SlideShare a Scribd company logo
Chapter 10 Review Clickers
© 2014 Pearson Education, Inc.
The Cosmic Perspective
Seventh Edition
Planetary
Atmospheres:
Earth and the Other
Terrestrial Worlds
© 2014 Pearson Education, Inc.
Chapter 10
What are the main constituents of Earth's
atmosphere?
a) hydrogen and helium
b) nitrogen and oxygen
c) oxygen and carbon dioxide
d) oxygen and carbon monoxide
e) water vapor and oxygen
© 2014 Pearson Education, Inc.
Chapter 10
What are the main constituents of Earth's
atmosphere?
a) hydrogen and helium
b) nitrogen and oxygen
c) oxygen and carbon dioxide
d) oxygen and carbon monoxide
e) water vapor and oxygen
© 2014 Pearson Education, Inc.
Chapter 10
Why is atmospheric pressure less on top of a
mountain than at sea level?
a) It is cooler in the mountains.
b) Denser air sinks to sea level; the air on mountains
is lighter.
c) The pressure at every height in the atmosphere
equals the weight of the air above it.
d) none of the above
© 2014 Pearson Education, Inc.
Chapter 10
Why is atmospheric pressure less on top of a
mountain than at sea level?
a) It is cooler in the mountains.
b) Denser air sinks to sea level; the air on mountains
is lighter.
c) The pressure at every height in the atmosphere
equals the weight of the air above it.
d) none of the above
© 2014 Pearson Education, Inc.
Chapter 10
If there was no greenhouse effect, Earth
a) would be warmer than it is today.
b) would have a thicker atmosphere.
c) would be colder than freezing.
d) would have no protection from ultraviolet radiation.
© 2014 Pearson Education, Inc.
Chapter 10
If there was no greenhouse effect, Earth
a) would be warmer than it is today.
b) would have a thicker atmosphere.
c) would be colder than freezing.
d) would have no protection from ultraviolet radiation.
© 2014 Pearson Education, Inc.
Chapter 10
If Earth was more reflective (had a higher
albedo), what would happen to its temperature?
a) It would go up.
b) It would go down.
c) It wouldn't change.
© 2014 Pearson Education, Inc.
Chapter 10
If Earth was more reflective (had a higher
albedo), what would happen to its temperature?
a) It would go up.
b) It would go down.
c) It wouldn't change.
© 2014 Pearson Education, Inc.
Chapter 10
If Earth didn't have an atmosphere, what would
happen to its temperature?
a) It would go up a little.
b) It would go up a lot.
c) It would go down a little.
d) It would go down a lot.
e) It wouldn't change.
© 2014 Pearson Education, Inc.
Chapter 10
If Earth didn't have an atmosphere, what would
happen to its temperature?
a) It would go up a little.
b) It would go up a lot.
c) It would go down a little.
d) It would go down a lot.
e) It wouldn't change.
© 2014 Pearson Education, Inc.
Chapter 10
Which of the following correctly states the
layers of Earth's atmosphere from closest to the
surface to closest to space?
a) troposphere, stratosphere, exosphere, thermosphere
b) stratosphere, exosphere, thermosphere, troposphere
c) troposphere, stratosphere, thermosphere, exosphere
d) thermosphere, troposphere, stratosphere, exosphere
© 2014 Pearson Education, Inc.
Chapter 10
Which of the following correctly states the
layers of Earth's atmosphere from closest to the
surface to closest to space?
a) troposphere, stratosphere, exosphere, thermosphere
b) stratosphere, exosphere, thermosphere, troposphere
c) troposphere, stratosphere, thermosphere,
exosphere
d) thermosphere, troposphere, stratosphere, exosphere
© 2014 Pearson Education, Inc.
Chapter 10
Infrared radiation emitted by Earth's surface
a) heats the troposphere from below.
b) causes convection.
c) causes weather (storms).
d) all of the above
e) none of the above
© 2014 Pearson Education, Inc.
Chapter 10
Infrared radiation emitted by Earth's surface
a) heats the troposphere from below.
b) causes convection.
c) causes weather (storms).
d) all of the above
e) none of the above
© 2014 Pearson Education, Inc.
Chapter 10
The stratosphere is heated by
a) warm air rising from the troposphere.
b) ultraviolet light from the Sun.
c) convection.
d) X-rays.
e) all of the above
© 2014 Pearson Education, Inc.
Chapter 10
The stratosphere is heated by
a) warm air rising from the troposphere.
b) ultraviolet light from the Sun.
c) convection.
d) X-rays.
e) all of the above
© 2014 Pearson Education, Inc.
Chapter 10
The sky is blue because
a) of the reflection of the oceans.
b) blue is the color of oxygen gas.
c) blue is the color of nitrogen gas.
d) the blue light in sunlight scatters more than the red
light.
e) of clouds.
© 2014 Pearson Education, Inc.
Chapter 10
The sky is blue because
a) of the reflection of the oceans.
b) blue is the color of oxygen gas.
c) blue is the color of nitrogen gas.
d) the blue light in sunlight scatters more than the
red light.
e) of clouds.
© 2014 Pearson Education, Inc.
Chapter 10
What protects Earth from the high energy
particles shot from the Sun (the solar wind)?
a) the troposphere
b) the stratosphere
c) the exosphere
d) the magnetosphere
e) the Van Allen radiation belts
© 2014 Pearson Education, Inc.
Chapter 10
What protects Earth from the high energy
particles shot from the Sun (the solar wind)?
a) the troposphere
b) the stratosphere
c) the exosphere
d) the magnetosphere
e) the Van Allen radiation belts
© 2014 Pearson Education, Inc.
Chapter 10
What affects the global circulation pattern of
Earth's atmosphere?
a) hot air from the equator rising, cool air at the poles
falling
b) Earth's rotation
c) convection
d) coriolis forces
e) all of the above
© 2014 Pearson Education, Inc.
Chapter 10
What affects the global circulation pattern of
Earth's atmosphere?
a) hot air from the equator rising, cool air at the poles
falling
b) Earth's rotation
c) convection
d) coriolis forces
e) all of the above
© 2014 Pearson Education, Inc.
Chapter 10
What effects long-term climate change?
a) changes in the Sun's brightness
b) changes in Earth's reflectivity
c) change in the tilt of Earth's axis
d) changes is greenhouse gas abundance
e) all of the above
© 2014 Pearson Education, Inc.
Chapter 10
What effects long-term climate change?
a) changes in the Sun's brightness
b) changes in Earth's reflectivity
c) change in the tilt of Earth's axis
d) changes is greenhouse gas abundance
e) all of the above
© 2014 Pearson Education, Inc.
Chapter 10
What is the main source of the original
atmospheres of the terrestrial planets?
a) gas accreted from the solar nebula
b) comets
c) gas released from interior rocks (outgassing)
d) evaporation from ice
© 2014 Pearson Education, Inc.
Chapter 10
What is the main source of the original
atmospheres of the terrestrial planets?
a) gas accreted from the solar nebula
b) comets
c) gas released from interior rocks (outgassing)
d) evaporation from ice
© 2014 Pearson Education, Inc.
Chapter 10
Where did the hydrogen in Earth's atmosphere
go?
a) We never had any.
b) It escaped into space.
c) It dissolved in the oceans and was incorporated
into rocks.
d) none of the above
© 2014 Pearson Education, Inc.
Chapter 10
Where did the hydrogen in Earth's atmosphere
go?
a) We never had any.
b) It escaped into space.
c) It dissolved in the oceans and was incorporated
into rocks.
d) none of the above
© 2014 Pearson Education, Inc.
Chapter 10
Where did the carbon dioxide in Earth's
atmosphere go?
a) We never had any.
b) It escaped into space.
c) It dissolved in the oceans and was incorporated
into rocks.
d) none of the above
© 2014 Pearson Education, Inc.
Chapter 10
Where did the carbon dioxide in Earth's
atmosphere go?
a) We never had any.
b) It escaped into space.
c) It dissolved in the oceans and was incorporated
into rocks.
d) none of the above
© 2014 Pearson Education, Inc.
Chapter 10
Why do we think Mars was once warmer and
wetter?
a) It has plenty of volcanoes to outgas an atmosphere.
b) It doesn't have strong magnetic field to protect from
solar wind stripping.
c) There is evidence it once had liquid water. It is too
cold for that now.
d) all of the above
e) A and C
© 2014 Pearson Education, Inc.
Chapter 10
Why do we think Mars was once warmer and
wetter?
a) It has plenty of volcanoes to outgas an atmosphere.
b) It doesn't have strong magnetic field to protect from
solar wind stripping.
c) There is evidence it once had liquid water. It is too
cold for that now.
d) all of the above
e) A and C
© 2014 Pearson Education, Inc.
Chapter 10
What is the main reason that Venus is warmer
than Earth?
a) Venus is closer to the Sun than Earth.
b) Venus has a higher reflectivity than Earth.
c) Venus has a lower reflectivity than Earth.
d) The greenhouse effect is much higher on Venus
than on Earth.
e) Human presence on Earth has led to declining
temperatures.
© 2014 Pearson Education, Inc.
Chapter 10
What is the main reason that Venus is warmer
than Earth?
a) Venus is closer to the Sun than Earth.
b) Venus has a higher reflectivity than Earth.
c) Venus has a lower reflectivity than Earth.
d) The greenhouse effect is much higher on
Venus than on Earth.
e) Human presence on Earth has led to declining
temperatures.
© 2014 Pearson Education, Inc.
Chapter 10
Suppose we could magically replace Venus'
actual atmosphere with an atmosphere
identical to Earth's. Could liquid water exist
on its surface?
a) No, the runaway greenhouse effect would ensure that
liquid water would immediately evaporate.
b) No, the low pressure would ensure that liquid water
would immediately evaporate.
c) Yes, the surface temperature would be well below the
boiling point of water.
d) Yes, the conditions would be exactly as on Earth.
e) Yes, but only at the poles.
© 2014 Pearson Education, Inc.
Chapter 10
Suppose we could magically replace Venus'
actual atmosphere with an atmosphere
identical to Earth's. Could liquid water exist
on its surface?
a) No, the runaway greenhouse effect would ensure that
liquid water would immediately evaporate.
b) No, the low pressure would ensure that liquid water
would immediately evaporate.
c) Yes, the surface temperature would be well below
the boiling point of water.
d) Yes, the conditions would be exactly as on Earth.
e) Yes, but only at the poles.
© 2014 Pearson Education, Inc.
Chapter 10
Suppose that, somehow, all plants died out.
What would happen to the oxygen in our
atmosphere?
a) The oxygen would eventually be used up in oxidation
reactions with the surface.
b) The oxygen would initially decrease, but as greenhouse
gases and temperature increased, it would recover to its
normal value.
c) The oxygen would increase as plants would not exist to
remove it from the atmosphere.
d) Plants grow by intaking carbon and therefore the oxygen
content would be unaffected.
© 2014 Pearson Education, Inc.
Chapter 10
Suppose that, somehow, all plants died out.
What would happen to the oxygen in our
atmosphere?
a) The oxygen would eventually be used up in oxidation
reactions with the surface.
b) The oxygen would initially decrease, but as greenhouse
gases and temperature increased, it would recover to its
normal value.
c) The oxygen would increase as plants would not exist to
remove it from the atmosphere.
d) Plants grow by intaking carbon and therefore the oxygen
content would be unaffected.
© 2014 Pearson Education, Inc.
Chapter 10
Surprising discovery? - A planet in another
solar system that has an Earth-like atmosphere
with plentiful oxygen, but no life of any kind.
a) Plausible. Life requires far more than oxygen to exist.
b) Plausible. The oxygen may have been transported
there by cometary impacts.
c) Implausible. Oxygen is highly reactive and its
presence in an atmosphere suggests replenishment
by a living organism of some sort.
d) Implausible. Oxygen is essential to life.
© 2014 Pearson Education, Inc.
Chapter 10
Surprising discovery? - A planet in another
solar system that has an Earth-like atmosphere
with plentiful oxygen, but no life of any kind.
a) Plausible. Life requires far more than oxygen to exist.
b) Plausible. The oxygen may have been transported
there by cometary impacts.
c) Implausible. Oxygen is highly reactive and its
presence in an atmosphere suggests
replenishment by a living organism of some sort.
d) Implausible. Oxygen is essential to life.

