Friday, October 12, 2012

Atmosphere and Climate



Atmosphere and Climate

Origin of the Atmosphere

Since the creation of the Earth the atmosphere underwent many changes in different geological ages. It became more or less stable since 580 million years ago (Cambrian period). Geological changes shaped the present lithosphere and hydrosphere.
At the beginning the atmosphere probably had water vapour (60–70%), carbon dioxide (10–15%) and nitrogen (8–10%) but no oxygen. As the Earth cooled down from its very hot state, there was massive condensation of water vapour which resulted in incessant rainfall for thousands of years. The rainwater filled in the cavities of Earth’s surface forming seas, oceans and lakes.
Life forms first appeared in the seas some 3.5 billion years ago as blue–green algae. The evolution of plant life on Earth transformed the atmosphere. Plants assimilated carbon dioxide from the atmosphere for photosynthesis and in the process released oxygen into the atmosphere. The present atmosphere consists of nitrogen (78.08%), oxygen (20.95%), argon (0.93%) and carbon dioxide (0.33%).
The process of evolution went on—the living world appeared in the sequence: plants, animals and man. Some 5 million years ago man appeared last of all only when the atmosphere built enough stock of oxygen and the optimum environment for life forms prevailed.

The Climate of the Earth

The earth is a complex system in which the oceans, atmosphere and living species (biosphere) interact with one another and this has ultimately protected life on earth for about 3 billion years.
The earth has a unique mechanism for stabilising and controlling the global climate:
(i) The plants and animals balance carbon dioxide level of the atmosphere which in turn acts as a global thermostat rewriting earth’s temperature within optimum limits.
(ii) The ocean plankton (plant and animal species) plays important role in regulating global climate.
(iii) Sudden shifts in ocean current, e.g. gulf stream can initiate mini ice ages which last for centuries.
(iv) Tiny changes in the earth’s orbit, favoured by changes in the proportions of atmospheric gases, control the advance and retreat of glaciers. The mechanism with which carbon is handled helps in the stability of the earth’s climate.
Carbon, the backbone of biological chemistry, is the component of rock and in the form
of carbon dioxide, keeps the earth warm. With rise in carbon dioxide level in the atmosphere, say by a volcanic explosion or burning of fossil fuel, there is a corresponding increase of uptake of carbon dioxide by green plants from air and also by the oceans where it is turned into rock at the ocean floor. Similarly, if there is decrease of carbon dioxide in the atmosphere, there is less evaporation of sea water and less rainfall and carbon in the ocean rock in the floor burns through volcanoes and makes up the carbon dioxide deficiency in the atmosphere.
The earth swings back and forth between hot and cold periods with rise and fall of carbon dioxide level in the atmosphere. Thus during the dinosaur era some 100 million years ago carbon dioxide content was 4–5 times higher than to-day’s and the earth was warmer by about 5° C. But during the Ice Age about 18000 years ago carbon dioxide dropped to 60 per cent of its present level and the dinosaurs were extinct for lack of vegetation, i.e. their food.
The oceans provide another mechanism for governing climate. Covering 70 per cent of the planet, oceans act as a huge fly wheel in the earth’s machinery. As a huge reservoir of carbon (fixed as HCO3 mineral deposit on the ocean floor), the oceans regulate the carbon dioxide level and hence global climate. Ocean currents also play major role in setting long term climate patterns.

EVOLUTION OF THE EARTH



EVOLUTION OF THE EARTH

The planet earth initially was a barren, rocky and hot object with a thin atmosphere of hydrogen and helium. This is far from the present day picture of the earth. Hence, there must have been some events– processes, which may have caused this change from rocky, barren and hot earth to a beautiful planet with ample amount of water and conducive atmosphere favouring the existence of life
The earth has a layered structure.From the outermost end of the atmosphere to the to the centre of the earth, the material that existis not uniform. The atmospheric matter has the least density. From the surface to deeper depths, the earth’s interior has different zones and each of these contains materials with different characteristics.

