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Asteroids



















Space Background with Welcome








































250px-innersolarsystem-en.jpg

Photo of the inner solar system with the asteroid belt depicted in white






All about Asteroids:
 
Asteroids were first discovered in 1801 by Giuseppe Piazzi, when a search for a missing planet was conducted based on Bode's Law.  While Piazzi was searching for the planet, he happened upon the largest of teh asteroids in the asteroid belt and named it Ceres (see hubble photo below).  Futher information on the discovery of asteroids can be found by visiting http://near.jhuapl.edu/eros/history/index.html . This web site is titled: A Brief Historical Account of the Discovery of the Asteroids.  It was written by Ray Sterner. 
 
Asteroids recieved their name from Sir William Hershel, who felt they had a star like quality.  He derived the word asteroid from the greek aster which means star.
 
Asteroids are small, rocky planetoidal bodies orbiting the sun between Mars and Jupiter.
 
Asteroids are thought to be remainders of planets left over after the planets formed.
 
Types of Asteroids:
 

90% of asteroids can be divided into two groups based on albedo and color.

 

75% of all asteroids are the C-Type.  they are extremely dark. These asteroids contain high amounts of carbon and some contain water.

 

16% of all asteroids are the S - type.  They are of moderate albedo and reddish  in color.  Spectra indicates these asteroids contain iron and magnesium silicates mixed with pure nickel-iron.

 

5% of all asteroids are the M - type. They are of ambiguous spectrum and moderate albedos.  they have no silica absorption bands so they may be metallic asteroids.  They may be remnant cores of larger differentiated precursor bodies.       

            

The remaning 4% are rare types

Eros
eros19.jpg






There is still much to be known about asteroids.  The Near Earth Asteroid Rendezvous or NEAR Launched on the 17th of February, 1996.  NEAR’s mission was to travel to the Asteroid Eros and orbit it for over a year.  NEAR went into orbit around Eros on the 14th of February, 200 and remained in orbit at various altitudes until the 12th of February, 2001, when NEAR became the first spacecraft to touchdown on an asteroid.  NEAR continued to transmit information until the 28th of February, there has been no contact made since.

 

More about asteroids

Recommended Reading on Asteroids:
 
  • Asteroids III, Edited by W. Bottke, A. Cellino, P. Paolicchi, and P. Binzel, University of Arizona Press, Tucson, 2002
  • The First Asteroid: Ceres, 1801-2001, C. Cunningham, Star Lab Press, Surfside, Florida, 2001
  • Asteroids : A History, C. Peebles, Smithsonian Institution Press, Washington, D.C., 2000
  • Asteroid: Earth Destroyer or New Frontier?, P. Barnes-Svarney, Plenum Press, New York, 1996
  • Asteroids II, Edited by R. Binzel, T, Gehrels, and M. Matthews, University of Arizona Press, Tucson, 1989
  • Asteroids : Their Nature and Utilization, C. Kowal, Halstead Press, New York, 1988
  • Asteroids - Dynamic site: This is the Asteroid Dynamic site. This site contains information on numbered and multiopposition asteroids.








































    Ceres as viewed from the Hubble Space Telescope

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    Eros in motion
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