and in nearly the same plane?
A) The original solar nebula happened to be disk-shaped by chance.
B) Any planets that once orbited in the opposite

C) The laws of conservation of energy and conservation of angular momentum ensure that any rotating, collapsing cloud will end up as a spinning disk.

Which of the following lists the ingredients of the solar nebula from highest to lowest percentage of mass of the nebula?
A) light gases (H, He), hydrogen compounds (H2O, CH4, NH3), rocks, metals
B) hydrogen compounds (H2O, CH4, NH3), light gases (H, He),

A) light gases (H, He), hydrogen compounds (H2O, CH4, NH3), rocks, metals

What percentage of the solar nebula's mass consisted of hydrogen and helium gases?
A) 0.5 percent
B) 5 percent
C) 50 percent
D) 98 percent
E) 100 percent

D) 98 percent

What percentage of the solar nebula's mass consisted of rocky material?
A) 0 percent
B) 0.4 percent
C) 2 percent
D) 20 percent
E) 80 percent

B) 0.4 percent

What kind of material in the solar nebula could remain solid at temperatures as high as 1,500 K, such as existed in the inner regions of the nebula?
A) rocks
B) metals
C) silicon-based minerals
D) hydrogen compounds
E) molecules such as methane and ammoni

B) metals

What was the frost line of the solar system?
A) the distance from the Sun where temperatures were low enough for metals to condense, between the Sun and the present-day orbit of Mercury
B) the distance from the Sun where temperatures were low enough for r

C) the distance from the Sun where temperatures were low enough for hydrogen compounds to condense into ices, between the present-day orbits of Mars and Jupiter

Why are the inner planets made of denser materials than the outer planets?
A) The Sun's gravity pulled denser materials toward the inner part of the solar nebula, while lighter gases escaped more easily.
B) Denser materials were heavier and sank to the ce

C) In the inner part of the nebula only metals and rocks were able to condense because of the high temperatures, whereas hydrogen compounds, although more abundant, were only able to condense in the cooler outer regions.

Which of the following is the origin of almost all the large moons around the jovian planets?
A) They are captured asteroids.
B) They are captured comets.
C) They are captured planets.
D) They were formed by condensation and accretion in a disk of gas aro

D) They were formed by condensation and accretion in a disk of gas around the planet.

What is the most likely reason that there are no giant planets beyond Neptune?
A) Any planets forming beyond Neptune would have drifted out of the solar system due to the weakness of the Sun's gravity at this distance.
B) There was no material to create p

C) By the time planetesimals grew to a large enough mass to hold onto an atmosphere, the solar nebula had been blown away.

Observations of young stars (as well as theory) tell us that when the Sun was young the solar wind
A) was weaker than it is today.
B) was stronger than it is today.
C) was about the same strength as it is today. D) was nonexistent.
E) blew outward only al

B) was stronger than it is today.

Which of the following has not been detected around other stars in the Galaxy?
A) a collapsing nebula of gas
B) flattened, spinning disks
C) jovian planets
D) terrestrial planets
E) strong stellar winds

D) terrestrial planets

At first, the Sun's present-day rotation seems to contradict the prediction of the nebular theory because
A) the theory predicts that the axis of rotation should not be perpendicular to the orbital plane of the planets, but it is.
B) the axis of rotation

D) the theory predicts that the Sun should have been rotating fast when it formed, but the actual rotation
is fairly slow.

According to our theory of solar system formation, why does the Sun rotate slowly today?
A) The Sun once rotated much faster, but it transferred angular momentum to charged particles caught in its magnetic field and then blew the particles away with its s

A) The Sun once rotated much faster, but it transferred angular momentum to charged particles caught in its magnetic field and then blew the particles away with its strong solar wind.

Which of the following are relatively unchanged fragments from the early period of planet building in the solar system?
A) the moons of Mars
B) asteroids
C) Kuiper belt comets
D) Oort cloud comets
E) All of the above

E) All of the above

According to the nebular theory, what are asteroids and comets?
A) They are the shattered remains of collisions between planets.
B) They are the shattered remains of collisions between moons.
C) They are leftover planetesimals that never accreted into pla

C) They are leftover planetesimals that never accreted into planets.

