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Exploring space can tell us about where we come from
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Home
Observing Space
Introduction
Telescopes
Invisible Astronomy
Section 1.4
Section 1.5
Section 1.6
Section 1.7
Section 1.8
Section 1.9
Section 1.10
Section 1.11
Section 1.12
Section 1.13
Section 1.14
Section 1.15
Exploring Space
Introduction
Pioneers
Shuttles
Launchers
ISS
USA in Space
UK in Space
China in Space
France in Space
Russia in Space
The X-Prize
Section 2.12
Section 2.13
Section 2.14
Section 2.15
Planets
Introduction
Mercury
Venus
Earth
Mars
Jupiter
Saturn
Uranus
Neptune
Pluto
Section 3.11
Section 3.12
Section 3.13
Section 3.14
Section 3.15
Moons
Section 4.1
Section 4.2
Section 4.3
Section 4.4
Section 4.5
Section 4.6
Section 4.7
Section 4.8
Section 4.9
Section 4.10
Section 4.11
Section 4.12
Section 4.13
Section 4.14
Section 4.15
Stars
Introduction
The Sun
Sirius
Canopus
Alpha Centauri
Arcturus
Others
Section 5.8
Section 5.9
Section 5.10
Section 5.11
Section 5.12
Section 5.13
Section 5.14
Section 5.15
Comets, Meteors & Asteroids
Deep Impact Mission
Section 6.2
Section 6.3
Section 6.4
Section 6.5
Section 6.6
Section 6.7
Section 6.8
Section 6.9
Section 6.10
Section 6.11
Section 6.12
Section 6.13
Section 6.14
Section 6.15
Galaxies
Section 7.1
Section 7.2
Section 7.3
Section 7.4
Section 7.5
Section 7.6
Section 7.7
Section 7.8
Section 7.9
Section 7.10
Section 7.11
Section 7.12
Section 7.13
Section 7.14
Section 7.15
The Universe
Section 8.1
Section 8.2
Section 8.3
Section 8.4
Section 8.5
Section 8.6
Section 8.7
Section 8.8
Section 8.9
Section 8.10
Section 8.11
Section 8.12
Section 8.13
Section 8.14
Section 8.15
Eclipses
Solar Eclipse
Lunar Eclipse
Lunar Eclipse 2008
What Eclipses Have Taught Us
Significant Eclipses in History
The Blood Red Moon
Section 9.7
Section 9.8
Section 9.9
Section 9.10
Section 9.11
Section 9.12
Section 9.13
Section 9.14
Section 9.15
Amazing Facts
Section 10.1
Section 10.2
Section 10.3
Section 10.4
Section 10.5
Section 10.6
Section 10.7
Section 10.8
Section 10.9
Section 10.10
Section 10.11
Section 10.12
Section 10.13
Section 10.14
Section 10.15
Play: Comet Impact
Section 11.1
Section 11.2
Section 11.3
Section 11.4
Section 11.5
Section 11.6
Section 11.7
Section 11.8
Section 11.9
Section 11.10
Section 11.11
Section 11.12
Section 11.13
Section 11.14
Section 11.15
Space Blog
Section 12.1
Section 12.2
Section 12.3
Section 12.4
Section 12.5
Section 12.6
Section 12.7
Section 12.8
Section 12.9
Section 12.10
Section 12.11
Section 12.12
Section 12.13
Section 12.14
Section 12.15
Section 13
Section 13.1
Section 13.2
Section 13.3
Section 13.4
Section 13.5
Section 13.6
Section 13.7
Section 13.8
Section 13.9
Section 13.10
Section 13.11
Section 13.12
Section 13.13
Section 13.14
Section 13.15
Section 14
Section 14.1
Section 14.2
Section 14.3
Section 14.4
Section 14.5
Section 14.6
Section 14.7
Section 14.8
Section 14.9
Section 14.10
Section 14.11
Section 14.12
Section 14.13
Section 14.14
Section 14.15
Section 15
Section 15.1
Section 15.2
Section 15.3
Section 15.4
Section 15.5
Section 15.6
Section 15.7
Section 15.8
Section 15.9
Section 15.10
Section 15.11
Section 15.12
Section 15.13
Section 15.14
Section 15.15
Eclipses
Solar Eclipse

Of all the types of eclipse we can witness, a total solar eclipse ranks as the most spectacular and awe-inspiring. This breathtaking natural phenomenon occurs when the Moon, moving in its orbit, passes between the Earth and the Sun, casting its shadow across the Earth (as in the diagram).

From our viewpoint on Earth, the Moon appears to move in front of the Sun, gradually covering up more and more of the Sun’s disk and blotting out the daylight. When the Sun is completely covered over by the Moon, an eerie silence descends, the sky turns dark and everything is enveloped in a deep twilight. Confused birds stop singing and return to their roosts, farm animals go to their pens to sleep, while the brighter stars and planets become visible in the sky. For a brief moment, we can see the Sun’s corona – its pearly white outer atmosphere - around the outside of the eclipsed Sun. To see a total solar eclipse, you need to be in exactly the right place: within an 80-100km strip of the eclipse’s centre line. Outside this narrow strip, you’ll only see a partial eclipse. Totality only lasts for a short while and never more than seven and a half minutes before the Sun’s rays become visible once more.

Warning! Never look at the partial phase of a total solar eclipse unless you are looking through an appropriate solar filter: otherwise, you may permanently damage your eyes. Only totality – when the Moon covers the Sun completely, is safe to observe with the naked eye.

Calendar of Solar Eclipses

  • Date: 7 February 2008
    Eclipse Type: Annular
    Where: Antarctica
  • Date: 1 August 2008
    Eclipse Type: Total
    Where: Russia, Mongolia
  • Date: 26 January 2009
    Eclipse Type: Annular
    Where: Indonesia
  • Date: 22 July 2009
    Eclipse Type: Total
    Where: Asia, Pacific
  • Date: 15 January 2010
    Eclipse Type: Annular
    Where: Africa, Asia
  • Date: 11 July 2010
    Eclipse Type: Total
    Where: Pacific, S. America

Photos: DCL/Perry Vlahos

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