Page 207 - NS-2 Textbook
P. 207

Earth's Oceanographic History





          Our study of oceanography will begm with a discussion   oxygen. Because the hydrogen was lightel; much of it es-
          of  the  origin  of  Earth  and  its  seas.  Where  did  it  all   caped into space, ,,,,hile  the heavier oxygen atoms vvere
          begin-how and why? A basic idea of how our planet      retained in the atmosphere by gravity. Gradually, poison-
          Earth began is  essential in our. study of the life-giving   ous ammonia and methane gases in the atmosphere were
          seas. More about the scientific theory of the formation of   dissipated by the S,m as both it and Earth cooled. Slowly,
          the universe and the solar system is given in the astron-  the atmosphere cooled enough to cause the water ,;apor in
          omy unit (unit 4) of this text.                        the air to condense and return to the surface in the form of
                                                                 rain. Falling on Earth's hot surface, some water hissed into
                                                                 steam, joined with new water vapor brought to the surface
                    FORMATION  OF THE  OCEANS
                                                                 by volcanoes, and rose to be condensed and fall again and
          Modern science has given scientists a good idea of how   again as rain and, later, as snow.
          Earth began. This study is a part of astronomy called C08-  This continuous precipitation (rain and snow) prob-
          lIIologlj,  the science concerned with the nature of the uni-  ably went on for thousands, maybe millions, of years. Fi-
          verse and its origin. Scientists who study cosmology are   nally, about 4 billion years ago, Earth had cooled to about
          called cosmologists.                                   its present size and temperature. Lighter granite (granitic
             Cosmologists believe that what is now our solar sys-  rocks) had risen to higher elevations on the surface, and
          tem (the Sun, the planets, and their moons) began about   the heavier basalt (basaltic rocks) sank, creating high and
          4.5  billion years  ago  as  a  large  cloud of gas  and dust.   low areas. Eventually most of the low spots in the crust
          Gradually,  gravity  and  centripetal  forces  caused  this   filled ·with rain,vater. These gigantic ,vater pools eventu-
          cloud to spin and take the shape of a huge disk, with the   ally  formed  the  world  ocean-not  in  the  same  geo-
          infant Sun in its center. From time to time, eddies, s'\vids}   graphic shape we see the oceans today but, nevertheless,
          and collisions occurred in this disk, causing a number of   covering about 70 percent of Earth's surface.
          smaller clusters of materials to separate and whirl in or-  TIle cycle of evaporation and condensation continues
          bits  arolmd  the  large  cluster forming  the  S,m.  One  of   today, though now only a small percentage of the vapor
          these swirling masses became the planet Earth.         ascending into the ahnosphere COTIleS fronl volcanoes and
             After millions of years of increasing pressure and tem-  other cracks in the Earth. Most of the water vapor today
          perature, metallic crystals of iron and nickel melted and   conles fron1 the ocean surface and trapped ground\vater,
          sank toward the core, or center, of the Earth. Because of the   which is heated and recycled by the S,m. Over millions of
          intense  heat  created  within  the  Earth  by  compression,   years, the oceans have overrun some coastal edges of the
          molten rock (magma) called lava  often broke through the   early continents as the result of ,vind and ,vater erosion,
          surface, either in large cracks in the Earth's crust or in ac-  earthquakes, and landslides in those areas. At the same
          tive volcanoes that expelled gases and solid materials. The   time, the buildup of polar icecaps has kept an almost con-
          hydrogen molecules, other gases, and water vapor that es-  stant an10lult of water in the seas.  Ours  is a continually
          caped from the Earth gradually rose. The Sun's rays acted   changmg geologic  world.  However,  these changes hap-
          on the released gases and soon distributed them arOlUld   pen too slowly to be seen in the lifetimes of humans, ex-
          the new planet to  form  an atmosphere.  Meanwhile,  the   cept in instances of violent natural change, such as  vol-
          Earth continued to contract into a lllore solid mass, devel-  ·canie eruption or massive earthquake.
          oping what is now the planet's crust.
             The intense heat created by the compression of the     THE  EARTH'S  CRUST:  CONTINENTAL DRIFT
          Earth continued to  cause thousands of volcanoes to bring
          lava and water vapor to  the surface. Radiation from the   Earth  is  made  up  of several  "shells,"  some,vhat like  a
          Sun also continued to form Earth's atmosphere by breaking   golf ball. Earth's core consists of two parts: a solid inner
          up water molecules into separate atoms of hydrogen and   core  of  nickel  and  iron  with  a  diameter  of  about  860


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