Geologic Time, time scale that covers Earth’s entire geologic history from its origin to the present. Before the growth of a geologic time scale in the 19th century natural historians recognized that Earth has a lengthy history, but the scale used today developed over the last 200 years and continues to evolve. A geologic time scale helps scientists think about the history of the planet in manageable sections of time.

The present geologic time scale is based on radiometric dating and the record of ancient life preserved in layers of rock. Most boundaries in recent geologic time coincide with periodic extinctions and appearances of new species. Divisions in the older part of the record are based on dates provided by radiometric dating methods.
Division of Time:
The geologic time scale adopted by the International Union of Geological Sciences in 2004 breaks Earth’s history into distinct intervals of varying lengths measured in calendar years. The longest intervals are eons. Each eon is subdivided into eras. Each era is made up of periods, which are further divided into epochs.
There are three eons: the Archean, the Proterozoic, and the Phanerozoic. The Archean, the earliest eon, is defined as about 3.8 billion to 2.5 billion years before present. The time before the Archean Eon, simply called pre-Archean, is marked by the formation of the planet. The Proterozoic Eon lasted from about 2.5 billion to 542 million years before present. The Archean and Proterozoic eons are also collectively called Precambrian time. An explosion of invertebrate life marks the end of the Proterozoic and the beginning of the Phanerozoic.
The Phanerozoic Eon started about 542 million years ago and continues into the present. It is divided into three eras: the Paleozoic (542 million to 251 million years before present), Mesozoic (251 million to 65 million years before present), and Cenozoic (65 million years before present to present).
The Paleozoic Era is divided into six periods. From oldest to youngest they are the Cambrian (542 million to 488 million years before present), Ordovician (488 million to 444 million years before present), Silurian (444 million to 416 million years before present), Devonian (416 million to 359 million years before present), Carboniferous (359 million to 299 million years before present), and Permian (299 million to 251 million years before present). The Paleozoic began with the appearance of many different life-forms, which are preserved as abundant fossils in rock sequences all over the world. It ended with the extinction of over 90 percent of all living organisms at the end of the Permian Period. The cause of this event is currently unknown.
The Mesozoic Era is made up of the Triassic (251 million to 200 million years before present), Jurassic (200 million to 145 million years before present), and Cretaceous (145 million to 65 million years before present) periods. The Mesozoic began with the appearance of many new kinds of animals, including the dinosaurs and the ammonites, or extinct relatives of modern squid. The Mesozoic ended with another major extinction in which about 80 percent of all living organisms died. This extinction may have been the result of a large asteroid that crashed into Earth on the present-day northern Yucatán Peninsula of Mexico.
The Cenozoic Era has two geologic periods, the Paleogene (65 million to 23 million years before present) and the Neogene (23 million years before present to the present). The Paleogene Period is made up of three epochs: the Paleocene (65 million to 56 million years before present), Eocene (56 million to 34 million years before present), and Oligocene (34 million to 23 million years before present). The Neogene Period is divided into four epochs: the Miocene (23 million to 5.3 million years before present), Pliocene (5.3 million to 1.8 million years before present), Pleistocene (1.8 million to 11,500 years before present), and Holocene (11,500 years to the present) epochs. The Holocene is marked by the rapid retreat of the last continental ice sheets in Europe and North America, an accelerated rise in sea level, climatic moderation, and the expansion of human societies in every part of the world.

Geologic Time

The Precambrian is a time span that includes the Archean and Proterozoic eons and began about 4 billion years ago. The Precambrian marks the first formation of continents, the oceans, the atmosphere, and life. The Precambrian represents the oldest chapter in Earth’s history that can still be studied. Very little remains of Earth from the period of 4.6 billion to about 4 billion years ago due to the melting of rock caused by the early period of meteorite bombardment. Rocks dating from the Precambrian, however, have been found in Africa, Antarctica, Australia, Brazil, Canada, and Scandinavia. Some zircon mineral grains deposited in Australian rock layers have been dated to 4.2 billion years.

