Science Advances
Supplementary Materials
Oxygen isotopic heterogeneity in the early Solar System inherited from the protosolar molecular cloud
Alexander N. Krot, Kazuhide Nagashima, James R. Lyons, Jeong-Eun Lee, Martin Bizzarro
This PDF file includes:
- Mineralogical observations
- Gas/dust fractionation during disk accretion
- Solar nebula model
- Radial transport time scales assuming an active MRI
- FUV and x-ray surfaces of solar nebula
- Inward flux of surface disk material
- Time scales for CO photodissociation by FUV and H ionization by x-rays
- Time scales for loss of O onto grains in disk surface and for grains settling
- Δ17O of mixed material in CAI-forming region
- Table S1
- Figs. S1 to S5
- References
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