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Predicting the water content of interstellar objects from galactic star formation histories

Abstract:

Planetesimals inevitably bear the signatures of their natal environment, preserving in their composition a record of the metallicity of their system's original gas and dust, albeit one altered by the formation processes. When planetesimals are dispersed from their system of origin, this record is carried with them. As each star is likely to contribute at least 1012 interstellar objects (ISOs), the Galaxy's drifting population of ISOs provides an overview of the properties of its stellar population through time. Using the EAGLE cosmological simulations and models of protoplanetary formation, our modeling predicts an ISO population with a bimodal distribution in their water mass fraction: objects formed in low-metallicity, typically older, systems have a higher water fraction than their counterparts formed in high-metallicity protoplanetary disks, and these water-rich objects comprise the majority of the population. Both detected ISOs seem to belong to the lower water fraction population; these results suggest they come from recently formed systems. We show that the population of ISOs in galaxies with different star formation histories will have different proportions of objects with high and low water fractions. This work suggests that it is possible that the upcoming Vera C. Rubin Observatory Legacy Survey of Space and Time will detect a large enough population of ISOs to place useful constraints on models of protoplanetary disks, as well as galactic structure and evolution.

Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.3847/2041-8213/ac41d5

Authors


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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Oxford college:
Mansfield College
Role:
Author
ORCID:
0000-0001-5578-359X


Publisher:
IOP Science
Journal:
Astrophysical Journal Letters More from this journal
Volume:
294
Article number:
1
Publication date:
2021-12-29
Acceptance date:
2021-12-09
DOI:
EISSN:
2041-8213
ISSN:
2041-8205


Language:
English
Keywords:
Pubs id:
1226769
Local pid:
pubs:1226769
Deposit date:
2021-12-21

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