The Precambrian is also the longest chapter in Earth’s history, spanning a period of about 3.5 billion years. During this timeframe, the atmosphere and the oceans formed from gases that escaped from the hot interior of the planet as a result of widespread volcanic eruptions. The early atmosphere consisted primarily of nitrogen, carbon dioxide, and water vapor. As Earth continued to cool, the water vapor condensed out and fell as precipitation to form the oceans. Some scientists believe that much of Earth’s water vapor originally came from comets containing frozen water that struck Earth during the period of meteorite bombardment.
By studying 2-billion-year-old rocks found in northwestern Canada, as well as 2.5-billion-year-old rocks in China, scientists have found evidence that plate tectonics began shaping Earth’s surface as early as the middle Precambrian. About a billion years ago, the Earth’s plates were centered around the South Pole and formed a supercontinent called Rodinia. Slowly, pieces of this supercontinent broke away from the central continent and traveled north, forming smaller continents.
Life originated during the Precambrian. The earliest fossil evidence of life consists of prokaryotes, one-celled organisms that lacked a nucleus and reproduced by dividing, a process known as asexual reproduction. Asexual division meant that a prokaryote’s hereditary material was copied unchanged. The first prokaryotes were bacteria known as archaebacteria. Scientists believe they came into existence perhaps as early as 3.8 billion years ago, but certainly by about 3.5 billion years ago, and were anaerobic—that is, they did not require oxygen to produce energy. Free oxygen barely existed in the atmosphere of the early Earth.
Archaebacteria were followed about 3.46 billion years ago by another type of prokaryote known as cyanobacteria or blue-green algae. These cyanobacteria gradually introduced oxygen in the atmosphere as a result of photosynthesis. In shallow tropical waters, cyanobacteria formed mats that grew into humps called stromatolites. Fossilized stromatolites have been found in rocks in the Pilbara region of western Australia that are more than 3.4 billion years old and in rocks of the Gunflint Chert region of northwest Lake Superior that are about 2.1 billion years old.
For billions of years, life existed only in the simple form of prokaryotes. Prokaryotes were followed by the relatively more advanced eukaryotes, organisms that have a nucleus in their cells and that reproduce by combining or sharing their heredity makeup rather than by simply dividing. Sexual reproduction marked a milestone in life on Earth because it created the possibility of hereditary variation and enabled organisms to adapt more easily to a changing environment. The very latest part of Precambrian time some 560 million to 545 million years ago saw the appearance of an intriguing group of fossil organisms known as the Ediacaran fauna. First discovered in the northern Flinders Range region of Australia in the mid-1940s and subsequently found in many locations throughout the world, these strange fossils appear to be the precursors of many of the fossil groups that were to explode in Earth's oceans in the Paleozoic Era.
Paleozoic Era.
At the start of the Paleozoic Era about 543 million years ago, an enormous expansion in the diversity and complexity of life occurred. This event took place in the Cambrian Period and is called the Cambrian explosion. Nothing like it has happened since. Almost all of the major groups of animals we know today made their first appearance during the Cambrian explosion. Almost all of the different “body plans” found in animals today—that is, the way an animal’s body is designed, with heads, legs, rear ends, claws, tentacles, or antennae—also originated during this period.
Fishes first appeared during the Paleozoic Era, and multicellular plants began growing on the land. Other land animals, such as scorpions, insects, and amphibians, also originated during this time. Just as new forms of life were being created, however, other forms of life were going out of existence. Natural selection meant that some species were able to flourish, while others failed. In fact, mass extinctions of animal and plant species were commonplace.
Most of the early complex life forms of the Cambrian explosion lived in the sea. The creation of warm, shallow seas, along with the buildup of oxygen in the atmosphere, may have aided this explosion of life forms. The shallow seas were created by the breakup of the supercontinent Rodinia. During the Ordovician, Silurian, and Devonian periods, which followed the Cambrian Period and lasted from 490 million to 354 million years ago, some of the continental pieces that had broken off Rodinia collided. These collisions resulted in larger continental masses in equatorial regions and in the Northern Hemisphere. The collisions built a number of mountain ranges, including parts of the Appalachian Mountains in North America and the Caledonian Mountains of northern Europe.
Toward the close of the Paleozoic Era, two large continental masses, Gondwanaland to the south and Laurasia to the north, faced each other across the equator. Their slow but eventful collision during the Permian Period of the Paleozoic Era, which lasted from 290 million to 248 million years ago, assembled the supercontinent Pangaea and resulted in some of the grandest mountains in the history of Earth. These mountains included other parts of the Appalachians and the Ural Mountains of Asia. At the close of the Paleozoic Era, Pangaea represented over 90 percent of all the continental landmasses. Pangaea straddled the equator with a huge mouthlike opening that faced east. This opening was the Tethys Ocean, which closed as India moved northward creating the Himalayas. The last remnants of the Tethys Ocean can be seen in today’s Mediterranean Sea.
The Paleozoic came to an end with a major extinction event, when perhaps as many as 90 percent of all plant and animal species died out. The reason is not known for sure, but many scientists believe that huge volcanic outpourings of lavas in central Siberia, coupled with an asteroid impact, were joint contributing factors.
Mesozoic Era
The Mesozoic Era, beginning 248 million years ago, is often characterized as the Age of Reptiles because reptiles were the dominant life forms during this era. Reptiles dominated not only on land, as dinosaurs, but also in the sea, in the form of the plesiosaurs and ichthyosaurs, and in the air, as pterosaurs, which were flying reptiles. See also Dinosaur; Plesiosaur; Ichthyosaur; Pterosaur.
The Mesozoic Era is divided into three geological periods: the Triassic, which lasted from 248 million to 206 million years ago; the Jurassic, from 206 million to 144 million years ago; and the Cretaceous, from 144 million to 65 million years ago. The dinosaurs emerged during the Triassic Period and were one of the most successful animals in Earth’s history, lasting for about 180 million years before going extinct at the end of the Cretaceous Period. The first birds and mammals and the first flowering plants also appeared during the Mesozoic Era. Before flowering plants emerged, plants with seed-bearing cones known as conifers were the dominant form of plants. Flowering plants soon replaced conifers as the dominant form of vegetation during the Mesozoic Era.
The Mesozoic was an eventful era geologically with many changes to Earth’s surface. Pangaea continued to exist for another 50 million years during the early Mesozoic Era. By the early Jurassic Period, Pangaea began to break up. What is now South America began splitting from what is now Africa, and in the process the South Atlantic Ocean formed. As the landmass that became North America drifted away from Pangaea and moved westward, a long subduction zone extended along North America’s western margin. This subduction zone and the accompanying arc of volcanoes extended from what is now Alaska to the southern tip of South America. Much of this feature, called the American Cordillera, exists today as the eastern margin of the Pacific Ring of Fire.
During the Cretaceous Period, heat continued to be released from the margins of the drifting continents, and as they slowly sank, vast inland seas formed in much of the continental interiors. The fossilized remains of fishes and marine mollusks called ammonites can be found today in the middle of the North American continent because these areas were once underwater. Large continental masses broke off the northern part of southern Gondwanaland during this period and began to narrow the Tethys Ocean. The largest of these continental masses, present-day India, moved northward toward its collision with southern Asia. As both the North Atlantic Ocean and South Atlantic Ocean continued to open, North and South America became isolated continents for the first time in 450 million years. Their westward journey resulted in mountains along their western margins, including the Andes of South America.
Cenozoic Era


