Abstract
The origin of the isotopically anomalous oxygen components found in various meteorites can be attributed to an intense irradiation of the solar system materials during the T-Tauri phase of the young Sun. Such an irradiation is expected to have produced large isotopic anomalies for oxygen, but not for silicon, in the meteorites.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
