The Sun's origin and composition: implications from meteorite studies

Details The Sun's origin and composition: implications from meteorite studies The Sun's origin and composition: implications from meteorite studies

Nov 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.500..787m&link_type=abstract

In: Proceedings of Asteroids, Comets, Meteors - ACM 2002. International Conference, 29 July - 2 August 2002, Berlin, Germany. Ed

Computer Science

1

Sun: Chemical Composition, Meteorites

Scientific paper

In the 1970s meteorite studies indicated the Sun might be a supernova
remnant. Decay products of short-lived nuclides, nucleogenetic isotopic
anomalies in meteorites, and evidence of mass separation in the Sun
confirmed that iron is the Sun's most abundant element.

Affiliated with

Also associated with

No associations

Rating

The Sun's origin and composition: implications from meteorite studies 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 The Sun's origin and composition: implications from meteorite studies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Sun's origin and composition: implications from meteorite studies will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-738701