Solar eclipse

From Wikipedia, the free encyclopedia
Jump to: navigation, search
Photo taken during the 1999 eclipse.

When seen from Earth, a solar eclipse (ee klips') happens when the Moon passes between the Earth and the Sun. This makes the Moon fully or partially (partly) cover the sun. Solar eclipses can only happen during a new moon. Every year about two solar eclipses occur. Sometimes there are even five solar eclipses in a year. However, only two of these can be total solar eclipses,[1][2] and they are quite uncommon.

Eclipses are total only in a narrow track along the Earth, and only for a few minutes. Outside this path, all eclipses are partial, and places far from the track get no eclipse at all. The track can be predicted many years before it happens. Many people who are sometimes called "eclipse chasers" or "umbraphiles"[3] (the moon's shadow is called an umbra)[4] travel to faraway places to see solar eclipses. After the solar eclipse on August 11, 1999, in Europe, people began to show more interest in solar eclipses. On October 3, 2005, there was another solar eclipse, and unusually many people came to see it.

The last total eclipse was the solar eclipse of November 13, 2012.

A total solar eclipse is a natural phenomenon (event). Yet long ago, solar eclipses were thought to happen because of something supernatural or as a sign that something bad was going to happen. This is still believed in some cultures today. A total solar eclipse can frighten people who do not know what it means, because the Sun seems to disappear during the day and the sky turns dark in just a few minutes.

Solar eclipses happen somewhere on Earth almost every year, and very similar solar eclipses happen every 18 years, 11.3 days. This period is called the Saros cycle

Types[change | edit source]

Hybrid solar eclipse on October 3, 2005

There are four different types of solar eclipses:

  • A total eclipse is when the Sun is completely hidden behind the Moon. The dark shadow of the Moon covers the very bright surface of the Sun. This makes the corona easier to see.
  • An annular eclipse is when the Sun is directly behind the moon, but it looks like the Moon is smaller. This makes the Sun appear as a very bright ring or annulus around the shape of the Moon.
  • A hybrid eclipse (also called annular/total eclipse) is when it looks like a total eclipse in some parts of the Earth, and an annular eclipse in other parts. Hybrid eclipses do not happen as often as other eclipses.
  • A partial eclipse is when the moon is not exactly between the Sun and Earth, so it does not hide the Sun completely. This can usually be seen from a large part of the Earth.

The Sun's distance from the Earth is about 400 times the Moon's distance, and the Sun's diameter is about 400 times as big as the Moon's. This is why the Sun and Moon seem to be about the same size from Earth.

Looking at a solar eclipse[change | edit source]

Solar eclips 1999 1.jpg Solar eclips 1999 2.jpg Solar eclips 1999 3.jpg Solar eclipse 1999 4 NR.jpg Solar eclips 1999 5.jpg Solar eclips 1999 6.jpg Solar eclips 1999 7.jpg

Looking directly at the bright surface of the Sun itself can hurt the retina of the eye greatly because of the radiation that comes from the Sun. It can even blind people. The retina does not feel pain, so damage may not be felt for hours.[5]

The Sun is usually so bright that it is hard to look at it directly. However, when the Sun is covered in an eclipse, it is easier to look at it. Looking at the Sun during an eclipse is equally dangerous, except in the very short time when the Sun's surface is completely covered. Looking at the Sun's surface through binoculars, a telescope, or even a camera is extremely dangerous and can damage the eye in less than a second.[6][7]

Looking at the Sun without an eclipse does not usually hurt the eye very greatly, because the pupil of the eye closes down and makes everything darker. If the Sun is almost completely covered, the pupil opens because there is not as much light. However, the parts of the Sun that can be seen are still equally bright, and can hurt the eye very much.

References[change | edit source]

  1. Littmann, Mark; Fred Espenak, Ken Willcox (2008). Totality: Eclipses of the Sun. Oxford University Press. pp. 18–19. ISBN 0199532095.
  2. Five solar eclipses occurred in 1935. NASA (6 September, 2009). "Five Millennium Catalog of Solar Eclipses". NASA Eclipse Web Site. Fred Espenak, Project and Website Manager. http://eclipse.gsfc.nasa.gov/SEcat5/SE1901-2000.html. Retrieved 26 January 2010.
  3. "Op-Ed Contributor - Why I Never Miss a Solar Eclipse - NYTimes.com". nytimes.com. http://www.nytimes.com/2010/07/11/opinion/11pasachoff.html. Retrieved 2 September 2010.
  4. "Journeys - Eclipse Chasing, in Pursuit of Total Awe - NYTimes.com". nytimes.com. http://www.nytimes.com/2009/05/17/travel/17journeys.html?_r=1. Retrieved 2 September 2010.
  5. F. Espenak. "Eye Safety During Solar Eclipses". http://sunearth.gsfc.nasa.gov/eclipse/SEhelp/safety.html.
  6. A. M. MacRobert. "How to Watch a Partial Solar Eclipse Safely". Sky & Telescope magazine. http://www.skyandtelescope.com/observing/objects/eclipses/3306081.html. Retrieved 2007-08-04.
  7. B. Ralph Chou, MSc, OD. "Eye safety during solar eclipses". National Aeronautics and Space Administration. http://eclipse.gsfc.nasa.gov/SEhelp/safety2.html. Retrieved 2010-12-03.

Other websites[change | edit source]

Eye safety[change | edit source]