According to the nebular theory, how did the Kuiper belt form?
A) It is material left over from the interstellar cloud that never contracted with the rest of the gases to form the solar nebula.
B) It is made of planetesimals that formed beyond Neptune's o

B) It is made of planetesimals that formed beyond Neptune's orbit and never accreted to form a planet.

According to the nebular theory, how did the Oort cloud form?
A) It is material left over from the interstellar cloud that never contracted with the rest of the gases to form the solar nebula.
B) It is made of planetesimals that formed beyond Neptune's or

E) It is made of planetesimals formed in the outer solar system that were flung into distant orbits by encounters with the jovian planets.

According to our theory of solar system formation, why do we find some exceptions to the general rules and patterns of the planets?
A) Our theory is not quite correct because it cannot explain these exceptions.
B) Most of the exceptions are the result of

B) Most of the exceptions are the result of giant impacts.

According to our theory of solar system formation, what is Pluto?
A) Pluto is a terrestrial planet that was shot out from the inner solar system to its present location.
B) Pluto is a terrestrial planet that happened to form at a large distance from the S

D) Pluto is a large Kuiper-belt comet.

Based on our current theory of Earth's formation, the water we drink comes from
A) ice that condensed in the solar nebula in the region where Earth formed.
B) chemical reactions that occurred in Earth's crust after Earth formed.
C) chemical reactions that

E) comets that impacted Earth.

The heavy bombardment phase of the solar system lasted
A) several million years.
B) several tens of millions of years.
C) several hundreds of millions of years.
D) about a billion years.
E) to the present time.

C) several hundreds of millions of years.

Which of the following is not evidence supporting the giant impact theory for the formation of the Moon?
A) Computer simulations show that the Moon could really have formed in this way.
B) The composition of the Moon is similar to that of Earth's outer la

D) Scientists have found several meteorites that appear to be the remains of the object that caused the giant impact.

Which of the following puzzles in the solar system cannot be explained by a giant impact event?
A) the formation of the Moon
B) the large metallic core of Mercury
C) the backward rotation of Venus
D) the extreme axis tilt of Uranus
E) the orbit of Triton

E) the orbit of Triton in the opposite direction to Neptune's rotation

The nebular theory of the formation of the solar system successfully predicts all but one of the following. Which one does the theory not predict?
A) Planets orbit around the Sun in nearly circular orbits in a flattened disk.
B) the compositional differen

C) the equal number of terrestrial and jovian planets

The age of our solar system is approximately A) 10,000 years.
B) 3.8 million years.
C) 4.6 million years.
D) 4.6 billion years.
E) 14 billion years.

D) 4.6 billion years.

The age of the solar system can be established by radioactive dating of
A) the oldest Earth rocks.
B) the oldest rocks on the Moon.
C) the oldest meteorites.
D) the atmosphere of Mars.
E) It hasn't been done yet, but the age of the solar system could be o

C) the oldest meteorites.

What do meteorites reveal about the solar system?
A) They reveal that meteorites are much older than the comets and planets.
B) Nothing, because they come from other star systems.
C) They reveal that the solar system once contained 10 planets.
D) They rev

D) They reveal that the age of the solar system is approximately 4.6 billion years.

Suppose you find a rock that contains some potassium-40 (half-life of 1.3 billion years). You measure the amount and determine that there are 5 grams of potassium-40 in the rock. By measuring the amount of its decay product (argon-40) present in the rock,

C) 3.9 billion years

In essence, the nebular theory holds that ________.
A) our solar system formed from the collapse of an interstellar cloud of gas and dust
B) nebulae are clouds of gas and dust in space
C) the planets each formed from the collapse of its own separate nebul

A) our solar system formed from the collapse of an interstellar cloud of gas and dust

According to modern science, what was the approximate chemical composition of the solar nebula?
A) 50% hydrogen and helium, 50% everything else
B) 98% hydrogen and helium, 2% everything else
C) 98% hydrogen, 2% helium
D) roughly equal proportions of hydro

B) 98% hydrogen and helium, 2% everything else

The terrestrial planets are made almost entirely of elements heavier than hydrogen and helium. According to modern science, where did these elements come from?
A) They were produced by stars that lived and died before our solar system was born.
B) They we

A) They were produced by stars that lived and died before our solar system was born.

