Uni

t 3, S

lide

3.2.

44—

Oce

an S

cien

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Sequ

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6–8

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Session 1.10The Puzzling Case of the Daily Rains

Uni

t 1, S

lide

1.10

.1—

Oce

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Sequ

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6–8

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1.10

x.x

1.10

1.10Answer for DAY

☀ ☁☁♒♒♒♒♒♒Ocean

65ºF18ºC

Air

Land80ºF27ºC

65˚F18˚C

80˚F27˚C

Uni

t 1, S

lide

1.10

.2—

Oce

an S

cien

ces

Sequ

ence

6–8

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ccc

c

Uni

t 1, S

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1.10

.3—

Oce

an S

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Sequ

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6–8

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1.10Answer for NIGHT

☁☁♒♒♒♒♒♒Ocean

65ºF18ºC

Air

Land80ºF27ºC

65˚F18˚C

55˚F13˚C

cc

cc

c

c

1.10Answer for NIGHT 1.10

Uni

t 1, S

lide

1.10

.4—

Oce

an S

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Sequ

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6–8

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Costa Rica: Near the Equator

�

1.10

Uni

t 1, S

lide

1.10

.5—

Oce

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Sequ

ence

6–8

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Morning: Clear

x.x

1.10Morning: Clear 1.10Afternoon: Clouds

Uni

t 1, S

lide

1.10

.6—

Oce

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Sequ

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6–8

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Late Afternoon: Rain

1.10

Uni

t 1, S

lide

1.10

.7—

Oce

an S

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Sequ

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6–8

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Evening: Clearing

x.x

1.10 Evening: Clearing 1.10

Uni

t 3, S

lide

1.10

.8—

Oce

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Sequ

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x.x

Unit 1, Slide 1.10.9—Ocean Sciences Sequence 6–8 © 2014 The Regents of the University of California

Night: Clear 1.10

Session 2.1xxxxxCarbon

Uni

t 3, S

lide

3.2.

53—

Oce

an S

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Sequ

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6–8

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x.x

x.x

1.10

Uni

t 1, S

lide

1.10

.10—

Oce

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Sequ

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Key Concept

•added to liquid water, some of the water molecules at the surface evaporate into the air as water vapor.

•taken away from water vapor, some of the water molecules condense into liquid water.

If enough heat energy is –

1.10

Session 1.1xxxxxCarbon

x.xKey

Concept

Uni

t 1, S

lide

1.10

.11—

Oce

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Sequ

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1.10

Evaporation and condensation move heat energy around Earth. Without this, Earth would be much hotter in some places and much colder in others.

Key Concept

Uni

t 1, S

lide

1.10

.11—

Oce

an S

cien

ces

Sequ

ence

6–8

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