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{{Orphan|date=February 2009}} {{Orphan|date=February 2009}}
In ], any material that condenses at high temperatures is called '''refractory'''<ref>{{cite web In ], any material that condenses at high temperatures is called '''refractory'''<ref>{{cite book
|title=Solar system evolution: a new perspective : an inquiry into the chemical composition, origin, and evolution of the solar system
|title=Glossary for Planetary Science Research Discoveries
|url=http://books.google.com/books?id=R3QKq4K0jIEC&vq=refractory&dq=refractory+ice+rock+gas&hl=ru&source=gbs_navlinks_s
|url=http://www.psrd.hawaii.edu/PSRDglossary.html#refractory
|publisher=Planetary Science Research Discoveries |publisher=Cambridge University Press
|year=2001
|pages=73–75
|last=Taylor
|first=Stuart Ross
|isbn= 9780521641302
}}</ref>. The opposite of refractory is ]. }}</ref>. The opposite of refractory is ].


The refractory group includes elements and compounds like metals and ] which make up the bulk of the mass of the ], ], ] and ]-type asteroids. A fraction of the mass of other ] and ]s. The refractory group includes elements and compounds like metals and ] which make up the bulk of the mass of the ], ], ] and ]-type asteroids. A fraction of the mass of other ] and ]s.


==References== ==References==

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In planetary science, any material that condenses at high temperatures is called refractory. The opposite of refractory is volatile.

The refractory group includes elements and compounds like metals and silicates which make up the bulk of the mass of the Terrestrial Planets, S, M and E-type asteroids. A fraction of the mass of other asteroids and Trans-Neptunian objects.

References

  1. Taylor, Stuart Ross (2001). Solar system evolution: a new perspective : an inquiry into the chemical composition, origin, and evolution of the solar system. Cambridge University Press. pp. 73–75. ISBN 9780521641302.
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