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	     The name
    'Asteroid' was given by Sir William Herschel in 1802, shortly after they were discovered.
    It means 'like a star' in Greek. 
	    What is an Asteroid? 
         Sometimes referred to as as 'minor planets', asteroids are small fragments of rock,
    not large enough to be classified as Planets or Dwarf Planets, left over from the formation of the Solar System
	about 4,500 million years ago. Over 8,000 of these have now been
    catalogued, though it is thought that vastly more lie undiscovered.
	Those catalogued range wildly in size from the odd metre to hundreds of
    kilometres wide, although only about 250 have diameters of over 100km, and most tend to be
    about 1km across. 
	    The largest discovered asteroid is 'Ceres', though it has subsequently been reclassified as a Dwarf planet, which is a massive 940km in diameter, and was discovered
	in 1801 by Italian astronomer Giuseppe Piazzi (Ceres was in fact also the first asteroid to be discovered, and the first, and so far only, to be recategorised as a Dwarf Planet).
    92.8% of all the asteroids so far examined are found to be made of rock whilst 5.7% are 
	made from a mixture of Nickel and Iron. Their shapes tend to be highly irregular, as they do not have strong enough gravitational fields to pull them into a sphere, and
	some asteroids have been found to have their own 'moons'. 
	    Asteroid Locations and Dangers 
        Most asteroids in the Solar
    System are to be found in the Asteroid Belt (or Main Belt) which is in an elliptical orbit
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	Asteroid Ida, from Galileo Credit: NASA/JpL |   
    around the Sun, between Mars and Jupiter, ranging from 2.2 to 3.3 AUs from the Sun (see illustration).
    There is also another lesser-known group of asteroids, the 'Trojans', which follow Jupiter's orbit around the Sun, roughly
	60° ahead or behind the planet.
	    However, small bodies such as asteroids don't all just stay put in a regular orbit all the time. 
	In fact, some can be found inside the Earth's own orbit.
	All it takes is for one asteroid to hit another for them both to end up hurtling away at high speed into the rest of the
	Solar Sysyem. Obviously this presents a potentially dangerous situation if a sizeable asteroid happens to end up hitting Earth.
	     There is even a theory, which has recieved a lot of support in recent years, which suggests that 
	the dinosaurs were wiped out when an asteroid or comet hit the
    Earth near the Yucatan peninsula, forming the Chicxulub Crater, although this is in no way known for sure. Nevertheless, the potential for damage
	is catastrophic for humans, if an asteroid of a kilometre were to collide with the Earth, and it is primarily for this reason
	that both public curiosity and scientific research on asteroids have been increasing substantially in recent decades. 
	    Origin of Asteroids 
        There are many
    theories as to how asteroids originated but the most likely one is that they are
    left-overs from when the Solar System was created. Originally, there may have been as many as
    eight Mars sized objects in the main belt, but if this were the case, Jupiter's gravitational
    influence would have slowly caused them to fragment, which would explain the asteroid belt as we see it today.
	One of these 'Mars-like' objects probably crashed into the young
    Earth creating the moon (this is known as the 'Big Splash', see the Earth section for more
    details), another one must have survived and is now called Mars
    and the rest got broken up in collisions, with most of the debris now scattered around the
    Solar System or burned in the Sun and the rest in the Asteroid Belt.
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	Asteroid Eros, from NEAR Credit: NASA/JpL |   
	The mass of all the known asteroids added together is less that half that of the Earth's Moon.
        The NEAR Mission 
	    The NEAR (Near Earth Asteroid
    Rendezvous) spacecraft was launched in 1996 too examine a certain asteroid called Eros
    (which is not actually part of the Main Belt) and on its way, it passed just 1,200 km away from
    asteroid Matilde. The NEAR mission was very fruitful, and it revealed a lot of useful information about Eros, 
	before it crashed, as planned, into the asteroid itself, taking photos from as close as 130 metres above the surface of Eros. 
	For many fascinating pictures of this asteroid, including some as
    close as a few miles, go to the NEAR website. 
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