Isotopically Primitive Interplanetary Dust Particles of Cometary Origin: Evidence from Nitrogen Isotopic Compositions

Details Isotopically Primitive Interplanetary Dust Particles of Cometary Origin: Evidence from Nitrogen Isotopic Compositions Isotopically Primitive Interplanetary Dust Particles of Cometary Origin: Evidence from Nitrogen Isotopic Compositions

Mar 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004lpi....35.1281f&link_type=abstract

35th Lunar and Planetary Science Conference, March 15-19, 2004, League City, Texas, abstract no.1281

Computer Science

15

Scientific paper

We report on a subgroup of isotopically primitive IDPs characterized by
anomalous bulk N compositions and abundant ^15N-rich hotspots,
occasionally with associated C isotopic anomalies. These IDPs have a
presolar silicate grain abundance of ~450 ppm.

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