More Related Content

What's hot

08 lecture outline
08 lecture outline08 lecture outline
08 lecture outline
Asma Said,PhD
 
Geochemistry chapt 1
Geochemistry chapt 1Geochemistry chapt 1
Geochemistry chapt 1
BelisumaHirpa
 
HPU NCS2200 Universe Formation 1
HPU NCS2200 Universe Formation 1HPU NCS2200 Universe Formation 1
HPU NCS2200 Universe Formation 1
cooperk2
 
Young And Hot Big Bang
Young And Hot Big BangYoung And Hot Big Bang
Young And Hot Big Bang
Gilroy ECA
 
The solar system - Phoenix University Guide
The solar system - Phoenix University GuideThe solar system - Phoenix University Guide
The solar system - Phoenix University Guide
phoenixuniversityguide
 
Origin of universe
Origin of universe Origin of universe
Origin of universe
P.K. Mani
 
Geochemistry chapt 1
Geochemistry chapt 1Geochemistry chapt 1
Geochemistry chapt 1
BelisumaHirpa
 
Chapter 19 – formation of the universe
Chapter 19 – formation of the universeChapter 19 – formation of the universe
Chapter 19 – formation of the universeAnnie cox
 
Ch09 Tutorial
Ch09 TutorialCh09 Tutorial
Ch09 TutorialJT T
 
History of earth Chapter for SEE Nepal
History of earth Chapter for SEE NepalHistory of earth Chapter for SEE Nepal
History of earth Chapter for SEE Nepal
Anjan Nepal
 
Big Bang And Starlight Travel
Big  Bang And  Starlight  TravelBig  Bang And  Starlight  Travel
Big Bang And Starlight Travel
Larry Kisner
 
Astonishing Astronomy 101 - Chapter 6
Astonishing Astronomy 101 - Chapter 6Astonishing Astronomy 101 - Chapter 6
Astonishing Astronomy 101 - Chapter 6
Don R. Mueller, Ph.D.
 
