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2016 | OriginalPaper | Chapter

2. Raw Materials

Author : Claudio Vita-Finzi

Published in: A History of the Solar System

Publisher: Springer International Publishing

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Abstract

A presolar (molecular) cloud supplied dust and gas to the solar nebula ancestral to our solar system. The dust originated in different varieties of star including low mass stars at the end of their evolution and exploding supernovae. They include silicates and graphite. The gas is predominantly molecular hydrogen (H2). Calcium-aluminium-rich inclusions (CAIs) and chondrules are found in meteorites which yield some of the oldest ages for the solar system. Polycyclic aromatic hydrocarbons (PAHs) are widespread; at low temperatures they may be transformed into more complex organic molecules by UV radiation.

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Metadata
Title
Raw Materials
Author
Claudio Vita-Finzi
Copyright Year
2016
Book
A History of the Solar System

Print ISBN: 978-3-319-33848-4

Electronic ISBN: 978-3-319-33850-7

Copyright Year: 2016

DOI
https://doi.org/10.1007/978-3-319-33850-7_2