According to our theory of solar system formation, what three major changes occurred in the solar nebula as it shrank in size?
A) It got hotter, its rate of rotation increased, and it flattened into a disk.
B) Its mass, temperature, and density all increa

A) It got hotter, its rate of rotation increased, and it flattened into a disk.

Which of the following types of material can condense into what we call ice at low temperatures?
A) hydrogen and helium
B) rock
C) metal
D) hydrogen compounds

D) hydrogen compounds

According to our present theory of solar system formation, which of the following lists the major ingredients of the solar nebula in order from the most abundant to the least abundant?
A) hydrogen compounds; hydrogen and helium gas; metal; rock
B) hydroge

C) hydrogen and helium gas; hydrogen compounds; rock; metal

What do we mean by the frost line when we discuss the formation of planets in the solar nebula?
A) It is a circle at a particular distance from the Sun, beyond which the temperature was low enough for ices to condense.
B) It is another way of stating the

A) It is a circle at a particular distance from the Sun, beyond which the temperature was low enough for ices to condense.

What do we mean by accretion in the context of planet formation?
A) the formation of moons around planets
B) the growth of planetesimals from smaller solid particles that collided and stuck together C) the solidification of ices, rocks, and metal from the

B) the growth of planetesimals from smaller solid particles that collided and stuck together

According to our present theory of solar system formation, why were solid planetesimals able to grow larger in the outer solar system than in the inner solar system?
A) because the Sun's gravity was stronger in the outer solar system, allowing more solid

B) because only metal and rock could condense in the inner solar system, while ice also condensed in the outer solar system

According to our basic scenario of solar system formation, why do the jovian planets have numerous large moons?
A) As the growing jovian planets captured gas from the solar nebula, the gas formed swirling disks around them, and moons formed from condensat

A) As the growing jovian planets captured gas from the solar nebula, the gas formed swirling disks around them, and moons formed from condensation accretion within these disks.

According to our theory of solar system formation, what are asteroids and comets?
A) the shattered remains of collisions between planets
B) chunks of rock or ice that condensed after the planets and moons finished forming
C) chunks of rock or ice that wer

D) leftover planetesimals that never accreted into planets

According to our theory of solar system formation, where did the comets of the Oort cloud form?
A) in the inner solar system
B) far beyond the orbit of Pluto
C) in the region of the jovian planets
D) in the asteroid belt

C) in the region of the jovian planets

What do we mean by the period of heavy bombardment in the context of the history of our solar system?
A) the first few hundred million years after the planets formed, which is when most impact craters were formed
B) the time before planetesimals finished

A) the first few hundred million years after the planets formed, which is when most impact craters were formed

What is the giant impact hypothesis for the origin of the Moon?
A) The Moon formed when two gigantic asteroids collided with one another.
B) The Moon originally was about the same size as Earth, but a giant impact blasted most of it away so that it ended

C) The Moon formed from material blasted out of the Earth's mantle and crust by the impact of a Mars- size object.

Suppose you start with 1 kilogram of a radioactive substance that has a half-life of 10 years. Which of the following statements will be true after 20 years pass?
A) You'll have 0.25 kilogram of the radioactive substance remaining.
B) All the material wil

A) You'll have 0.25 kilogram of the radioactive substance remaining.

According to modern scientific dating techniques, approximately how old is the solar system?
A) 10,000 years
B) 4.6 million years
C) 4.5 billion years
D) 14 billion years

C) 4.5 billion years

Which of the following best explains why we can rule out the idea that planets are usually formed by near- collisions between stars?
A) Studies of the trajectories of nearby stars relative to the Sun show that the Sun is not in danger of a near-collision

B) Stellar near-collisions are far too rare to explain all the planets now known to orbit nearby stars.

According to our modern science, which of the following best explains why the vast majority of the mass of our solar system consists of hydrogen and helium gas?
A) Hydrogen and helium are the most common elements throughout the universe, because they were

A) Hydrogen and helium are the most common elements throughout the universe, because they were the only elements present when the universe was young.

