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Prebiotic Matter in Interstellar Molecules

Published online by Cambridge University Press:  04 August 2017

Ronald D. Brown
Ronald D. Brown*
Affiliation:
Chemistry Department, Monash University, Clayton, Victoria, 3168, Australia

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With the discovery of the first polyatomic molecules, NH3, H2O and H2CO in 1968/9 there was immediate speculation as to how far biological chemical evolution - from atoms to small carbon compounds of biological significance - could have occurred in the Galaxy. There was also potential conflict with the canonical scientific view of the origin of life, traceable to the production of simple bio-molecules from the influence of energetic atmospheric events on the simple gaseous mixture (CH4, H2, H2O and NH3) presumed to compose the atmosphere of the very young Earth.

Information

Type
Section III. Planetary, Interplanetary and Interstellar Organic Matter
Information
Symposium - International Astronomical Union , Volume 112: The Search for Extraterrestrial Life: Recent Developments , 1985, pp. 123 - 137
Copyright
Copyright © Reidel 1985 

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