A neon-E-rich phase in the Orgueil carbonaceous chondrite

Details A neon-E-rich phase in the Orgueil carbonaceous chondrite A neon-E-rich phase in the Orgueil carbonaceous chondrite

Dec 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974e%26psl..24..182e&link_type=abstract

Earth and Planetary Science Letters, vol. 24, no. 2, Dec. 1974, p. 182-187.

Computer Science

36

Carbonaceous Meteorites, Interstellar Matter, Meteoritic Composition, Neon Isotopes, Orgueil Meteorite, Geochemistry, Isotope Separation, Silicates, Trapped Particles

Scientific paper

Attention is given to a procedure for separating a silicate fraction which contains large amounts of neon-E from the carbonaceous chondrite Orgueil. In this fraction a 20Ne/22Ne ratio of 4.56 is measured. The obtained data support the hypothesis that neon-E might be associated with interstellar dust grains of the type not fully homogenized with the solar system and which retain some of their trapped neon. Neon results in a three-isotope diagram are presented.

Affiliated with

Also associated with

No associations

Rating

A neon-E-rich phase in the Orgueil carbonaceous chondrite does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with A neon-E-rich phase in the Orgueil carbonaceous chondrite, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A neon-E-rich phase in the Orgueil carbonaceous chondrite will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1337819