The role of protostellar jets in star formation and the evolution of the early solar system: Astrophysical and meteoritical perspectives

Article


Salmeron, Raquel and Ireland, Trevor. 2012. "The role of protostellar jets in star formation and the evolution of the early solar system: Astrophysical and meteoritical perspectives." Meteoritics and Planetary Science. 47 (12), pp. 1-19. https://doi.org/10.1111/maps.12029
Article Title

The role of protostellar jets in star formation and the evolution of the early solar system: Astrophysical and meteoritical perspectives

ERA Journal ID1902
Article CategoryArticle
AuthorsSalmeron, Raquel (Author) and Ireland, Trevor (Author)
Journal TitleMeteoritics and Planetary Science
Journal Citation47 (12), pp. 1-19
Number of Pages19
Year2012
PublisherJohn Wiley & Sons
Place of PublicationUnited Kingdom
ISSN1086-9379
Digital Object Identifier (DOI)https://doi.org/10.1111/maps.12029
Web Address (URL)https://onlinelibrary.wiley.com/doi/full/10.1111/maps.12029
Abstract

The rock record from the early solar system indicates high-temperature thermal processing sufficient to melt refractory oxides and silicates. The astrophysical context for the formation and evolution of our solar system, from a molecular cloud to a “clean” planetary system, is difficult to constrain tightly because of the large scales and lack of resolution of astronomical observations. Protostellar jets and winds, commonly associated with forming stars, are likely to play a role in heating and redistribution of the processed material in the solar system. We have recently proposed that disk-winds can cause melting of small inclusions to distances out to several AU. Particularly energetic outbursts, such as the FU-Orionis and EXor events, occur over relatively short time scales (approximately 100 and 1 yr, respectively), and are probably events related to formation of the refractory solids present in primitive meteorites.

KeywordsAluminum-rich inclusion; t-tauriprotoplanetary disks; refractory inclusions; accretion disks; isotope heterogeneity; crystalline silicates; ambipolar-diffusion; molecular clouds; young objects
ANZSRC Field of Research 2020510107. Planetary science (excl. solar system and planetary geology)
510109. Stellar astronomy and planetary systems
Byline AffiliationsAustralian National University
Institution of OriginUniversity of Southern Queensland
Funding source
Grant ID
DP120101792
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