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Showing posts with label Education. Show all posts
Showing posts with label Education. Show all posts

Tuesday, December 17, 2013

Cosmic Journeys : Earth in 1000 Years


This edition of COSMIC JOURNEYS explores the still unfolding story of Earth's past and the light it sheds on the science of climate change today. While that story can tell us about the mechanisms that can shape our climate. it's still the unique conditions of our time that will determine sea levels, ice coverage, and temperatures.


Ice, in its varied forms, covers as much as 16% of Earth's surface, including 33% of land areas at the height of the northern winter. Glaciers, sea ice, permafrost, ice sheets and snow play an important role in Earth's climate. They reflect energy back to space, shape ocean currents, and spawn weather patterns.

But there are signs that Earth's great stores of ice are beginning to melt. To find out where Earth might be headed, scientists are drilling down into the ice, and scouring ancient sea beds, for evidence of past climate change. What are they learning about the fate of our planet... a thousand years into the future and even beyond?

30,000 years ago, Earth began a relentless descent into winter. Glaciers pushed into what were temperate zones. Ice spread beyond polar seas. New layers of ice accumulated on the vast frozen plateau of Greenland. At three kilometers thick, Greenland's ice sheet is a monumental formation built over successive ice ages and millions of years. It's so heavy that it has pushed much of the island down below sea level. And yet, today, scientists have begun to wonder how resilient this ice sheet really is.

Average global temperatures have risen about one degree Celsius since the industrial revolution. They could go up another degree by the end of this century. If Greenland's ice sheet were to melt, sea levels would rise by over seven meters. That would destroy or threaten the homes and livelihoods of up to a quarter of the world's population.

With so much at stake, scientists are monitoring Earth's frozen zones... with satellites, radar flights, and expeditions to drill deep into ice sheets. And they are reconstructing past climates, looking for clues to where Earth might now be headed... not just centuries, but thousands of years in the future.

Periods of melting and freezing, it turns out, are central events in our planet's history.
That's been born out by evidence ranging from geological traces of past sea levels... the distribution of fossils... chemical traces that correspond to ocean temperatures, and more.

Going back over two billion years, earth has experienced five major glacial or ice ages. The first, called the Huronian, has been linked to the rise of photosynthesis in primitive organisms. They began to take in carbon dioxide, an important greenhouse gas. That decreased the amount of solar energy trapped by the atmosphere, sending Earth into a deep freeze.

The second major ice age began 580 million years ago. It was so severe, it's often referred to as "snowball earth." The Andean-Saharan and the Karoo ice ages began 460 and 360 million years ago. Finally, there's the Quaternary... from 2.6 million years ago to the present. Periods of cooling and warming have been spurred by a range of interlocking factors: the movement of continents, patterns of ocean circulation, volcanic events, the evolution of plants and animals.

The world as we know it was beginning to take shape in the period from 90 to 50 million years ago. The continents were moving toward their present positions. The Americas separated from Europe and Africa. India headed toward a merger with Asia. The world was getting warmer. Temperatures spiked roughly 55 million years ago, going up about 5 degrees Celsius in just a few thousand years. CO2 levels rose to about 1000 parts per million compared to 280 in pre-industrial times, and 390 today.

But the stage was set for a major cool down. The configuration of landmasses had cut the Arctic off from the wider oceans. That allowed a layer of fresh water to settle over it, and a sea plant called Azolla to spread widely. In a year, it can soak up as much as 6 tons of CO2 per acre. Plowing into Asia, the Indian subcontinent caused the mighty Himalayan Mountains to rise up. In a process called weathering, rainfall interacting with exposed rock began to draw more CO2 from the atmosphere... washing it into the sea. Temperatures steadily dropped.

By around 33 million years ago, South America had separated from Antarctica. Currents swirling around the continent isolated it from warm waters to the north. An ice sheet formed. In time, with temperatures and CO2 levels continuing to fall, the door was open for a more subtle climate driver. It was first described by the 19th century Serbian scientist, Milutin Milankovic.

