Origins of the Ocean Planet

1. Origins of the Ocean Planet Resources from Garrison Textbook (2010)

2. It’s Only a Theory Laws: • Well supported explanations that describe a situation • Have been supported through observable and testable experiments • Considered facts Theories: • Cannot become laws • They explain a series of observations to try and explain the phenomenon or situation

3. It’s Only a Theory http://youtu.be/9Re8QxKZdm0

4. Objective 1 & 2 • Be able to describe how marine scientists conduct investigations • Be able to distinguish what information about the ocean is of utmost importance to us now-a-days and in the future

5. Earth is an Ocean World • Facts about the Ocean • 97% of Earth’s water is found in or near the ocean • < 3% is found on land, ice, groundwater, and all freshwater lakes/rivers • Functions of the Ocean • Moderate temperature • Influences weather • Nurtures life • Crucial natural resource (renewable)

6. Water Amounts by Location (Garrison, 2010)

7. Ocean Divisions • Imaginary divisions that compartmentalize the oceans and seas, by using continental boundaries • Truly the entire ocean (world ocean) is connected, the terms for the oceans is meant to simplify the compartmentalization

8. Ocean’s Size • 361 million km2 (square kilometers) = 139 million squared miles • Depth = 3,796 meters (12,451 feet) • Volume = 1.37 billion km3 (cubic kilometers) [329 million cubic miles] • Average temperature = 39OF • Mass = 1.41 billion billion metric tons

9. Earth Is an Ocean World Average ocean depth is 4 ½ times as great as average land elevation. (Garrison, 2010)

10. Proportion of Sea vs. Land (Garrison, 2010)

11. Comparison’s • On a planetary scale, the Earth’s ocean is insignificant in size • There is more water inside the Earth’s interior than there is in the ocean and atmosphere

12. S.T.E.M. Career Connection • Marine Geologists • Chemical Oceanographers • Physical Oceanographers • Climatologists • Marine Biologists • Marine Engineers

13. What do they do… • Marine Geologists • Study earth’s crust and composition • Chemical Oceanographers • Study the ocean’s chemical composition (gases/solids dissolved in the ocean) • Physical Oceanographers • Study of the waves, currents, and climate prediction • Climatologists • Determine the role the ocean play’s within the changes in the climate • Marine Biologists • Study the nature and distribution of marine organisms • Marine Engineers • Design and create structures utilized in the ocean

14. Studying what????? • Oceanography • is the study of the earth's oceans and their interlinked ecosystems , geological, chemicaland physical processes. • Geological oceanography • the study of geologic processes in the oceans (plate tectonics, coastal morphology) • Chemical oceanography • the study of the chemistry of the oceans • Meteorological oceanography • the study of the interaction between atmosphere and the oceans • Physical oceanography • the study of the physical attributes of the oceans (temperature-salinity structure, waves, tides, currents) • Biological oceanography • the study of the flora and fauna of the oceans

15. Three of the most prominent oceanographic institutions in the US: Lamont-Doherty Earth Observatory of Columbia University, NY Woods Hole Oceanographic Institute, Cape Code, MA (MIT) Scripps Institution of Oceanography, La Jolla CA (UC-San Diego)

16. Objective 3 • Describe how the study of the past can help us predict the future of our oceans

17. Understanding the Ocean Began with Voyaging for Trade and Exploration • Voyaging on water was important to many early civilizations. The Egyptians, Cretans, and Phoenicians were all skilled sailors. • Cartographers, or chart makers, recorded information about locations and landmarks and currents. • Today, charts are detailed graphic representations of water and water-related information. • The Library at Alexandria, in Egypt, was founded in the third century B.C. This library stored information on every area of human endeavor. • Eratosthenes of Cyrene was the second librarian at Alexandria. He was the first to calculate the circumference of Earth. He also invented a system of longitude and latitude. • The principles of celestial navigation were invented at the Library at Alexandria. (Garrison, 2010)

18. Objective 5 & 6 • Be able to describe how life begun in the ocean environment • Be able to describe the intercorrelation of studying the cosmos and the ocean

19. Stars and Seas • To understand the ocean, we need to understand how it formed and evolved through time. • Because the world ocean is the largest feature of Earth’s surface, scientists believe the origin of the ocean is linked to Earth’s origin. • The origin of Earth is linked to that of the solar system and the galaxies.

20. Earth Was Formed of Material Made in Stars • The universe apparently had a beginning called the big bang that occurred ~13.7 billion years ago. • All of the mass and energy of the universe was concentrated at a geometric point at the beginning of space and time, the moment when the expansion of the universe began. • We don’t know what initiated the expansion, but it continues today and will probably continue for billions of years, perhaps forever.

