Cometary Delivery of Organic Molecules to the Early Earth
- 27 July 1990
- journal article
- research article
- Published by American Association for the Advancement of Science (AAAS) in Science
- Vol. 249 (4967), 366-373
- https://doi.org/10.1126/science.11538074
Abstract
It has long been speculated that Earth accreted prebiotic organic molecules important for the origins of life from impacts of carbonaceous asteroids and comets during the period of heavy bombardment 4.5 x 10(9) to 3.8 x 10(9) years ago. A comprehensive treatment of comet-asteroid interaction with the atmosphere, surface impact, and resulting organic pyrolysis demonstrates that organics will not survive impacts at velocities greater than about 10 kilometers per second and that even comets and asteroids as small as 100 meters in radius cannot be aerobraked to below this velocity in 1-bar atmospheres. However, for plausible dense (10-bar carbon dioxide) early atmospheres, we find that 4.5 x 10(9) years ago Earth was accreting intact cometary organics at a rate of at least approximately 10(6) to 10(7) kilograms per year, a flux that thereafter declined with a half-life of approximately 10(8) years. These results may be put in context by comparison with terrestrial oceanic and total biomasses, approximately 3 x 10(12) kilograms and approximately 6 x 10(14) kilograms, respectively.Keywords
This publication has 74 references indexed in Scilit:
- Extraterrestrial amino acids in Cretaceous/Tertiary boundary sediments at Stevns Klint, DenmarkNature, 1989
- The chemistry of cometsPhilosophical Transactions of the Royal Society of London. Series A, Mathematical and Physical Sciences, 1988
- Cometary magnitude distribution and the ratio between the numbers of long- and short-period cometsIcarus, 1988
- Unusual stable isotope ratios in amino acid and carboxylic acid extracts from the Murchison meteoriteNature, 1987
- Chemical effects of large impacts on the Earth's primitive atmosphereNature, 1986
- Carbon dioxide on the early earthOrigins of Life and Evolution of Biospheres, 1985
- Terrestrial impactors at geological boundary events: comets or asteroids?Nature, 1985
- The composition of the Trojan asteroidsNature, 1980
- Expressions for the internal energy and entropy of water over a wide range of thermodynamic parametersFluid Dynamics, 1971
- Early Terrestrial Conditions That May Have Favored Organic SynthesisScience, 1908