7th Grade Chapter 5 Lesson 1
7th Grade Chapter 5 Lesson 17th Grade Chapter 5 Lesson 1
7th Grade Chapter 5 Lesson 1
MRS.KDUNCAN
 
C. the solar system
C. the solar systemC. the solar system
C. the solar system
Jan Crisides Corrado
 
Earths formation
Earths formationEarths formation
Earths formation
FelixCarbonell2
 
Origin of the earth
Origin of the earthOrigin of the earth
origin of earth
origin of earthorigin of earth
origin of earth
Madhavan Natarajan
 
Module 1 origin and systems of earth
Module 1 origin and systems of earthModule 1 origin and systems of earth
Module 1 origin and systems of earth
brionesako
 
FROM BIG BANG TO THE PRESENT TIME
FROM BIG BANG TO THE PRESENT TIMEFROM BIG BANG TO THE PRESENT TIME
FROM BIG BANG TO THE PRESENT TIME
Nepal Flying Labs
 

What's hot (20)

08 lecture outline
08 lecture outline08 lecture outline
08 lecture outline
 
Geochemistry chapt 1
Geochemistry chapt 1Geochemistry chapt 1
Geochemistry chapt 1
 
HPU NCS2200 Universe Formation 1
HPU NCS2200 Universe Formation 1HPU NCS2200 Universe Formation 1
HPU NCS2200 Universe Formation 1
 
Young And Hot Big Bang
Young And Hot Big BangYoung And Hot Big Bang
Young And Hot Big Bang
 
The solar system - Phoenix University Guide
The solar system - Phoenix University GuideThe solar system - Phoenix University Guide
The solar system - Phoenix University Guide
 
Origin of universe
Origin of universe Origin of universe
Origin of universe
 
Geochemistry chapt 1
Geochemistry chapt 1Geochemistry chapt 1
Geochemistry chapt 1
 
Galaxies
GalaxiesGalaxies
Galaxies
 
Chapter 19 – formation of the universe
Chapter 19 – formation of the universeChapter 19 – formation of the universe
Chapter 19 – formation of the universe
 
Ch09 Tutorial
Ch09 TutorialCh09 Tutorial
Ch09 Tutorial
 
History of earth Chapter for SEE Nepal
History of earth Chapter for SEE NepalHistory of earth Chapter for SEE Nepal
History of earth Chapter for SEE Nepal
 
Big Bang And Starlight Travel
Big  Bang And  Starlight  TravelBig  Bang And  Starlight  Travel
Big Bang And Starlight Travel
 
Astonishing Astronomy 101 - Chapter 6
Astonishing Astronomy 101 - Chapter 6Astonishing Astronomy 101 - Chapter 6
Astonishing Astronomy 101 - Chapter 6
 
7th Grade Chapter 5 Lesson 1
7th Grade Chapter 5 Lesson 17th Grade Chapter 5 Lesson 1
7th Grade Chapter 5 Lesson 1
 
C. the solar system
C. the solar systemC. the solar system
C. the solar system
 
Earths formation
Earths formationEarths formation
Earths formation
 
Origin of the earth
Origin of the earthOrigin of the earth
Origin of the earth
 
origin of earth
origin of earthorigin of earth
origin of earth
 
Module 1 origin and systems of earth
Module 1 origin and systems of earthModule 1 origin and systems of earth
Module 1 origin and systems of earth
 
FROM BIG BANG TO THE PRESENT TIME
FROM BIG BANG TO THE PRESENT TIMEFROM BIG BANG TO THE PRESENT TIME
FROM BIG BANG TO THE PRESENT TIME
 

Viewers also liked

12 review clickers
12 review clickers12 review clickers
12 review clickers
Asma Said,PhD
 
Technology Driven Differentiated Instruction #KCDTTL
Technology Driven Differentiated Instruction #KCDTTLTechnology Driven Differentiated Instruction #KCDTTL
Technology Driven Differentiated Instruction #KCDTTL
Vicki Davis
 
Gaga quiz
Gaga quizGaga quiz
Gaga quiz
Willish Brunt
 
Irregular verbs
Irregular verbsIrregular verbs
Irregular verbs
Charisse Marie Verallo
 
Irregular nouns sva
Irregular nouns svaIrregular nouns sva
Irregular nouns sva
Charisse Marie Verallo
 
Teoria do campo cristalino
Teoria do campo cristalinoTeoria do campo cristalino
Teoria do campo cristalino
João Paulo Costa
 
FRENCH: LES NOMBRES DE ZÉRO À UN MILLION
FRENCH: LES NOMBRES DE  ZÉRO À UN MILLIONFRENCH: LES NOMBRES DE  ZÉRO À UN MILLION
FRENCH: LES NOMBRES DE ZÉRO À UN MILLION
M, Michelle Jeannite
 
Educational Data Mining in Program Evaluation: Lessons Learned
Educational Data Mining in Program Evaluation: Lessons LearnedEducational Data Mining in Program Evaluation: Lessons Learned
Educational Data Mining in Program Evaluation: Lessons Learned
Kerry Rice
 
Infographic Recipes 4 Students
Infographic Recipes 4 StudentsInfographic Recipes 4 Students
Infographic Recipes 4 Students
Lisa Johnson
 
Історія розвитку обчислювальної техніки. Покоління ЕОМ
Історія розвитку обчислювальної техніки. Покоління ЕОМІсторія розвитку обчислювальної техніки. Покоління ЕОМ
Історія розвитку обчислювальної техніки. Покоління ЕОМ
Yulia Vlasenko
 
นำเสนอกองสาธารณสุข 58 new
นำเสนอกองสาธารณสุข 58 newนำเสนอกองสาธารณสุข 58 new
นำเสนอกองสาธารณสุข 58 new
yahapop
 
Eha 3002
Eha 3002Eha 3002
Eha 3002
yahapop
 
Етапи створення веб сайтів
Етапи створення веб сайтівЕтапи створення веб сайтів
Етапи створення веб сайтів
Yulia Vlasenko
 
02 reading quiz_clickers
02 reading quiz_clickers02 reading quiz_clickers
02 reading quiz_clickers
Asma Said,PhD
 
06 lecture outline
06 lecture outline06 lecture outline
06 lecture outline
Asma Said,PhD
 
04 reading quiz clickers
04 reading quiz clickers04 reading quiz clickers
04 reading quiz clickers
Asma Said,PhD
 
06 review clickers_cooney
06 review clickers_cooney06 review clickers_cooney
06 review clickers_cooney
Asma Said,PhD
 
13 review clickers
13 review clickers13 review clickers
13 review clickers
Asma Said,PhD
 
02 lecture outline
02 lecture outline02 lecture outline
02 lecture outline
Asma Said,PhD
 
07 review clickers
07 review clickers07 review clickers
07 review clickers
Asma Said,PhD
 

Viewers also liked (20)

12 review clickers
12 review clickers12 review clickers
12 review clickers
 
Technology Driven Differentiated Instruction #KCDTTL
Technology Driven Differentiated Instruction #KCDTTLTechnology Driven Differentiated Instruction #KCDTTL
Technology Driven Differentiated Instruction #KCDTTL
 
Gaga quiz
Gaga quizGaga quiz
Gaga quiz
 
Irregular verbs
Irregular verbsIrregular verbs
Irregular verbs
 
Irregular nouns sva
Irregular nouns svaIrregular nouns sva
Irregular nouns sva
 
Teoria do campo cristalino
Teoria do campo cristalinoTeoria do campo cristalino
Teoria do campo cristalino
 
