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 ID | 1902 |
| Article Category | Article |
| Authors | Salmeron, Raquel (Author) and Ireland, Trevor (Author) |
| Journal Title | Meteoritics and Planetary Science |
| Journal Citation | 47 (12), pp. 1-19 |
| Number of Pages | 19 |
| Year | 2012 |
| Publisher | John Wiley & Sons |
| Place of Publication | United Kingdom |
| ISSN | 1086-9379 |
| 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. |
| Keywords | Aluminum-rich inclusion; t-tauriprotoplanetary disks; refractory inclusions; accretion disks; isotope heterogeneity; crystalline silicates; ambipolar-diffusion; molecular clouds; young objects |
| ANZSRC Field of Research 2020 | 510107. Planetary science (excl. solar system and planetary geology) |
| 510109. Stellar astronomy and planetary systems | |
| Byline Affiliations | Australian National University |
| Institution of Origin | University of Southern Queensland |
| Funding source | Grant ID DP120101792 |
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