2010/07/22 by Nicolas Dauphas, Laurent Remusat, Laurent Rémusat +10 · 1 citation
Medicine · Physics and Astronomy · #Astro and Planetary Science #Astronomy #Astrophysics #Boron Compounds in Chemistry #Chromium #Isotope #Metallurgy #Nanoparticle #Neutron #Neutron star #Nuclear Physics and Applications #Nuclear physics #Nucleosynthesis #Physics #Supernova #astro-ph.SR
paper · pdf · doi:10.1088/0004-637x/720/2/1577
accepted for publication in the Astrophysical Journal; 41 pages, 13 figures, 4 tables
arxiv created 2010/07/22 · openalex publication_date 2010/08/23 · arxiv updated 2015/05/19 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
Neutron-rich isotopes with masses near that of iron are produced in Type Ia and II supernovae (SNeIa and SNeII). Traces of such nucleosynthesis are found in primitive meteorites in the form of variations in the isotopic abundance of 54 Cr, the most neutron-rich stable isotope of chromium. The hosts of these isotopic anomalies must be presolar grains that condensed in the outflows of SNe, offering the opportunity to study the nucleosynthesis of iron-peak nuclei in ways that complement spectroscopic observations and can inform models of stellar evolution. However, despite almost two decades of extensive search, the carrier of 54 Cr anomalies is still unknown, presumably because it is fine grained and is chemically labile. Here, we identify in the primitive meteorite Orgueil the carrier of 54 Cr anomalies as nanoparticles (<100 nm), most likely spinels that show large enrichments in 54 Cr relative to solar composition ( 54 Cr/ 52 Cr ratio >3.6 × solar). Such large enrichments in 54 Cr can only be produced in SNe. The mineralogy of the grains supports condensation in the O/Ne–O/C zones of an SNII, although a Type Ia origin cannot be excluded. We suggest that planetary materials incorporated different amounts of these nanoparticles, possibly due to late injection by a nearby SN that also delivered 26 Al and 60 Fe to the solar system. This idea explains why the relative abundance of 54 Cr and other neutron-rich isotopes vary between planets and meteorites. We anticipate that future isotopic studies of the grains identified here will shed new light on the birth of the solar system and the conditions in SNe.