Literature DB >> 11538074

Cometary delivery of organic molecules to the early Earth.

C F Chyba1, P J Thomas, L Brookshaw, C Sagan.   

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.

Entities:  

Keywords:  NASA Discipline Exobiology; NASA Discipline Number 52-20; NASA Program Exobiology; Non-NASA Center

Mesh:

Substances:

Year:  1990        PMID: 11538074     DOI: 10.1126/science.11538074

Source DB:  PubMed          Journal:  Science        ISSN: 0036-8075            Impact factor:   47.728


  69 in total

1.  The occurrence of Jovian planets and the habitability of planetary systems.

Authors:  J Lunine
Journal:  Proc Natl Acad Sci U S A       Date:  2001-01-30       Impact factor: 11.205

2.  Probing the structure of cometary ice.

Authors:  M A Wilson; A Pohorille; P Jenniskens; D F Blake
Journal:  Orig Life Evol Biosph       Date:  1995-06       Impact factor: 1.950

3.  The origin of life--did it occur at high temperatures?

Authors:  S L Miller; A Lazcano
Journal:  J Mol Evol       Date:  1995       Impact factor: 2.395

4.  How long did it take for life to begin and evolve to cyanobacteria?

Authors:  A Lazcano; S L Miller
Journal:  J Mol Evol       Date:  1994-12       Impact factor: 2.395

Review 5.  Carbonaceous micrometeorites and the origin of life.

Authors:  M Maurette
Journal:  Orig Life Evol Biosph       Date:  1998-10       Impact factor: 1.950

Review 6.  Asymmetric photoreactions as the origin of biomolecular homochirality: a critical review.

Authors:  Alain Jorissen; Corinne Cerf
Journal:  Orig Life Evol Biosph       Date:  2002-04       Impact factor: 1.950

7.  Survivability of bacteria ejected from icy surfaces after hypervelocity impact.

Authors:  Mark J Burchell; James A Galloway; Alan W Bunch; Pedro F B Brandão
Journal:  Orig Life Evol Biosph       Date:  2003-02       Impact factor: 1.950

Review 8.  Cosmic carbon chemistry: from the interstellar medium to the early Earth.

Authors:  Pascale Ehrenfreund; Jan Cami
Journal:  Cold Spring Harb Perspect Biol       Date:  2010-06-16       Impact factor: 10.005

Review 9.  Earth's earliest atmospheres.

Authors:  Kevin Zahnle; Laura Schaefer; Bruce Fegley
Journal:  Cold Spring Harb Perspect Biol       Date:  2010-06-23       Impact factor: 10.005

10.  Steps towards the formation of a protocell: the possible role of short peptides.

Authors:  Maya Fishkis
Journal:  Orig Life Evol Biosph       Date:  2007-09-14       Impact factor: 1.950

View more

北京卡尤迪生物科技股份有限公司 © 2022-2023.