The Cenozoic Era, beginning about 65 million years ago, is the period when mammals became the dominant form of life on land. Human beings first appeared in the later stages of the Cenozoic Era. In short, the modern world as we know it, with its characteristic geographical features and its animals and plants, came into being. All of the continents that we know today took shape during this era.
A single catastrophic event may have been responsible for this relatively abrupt change from the Age of Reptiles to the Age of Mammals. Most scientists now believe that a huge asteroid or comet struck the Earth at the end of the Mesozoic and the beginning of the Cenozoic eras, causing the extinction of many forms of life, including the dinosaurs. Evidence of this collision came with the discovery of a large impact crater off the coast of Mexico’s Yucatán Peninsula and the worldwide finding of iridium, a metallic element rare on Earth but abundant in meteorites, in rock layers dated from the end of the Cretaceous Period. The extinction of the dinosaurs opened the way for mammals to become the dominant land animals.
The Cenozoic Era is divided into the Tertiary and the Quaternary periods. The Tertiary Period lasted from about 65 million to about 1.8 million years ago. The Quaternary Period began about 1.8 million years ago and continues to the present day. These periods are further subdivided into epochs, such as the Pleistocene, from 1.8 million to 10,000 years ago, and the Holocene, from 10,000 years ago to the present.
Early in the Tertiary Period, Pangaea was completely disassembled, and the modern continents were all clearly outlined. India and other continental masses began colliding with southern Asia to form the Himalayas. Africa and a series of smaller microcontinents began colliding with southern Europe to form the Alps. The Tethys Ocean was nearly closed and began to resemble today’s Mediterranean Sea. As the Tethys continued to narrow, the Atlantic continued to open, becoming an ever-wider ocean. Iceland appeared as a new island in later Tertiary time, and its active volcanism today indicates that seafloor spreading is still causing the country to grow.
Late in the Tertiary Period, about 6 million years ago, humans began to evolve in Africa. These early humans began to migrate to other parts of the world between 2 million and 1.7 million years ago.
The Quaternary Period marks the onset of the great ice ages. Many times, perhaps at least once every 100,000 years on average, vast glaciers 3 km (2 mi) thick invaded much of North America, Europe, and parts of Asia. The glaciers eroded considerable amounts of material that stood in their paths, gouging out U-shaped valleys. Anatomically modern human beings, known as Homo sapiens, became the dominant form of life in the Quaternary Period. Most anthropologists (scientists who study human life and culture) believe that anatomically modern humans originated only recently in Earth’s 4.6-billion-year history, within the past 200,000 years.