21. Stars and Planets are Contained within Galaxies Our Milky Way Galaxy pictured from afar. We’re inside and dust obscures our view, but this painting is a good guess about what our galaxy looks like, based on many different types of observations. Our solar system is a little more than half-way out from the center in one of the blue spiral arms.

22. Stars and Planets Are Contained within Galaxies • What do stars have to do with the ocean? • Most of the substance of Earth, its ocean, and all living things, was formed by stars. • Every chemical element heavier than hydrogen was manufactured and released into space by stars. • Our sun, like all normal stars, is powered by nuclear fusion.

23. Stars and Planets Are Contained within Galaxies A filament of hot gas erupts from the face of our sun. Like all normal stars, the sun is powered by nuclear fusion – the welding together of small atoms to make larger ones. The entire Earth could easily fit into this filament’s outstretched arms.

24. Stars Make Heavy Elements from Lighter Ones The origin of a solar system in the spiral arm of a galaxy. Our sun and its family of planets were formed in this way about 5 billion years ago.

25. Solar Systems Form by Accretion Planet-building in progress. Accretion of planets occurs when small particles clump into large masses.

26. Earth Accumulated in Layers Sorted by Density • How did Earth become density stratified? • Young Earth was probably homogeneous • Heat and gravitational pressure caused Earth to partially melt • Gravity then pulled the iron present into the center of Earth • This heated Earth further and lighter minerals migrated to Earth’s surface and formed the crust

27. Earth Accumulated in Layers Sorted by Density (top) The planet grew by the aggregation of particles. Meteors and asteroids bombarded the surface, heating the new planet and adding to its growing mass. At the time, Earth was composed of a homogeneous mixture of materials. (middle) Earth lost volume because of gravitational compression. High temperatures in the interior turned the inner Earth into a semisolid mass; dense iron (red drops) fell toward the center to form the core, while less dense silicates move outward. Friction generated by this movement heated Earth even more. (bottom) The result of density stratification is evident in the formation of an inner and outer core, a mantle, and the crust.

28. Earth Accumulated in Layers Sorted by Density • How did water and water vapor form on early Earth? • The Sun stripped away Earth’s first atmosphere • Gases, including water vapor, released by the process of out-gassing, replaced the first atmosphere. • Water vapor in the atmosphere condensed into clouds. • Eventually, the surface cooled enough for water to collect in basins.

29. Earth Accumulated in Layers Sorted by Density Comets may have delivered some of Earth’s surface water. Intense bombardment of the early Earth by large bodies – comets and asteroids – probably lasted until about 3.8 billion years ago.

30. Earth Accumulated in Layers Sorted by Density The early atmosphere was very different from the atmosphere today.

31. Life Probably Originated in the Ocean Fossil of a bacteria-like organism (with an artist’s reconstruction) that photosynthesized and released oxygen into the atmosphere. Among the oldest fossils ever discovered, this microscopic filament from northwestern Australia is about 3.5 billion years old.

32. What Will Be the Future of Earth? • How long can Earth exist? • Our Sun will begin to die in 5 billion years. • 6 billion years from now the sun will enter the red giant phase and will engulf the inner planets. • At that time, Earth will probably be recycled into component atoms. • See Figure 1.8 for a timeline of Earth.

33. What Will Be the Future of Earth?

34. Are There Other Ocean Worlds? • Where have scientists found evidence of water? • Europa • The gravitational pull of Jupiter twists Europa, cracking the ice crust and warming the interior. • In some areas the ice has broken into large pieces that have shifted away from one another but fit together like a jigsaw puzzle. • This suggests the ice crust is lubricated by slush or water. A global ocean greater in volume than Earth’s ocean may lie beneath the movable crust. It may also be salty - salinity has been detected by Galileo’s magnetometers.

35. Are There Other Ocean Worlds? In 2005, Europe’s Mars Express orbiter imaged a glacier in an unnamed crater in the vast plains of northern Mars. This 200 meter (656 foot) thick remnant of a larger ice sheet is shielded by the frosty shade of the crater walls.

36. Are There Other Ocean Worlds? • Where have scientists found evidence of water? • Titan – Saturn’s largest moon, may have an ocean of hydrocarbons. • Mars • Early in its history, Mars may have had a thick atmosphere of carbon-dioxide, much like the atmosphere of the early Earth. • An ocean may have existed on Mars about 3.2 billion years ago. • Over the eons, rocks on the Martian surface absorbed the carbon dioxide and the atmosphere grew thin and cold and the ocean disappeared

37. Resources Garrison, T. (2010). Oceanography: An invitation to marine science (7th ed.). Brooks & Cole: Australia