According to our theory of solar system formation, which law best explains why the central regions of the solar nebula got hotter as the nebula shrank in size?
A) the law of conservation of angular momentum
B) Newton's third law
C) the two laws of thermal

D) the law of conservation of energy

According to our theory of solar system formation, which law best explains why the solar nebula spun faster as it shrank in size?
A) the law of conservation of angular momentum
B) the law of conservation of energy
C) the law of universal gravitation
D) Ei

A) the law of conservation of angular momentum

According to our present theory of solar system formation, which of the following best explains why the solar nebula ended up with a disk shape as it collapsed?
A) It was fairly flat to begin with, and retained this flat shape as it collapsed.
B) The forc

D) It flattened as a natural consequence of collisions between particles in the nebula.

What is the primary basis upon which we divide the ingredients of the solar nebula into four categories (hydrogen/helium; hydrogen compound; rock; metal)?
A) the temperatures at which various materials will condense from gaseous form to solid form B) the

A) the temperatures at which various materials will condense from gaseous form to solid form

According to our present theory of solar system formation, which of the following statements about the growth of terrestrial and jovian planets is not true?
A) Both types of planet begun with planetesimals growing through the process of accretion, but onl

B) The jovian planets began from planetesimals made only of ice, while the terrestrial planets began from planetesimals made only of rock and metal.

Many meteorites appear to have formed very early in the solar system's history. How do these meteorites support our theory about how the terrestrial planets formed?
A) The meteorites sizes are just what we'd expect if metal and rock condensed and accreted

B) The meteorites appearance and composition is just what we'd expect if metal and rock condensed and accreted as our theory suggests.

According to present understanding, which of the following statements about the solar wind is not true?
A) It is even stronger today than it was when the Sun was young.
B) It helped in the transfer of angular momentum from the young Sun to particles that

A) It is even stronger today than it was when the Sun was young.

According to our present theory of solar system formation, how did Earth end up with enough water to make oceans?
A) The water was mixed in the other materials in the planetesimals that accreted at our distance from the Sun.
B) The water was formed by che

C) The water was brought to the forming Earth by planetesimals that accreted beyond the orbit of Mars.

According to our present theory of solar system formation, which of the following objects now reside quite far from the place where they formed originally?
A) Oort cloud comets
B) Kuiper belt comets
C) asteroids of the asteroid belt
D) the terrestrial pla

A) Oort cloud comets

What is the primary reason that astronomers suspect that some jovian moons were captured into their current orbits?
A) Some moons have a composition that differs from the composition of the planets.
B) Astronomers have observed moons being captured.
C) So

D) Some moons have orbits that are "backwards" (compared to their planet's rotation) or highly inclined to their planet's equator.

Which of the following is not a line of evidence supporting the hypothesis that our Moon formed as a result of a giant impact?
A) The Pacific Ocean appears to be a large craterprobably the one made by the giant impact.
B) Computer simulations show that th

A) The Pacific Ocean appears to be a large craterprobably the one made by the giant impact.

Why are terrestrial planets denser than jovian planets?
A) Only dense materials could condense in the inner solar nebula.
B) The Sun's gravity gathered dense materials into the inner solar system.
C) Gravity compresses terrestrial planets to a higher degr

A) Only dense materials could condense in the inner solar nebula.

Suppose you find a rock that contains 10 micrograms of radioactive potassium-40, which has a half-life of 1. 25 billion years. By measuring the amount of its decay product (argon-40) present in the rock, you conclude that there must have been 80 microgram

C) 3.75 billion years

How do scientists determine the age of the solar system?
A) radiometric dating of Moon rocks
B) radiometric dating of the oldest Earth rocks
C) radiometric dating of meteorites
D) Theoretical calculations tell us how long it has taken the planets to evolv

C) radiometric dating of meteorites

The region of our solar system between Mercury and Mars has very few asteroids, while the region between Mars and Jupiter has many asteroids. Based on what you have learned, what is the most likely explanation for the lack of asteroids between Mercury and

A) There were very few planetary leftovers in this region, because most of the solid material was accreted by the terrestrial planets as the planets formed.