Thursday, October 11, 2012

Earth Systems (4 physical systems)

    Lecture 3

    Earth Systems  (4 physical systems)
    Atmosphere 
derived from the Greek words for air (atmo), 
      – Layer of gases that surround Earth. Allows you to breathe and protects earth.
    The air of our planet is composed of  79% nitrogen, and just under 21% oxygen,
      – Troposphere, Stratosphere, Mesosphere, Ionosphere (or Thermosphere), Exosphere and the Magnetosphere
               Lithosphere
§  Surface of the planet that forms the continents and the ocean floor.
§  derived from the Greek word for stone (litho)
§  This crust is inorganic and is composed of minerals.
§  It covers the entire surface of the earth from the top of Mount Everest to the bottom of the Mariana Trench.
    Hydrosphere
–       derived from the Greek words for water (hydro)
–       All the water on Earth (ocean, ice, and water vapor in the atmosphere)
–       Ninety-seven percent of the earth's water is in the oceans.
–       The remaining three percent is fresh water; three-quarters of the fresh water is solid and exists in ice sheets
    Biosphere
–       derived from the Greek word for life (bio).
–       Part of Earth where life exists.
–       Plants, animals, and one-celled organisms are all part of the biosphere
–       Most of the planet's life is found from three meters below the ground to thirty meters above it and in the top 200 meters of the oceans and seas.
•         All four spheres can be and often are present in a single location.
•         a piece of soil will of course have mineral material from the lithosphere.
•         Additionally, there will be elements of the hydrosphere present as moisture within the soil,
•          the biosphere as insects and plants,
•         the atmosphere as pockets of air between soil pieces.