A Solar System formation analogue in the Ophiuchus star-forming complex

Author(s)
John C. Forbes, João Alves, Douglas N. C. Lin
Abstract

Anomalies among the daughter nuclei of the extinct short-lived radionuclides in calcium-aluminium-rich inclusions indicate that the Solar System must have been born near a source of the short-lived radionuclides so that they could be incorporated before they decayed away. γ-rays from one such living short-lived radionuclide, 26Al, are detected in only a few nearby star-forming regions. Here we employ multiwavelength observations to demonstrate that one such region, Ophiuchus, containing many prestellar cores that may serve as analogues for the emerging Solar System, is inundated with 26Al from the neighbouring Upper Scorpius association, and so may provide concrete guidance for how short-lived radionuclide enrichment proceeded in the Solar System, complementary to the meteoritics. We demonstrate via Bayesian forward modelling drawing on a wide range of observational and theoretical results that this 26Al probably (1) arises from supernova explosions, (2) arises from multiple stars, (3) has enriched the gas before the formation of the cores and (4) gives rise to a broad distribution of core enrichment spanning about two orders of magnitude. This means that if the spread in calcium-aluminium-rich inclusion ages is small, as it is in the Solar System, protoplanetary disks must suffer a global heating event.

Organisation(s)
Department of Astrophysics
External organisation(s)
Flatiron Institute, University of California, Santa Cruz, Tsinghua University, Harvard University
Journal
Nature Astronomy
Volume
5
Pages
1009–1016
DOI
https://doi.org/10.1038/s41550-021-01442-9
Publication date
08-2021
Peer reviewed
Yes
Austrian Fields of Science 2012
103004 Astrophysics, 103003 Astronomy
Keywords
Portal url
https://ucris.univie.ac.at/portal/en/publications/a-solar-system-formation-analogue-in-the-ophiuchus-starforming-complex(635cbf76-0bd3-4a60-9d7b-ac1364f0fad0).html