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Possible mass distributions in the nebulae of other solar systems

โœ Scribed by Wilbur K. Brown


Publisher
Springer Netherlands
Year
1987
Tongue
English
Weight
767 KB
Volume
37
Category
Article
ISSN
1573-0794

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โœฆ Synopsis


The supernova shell fragmentation model of solar system formation -previously shown to be successful in describing the mass distribution of our solar system -is used to calculate the mass distributions of other solar nebulae.


๐Ÿ“œ SIMILAR VOLUMES


The distributions and ages of refractory
โœ F.J. Ciesla ๐Ÿ“‚ Article ๐Ÿ“… 2010 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 680 KB

Refractory objects such as Calcium, Aluminum-rich Inclusions, Amoeboid Olivine Aggregates, and crystalline silicates, are found in primitive bodies throughout our Solar System. It is believed that these objects formed in the hot, inner solar nebula and were redistributed during the mass and angular