FRENCH: LES NOMBRES DE ZÉRO À UN MILLION
FRENCH: LES NOMBRES DE  ZÉRO À UN MILLIONFRENCH: LES NOMBRES DE  ZÉRO À UN MILLION
FRENCH: LES NOMBRES DE ZÉRO À UN MILLION
 
Educational Data Mining in Program Evaluation: Lessons Learned
Educational Data Mining in Program Evaluation: Lessons LearnedEducational Data Mining in Program Evaluation: Lessons Learned
Educational Data Mining in Program Evaluation: Lessons Learned
 
Infographic Recipes 4 Students
Infographic Recipes 4 StudentsInfographic Recipes 4 Students
Infographic Recipes 4 Students
 
Історія розвитку обчислювальної техніки. Покоління ЕОМ
Історія розвитку обчислювальної техніки. Покоління ЕОМІсторія розвитку обчислювальної техніки. Покоління ЕОМ
Історія розвитку обчислювальної техніки. Покоління ЕОМ
 
นำเสนอกองสาธารณสุข 58 new
นำเสนอกองสาธารณสุข 58 newนำเสนอกองสาธารณสุข 58 new
นำเสนอกองสาธารณสุข 58 new
 
Eha 3002
Eha 3002Eha 3002
Eha 3002
 
Етапи створення веб сайтів
Етапи створення веб сайтівЕтапи створення веб сайтів
Етапи створення веб сайтів
 
02 reading quiz_clickers
02 reading quiz_clickers02 reading quiz_clickers
02 reading quiz_clickers
 
06 lecture outline
06 lecture outline06 lecture outline
06 lecture outline
 
04 reading quiz clickers
04 reading quiz clickers04 reading quiz clickers
04 reading quiz clickers
 
06 review clickers_cooney
06 review clickers_cooney06 review clickers_cooney
06 review clickers_cooney
 
13 review clickers
13 review clickers13 review clickers
13 review clickers
 
02 lecture outline
02 lecture outline02 lecture outline
02 lecture outline
 
07 review clickers
07 review clickers07 review clickers
07 review clickers
 

Similar to 10 review clickers

14 review clickers
14 review clickers14 review clickers
14 review clickers
Asma Said,PhD
 
17 clicker questions
17 clicker questions17 clicker questions
17 clicker questions
Asma Said,PhD
 
09 clicker questions
09 clicker questions09 clicker questions
09 clicker questions
Asma Said,PhD
 
1. What drives currents deep in the oceanA. Differences in water .docx
1. What drives currents deep in the oceanA. Differences in water .docx1. What drives currents deep in the oceanA. Differences in water .docx
1. What drives currents deep in the oceanA. Differences in water .docx
mansonagnus
 
EXERCISES ABOUT THE SUBSYSTEM.pptx
EXERCISES ABOUT THE SUBSYSTEM.pptxEXERCISES ABOUT THE SUBSYSTEM.pptx
EXERCISES ABOUT THE SUBSYSTEM.pptx
Juvy41
 
Ch08 Tutorial
Ch08 TutorialCh08 Tutorial
Ch08 TutorialJT T
 
science 8 3 review exam.pptxdddddddddddd
science 8 3 review exam.pptxddddddddddddscience 8 3 review exam.pptxdddddddddddd
science 8 3 review exam.pptxdddddddddddd
JESSANDEPEDRO
 
1. How many time zones are there across the world2. Which map wou.docx
1. How many time zones are there across the world2. Which map wou.docx1. How many time zones are there across the world2. Which map wou.docx
1. How many time zones are there across the world2. Which map wou.docx
corbing9ttj
 
How sun and ocean interact in water cycle.pptx
How sun and ocean interact in water cycle.pptxHow sun and ocean interact in water cycle.pptx
How sun and ocean interact in water cycle.pptx
VivekRaval22
 
Science NAT Review.pptx
Science NAT Review.pptxScience NAT Review.pptx
Science NAT Review.pptx
TeddyCatimbang3
 
10 clicker questions
10 clicker questions10 clicker questions
10 clicker questions
Asma Said,PhD
 
05 review clickers
05 review clickers05 review clickers
05 review clickers
Asma Said,PhD
 
02 review clickers
02 review clickers02 review clickers
02 review clickers
Asma Said,PhD
 
13 review clickers
13 review clickers13 review clickers
13 review clickers
Asma Said,PhD
 
26 clicker questions
26 clicker questions26 clicker questions
26 clicker questions
Asma Said,PhD
 
04 clicker questions
04 clicker questions04 clicker questions
04 clicker questions
Asma Said,PhD
 
15 clicker questions
15 clicker questions15 clicker questions
15 clicker questions
Asma Said,PhD
 
15 clicker questions
15 clicker questions15 clicker questions
15 clicker questions
Asma Said,PhD
 
Climate change101 esip_2011
Climate change101 esip_2011Climate change101 esip_2011
Climate change101 esip_2011
Rebreid
 
BALASABAS, THRECIA GAILE B..docx.pdf
BALASABAS, THRECIA GAILE B..docx.pdfBALASABAS, THRECIA GAILE B..docx.pdf
BALASABAS, THRECIA GAILE B..docx.pdf
PatrickJhonBinasBala
 

Similar to 10 review clickers (20)

14 review clickers
14 review clickers14 review clickers
14 review clickers
 
17 clicker questions
17 clicker questions17 clicker questions
17 clicker questions
 
09 clicker questions
09 clicker questions09 clicker questions
09 clicker questions
 
1. What drives currents deep in the oceanA. Differences in water .docx
1. What drives currents deep in the oceanA. Differences in water .docx1. What drives currents deep in the oceanA. Differences in water .docx
1. What drives currents deep in the oceanA. Differences in water .docx
 
EXERCISES ABOUT THE SUBSYSTEM.pptx
EXERCISES ABOUT THE SUBSYSTEM.pptxEXERCISES ABOUT THE SUBSYSTEM.pptx
EXERCISES ABOUT THE SUBSYSTEM.pptx
 
Ch08 Tutorial
Ch08 TutorialCh08 Tutorial
Ch08 Tutorial
 
science 8 3 review exam.pptxdddddddddddd
science 8 3 review exam.pptxddddddddddddscience 8 3 review exam.pptxdddddddddddd
science 8 3 review exam.pptxdddddddddddd
 
1. How many time zones are there across the world2. Which map wou.docx
1. How many time zones are there across the world2. Which map wou.docx1. How many time zones are there across the world2. Which map wou.docx
1. How many time zones are there across the world2. Which map wou.docx
 
How sun and ocean interact in water cycle.pptx
How sun and ocean interact in water cycle.pptxHow sun and ocean interact in water cycle.pptx
How sun and ocean interact in water cycle.pptx
 
Science NAT Review.pptx
Science NAT Review.pptxScience NAT Review.pptx
Science NAT Review.pptx
 
10 clicker questions
10 clicker questions10 clicker questions
10 clicker questions
 
05 review clickers
05 review clickers05 review clickers
05 review clickers
 
02 review clickers
02 review clickers02 review clickers
02 review clickers
 
13 review clickers
13 review clickers13 review clickers
13 review clickers
 
26 clicker questions
26 clicker questions26 clicker questions
26 clicker questions
 
04 clicker questions
04 clicker questions04 clicker questions
04 clicker questions
 
15 clicker questions
15 clicker questions15 clicker questions
15 clicker questions
 
15 clicker questions
15 clicker questions15 clicker questions
15 clicker questions
 
