Observational constraints on the origin of the elements. IV: The  standard composition of the Sun

[en] The chemical composition of the Sun is requested in the context of various studies in astrophysics, among them in the calculation of the standard solar models (SSMs), which describe the evolution of the Sun from the pre-main-sequence to its present age. In this work, we provide a critical re-analysis of the solar chemical abundances and corresponding SSMs. For the photospheric values, we employ new high-quality solar observational data collected with the IAG facility, state-of-the art non-equilibrium modelling, new oscillator strengths, and different atmospheric models, including the MARCS model, but also averages based on Stagger and CO5BOLD 3D radiation-hydrodynamics simulations of stellar convection. We perform new calculations of oscillator strengths for transitions in O I and N I. For O I - the critical element for the interior models - calculations are carried out using several independent methods. We find unprecedented agreement between the new estimates of transition probabilities, thus supporting our revised solar oxygen abundance. We also provide new estimates of the noble gas Ne abundance. We investigate our results in comparison with the previous estimates. We discuss the consistency of our photospheric measurements with meteoritic values taking into account systematic and correlated errors. Finally, we provide revised chemical abundances, leading to a new value of the solar photospheric present-day metallicity $Z/X = 0.0225$, and employ them in the calculations of the SSM. We find that the puzzling mismatch between the helioseismic constraints on the solar interior structure and the model is resolved with the new chemical composition.

Disciplines :

Physique

Auteur, co-auteur :

Magg, Ekaterina

Bergemann, Maria

Serenelli, Aldo

Bautista, Manuel

Plez, Bertrand

Heiter, Ulrike

Gerber, Jeffrey M.

Ludwig, Hans-Günter

Basu, Sarbani

Ferguson, Jason W.

Plus d'auteurs (4 en +)

Langue du document :

Anglais

Titre :

Observational constraints on the origin of the elements. IV: The standard composition of the Sun

Date de publication/diffusion :

20 mai 2022

Titre du périodique :

Astronomy and Astrophysics

ISSN :

0004-6361

eISSN :

1432-0746

Maison d'édition :

EDP Sciences

Volume/Tome :

661

Pagination :

A140

Peer reviewed :

Peer reviewed vérifié par ORBi

URL complémentaire :

https://www.aanda.org/10.1051/0004-6361/202142971/pdf

Institut de recherche :

Complexys

Commentaire :

accepted for publication in A&A

Disponible sur ORBi UMONS :

depuis le 16 juin 2022

Statistiques

Nombre de vues

36 (dont 3 UMONS)

Nombre de téléchargements

4 (dont 4 UMONS)

Voir plus de statistiques

citations Scopus^®

127

citations Scopus^®
sans auto-citations

112

OpenCitations

citations OpenAlex

129

Bibliographie

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