About 2% of our solar nebula consisted of elements besides hydrogen and helium. However, the very first generation of star systems in the universe probably consisted only of hydrogen and helium. Which of the following statements is most likely to have bee

A) There were no comets or asteroids in these first-generation star systems.

All the planets in the solar system rotate in the same direction as they orbit the Sun.

False

As viewed from above Earth's North Pole, all of the planets orbit the Sun in the same (counterclockwise) direction.

True

The more massive planets in the solar system tend to be less dense than the lower mass planets.

True

Within the frost line, planetesimals were composed entirely of rock and outside the frost line planetesimals were composed entirely of ice.

False

Impacts were extremely common in the young solar system but no longer occur today.

False

Earth's atmosphere resulted from the impact of icy planetesimals that originated in the outer regions of the Solar System.

True

The Moon probably formed at the same time that Earth formed, rather like the formation of a double planet.

False

Some radioactive isotopes found in meteorites suggest that the solar system may have been formed shortly after a supernova occurred nearby.

True

Based on our theory of how our own solar system formed, we would expect that other solar systems would be quite common.

True

Nebular theory predicts that other solar systems that formed in the same way should also have 8 planets.

False

Briefly summarize the observed patterns of motion in our solar system that are consistent with the nebular theory .

(a) All planets orbit the Sun counterclockwise when seen from above Earth's North Pole.
(b) All planetary orbits lie nearly in the same plane.
(c) Almost all planets travel on nearly circular orbits.
(d) The spacing between planetary orbits increases with

List at least three of the notable exceptions to the general patterns of the solar system.
Several possibilities:

(a) Mercury and Pluto have large orbital eccentricities and inclinations.
(b) The rotational axes of Uranus and Pluto are substantially tilted.
(c) Venus rotates backward, that is, clockwise.
(d) Unlike other terrestrial planets, Earth has a large Moon.
(

Suppose the entire solar nebula had cooled to a very low temperature before the solar wind cleared it away. Do you think Earth would be the same? Why or why not?

Ices would have condensed in the inner solar system, significantly increasing the size and mass (or possibly number) of terrestrial planets. Water and other hydrogen compounds would be much more abundant.

Suppose the planet Jupiter had never formed. How do you think the distribution of asteroids and comets in our solar system would be different? Explain.

If Jupiter had never existed, its gravity would not have prevented asteroidal material from accreting into a single planet outside of Mars. Comets would not have been flung into the Oort cloud or completely out of the solar system to as great a degree (th

Explain why the early Earth did not form with water, and how it gained it later in its formation.

Earth, and all terrestrial planets, formed inside the frost line from rocky and metallic planetesimals. The temperature of the solar nebula was too hot for water ice to exist and Earth was too small to hold onto a substantial atmosphere of hot gases. Eart

Briefly describe the modern theory of how our Moon formed.

The Moon formed from a giant impact of a Mars-size object with Earth. This impact blasted material into Earth orbit that eventually coalesced to form the Moon.

Suppose you discovered a meteorite that contains small amounts of potassium-40, which has a half-life of 1.3 billion years, and its decay product argon-40. You determine that 1/16 of the original potassium-40 remains; the other 15/16 has decayed into argo

To reach a fraction of 1/16, the meteorite has been through four half-lives, which means it is 4 � 1.3 billion = 5.2 billion years old. Since this is older than the solar system, it is probably a rock from interstellar space.

Explain how the age of a rock can be determined by radiometric dating.

The minerals in rocks contain small amounts of radioactive isotopes (for example carbon-14 or potassium-40). Over time, these parent isotopes decay into a different, stable element, the daughter isotope. By precisely counting the number of parent and daug

If we were to re-run the formation of the solar system, what would likely be the same and what would likely be different?

As with our solar system, planets would likely orbit in a thin disk, with small, dense planets close to the Sun and larger, jovian-like planets further away because these properties are due to the cumulative effects of cloud flattening during collapse and

Process of Science: A scientific theory must produce testable hypotheses that are then evaluated when data are available. What testable hypotheses does nebular theory predict? Describe two hypotheses about solar systems that come from nebular theory that

1. Larger planets should be in the outer solar system.
2. Planets should orbit in the same direction.
3. Planets should lie in approximately the same plane.