Beryllium-10 production in gaseous protoplanetary disks and implications for the astrophysical setting of refractory inclusions

Muséum national d’Histoire naturelle, IMPMC, Département Origines et Evolution, 57 rue Cuvier, 75005 Paris, France
e-mail: emmanuel.jacquet@mnhn.fr

Received: 30 November 2018
Accepted: 7 March 2019

Abstract

Calcium-aluminum-rich inclusions (CAIs), the oldest known solids of the solar system, show evidence for the past presence of short-lived radionuclide beryllium-10, which was likely produced by spallation during protosolar flares. While such ¹⁰Be production has hitherto been modeled at the inner edge of the protoplanetary disk, I calculate here that spallation at the disk surface may reproduce the measured ¹⁰Be/⁹Be ratios at larger heliocentric distances. Beryllium-10 production in the gas prior to CAI formation would dominate that in the solid. Interestingly, provided the Sun’s proton to X-ray output ratio does not decrease strongly, ¹⁰Be/⁹Be at the CAI condensation front would increase with time, explaining the reduced values in a (presumably early) generation of CAIs with nucleosynthetic anomalies. CAIs thus need not have formed very close to the Sun and may have condensed at 0.1–1 AU where sufficiently high temperatures originally prevailed.