Climate change101 esip_2011
Climate change101 esip_2011Climate change101 esip_2011
Climate change101 esip_2011
 
BALASABAS, THRECIA GAILE B..docx.pdf
BALASABAS, THRECIA GAILE B..docx.pdfBALASABAS, THRECIA GAILE B..docx.pdf
BALASABAS, THRECIA GAILE B..docx.pdf
 

More from Asma Said,PhD

Cosmology CSUDH Telescopes
Cosmology CSUDH TelescopesCosmology CSUDH Telescopes
Cosmology CSUDH Telescopes
Asma Said,PhD
 
Cosmology CSUDH
Cosmology CSUDHCosmology CSUDH
Cosmology CSUDH
Asma Said,PhD
 
24 clicker questions
24 clicker questions24 clicker questions
24 clicker questions
Asma Said,PhD
 
24 lecture outline
24 lecture outline24 lecture outline
24 lecture outline
Asma Said,PhD
 
S2 review clickers
S2 review clickersS2 review clickers
S2 review clickers
Asma Said,PhD
 
S2 lecture outline
S2 lecture outlineS2 lecture outline
S2 lecture outline
Asma Said,PhD
 
22 clicker questions
22 clicker questions22 clicker questions
22 clicker questions
Asma Said,PhD
 
22 lecture outline
22 lecture outline22 lecture outline
22 lecture outline
Asma Said,PhD
 
14 lecture outline
14 lecture outline14 lecture outline
14 lecture outline
Asma Said,PhD
 
19 clicker questions
19 clicker questions19 clicker questions
19 clicker questions
Asma Said,PhD
 
19 lecture outline 3
19 lecture outline 319 lecture outline 3
19 lecture outline 3
Asma Said,PhD
 
13 lecture outline
13 lecture outline13 lecture outline
13 lecture outline
Asma Said,PhD
 
15 lecture outline
15 lecture outline15 lecture outline
15 lecture outline
Asma Said,PhD
 
12 review clickers
12 review clickers12 review clickers
12 review clickers
Asma Said,PhD
 
11 lecture outline 2
11 lecture outline 211 lecture outline 2
11 lecture outline 2
Asma Said,PhD
 
09 lecture outline
09 lecture outline09 lecture outline
09 lecture outline
Asma Said,PhD
 
07 review clickers
07 review clickers07 review clickers
07 review clickers
Asma Said,PhD
 
06 lecture outline
06 lecture outline06 lecture outline
06 lecture outline
Asma Said,PhD
 
In class problems fall 2016
In class problems fall 2016In class problems fall 2016
In class problems fall 2016
Asma Said,PhD
 
Why study physics
Why study physicsWhy study physics
Why study physics
Asma Said,PhD
 

More from Asma Said,PhD (20)

Cosmology CSUDH Telescopes
Cosmology CSUDH TelescopesCosmology CSUDH Telescopes
Cosmology CSUDH Telescopes
 
Cosmology CSUDH
Cosmology CSUDHCosmology CSUDH
Cosmology CSUDH
 
24 clicker questions
24 clicker questions24 clicker questions
24 clicker questions
 
24 lecture outline
24 lecture outline24 lecture outline
24 lecture outline
 
S2 review clickers
S2 review clickersS2 review clickers
S2 review clickers
 
S2 lecture outline
S2 lecture outlineS2 lecture outline
S2 lecture outline
 
22 clicker questions
22 clicker questions22 clicker questions
22 clicker questions
 
22 lecture outline
22 lecture outline22 lecture outline
22 lecture outline
 
14 lecture outline
14 lecture outline14 lecture outline
14 lecture outline
 
19 clicker questions
19 clicker questions19 clicker questions
19 clicker questions
 
19 lecture outline 3
19 lecture outline 319 lecture outline 3
19 lecture outline 3
 
13 lecture outline
13 lecture outline13 lecture outline
13 lecture outline
 
15 lecture outline
15 lecture outline15 lecture outline
15 lecture outline
 
12 review clickers
12 review clickers12 review clickers
12 review clickers
 
11 lecture outline 2
11 lecture outline 211 lecture outline 2
11 lecture outline 2
 
09 lecture outline
09 lecture outline09 lecture outline
09 lecture outline
 
07 review clickers
07 review clickers07 review clickers
07 review clickers
 
06 lecture outline
06 lecture outline06 lecture outline
06 lecture outline
 
In class problems fall 2016
In class problems fall 2016In class problems fall 2016
In class problems fall 2016
 
Why study physics
Why study physicsWhy study physics
Why study physics
 

Recently uploaded

(May 29th, 2024) Advancements in Intravital Microscopy- Insights for Preclini...
(May 29th, 2024) Advancements in Intravital Microscopy- Insights for Preclini...(May 29th, 2024) Advancements in Intravital Microscopy- Insights for Preclini...
(May 29th, 2024) Advancements in Intravital Microscopy- Insights for Preclini...
Scintica Instrumentation
 
Cancer cell metabolism: special Reference to Lactate Pathway
Cancer cell metabolism: special Reference to Lactate PathwayCancer cell metabolism: special Reference to Lactate Pathway
Cancer cell metabolism: special Reference to Lactate Pathway
AADYARAJPANDEY1
 
Anemia_ different types_causes_ conditions
Anemia_ different types_causes_ conditionsAnemia_ different types_causes_ conditions
Anemia_ different types_causes_ conditions
muralinath2
 
Circulatory system_ Laplace law. Ohms law.reynaults law,baro-chemo-receptors-...
Circulatory system_ Laplace law. Ohms law.reynaults law,baro-chemo-receptors-...Circulatory system_ Laplace law. Ohms law.reynaults law,baro-chemo-receptors-...
Circulatory system_ Laplace law. Ohms law.reynaults law,baro-chemo-receptors-...
muralinath2
 
Lateral Ventricles.pdf very easy good diagrams comprehensive
Lateral Ventricles.pdf very easy good diagrams comprehensiveLateral Ventricles.pdf very easy good diagrams comprehensive
Lateral Ventricles.pdf very easy good diagrams comprehensive
silvermistyshot
 
plant biotechnology Lecture note ppt.pptx
plant biotechnology Lecture note ppt.pptxplant biotechnology Lecture note ppt.pptx
plant biotechnology Lecture note ppt.pptx
yusufzako14
 
GBSN - Biochemistry (Unit 5) Chemistry of Lipids
GBSN - Biochemistry (Unit 5) Chemistry of LipidsGBSN - Biochemistry (Unit 5) Chemistry of Lipids
GBSN - Biochemistry (Unit 5) Chemistry of Lipids
Areesha Ahmad
 
Unveiling the Energy Potential of Marshmallow Deposits.pdf
Unveiling the Energy Potential of Marshmallow Deposits.pdfUnveiling the Energy Potential of Marshmallow Deposits.pdf
Unveiling the Energy Potential of Marshmallow Deposits.pdf
Erdal Coalmaker
 
general properties of oerganologametal.ppt
general properties of oerganologametal.pptgeneral properties of oerganologametal.ppt
general properties of oerganologametal.ppt
IqrimaNabilatulhusni
 
Citrus Greening Disease and its Management
Citrus Greening Disease and its ManagementCitrus Greening Disease and its Management
Citrus Greening Disease and its Management
subedisuryaofficial
 
