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GLY150: INTRODUCTION TO OCEANOGRAPHY


University of North Carolina Wilmington

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Lecture Outline

Scientific Methods, Origin of Solar System and Earth


I. Scientific Methods

II. Origin of Universe, Solar System, Earth

III. The Earth in the Solar System

Planet 

Radius [km]

Mass 1=Earth

Density [g/cm3] 

Distance from Sun [AU]

Rotation [hours, days]

Ts [k]

Atmos. Gases

Sun

695000

329000

1.41

0.0

 

6000

 

Mercury

2439

0.055

5.43

0.39

58.6d

450

Na

Venus

6051

0.815

5.24

0.72

-243d

283 

CO2, N

Earth

6370

1.000

5.51

1.00

23.94h

250

N,O

Mars

3390

0.107

3.93

1.52

24.62h

220 

CO2,N,Ar

Jupiter

71600

317.8

1.33

5.2

9.3h

105 

H,He,CH4,NH3

Saturn

60300

95.20

0.68

9.54

10.5h 

75 

H,He,CH4,NH3

Uranus

24100

14.5

1.60

19.18 

-17.24h 

50 

H,He,CH4

Neptune 

22500

17.2

1.65

30.07

16h

40 

H,CH4,He?

Pluto

~1140

0.002

0.5

39.44

6.4d 

40 

CH4

1K=-273C, Ts=surface temperature, A.U.=Astronomical Unit, negative rotation period indicates rotation opposite to orbit direction about the sun.

IV. Earth's Interior Structure


Some helpful links relevant to these lectures:
Ocean Planet
Views of the Solar System
Origin of Earth's ocean and atmosphere


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