The Solar Nebula's First Accretionary Particles (FAPs) — Are They Preserved in Collected Interplanetary Dust Samples?

Details The Solar Nebula's First Accretionary Particles (FAPs) — Are They Preserved in Collected Interplanetary Dust Samples? The Solar Nebula's First Accretionary Particles (FAPs) — Are They Preserved in Collected Interplanetary Dust Samples?

Mar 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004lpi....35.1944b&link_type=abstract

35th Lunar and Planetary Science Conference, March 15-19, 2004, League City, Texas, abstract no.1944

Physics

1

Scientific paper

The first generation of accretionary particles in the solar nebula
initiated the growth processes that led to the formation of rocks,
boulders, planetismals and ultimately planets. The first (also the
fundamental) accretionary particles (FAPs) were grains of nebular and
pre-solar origin.

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