THE IMPORTANCE OF MARTIAN ATMOSPHERE SAMPLE RETURN.
THE IMPORTANCE OF MARTIAN ATMOSPHERE SAMPLE RETURN.THE IMPORTANCE OF MARTIAN ATMOSPHERE SAMPLE RETURN.
THE IMPORTANCE OF MARTIAN ATMOSPHERE SAMPLE RETURN.
Sérgio Sacani
 
FAIR & AI Ready KGs for Explainable Predictions
FAIR & AI Ready KGs for Explainable PredictionsFAIR & AI Ready KGs for Explainable Predictions
FAIR & AI Ready KGs for Explainable Predictions
Michel Dumontier
 
Nutraceutical market, scope and growth: Herbal drug technology
Nutraceutical market, scope and growth: Herbal drug technologyNutraceutical market, scope and growth: Herbal drug technology
Nutraceutical market, scope and growth: Herbal drug technology
Lokesh Patil
 
Structural Classification Of Protein (SCOP)
Structural Classification Of Protein  (SCOP)Structural Classification Of Protein  (SCOP)
Structural Classification Of Protein (SCOP)
aishnasrivastava
 
Large scale production of streptomycin.pptx
Large scale production of streptomycin.pptxLarge scale production of streptomycin.pptx
Large scale production of streptomycin.pptx
Cherry
 
Body fluids_tonicity_dehydration_hypovolemia_hypervolemia.pptx
Body fluids_tonicity_dehydration_hypovolemia_hypervolemia.pptxBody fluids_tonicity_dehydration_hypovolemia_hypervolemia.pptx
Body fluids_tonicity_dehydration_hypovolemia_hypervolemia.pptx
muralinath2
 
insect morphology and physiology of insect
insect morphology and physiology of insectinsect morphology and physiology of insect
insect morphology and physiology of insect
anitaento25
 
EY - Supply Chain Services 2018_template.pptx
EY - Supply Chain Services 2018_template.pptxEY - Supply Chain Services 2018_template.pptx
EY - Supply Chain Services 2018_template.pptx
AlguinaldoKong
 
Orion Air Quality Monitoring Systems - CWS
Orion Air Quality Monitoring Systems - CWSOrion Air Quality Monitoring Systems - CWS
Orion Air Quality Monitoring Systems - CWS
Columbia Weather Systems
 
extra-chromosomal-inheritance[1].pptx.pdfpdf
extra-chromosomal-inheritance[1].pptx.pdfpdfextra-chromosomal-inheritance[1].pptx.pdfpdf
extra-chromosomal-inheritance[1].pptx.pdfpdf
DiyaBiswas10
 

Recently uploaded (20)

(May 29th, 2024) Advancements in Intravital Microscopy- Insights for Preclini...
(May 29th, 2024) Advancements in Intravital Microscopy- Insights for Preclini...(May 29th, 2024) Advancements in Intravital Microscopy- Insights for Preclini...
(May 29th, 2024) Advancements in Intravital Microscopy- Insights for Preclini...
 
Cancer cell metabolism: special Reference to Lactate Pathway
Cancer cell metabolism: special Reference to Lactate PathwayCancer cell metabolism: special Reference to Lactate Pathway
Cancer cell metabolism: special Reference to Lactate Pathway
 
Anemia_ different types_causes_ conditions
Anemia_ different types_causes_ conditionsAnemia_ different types_causes_ conditions
Anemia_ different types_causes_ conditions
 
Circulatory system_ Laplace law. Ohms law.reynaults law,baro-chemo-receptors-...
Circulatory system_ Laplace law. Ohms law.reynaults law,baro-chemo-receptors-...Circulatory system_ Laplace law. Ohms law.reynaults law,baro-chemo-receptors-...
Circulatory system_ Laplace law. Ohms law.reynaults law,baro-chemo-receptors-...
 
Lateral Ventricles.pdf very easy good diagrams comprehensive
Lateral Ventricles.pdf very easy good diagrams comprehensiveLateral Ventricles.pdf very easy good diagrams comprehensive
Lateral Ventricles.pdf very easy good diagrams comprehensive
 
plant biotechnology Lecture note ppt.pptx
plant biotechnology Lecture note ppt.pptxplant biotechnology Lecture note ppt.pptx
plant biotechnology Lecture note ppt.pptx
 
GBSN - Biochemistry (Unit 5) Chemistry of Lipids
GBSN - Biochemistry (Unit 5) Chemistry of LipidsGBSN - Biochemistry (Unit 5) Chemistry of Lipids
GBSN - Biochemistry (Unit 5) Chemistry of Lipids
 
Unveiling the Energy Potential of Marshmallow Deposits.pdf
Unveiling the Energy Potential of Marshmallow Deposits.pdfUnveiling the Energy Potential of Marshmallow Deposits.pdf
Unveiling the Energy Potential of Marshmallow Deposits.pdf
 
general properties of oerganologametal.ppt
general properties of oerganologametal.pptgeneral properties of oerganologametal.ppt
general properties of oerganologametal.ppt
 
Citrus Greening Disease and its Management
Citrus Greening Disease and its ManagementCitrus Greening Disease and its Management
Citrus Greening Disease and its Management
 
THE IMPORTANCE OF MARTIAN ATMOSPHERE SAMPLE RETURN.
THE IMPORTANCE OF MARTIAN ATMOSPHERE SAMPLE RETURN.THE IMPORTANCE OF MARTIAN ATMOSPHERE SAMPLE RETURN.
THE IMPORTANCE OF MARTIAN ATMOSPHERE SAMPLE RETURN.
 
FAIR & AI Ready KGs for Explainable Predictions
FAIR & AI Ready KGs for Explainable PredictionsFAIR & AI Ready KGs for Explainable Predictions
FAIR & AI Ready KGs for Explainable Predictions
 
Nutraceutical market, scope and growth: Herbal drug technology
Nutraceutical market, scope and growth: Herbal drug technologyNutraceutical market, scope and growth: Herbal drug technology
Nutraceutical market, scope and growth: Herbal drug technology
 
Structural Classification Of Protein (SCOP)
Structural Classification Of Protein  (SCOP)Structural Classification Of Protein  (SCOP)
Structural Classification Of Protein (SCOP)
 
Large scale production of streptomycin.pptx
Large scale production of streptomycin.pptxLarge scale production of streptomycin.pptx
Large scale production of streptomycin.pptx
 
Body fluids_tonicity_dehydration_hypovolemia_hypervolemia.pptx
Body fluids_tonicity_dehydration_hypovolemia_hypervolemia.pptxBody fluids_tonicity_dehydration_hypovolemia_hypervolemia.pptx
Body fluids_tonicity_dehydration_hypovolemia_hypervolemia.pptx
 
insect morphology and physiology of insect
insect morphology and physiology of insectinsect morphology and physiology of insect
insect morphology and physiology of insect
 
EY - Supply Chain Services 2018_template.pptx
EY - Supply Chain Services 2018_template.pptxEY - Supply Chain Services 2018_template.pptx
EY - Supply Chain Services 2018_template.pptx
 
Orion Air Quality Monitoring Systems - CWS
Orion Air Quality Monitoring Systems - CWSOrion Air Quality Monitoring Systems - CWS
Orion Air Quality Monitoring Systems - CWS
 
extra-chromosomal-inheritance[1].pptx.pdfpdf
extra-chromosomal-inheritance[1].pptx.pdfpdfextra-chromosomal-inheritance[1].pptx.pdfpdf
extra-chromosomal-inheritance[1].pptx.pdfpdf
 

