Chemical Abundances of Rock-forming Elements of Cometary Streams Obtained from Meteor Spectroscopy

Details Chemical Abundances of Rock-forming Elements of Cometary Streams Obtained from Meteor Spectroscopy Chemical Abundances of Rock-forming Elements of Cometary Streams Obtained from Meteor Spectroscopy

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003lpi....34.1029l&link_type=abstract

34th Annual Lunar and Planetary Science Conference, March 17-21, 2003, League City, Texas, abstract no.1029

Computer Science

1

Scientific paper

Relative chemical abundances of Si, Mg, Fe and Ca obtained from meteor
spectroscopy of eight fireballs belonging to well-known cometary streams
(Perseid, Cignid, Andromedid, Leonid) are discussed and compared to
1P/Halley dust, IDPs and CI chondrites.

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