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NASA gave people a front row seat to today's total solar eclipse, thanks to a partnership with the University of California at Berkeley and the Exploratorium. A streaming webcast brought the eclipse -- visible along a path from South America to Africa to Asia -- to schools and museums and computer desktops worldwide.

 

lefthttp://hypography.com/gallery/files/9/9/8/eclipse_thumb.jpg[/img]The eclipse coverage was part of Sun-Earth Day, celebrated every year to help everyone better understand how our sun interacts with the Earth and other planets in the solar system. This year's theme, "Eclipse: In a Different Light" shows how eclipses have inspired people to observe and understand the Sun-Earth-Moon system.

 

NASA and Libyan scientists also conducted joint scientific activities in Libya to observe and study the event.

 

A total solar eclipse is very rare because all parts of this puzzle must line up correctly in order for it to occur. The moon must be in its new phase for a solar eclipse to take place. The moon's shadow has two parts—a central region called the umbra and an outer region called the penumbra. The part of the moon’s shadow which passes over you determines what kind of eclipse you will see.

 

This eclipse's path begins in Brazil and extends across the Atlantic Ocean, Northern Africa, and Central Asia where it ends at sunset in Northern Mongolia. A partial eclipse path, within the much broader path of the moon's penumbral shadow, includes the northern two thirds of Africa, Europe, and Central Asia.

 

In a total eclipse like this one, the entire central portion of the Sun is blocked out. The sky darkens as though it is nighttime and -- for the only time -- you can see the Sun’s corona, or outer atmosphere. Total solar eclipses are of special interest to astronomers because it's the only time they can study the corona. Scientists still don't understand why the corona is so hot. Its temperature is 1 to 2 million degrees Fahrenheit while the Sun's bright surface is only 10,000° F. Careful measurements and experiments made during a total eclipse can help to unravel this enigma.

 

This year's eclipse is also special because the total phase lasts over 4 minutes at the center of the path. This is quite long for a total solar eclipse since most last just a minute or two. The next total eclipse,on August 1, 2008, will be seen in northern Canada, Greenland, Siberia, Mongolia and northern China. It will last about 2 minutes. The next total eclipse visible from the United States won’t happen until August 21, 2017.

 

Source: NASA

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