10 review clickers

  • 1. Chapter 10 Review Clickers © 2014 Pearson Education, Inc. The Cosmic Perspective Seventh Edition Planetary Atmospheres: Earth and the Other Terrestrial Worlds
  • 2. © 2014 Pearson Education, Inc. Chapter 10 What are the main constituents of Earth's atmosphere? a) hydrogen and helium b) nitrogen and oxygen c) oxygen and carbon dioxide d) oxygen and carbon monoxide e) water vapor and oxygen
  • 3. © 2014 Pearson Education, Inc. Chapter 10 What are the main constituents of Earth's atmosphere? a) hydrogen and helium b) nitrogen and oxygen c) oxygen and carbon dioxide d) oxygen and carbon monoxide e) water vapor and oxygen
  • 4. © 2014 Pearson Education, Inc. Chapter 10 Why is atmospheric pressure less on top of a mountain than at sea level? a) It is cooler in the mountains. b) Denser air sinks to sea level; the air on mountains is lighter. c) The pressure at every height in the atmosphere equals the weight of the air above it. d) none of the above
  • 5. © 2014 Pearson Education, Inc. Chapter 10 Why is atmospheric pressure less on top of a mountain than at sea level? a) It is cooler in the mountains. b) Denser air sinks to sea level; the air on mountains is lighter. c) The pressure at every height in the atmosphere equals the weight of the air above it. d) none of the above
  • 6. © 2014 Pearson Education, Inc. Chapter 10 If there was no greenhouse effect, Earth a) would be warmer than it is today. b) would have a thicker atmosphere. c) would be colder than freezing. d) would have no protection from ultraviolet radiation.
  • 7. © 2014 Pearson Education, Inc. Chapter 10 If there was no greenhouse effect, Earth a) would be warmer than it is today. b) would have a thicker atmosphere. c) would be colder than freezing. d) would have no protection from ultraviolet radiation.
  • 8. © 2014 Pearson Education, Inc. Chapter 10 If Earth was more reflective (had a higher albedo), what would happen to its temperature? a) It would go up. b) It would go down. c) It wouldn't change.
  • 9. © 2014 Pearson Education, Inc. Chapter 10 If Earth was more reflective (had a higher albedo), what would happen to its temperature? a) It would go up. b) It would go down. c) It wouldn't change.
  • 10. © 2014 Pearson Education, Inc. Chapter 10 If Earth didn't have an atmosphere, what would happen to its temperature? a) It would go up a little. b) It would go up a lot. c) It would go down a little. d) It would go down a lot. e) It wouldn't change.
  • 11. © 2014 Pearson Education, Inc. Chapter 10 If Earth didn't have an atmosphere, what would happen to its temperature? a) It would go up a little. b) It would go up a lot. c) It would go down a little. d) It would go down a lot. e) It wouldn't change.
  • 12. © 2014 Pearson Education, Inc. Chapter 10 Which of the following correctly states the layers of Earth's atmosphere from closest to the surface to closest to space? a) troposphere, stratosphere, exosphere, thermosphere b) stratosphere, exosphere, thermosphere, troposphere c) troposphere, stratosphere, thermosphere, exosphere d) thermosphere, troposphere, stratosphere, exosphere
  • 13. © 2014 Pearson Education, Inc. Chapter 10 Which of the following correctly states the layers of Earth's atmosphere from closest to the surface to closest to space? a) troposphere, stratosphere, exosphere, thermosphere b) stratosphere, exosphere, thermosphere, troposphere c) troposphere, stratosphere, thermosphere, exosphere d) thermosphere, troposphere, stratosphere, exosphere
  • 14. © 2014 Pearson Education, Inc. Chapter 10 Infrared radiation emitted by Earth's surface a) heats the troposphere from below. b) causes convection. c) causes weather (storms). d) all of the above e) none of the above
  • 15. © 2014 Pearson Education, Inc. Chapter 10 Infrared radiation emitted by Earth's surface a) heats the troposphere from below. b) causes convection. c) causes weather (storms). d) all of the above e) none of the above
  • 16. © 2014 Pearson Education, Inc. Chapter 10 The stratosphere is heated by a) warm air rising from the troposphere. b) ultraviolet light from the Sun. c) convection. d) X-rays. e) all of the above
  • 17. © 2014 Pearson Education, Inc. Chapter 10 The stratosphere is heated by a) warm air rising from the troposphere. b) ultraviolet light from the Sun. c) convection. d) X-rays. e) all of the above
  • 18. © 2014 Pearson Education, Inc. Chapter 10 The sky is blue because a) of the reflection of the oceans. b) blue is the color of oxygen gas. c) blue is the color of nitrogen gas. d) the blue light in sunlight scatters more than the red light. e) of clouds.
  • 19. © 2014 Pearson Education, Inc. Chapter 10 The sky is blue because a) of the reflection of the oceans. b) blue is the color of oxygen gas. c) blue is the color of nitrogen gas. d) the blue light in sunlight scatters more than the red light. e) of clouds.
  • 20. © 2014 Pearson Education, Inc. Chapter 10 What protects Earth from the high energy particles shot from the Sun (the solar wind)? a) the troposphere b) the stratosphere c) the exosphere d) the magnetosphere e) the Van Allen radiation belts
  • 21. © 2014 Pearson Education, Inc. Chapter 10 What protects Earth from the high energy particles shot from the Sun (the solar wind)? a) the troposphere b) the stratosphere c) the exosphere d) the magnetosphere e) the Van Allen radiation belts
  • 22. © 2014 Pearson Education, Inc. Chapter 10 What affects the global circulation pattern of Earth's atmosphere? a) hot air from the equator rising, cool air at the poles falling b) Earth's rotation c) convection d) coriolis forces e) all of the above
  • 23. © 2014 Pearson Education, Inc. Chapter 10 What affects the global circulation pattern of Earth's atmosphere? a) hot air from the equator rising, cool air at the poles falling b) Earth's rotation c) convection d) coriolis forces e) all of the above
  • 24. © 2014 Pearson Education, Inc. Chapter 10 What effects long-term climate change? a) changes in the Sun's brightness b) changes in Earth's reflectivity c) change in the tilt of Earth's axis d) changes is greenhouse gas abundance e) all of the above
  • 25. © 2014 Pearson Education, Inc. Chapter 10 What effects long-term climate change? a) changes in the Sun's brightness b) changes in Earth's reflectivity c) change in the tilt of Earth's axis d) changes is greenhouse gas abundance e) all of the above
  • 26. © 2014 Pearson Education, Inc. Chapter 10 What is the main source of the original atmospheres of the terrestrial planets? a) gas accreted from the solar nebula b) comets c) gas released from interior rocks (outgassing) d) evaporation from ice
  • 27. © 2014 Pearson Education, Inc. Chapter 10 What is the main source of the original atmospheres of the terrestrial planets? a) gas accreted from the solar nebula b) comets c) gas released from interior rocks (outgassing) d) evaporation from ice
  • 28. © 2014 Pearson Education, Inc. Chapter 10 Where did the hydrogen in Earth's atmosphere go? a) We never had any. b) It escaped into space. c) It dissolved in the oceans and was incorporated into rocks. d) none of the above
  • 29. © 2014 Pearson Education, Inc. Chapter 10 Where did the hydrogen in Earth's atmosphere go? a) We never had any. b) It escaped into space. c) It dissolved in the oceans and was incorporated into rocks. d) none of the above
  • 30. © 2014 Pearson Education, Inc. Chapter 10 Where did the carbon dioxide in Earth's atmosphere go? a) We never had any. b) It escaped into space. c) It dissolved in the oceans and was incorporated into rocks. d) none of the above
  • 31. © 2014 Pearson Education, Inc. Chapter 10 Where did the carbon dioxide in Earth's atmosphere go? a) We never had any. b) It escaped into space. c) It dissolved in the oceans and was incorporated into rocks. d) none of the above
  • 32. © 2014 Pearson Education, Inc. Chapter 10 Why do we think Mars was once warmer and wetter? a) It has plenty of volcanoes to outgas an atmosphere. b) It doesn't have strong magnetic field to protect from solar wind stripping. c) There is evidence it once had liquid water. It is too cold for that now. d) all of the above e) A and C
  • 33. © 2014 Pearson Education, Inc. Chapter 10 Why do we think Mars was once warmer and wetter? a) It has plenty of volcanoes to outgas an atmosphere. b) It doesn't have strong magnetic field to protect from solar wind stripping. c) There is evidence it once had liquid water. It is too cold for that now. d) all of the above e) A and C
  • 34. © 2014 Pearson Education, Inc. Chapter 10 What is the main reason that Venus is warmer than Earth? a) Venus is closer to the Sun than Earth. b) Venus has a higher reflectivity than Earth. c) Venus has a lower reflectivity than Earth. d) The greenhouse effect is much higher on Venus than on Earth. e) Human presence on Earth has led to declining temperatures.
  • 35. © 2014 Pearson Education, Inc. Chapter 10 What is the main reason that Venus is warmer than Earth? a) Venus is closer to the Sun than Earth. b) Venus has a higher reflectivity than Earth. c) Venus has a lower reflectivity than Earth. d) The greenhouse effect is much higher on Venus than on Earth. e) Human presence on Earth has led to declining temperatures.
  • 36. © 2014 Pearson Education, Inc. Chapter 10 Suppose we could magically replace Venus' actual atmosphere with an atmosphere identical to Earth's. Could liquid water exist on its surface? a) No, the runaway greenhouse effect would ensure that liquid water would immediately evaporate. b) No, the low pressure would ensure that liquid water would immediately evaporate. c) Yes, the surface temperature would be well below the boiling point of water. d) Yes, the conditions would be exactly as on Earth. e) Yes, but only at the poles.
  • 37. © 2014 Pearson Education, Inc. Chapter 10 Suppose we could magically replace Venus' actual atmosphere with an atmosphere identical to Earth's. Could liquid water exist on its surface? a) No, the runaway greenhouse effect would ensure that liquid water would immediately evaporate. b) No, the low pressure would ensure that liquid water would immediately evaporate. c) Yes, the surface temperature would be well below the boiling point of water. d) Yes, the conditions would be exactly as on Earth. e) Yes, but only at the poles.
  • 38. © 2014 Pearson Education, Inc. Chapter 10 Suppose that, somehow, all plants died out. What would happen to the oxygen in our atmosphere? a) The oxygen would eventually be used up in oxidation reactions with the surface. b) The oxygen would initially decrease, but as greenhouse gases and temperature increased, it would recover to its normal value. c) The oxygen would increase as plants would not exist to remove it from the atmosphere. d) Plants grow by intaking carbon and therefore the oxygen content would be unaffected.
  • 39. © 2014 Pearson Education, Inc. Chapter 10 Suppose that, somehow, all plants died out. What would happen to the oxygen in our atmosphere? a) The oxygen would eventually be used up in oxidation reactions with the surface. b) The oxygen would initially decrease, but as greenhouse gases and temperature increased, it would recover to its normal value. c) The oxygen would increase as plants would not exist to remove it from the atmosphere. d) Plants grow by intaking carbon and therefore the oxygen content would be unaffected.
  • 40. © 2014 Pearson Education, Inc. Chapter 10 Surprising discovery? - A planet in another solar system that has an Earth-like atmosphere with plentiful oxygen, but no life of any kind. a) Plausible. Life requires far more than oxygen to exist. b) Plausible. The oxygen may have been transported there by cometary impacts. c) Implausible. Oxygen is highly reactive and its presence in an atmosphere suggests replenishment by a living organism of some sort. d) Implausible. Oxygen is essential to life.
  • 41. © 2014 Pearson Education, Inc. Chapter 10 Surprising discovery? - A planet in another solar system that has an Earth-like atmosphere with plentiful oxygen, but no life of any kind. a) Plausible. Life requires far more than oxygen to exist. b) Plausible. The oxygen may have been transported there by cometary impacts. c) Implausible. Oxygen is highly reactive and its presence in an atmosphere suggests replenishment by a living organism of some sort. d) Implausible. Oxygen is essential to life.