He saw that periodic variations in Earth's rotational motion altered the amount of solar radiation striking the poles. In combination, every 100,000 years or so, these variations have sent earth into a period of cool temperatures and spreading ice.
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Cosmic Journeys : Hyper Earth: the New World

Our world, Earth, is changing before our eyes. Go back millions of years. Forests reached into polar regions, sea levels rose, and temperatures soared with high levels of the greenhouse gas, carbon dioxide in the atmosphere. A long cooling period followed. But now CO2 is on the rise again. What will happen? How will we live in the New World that's now emerging?

Scientists are intensively tracking the workings of planet Earth with satellites that chart its winds, ocean currents, temperatures, plant growth, and more. And with a new virtual Earth, shrunk down and converted into physical equations, satellite data, and computer codes they are able to show the workings of our planet in whole new ways..

This other Earth, a mirror of the one in which we live, is designed to follow the flow of heat through the complex, dynamic engine known as the climate... and to predict its future evolution. You can see the pattern of heat input in this sequence showing surface temperatures. As the seasons shift, heat builds and dissipates, most notably across tropical and subtropical regions. How does Earth dissipate this build up of heat? Look below. The oceans cover 71% of the planet's surface, at an average depth of more than four kilometers.


They act like an immense battery that can store and release energy over long periods of time, while transporting heat from warm to cool regions. The oceans are set in motion by the unevenness of solar heating... due to the amount of sunlight striking the tropics versus the poles, along with the cycles of day and night and the seasons.

That causes warm, tropical winds to blow toward the poles, and cold polar air to push toward the equator. Wind currents, in turn, drive surface ocean currents. This computer simulation shows the Gulfstream winding its way north along the coast of North America. This great ocean river carries enough heat energy to power the industrial world a hundred times over.

It breaks down in massive whirlpools that spread warm tropical waters over northern seas. Below the surface, this current mixes with cold deep currents that swirl around undersea ledges and mountains. When heat builds within tropical oceans in late summer, it can be released in a fury.
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Cosmic Journeys : Voyager Journey to the Stars



Cosmic Journeys examines the great promise of the Voyager mission and where it will lead us in our grand ambition to move out beyond our home planet. The two Voyager spacecraft are part of an ancient quest to push beyond our boundaries... to see what lies beyond the horizon. Now tens of billions of kilometers from Earth, two spacecraft are streaking out into the void. What will we learn about the Galaxy, the Universe, and ourselves from Voyager's epic Journey to the stars?

December 19, 1972... the splashdown of the Apollo 17 crew capsule marked the end of the golden age of manned spaceflight. The Mercury.... Gemini... and Apollo programs had proven that we could send people into space... To orbit the Earth.... Fly out beyond our planet... Then land on the moon and walk among its ancient crater.

The collective will to send people beyond our planet faded in times of economic uncertainty, war, and shifting priorities. And yet, just five years after Apollo ended, scientists launched a new vision that was just as profound and even more far-reaching.



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The Known Universe by AMNH





















Το βίντεο ξεκινάει από τα Ιμαλάια για να φτάσει στο απώτατο άκρο του Κόσμου. Έναν Κόσμο που περιέχει περίπου 100 δισεκατομμύρια άστρα στον Γαλαξία μας, και κατά προσέγγιση 125 δισεκατομμύρια γαλαξίες συνολικά.

Έναν Κόσμο που έχει διάμετρο περίπου 40 δισεκατομμύρια έτη φωτός, ενώ το παρατηρήσιμο Σύμπαν είναι μόνο13.7 δισ. έτη φωτός. Τη δημιουργία του βίντεο, αλλά και τη συλλογή δεδομένων, επιμελήθηκε το τμήμα αστροφυσικών ερευνών του Αμερικανικού Μουσείου Φυσικής Ιστορίας.

