Formation of amorphous ice in the protoplanetary nebula

Details Formation of amorphous ice in the protoplanetary nebula Formation of amorphous ice in the protoplanetary nebula

Oct 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994p%26ss...42..865m&link_type=abstract

Planetary and Space Science (ISSN 0032-0633), vol. 42, no. 10, p. 865-870

Astronomy and Astrophysics

Astronomy

14

Astronomical Models, Comet Nuclei, Ice Formation, Nebulae, Protoplanets, Condensing, Solar Heating, Solar System Evolution, Sublimation

Scientific paper

The criteria for formation of amorphous ice in different models of the
protoplanetary nebula are developed. Assuming that comets are composed
mostly of amorphous ice, it is shown that the inner boundary of
formation of cometary nuclei is about 7 AU.

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