Editor's Notes

  1. Answer: b) nitrogen and oxygen
  2. Answer: b) nitrogen and oxygen
  3. Answer: c) The pressure at every height in the atmosphere equals the weight of the air above it.
  4. Answer: c) The pressure at every height in the atmosphere equals the weight of the air above it.
  5. Answer: c) would be colder than freezing.
  6. Answer: c) would be colder than freezing.
  7. Answer: b) It would go down.
  8. Answer: b) It would go down.
  9. Answer: d) It would go down a lot.
  10. Answer: d) It would go down a lot.
  11. Answer: c) troposphere, stratosphere, thermosphere, exosphere
  12. Answer: c) troposphere, stratosphere, thermosphere, exosphere
  13. Answer: d) all of the above
  14. Answer: d) all of the above
  15. Answer: b) ultraviolet light from the Sun.
  16. Answer: b) ultraviolet light from the Sun.
  17. Answer: d) the blue light in sunlight scatters more than the red light.
  18. Answer: d) the blue light in sunlight scatters more than the red light.
  19. Answer: d) the magnetosphere
  20. Answer: d) the magnetosphere
  21. Answer: e) all of the above
  22. Answer: e) all of the above
  23. Answer: e) all of the above
  24. Answer: e) all of the above
  25. Answer: c) gas released from interior rocks (outgassing)
  26. Answer: c) gas released from interior rocks (outgassing)
  27. Answer: b) It escaped into space.
  28. Answer: b) It escaped into space.
  29. Answer: c) It dissolved in the oceans and was incorporated into rocks.
  30. Answer: c) It dissolved in the oceans and was incorporated into rocks.
  31. Answer: d) all of the above.
  32. Answer: d) all of the above.
  33. Answer: d) The greenhouse effect is much higher on Venus than on Earth.
  34. Answer: d) The greenhouse effect is much higher on Venus than on Earth.
  35. Answer: c) Yes, the surface temperature would be well below the boiling point of water.
  36. Answer: c) Yes, the surface temperature would be well below the boiling point of water.
  37. Answer: a) The oxygen would eventually be used up in oxidation reactions with the surface.
  38. Answer: a) The oxygen would eventually be used up in oxidation reactions with the surface.
  39. Answer: c) Implausible. Oxygen is highly reactive and its presence in an atmosphere suggests replenishment by a living organism of some sort.
  40. Answer: c) Implausible. Oxygen is highly reactive and its presence in an atmosphere suggests replenishment by a living organism of some sort.