The Known Universe takes viewers from the Himalayas through our atmosphere and the inky black of space to the afterglow of the Big Bang. Every star, planet, and quasar seen in the film is possible because of the world's most complete four-dimensional map of the universe, the Digital Universe Atlas that is maintained and updated by astrophysicists at the American Museum of Natural History. The new film, created by the Museum, is part of an exhibition, Visions of the Cosmos: From the Milky Ocean to an Evolving Universe, at the Rubin Museum of Art in Manhattan through May 2010.

Data: Digital Universe, American Museum of Natural History
http://www.haydenplanetarium.org/univ...

Visualization Software: Uniview by SCISS

Director: Carter Emmart
Curator: Ben R. Oppenheimer
Producer: Michael Hoffman
Executive Producer: Ro Kinzler
Co-Executive Producer: Martin Brauen
Manager, Digital Universe Atlas: Brian Abbott

Music: Suke Cerulo

For more information visit http://www.amnh.org
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Monday, December 16, 2013

Pure Nature Specials : Mutation - The Science of Survival

Human mutation has always been fascinating, but beyond the spectacle is science.

 
 Research is uncovering how mutation works and how mutants may benefit future medicine.

They may even be the key to finding cures for life-threatening diseases.

 

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Under the Antarctic Ice - Beauty of The Nature


The Antarctic ice sheet is one of the two polar ice caps of the Earth. It covers about 98% of the Antarctic continent and is the largest single mass of ice on Earth. It covers an area of almost 14 million square km and contains 26.5 million cubic km of ice. That is, approximately 61 percent of all fresh water on the Earth is held in the Antarctic ice sheet, an amount equivalent to 70 m of water in the world's oceans. In East Antarctica, the ice sheet rests on a major land mass, but in West Antarctica the bed can extend to more than 2,500 m below sea level. The land in this area would be seabed if the ice sheet were not there.


The icing of Antarctica began with ice-rafting from middle Eocene times about 45.5 million years ago and escalated inland widely during the Eocene--Oligocene extinction event about 34 million years ago. CO2 levels were then about 760 ppm and had been decreasing from earlier levels in the thousands of ppm. Carbon dioxide decrease, with a tipping point of 600 ppm, was the primary agent forcing Antarctic glaciation.

The glaciation was favored by an interval when the Earth's orbit favored cool summers but Oxygen isotope ratio cycle marker changes were too large to be explained by Antarctic ice-sheet growth alone indicating an ice age of some size.The opening of the Drake Passage may have played a role as well though models of the changes suggest declining CO2 levels to have been more important.

Ice enters the sheet through precipitation as snow. This snow is then compacted to form glacier ice which moves under gravity towards the coast. Most of it is carried to the coast by fast moving ice streams. The ice then passes into the ocean, often forming vast floating ice shelves. These shelves then melt or calve off to give icebergs that eventually melt.


If the transfer of the ice from the land to the sea is balanced by snow falling back on the land then there will be no net contribution to global sea levels. A 2002 analysis of NASA satellite data from 1979--1999 showed that while overall the land ice is decreasing, areas of Antarctica where sea ice was increasing outnumbered areas of decreasing sea ice roughly 2:1.

The general trend shows that a warming climate in the southern hemisphere would transport more moisture to Antarctica, causing the interior ice sheets to grow, while calving events along the coast will increase, causing these areas to shrink. A 2006 paper derived from satellite data, measures changes in the gravity of the ice mass, suggests that the total amount of ice in Antarctica has begun decreasing in the past few years.


Another recent study compared the ice leaving the ice sheet, by measuring the ice velocity and thickness along the coast, to the amount of snow accumulation over the continent. This found that the East Antarctic Ice Sheet was in balance but the West Antarctic Ice Sheet was losing mass. This was largely due to acceleration of ice streams such as Pine Island Glacier. These results agree closely with the gravity changes.



The estimate published in November 2012 and based on the GRACE data as well as on an improved glacial isostatic adjustment model indicates that an average yearly mass loss was 69 ± 18 Gt/y from 2002 to 2010. The West Antarctic Ice Sheet was approximately in balance while the East Antarctic Ice Sheet gained mass. The mass loss was mainly concentrated along the Amundsen Sea coast.




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