A possible mechanism of origin of heavy elements in the solar system
E.P. Tito, V.I. Pavlov

TL;DR
This paper hypothesizes that a collision involving a neutron-rich compact object contributed to the formation of heavy elements in the early solar system and influenced terrestrial planet formation.
Contribution
It introduces a novel hypothesis linking neutron-rich compact object collisions to heavy element enrichment in the solar system.
Findings
Proposes a collision mechanism for heavy element origin.
Suggests a link between NRCO impacts and terrestrial planet formation.
Provides a new perspective on solar system chemical enrichment.
Abstract
We advance a hypothesis that a collision of a neutron-rich compact object (NRCO) with a massive dense object of the early solar system was responsible for the heavy element enrichment of the system and for the formation of the terrestrial planets.
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Taxonomy
TopicsAstro and Planetary Science · Stellar, planetary, and galactic studies · Gamma-ray bursts and supernovae
