Advanced search
Start date
Betweenand
Related content
(Reference retrieved automatically from Web of Science through information on FAPESP grant and its corresponding number as mentioned in the publication by the authors.)

Chemical evidence for planetary ingestion in a quarter of Sun-like stars

Full text
Author(s):
Spina, Lorenzo [1, 2, 3] ; Sharma, Parth [2, 3] ; Melendez, Jorge [4] ; Bedell, Megan [5] ; Casey, Andrew R. [2, 3] ; Carlos, Marilia [6] ; Franciosini, Elena [7] ; Vallenari, Antonella [1]
Total Authors: 8
Affiliation:
[1] INAF, Osservatorio Astron Padova, Padua - Italy
[2] Monash Univ, Sch Phys & Astron, Clayton, Vic - Australia
[3] ARC Ctr Excellence All Sky Astrophys Three Dimens, Canberra, ACT - Australia
[4] Univ Sao Paulo, Dept Astron, IAG, Sao Paulo - Brazil
[5] Simons Fdn, Flatiron Inst, New York, NY - USA
[6] Univ Padua, Dipartimento Fis & Astron Galileo Galilei, Padua - Italy
[7] INAF, Osservatorio Astrofis Arcetri, Florence - Italy
Total Affiliations: 7
Document type: Journal article
Source: NATURE ASTRONOMY; v. 5, n. 11 AUG 2021.
Web of Science Citations: 0
Abstract

Chemical inhomogeneities between the two members of a binary star system, where the stars presumably are formed from the same material, could be due to planetary engulfment. Such a fate has befallen planets around a quarter of Sun-like (in temperature and surface gravity) stars, according to this sample of more than 100 binary systems. Stellar members of binary systems are formed from the same material, and therefore they should be chemically identical. However, recent studies have unveiled chemical differences between the two members of binary pairs composed of Sun-like stars. These chemically inhomogeneous binaries represent one of the most contradictory examples in stellar astrophysics and a source of tension between theory and observations. It is still unclear whether the abundance variations are the result of inhomogeneities in the protostellar gas clouds or are due to planet engulfment events that occurred after the stellar formation. The former scenario undermines the general belief that the chemical makeup of stars provides the fossil information of the environment in which they formed, whereas the second scenario would shed light on the possible evolutionary paths of planetary systems. Our study provides compelling evidence in favour of the planet engulfment scenario. We also establish that planet engulfment events occur in Sun-like stars with a 20-35% probability. Therefore, an important fraction of planetary systems undergo very dynamical evolutionary paths that critically modify their architectures, unlike our calm Solar System. This study opens the possibility of using chemical abundances of stars to identify which ones are the most likely to host Solar System analogues. (AU)

FAPESP's process: 18/04055-8 - High precision spectroscopy: from the first stars to planets
Grantee:Jorge Luis Melendez Moreno
Support Opportunities: Research Projects - Thematic Grants