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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

Comets, Meteors & Asteroids

Comets, Meteors & Asteroids

The Hale-Bopp comet is 40km long and passes Earth every 4026 years.

Amongst the planets and moons, thousands of asteroids and comets that have been catalogued and their orbits calculated - thousands more remain unknown.

Comets
Comets, are small ‘dirty snowballs’ made from a mixture of ice, frozen gases, and dust. All comets are left over from the formation of the Solar System.

Comets travel three times faster than asteroids and are only visible when near the Sun. Haley’s comet is 16km long and passes the Sun every 76 years. 

Hale-Bopp, at 40km long, swings by only once every 4026 years. It’s believed that half of the near-Earth asteroids may be ‘dead’ comets.

Meteors
Approximately twice a week, a meteor about the size of a pillow will hurtle towards the Earth and detonate with the force of an atomic bomb.  Fortunately, our atmosphere means they vaporize around five miles above the ground. If a piece of meteor survives to reach the Earth's surface, it is known as a meteorite.

Millions of meteors strike the Earth every day - most of them the size of a grain of sand. HOwever, from time-to-time, something larger crashes through the Earth’s natural defence shield - sometimes with catastrophic effect. 

It was one of these fireballs that some scientists now believe caused the extinction of the dinosaurs when it smashed into the ground at the Chicxulub in the Yucatan province of Mexico, 65 million years ago.  That one was believed to have been 8km in diameter.

Asteroids
Most asteroids behave in an orderly fashion, orbiting the Sun in the asteroid belt between Mars and Jupiter.  Some escape their orbit and pose a threat to us. 

Asteroids are believed to be debris left over from the formation of the Solar System 4.6 billion years ago.

Thought to be made from rock and metal, asteroids range in size from pebbles to 934km across.

Photos: Corbis & Science Photo Library
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